Tag: space

  • Epic Trailer for 'The Martian' Questions the Value of a Human Life in Space

    An epic new trailer for the movie “The Martian” looks even more intense than the last one, and it raises some intriguing questions about the value of human life in space exploration.

    Set to the howling Jimi Hendrix song “All Along the Watchtower,” the new trailer for “The Martian,” directed by Ridley Scott, features some thrilling (and stressful) clips of astronauts braving Martian storms, rocket launches and other near-death experiences. The film focuses on astronaut Mark Watney (played by Matt Damon), who is mistakenly presumed dead by his fellow Mars explorers and is left behind on the Red Planet.

    When NASA officials discover that Watney is alive, they must decide whether to rescue him and, in doing so, risk the lives of the other six crewmembers. At one point in the trailer, the director of NASA (played by Jeff Daniels) grapples with the decision, stating, “It’s bigger than one person,” to which another character replies, “No. It’s not.” The film raises the question: If a person willingly embraces the risks of space exploration, should he or she be rescued at all costs? [Photos from ‘The Martian’]

    In an earlier trailer, Watney makes clear that he understands the risks of space exploration, saying, “It’s space. It doesn’t cooperate. I guarantee you that at some point, everything’s going to go south on you. And you’re going to say, ‘This is it. This is how I end.’”

    In the new trailer, we hear the end of that quote, in which Watney goes on to say, “Now, you can either accept that, or you can get to work.”

    Stranded on Mars with only enough food and water to last 50 days, Watney must wait four years for a rescue mission to arrive. As a result, he’s forced to find a way to grow food on a lifeless planet, and produce water. Other threats to his life and his safety arise, and he proclaims at the end, “No matter what happens, tell the world, tell my family, that I never stopped fighting to make it home.”

    Meanwhile, NASA and Watney’s crewmates must decide whether to rescue “the Martian.” By sending the crew back to the Red Planet, the agency would be risking six lives to save one, and thus rejects the proposal. The crewmembers must then decide whether they will not only risk their lives, but declare mutiny by going against NASA’s orders.

    Astronauts in 'The Martian'

    In the new movie “The Martian,” a group of astronauts must decide if they should rescue their stranded crewmate from the surface of Mars.
    Credit: 20th Century Fox/The Martian

    The plot of the film is a thought experiment: If a person understands the risks of space exploration, should the rest of humanity make every possible effort to save that person if (or when) things go wrong? Is NASA’s responsibility different from the individual responsibilities of its astronauts? 

    These are questions that humanity will have to seriously consider if a program like Mars One gets off the ground: If a private company sends people to space and something goes wrong, how much money and effort should the rest of the world spend to save them? Is it directly comparable to instances where hikers become lost or stranded, setting off costly and risky rescue missions? What do we lose if we reduce the value of one human life compared to multiple lives, and what do we lose if we don’t? 

    We’re excited to see how the movie tackles this question, and how closely it will follow the book by Andy Weir on which the movie is based. The film is set to be released Oct. 2 and, in addition to Damon and Daniels, stars Jessica Chastain, Kristen Wiig, Kate Mara, Michael Peña, Chiwetel Ejiofor and Donald Glover.

    Follow Calla Cofield @callacofieldFollow us @Spacedotcom, Facebook and Google+. Original article on Space.com.

  • 'Star Trek' Fan Film Recruits Real-Life Astronaut Samantha Cristoforetti

    Astronaut Samantha Cristoforetti in 'Voyager' Costume
    Astronaut Samantha Cristoforetti, the record-holder for the longest continuous spaceflight by a woman, joined on as a cast member in the fan project “Star Trek: Axanar.” In April, she tweeted this photo posing in the International Space Station in a “Star Trek: Voyager”-style uniform.
    Credit: ESA/NASA

    After spending 199 days on the International Space Station, a European astronaut is readying for her next big mission: joining an independent “Star Trek” production.

    Samantha Cristoforetti, an Italian astronaut for the European Space Agency, will join the fan-produced film “Star Trek: Axanar” in an as-yet-undisclosed role, film officials said in a blog post. Cristoforetti was the first Italian woman in space during the space station’s Expeditions 42 and 43, which wrapped up in June.

    The news comes as the production wrapped up a crowdfunding campaign  that raised $487,076, nearly double the original goal of $250,000. Filming will begin in early 2016.

    “Star Trek: Axanar” follows the story of Garth of Izar, a character who was introduced in the “Star Trek: The Original Series” episode “Whom Gods Destroy.” Garth’s story takes place about 21 years before the events of the first “Star Trek” episode, “Where No Man Has Gone Before.”

    The new, full-length film will follow from a 20-minute crowdfunded prelude that was released last year. Stars in the feature-length film include Richard Hatch, Kate Vernon (both of “Battlestar: Galactica”), Gary Graham (“Star Trek: Enterprise”) and Tony Todd (“Candyman”, “Chuck”, “24”). It is led by Executive Producer Alec Peters.

    After a crowdfunding campaign last year on Kickstarter that raised more than $600,000, the filmmakers have decided to break the feature-length film into four episodes costing at least $250,000 each.

    The base goal for the work is $1 million, but the filmmakers need at least $1.32 million in total to cover costs from using the crowdfunding site Indiegogo, which takes a cut of projects funded on its site, as well as “ongoing studio costs” and “payment processing,” according to the Indiegogo page.

    Cristoforetti wouldn’t be the first astronaut to appear on Star Trek. In 1993, NASA astronaut Mae Jemison played a small role on “Star Trek: The Next Generation.”

    Follow Elizabeth Howell @howellspace, or Space.com @Spacedotcom. We’re also on Facebook and Google+. Original article on Space.com.

  • Blast-Off! Japan's HTV Cargo Craft Launches To ISS | Video

    Credit: JAXA/NASA

  • To Pluto and Beyond: Planetarium Show Wows Space Fans

    Global Mosaic of Pluto Shown in True Color Image
    NASA’s New Horizons spacecraft obtained this view of Pluto at a distance of about 280,000 miles (450,000 kilometers) on July 14, 2015.
    Credit: NASA

    NEW YORK — The first-ever flyby of Pluto left scientists and the public wide-eyed, and the surprises will likely keep on coming.

    NASA’s New Horizons spacecraft zoomed through the Pluto system on July 14, coming within 7,800 miles (12,500 kilometers) of the dwarf planet’s surface. Images captured by the probe have revealed a world with its own cryogenic geology, situated in a diverse array of moons.

    At the American Museum of Natural History here, Emily Rice, an astrophysicist at the College of Staten Island, and Jackie Faherty, an astronomer with the Carnegie Institute, took an audience on a journey with New Horizons last week to highlight the science. [New Horizons’ Pluto Flyby: Complete Coverage]

    The Aug. 11 presentation was in the museum’s Hayden Planetarium and used its skylike dome to immerse people in the vastness of space. The show, called “Visiting Pluto and Friends in the 21st Century,” was part of the museum’s “Astronomy Live” series.

    Using new visualization technologies, Rice and Faherty offered views of Pluto and its five moons as New Horizons might have seen them and placed the dwarf planet system in relation to the sun and Earth.

    Carter Emmart, who directs Astrovisualization at the museum’s Rose Center for Earth and Space, Skyped in from Singapore to show off some of the technology, and to talk about how New Horizons made its way through the Pluto system.

    “I’m calling from the future,” he quipped, noting the time difference. (Singapore lies on the other side of the International Date Line.)

    The 3D view showed the shadows of Pluto and gave a feel for how the spacecraft was oriented, and how the craft had to move in space to get the pictures that NASA sent around the world.

    Rice said the accuracy of the flyby was quite good; the probe arrived within 90 seconds of its targeted time.

    “It’s like hitting a hole in one on a golf course in Los Angeles from New York,” she said.

    New Horizons also had to navigate among Pluto’s five moons — Charon, Nix, Hydra, Styx and Kerberos. Styx and Kerberos weren’t discovered until 2011 and 2012, when New Horizons was well on its way to Pluto. (The $720 million mission launched in January 2006.)

    Later in the show, Rice called up an old artist’s rendering of Pluto, which had been created long before New Horizons’ historic flyby. [‪Flying Over Pluto: Ice Mountains and ‘Young’ Plains (Video)]

    “We were so wrong,” she said. The old picture doesn’t show ice mountains, or even a surface that bears much resemblance to the one New Horizons showed.

    Faherty and Rice also demonstrated how New Horizons studied Pluto’s thin atmosphere, using a picture of Pluto “eclipsing” the sun. A hazy ring marked the edge of the dwarf planet, showing that there was some gas diffusing the light. The atmosphere contains methane-based chemicals called tholins.

    “The tholins probably rain out,” Faherty said, adding that they are what give Pluto its reddish-brown color.

    The big highlight of the mission, though, was finding that Pluto’s surface has been reworked in the recent past — it’s smooth in places, and cratered lightly or not at all. This suggests that some sort of internal heat source remained active until relatively recently, and may still be active today, mission scientists have said. 

    “But we don’t know what it is,” Faherty said.

    Many more pictures are coming from New Horizons; they’ll just take a long time to transmit. Mission team members have said the complete flyby data set probably won’t come down to Earth until late 2016. Emmart said the data-transmission rate is akin to that of a dial-up connection, and New Horizons is a good 3 billion miles (4.8 billion km) from Earth..

    Pluto wasn’t the only object that got attention during the planetarium show; Charon did as well. Faherty noted that Charon is “Pluto’s opposite” in that it’s made mostly of water ice rather than mostly rock, methane and nitrogen. She pointed out the tantalizing features that New Horizons saw, such as a large, miles-deep canyon and the dark spot near the moon’s north pole, which has been dubbed Mordor.

    The two scientists also mentioned the dwarf planet Ceres, which is currently being studied by NASA’s orbiting Dawn spacecraft. Dawn has spotted intriguing bright spots on Ceres’ surface that could be ice or salts of some sort; Dawn is moving down to a lower orbit to map the surface and get a better look.

    Then there is the European Space Agency’s Rosetta mission, which began orbiting Comet 67P/Churyumov–Gerasimenko in August 2014 and dropped a lander named Philae onto the icy object’s surface three months later.

    Comet 67P harbored its own surprises. “When they [Rosetta scientists] saw it, they said, ‘Oh damn, it looks like a rubber duck,’” Rice said.

    Philae didn’t manage to land in quite the way the mission planners hoped; it actually bounced off the comet twice and came to rest in a place where it couldn’t get as much sunlight as it needed to run its instruments continually.

    But Philae did gather data for more than two days on the comet’s surface, and the Rosetta mothership continues to study the object from orbit. Rice showed one photo taken by Philae during its November 2014 descent, at a distance of just 30 feet (9 meters) from 67P’s surface. It showed the place where scientists think the lander initially hit the surface. [Surprising Comet Discoveries by Rosetta and Philae (Infographic)]

    Rosetta’s mission will end when the lander is sent into the comet in September 2016. “I would call it crashing; Jackie would call it landing,” Rice said.

    Even Mercury got a place in the sun (no pun intended). NASA’s MESSENGER (Mercury Surface, Space Environment, Geochemistry, and Ranging) mission, which ended in April of this year, gathered a wealth of new data about the small planet, which is smaller than the Jupiter moon Ganymede, the solar system’s largest satellite.

    Rice brought up an emotional moment with one of the mission specialists on MESSENGER. “I asked if he was sad that the mission was over,” she said. “He said he woke up one morning and wanted to look for new images from MESSENGER, and there weren’t any.”

    Its fuel tank empty, MESSENGER was deliberately crashed into the planet’s surface on April 30.

    The show ended with a journey to the Oort Cloud, a huge comet repository that lies perhaps 2 light-years from the sun. None of the objects that inhabit this distant realm have been imaged yet.

    After the presentation, audience members got a chance to ask questions, some about the future of New Horizons. One person asked how long New Horizons would last. Rice noted that the probe’s plutonium power source could keep it going for years yet — perhaps another decade or two. But keeping New Horizons going has less to do with science and engineering than with Earthly politics.

    “It’s all dependent on the funding,” Rice said.

    Another question was whether New Horizons has solar panels in case it might pass another star. “It would take about 100,000 years for it to get to another star,” Rice said. “And it’s going in the wrong direction.” So the probe wasn’t designed with solar panels.

    New Horizons will fly by another object in the Kuiper Belt — the ring of icy bodies beyond Pluto — in 2019 if NASA approves and funds a proposed extended misison.

    “Maybe other Kuiper Belt objects won’t be as sexy as Pluto, but who knows?” Rice said.

    Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.

  • Lagrange Points: Parking Places in Space

    Diagram of the sun-Earth Lagrange points
    Diagram of the Lagrange points associated with the sun-Earth system. 
    Credit: NASA / WMAP Science Team

    A Lagrange point is a location in space where the combined gravitational forces of two large bodies, such as Earth and the sun or Earth and the moon, equal the centrifugal force felt by a much smaller third body. The interaction of the forces creates a point of equilibrium where a spacecraft may be “parked” to make observations.

    These points are named after Joseph-Louis Lagrange, an 18th-century mathematician who wrote about them in a 1772 paper concerning what he called the “three-body problem.” They are also called Lagrangian points and libration points.   

    Structure of Lagrange points

    There are five Lagrange points around major bodies such as a planet or a star. Three of them lie along the line connecting the two large bodies. In the Earth-sun system, for example, the first point, L1, lies between Earth and the sun at about 1 million miles from Earth. L1 gets an uninterrupted view of the sun, and is currently occupied by the Solar and Heliospheric Observatory (SOHO) and the Deep Space Climate Observatory. 

    L2 also lies a million miles from Earth, but in the opposite direction of the sun. At this point, with the Earth, moon and sun behind it, a spacecraft can get a clear view of deep space. NASA’s Wilkinson Microwave Anisotropy Probe (WMAP) is currently at this spot measuring the cosmic background radiation left over from the Big Bang. The James Webb Space Telescope will move into this region in 2018.

    The third Lagrange point, L3, lies behind the sun, opposite Earth’s orbit. For now, science has not found a use for this spot, although science fiction has.

    “NASA is unlikely to find any use for the L3 point since it remains hidden behind the sun at all times,” NASA wrote on a web page about Lagrange points. “The idea of a hidden ‘Planet-X’ at the L3 point has been a popular topic in science fiction writing. The instability of Planet X’s orbit (on a time scale of 150 years) didn’t stop Hollywood from turning out classics like ‘The Man from Planet X.’”

    L1, L2 and L3 are all unstable points with precarious equilibrium. If a spacecraft at L3 drifted toward or away from Earth, it would fall irreversibly toward the sun or Earth, “like a barely balanced cart atop a steep hill,” according to astronomer Neil DeGrasse Tyson. Spacecraft must make slight adjustments to maintain their orbits.

    Points L4 and L5, however, are stable, “like a ball in a large bowl,” according to the European Space Agency. These points lie along Earth’s orbit at 60 degrees ahead of and behind Earth, forming the apex of two equilateral triangles that have the large masses (Earth and the sun, for example) as their vertices.

    Because of the stability of these points, dust and asteroids tend to accumulate in these regions. Asteroids that surround the L4 and L5 points are called Trojans in honor of the asteroids Agamemnon, Achilles and Hector (all characters in the story of the siege of Troy) that are between Jupiter and the Sun. NASA states that there have been thousands of these types of asteroids found in our solar system, including Earth’s only known Trojan asteroid, 2010 TK7.

    L4 and L5 are also possible points for a space colony due to their relative proximity to Earth, at least according to the writings of Gerard O’Neill and related thinkers. In the 1970s and 1980s, a group called the L5 Society promoted this idea among its members. In the late 1980s, it merged into a group that is now known as the National Space Society, an advocacy organization that promotes the idea of forming civilizations beyond Earth.

    Benefits of Lagrange points

    If a spacecraft uses a Lagrange point close to Earth, there are many benefits to the location, the Jet Propulsion Laboratory’s Amy Mainzer told Space.com. 

    Mainzer is principal investigator of NEOWISE, a mission that searches for near-Earth asteroids using the Wide-field Infrared Survey Explorer (WISE) spacecraft that orbits close to our planet. While WISE is doing well with its current three-year mission that concludes in 2016, Mainzer said, a spacecraft placed at a Lagrange point would be able to do more.

    Far from the interfering heat and light of the sun, an asteroid-hunting spacecraft at a Lagrange point would be more sensitive to the tiny infrared signals from asteroids. It could point over a wide range of directions, except very close to the sun. And it wouldn’t need coolant to stay cool, as WISE required for the first phase of its mission between 2009 and 2011 — the location itself would allow for natural cooling. The James Webb Space Telescope will take advantage of the thermal environment at the sun-Earth L2 point to help keep cool.

    L1 and L2 also “allow you to have enormous bandwidth” because over conventional Ka-band radio, the communication speeds are very high, Mainzer said. “Otherwise, the data rates just become very slow,” she said, since a spacecraft in orbit around the sun (known as heliocentric orbit) would eventually drift far from Earth.

    Additional resources

    EDITOR’S RECOMMENDATIONS

  • Radical! Neon Found on the Moon

    LADEE Orbiting the Moon
    An illustration depicts NASA’s Lunar Atmosphere and Dust Environment Explorer (LADEE) spacecraft in orbit above the moon.
    Credit: NASA Ames/Dana Berry

    The moon doesn’t have any gaudy casinos or buzzing diner signs, but it does have neon.

    NASA’s LADEE spacecraft has made the first-ever detection of neon in the wispy lunar atmosphere, which is properly known as an “exosphere” because it’s so thin — about 100 trillion times less dense than that of Earth at sea level.

    “The presence of neon in the exosphere of the moon has been a subject of speculation since the Apollo missions, but no credible detections were made,” study lead author Mehdi Benna, of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and the University of Maryland, Baltimore County, said in a statement. “We were very pleased to not only finally confirm its presence, but to show that it is relatively abundant.” [The Moon: 10 Surprising Lunar Facts]

    But the gas is not abundant enough on the moon to generate the famous neon glow, NASA officials said.

    LADEE — which is short for Lunar Atmosphere and Dust Environment Explorer — studied the moon’s exosphere from orbit for seven months, from September 2013 through the end of its mission in April 2014.

    The spacecraft’s Neutral Mass Spectrometer (NMS) instrument determined that the moon’s atmosphere is composed mainly of helium, argon and neon. Most of this material comes from the solar wind, a diverse stream of particles flowing from the sun at about 1 million mph (1.6 million km/h). (Other elements in the solar wind tend to stick to the lunar surface, because they’re more volatile than helium, argon and neon, NASA officials said.)

    But the NMS data showed that some of the exospheric gases come from moon rocks, via the process of radioactive decay. About 20 percent of the helium probably came from the decay of uranium and thorium, and some of the argon from the decay of potassium-40 into argon-40, researchers said.

    “We were also surprised to find that argon-40 creates a local bulge above an unusual part of the moon’s surface, the region containing [the dark volcanic plains] Mare Imbrium and Oceanus Procellarum,” Benna said. “One could not help [but] notice that this region happens to be the place where potassium-40 is most abundant on the surface. So there may be a connection between the atmospheric argon, the surface potassium and deep interior sources.”

    LADEE’s measurements also revealed that argon abundance changed by about 25 percent over the course of the spacecraft’s mission, possibly as a result of outgassing caused by the Earth’s strong gravitational tug, researchers said.

    The new results, which were published May 28 in the journal Geophysical Research Letters, should give scientists a better understanding of exospheres in general, and that of the moon in particular, researchers said.

    “It’s critical to learn about the lunar exosphere before sustained human exploration substantially alters it,” Benna said.

    Follow Mike Wall on Twitter @michaeldwall and Google+. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.

  • Starship Enterprise vs. Superman: Who's the Fastest Sci-Fi Spacefarer? (Graphic)

    If the fictional USS Enterprise raced the ship from “Battlestar Galactica” to the nearest star system, which would get there first?

    A new graphic from Travelmath.com seeks to answer that question, which sounds like a typical opening argument over beers. The graphic shows fictional travel times across the universe for spaceships from several sci-fi franchises as well as comic-book characters such as Iron Man and Superman.

    When leaving Earth on a voyage to Alpha Centauri, it turns out, Galactica would get there in just 29 minutes, traveling at an average speed of 53.4 trillion miles per hour (85.9 trillion kilometers per hour). The USS Enterprise from “Star Trek” would take more than 161 days, at a speed of “just” 6.6 billion mph (10.6 km/h). [The 10 Greatest Sci-Fi Spaceships of All Time]

    Fictional Travel Times

    This fun graphic from Travelmath.com pits fictional spaceships and characters against each other in races across the universe.
    Credit: Travelmath

    To calculate the blazing-fast speeds for the various characters and spaceships portrayed, Travelmath.com consulted online fan encyclopedias from different franchises. You can actually race the sci-fi spaceships and fliers on Travelmath.com to see who wins, with each race accompanied by its own animation.

    From the Milky Way to Andromeda, the graphic pits three famous ships from the Star Wars universe: the Death Star, the Millennium Falcon and the X-Wing. It turns out to be not much of a contest, with the Millennium Falcon getting there in 100 days, two times faster than the X-Wing and eight times faster than the Death Star.

    Regardless, the superhero Dr. Manhattan from the comic miniseries “Watchmen” could beat all three of them, according to the graphic, because his travel is instantaneous.

    The graphic also claims that Superman would beat “Firefly’s” Serenity ship in a race from Earth to Neptune (4 hours as opposed to 42 days), and Iron Man could get around the world in 3 hours — 10 times faster than a TIE fighter from “Star Wars.”

    Travelmath is a service that offers information on travel distance, travel time and travel cost between Earth destinations, including flight and driving times. For real-life fliers, such as F-16 jets and passenger planes, the site uses information from aircraft manufacturers’ websites.

    Follow Elizabeth Howell @howellspace, or Space.com @Spacedotcom. We’re also on Facebook and Google+. Original article on Space.com.

  • Enormous Red Sprites Seen From Space (Update)

    Sorms Over Southern Mexico
    NASA photo ISS044-E-45576 showing storms over southern Mexico on Aug. 10, 2015.
    Credit: NASA

    Editor’s note: Updated to include a second photo of another sprite captured moments later by the same camera (added at bottom of article).

    This gorgeous photo, captured from the International Space Station on the night of Aug. 10, 2015, shows an orbital view of thunderstorms over the city lights of southern Mexico as a recumbent Orion rises over Earth’s limb. But wait, there’s more: along the right edge of the picture a cluster of bright red and purple streamers can be seen rising above a blue-white flash of lightning: it’s an enormous red sprite caught on camera!

    PHOTOS: Chasing Red Sprites and Blue Jets

    First photographed in 1989, red sprites are very brief flashes of optical activity that are associated with powerful lightning. So-called because of their elusive nature, sprites typically appear as branching red tendrils reaching up above the region of an exceptionally strong lightning flash. These electrical discharges can extend as high as 55 miles (90 kilometers) into the atmosphere, with the brightest region usually around altitudes of 40–45 miles (65–75 km). 

    Sprites don’t last very long  — 3–10 milliseconds at most — and so to catch one (technically here it’s a cluster of them) on camera is a real feat… or, in this case, a great surprise!

    PHOTO: Mysterious Sprite Photographed by ISS Astronaut

    Sprites have been photographed from the ISS before (it’s a great place from which to observe these phenomena, which are often obscured from the ground by storm clouds) but this is one of the best images of one I’ve seen yet.

    Sprite Over Mexico Aug. 10, 2015

    Detail of the sprite photographed over Mexico on Aug. 10, 2015.
    Credit: NASA

    ANALYSIS: Origin of Mysterious Jellyfish Lightning ‘Sprites’ Revealed

    (And in case you’re wondering that’s the moon (not the sun) shining brightly in the star-filled sky, and the yellow-green light surrounding the planet isn’t aurora — it’s a different phenomena called airglow.)

    Learn more about the history of sprite research at the University of Alaska Fairbanks website.

    Multiple sizes of the above image can be found on Johnson Space Center’s astronaut photography archive.

    UPDATE (11:50 p.m. ET): Just a few minutes earlier the same storm had created another sprite outburst, which was amazingly also captured on camera as the ISS was moving southeast:

    Another Sprite Outburst on Aug. 10, 2015

    This article was provided by Discovery News.

  • 'Eiffel Tower' Prominence Towers Over The Sun

    From his backyard in Östersund, Sweden, professional photographer and astrophotographer Göran Strand took a look at the sun using his portable solar telescope “to see if something interesting was going on.” And sure enough, there was something VERY interesting going onSomething was towering over the solar disk — something that looked like… the Eiffel Tower?

    Of course, this isn’t the famous Parisian landmark, nor is it some Photoshop trickery; the structure Strand had spotted was a solar prominence, and a beautiful one at that.

    PHOTOS: Simmering Solar Views from SDO

    “This big prominence got my attention right away, even in my small 50mm telescope it was a beautiful sight,” Strand told Discovery News via email. “While setting up my bigger solar telescope I thought of how the prominence looked and that it reminded me of the Eiffel Tower in Paris.”

    Using a larger Lunt 80mm hydrogen alpha pressure-tuned solar telescope hooked up to a Point Grey Grasshopper 3 camera, he captured a thousand photos and stacked the best 300 shots to produce this mesmerizing solar portrait:

    Colorized version of the 'Eiffel Tower' prominence on the sun

    Colorized version of the ‘Eiffel Tower’ prominence compiled from 300 solar observations.
    Credit: Göran Strand

    In the final image, the size of the Earth has been added to give a sense of scale. A rough comparison suggested that this prominence is approximately 7-Earth diameters high, reaching high into the sun’s atmosphere (the corona).

    NEWS: Sun Unleashes Spectacular Solar Eruption

    Prominences are large structures of magnetized plasma that can erupt from the sun’s chromosphere and arc high into the corona. As the plasma in the sun’s corona can have temperatures exceeding a million degrees Kelvin (Celsius), the plasma in prominences can be a hundred times cooler, at a similar temperature to the chromosphere.

    As they are cooler than the surrounding corona, they generate visible light and can therefore be spotted fairly easily though specialized equipment such as solar telescopes and eclipse glasses. (NOTE: Never look directly at the sun as serious eye injuries and even blindness can result.)

    Also, as the sun is rich in ionized hydrogen, astronomers use hydrogen alpha (or H-α) filters to produce observations of stunning detail of prominences and chromospheric features on the solar disk.

    PHOTOS: The Psychedelic Anatomy of a Solar Flare

    For more of Strand’s outstanding work, check out his websiteInstagramTwitter and Facebook.

    Original image of 'eiffel tower' prominence on sun

    The original, black and white view of the sun and prominence (in the lower-right).
    Credit: Göran Strand

    Originally published on Discovery News.

  • Viking Aurora: Northern Lights Wow Photographer in Newfoundland

    This stunning image of an aurora was taken was taken in Norstead, a Viking village replica.

    The Norstead Viking Village in L’anse aux Meadows, Newfoundland is the only confirmed Viking site in North America. Astrophotographer Adam Woodworth took the image on June 22 while visiting the area.

    “The aurora was coming from all directions it seemed like, this was the first time I’d witnessed a strong aurora display so far north. L’anse aux Meadows is near the northern most tip of Newfoundland, certainly the farthest north I’ve ever been. An experience I’ll never forget!” Woodworth wrote in an email to Space.com. [Amazing Aurora Photos of 2015]

    The image also shows Viking building replicas made out of sod and wood.  Woodworth’s image is a blend of two exposures for depth of field. He used a Nikon D810A, Nikon 14-24mm f/2.8 lens. The sky view was created with a single shot set at ISO 3200, 14mm, f/2.8, with a 1-second exposure.  The foreground was then taken as a single shot at ISO 1600, 14mm, f/5.6, with a 2-minute exposure.

    Auroras occur when charged particles from the sun’s solar wind interact with Earth’s upper atmosphere (at altitudes above 50 miles, or 80 km), causing a glow. The particles are funneled to Earth’s polar regions by the planet’s magnetic field. The auroras over the North Pole are known as the aurora borealis, or the northern lights. The lights over the South Pole are dubbed the aurora australis, or southern lights. 

    To see more amazing night sky photos submitted by SPACE.com readers, visit our astrophotography archive.

    Editor’s note: If you have a night sky photo you’d like to share for a possible story or image gallery, send images and comments in to Space.com at spacephotos@space.com.

    Follow Space.com on Twitter @Spacedotcom. We’re also on Facebook & Google+. Original story at Space.com.

  • Mars Hoax Returns to Mislead Stargazers

    Moon and Mars Hoax Image
    The image that accompanied the “Mars Spectacular” email of 2003, which sparked the recurring Mars Hoax.
    Credit: Origin Unknown

    Here we go again.

    The infamous Mars Hoax that has circulated widely through the Internet since its first appearance in 2003, when it originated in the form of an email message titled “Mars Spectacular,” has reared its ugly head yet again.

    The unknown source behind that 2003 email was likely honestly and earnestly trying to provide some interesting information to the general public in advance of a historically close approach of Mars to the Earth in late August 2003. [Quiz: Mars Myths and Misconceptions]

    Unfortunately, the message ended up giving countless people the wrong impression of what was to be seen in the night sky. The confusion arose from the following passage in the “Mars Spectacular” email:   

    “The encounter will culminate on Aug. 27 when Mars comes to within 34,649,589 miles (55,763,108 kilometers) of Earth and will be (next to the moon) the brightest object in the night sky. It will attain a magnitude of -2.9 and will appear 25.11 arc seconds wide. At a modest 75-power magnification, Mars will look as large as the full moon to the naked eye. Mars will be easy to spot.”      

    Many people, it seems, glossed over the words, “At a modest 75-power magnification” — partly because the email featured a line break just after this phrase — and fixated solely on “Mars will look as large as the full moon to the naked eye” (without realizing a telescope would be needed to pull of this trick).

    Of course, the message immediately went viral and was passed on to countless others who couldn’t resist forwarding it to their entire address book. Thus, the Mars Hoax was born. [7 Biggest Mysteries of Mars]

    And ever since, it has been all but impossible to get the proverbial genie back in the bottle.

    Many suckers

    The “Mars Spectacular” message was meant to apply only to August 2003, although every year since, during the month of August, the message has resurfaced and has propagated through cyberspace on to many other unsuspecting individuals. It amazes me that the hoax keeps drawing people in 12 years after it first emerged.

    To give you an idea of just how prevalent the Mars Hoax has become, consider this story:

    Back on Aug. 27, 2007, one of nature’s great sky shows, a total eclipse of the moon, occurred across the United States. On the day before the eclipse, the people who run the “answer line” at New York City’s Hayden Planetarium expected a heavy volume of phone inquiries from the general public concerning advice on how to view the eclipse. Fifty-one calls were logged that day, but amazingly, only three concerned the upcoming eclipse; the other 48 were calls asking about how to see Mars when it was due to appear as large as the full moon!

    Mars Myths & Misconceptions: Quiz

    No planet is more steeped in myth and misconception than Mars. This quiz will reveal how much you really know about some of the goofiest claims about the red planet.

    The original 'Face on Mars' image taken by NASA's Viking 1 orbiter, in grey scale, on July, 25 1976. Image shows a remnant massif located in the Cydonia region.

    0 of 10 questions complete

    Mars Myths & Misconceptions: Quiz

    No planet is more steeped in myth and misconception than Mars. This quiz will reveal how much you really know about some of the goofiest claims about the red planet.

    Start Quiz
    The original 'Face on Mars' image taken by NASA's Viking 1 orbiter, in grey scale, on July, 25 1976. Image shows a remnant massif located in the Cydonia region.

    0 of questions complete

    Many fallacies

    Interestingly, most of the original email message is substantially correct (for 2003). But there were also a few inaccuracies. For instance, after 2003, the next time that Mars will come closer to Earth will be in 2287, not 60,000 years from now. (The message confusingly implies that both of those figures are accurate.) And the 2003 rendezvous marked the closest Mars had come to Earth in more than 59,000 years, not merely 5,000 years.

    Furthermore, in 2003, Mars was not the brightest object in the night sky other than the moon. That honor went to Venus. In fact, even at its very brightest, Mars was a full magnitude fainterthan Venus.

    And even at its brightest, Mars appeared to the naked eye as nothing more than an extremely bright, yellowish-orange star, not at all like the full moon!

    So if you have already received this infamous Mars email, or if you receive it in the coming days, delete it! 

    In fact, why not take a few moments and forward this column to all those in your address book? Think of it as an antidote to the Mars Hoax virus.  

    So where is Mars now?

    This month, Mars is much dimmer and far less conspicuous than it was in August 2003. The Red Planet is 239 million miles (385 million km) from Earth, nearly seven times farther away than it was a dozen years ago. And at magnitude +1.7, Mars is about 70 times fainter compared to 2003, so you actually might need binoculars to pick up the planet in the twilight sky.   

    Currently, Mars is very slowly becoming evident in the dawn sky. It is rising 90 minutes before the sun. Search in the east-northeast sky, below the stars Castor and Pollux in Gemini.

    In terms of actual size, Mars is almost twice as big as the moon — about 4,213 miles (6,780 km) in diameter, compared to 2,160 miles (3,475 km) for the moon. 

    But the great distance between Mars and Earth means that the Red Planet never appears anywhere near as large as the moon in Earth’s sky. The average distance of the moon from Earth is 238,000 miles (382,900 km). For Mars to appear to loom as large as the moon does from Earth, it would have to be a mere two Earth-moon distances away, or roughly 476,000 miles (766,000 km).

    Joe Rao serves as an instructor and guest lecturer at New York’s Hayden Planetarium. He writes about astronomy for Natural History magazine, the Farmer’s Almanac and other publications, and he is also an on-camera meteorologist for News 12 Westchester, N.Y. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.

  • Yes, Even the Equator Can Get Slammed by Solar Storms

    2014 Solar Storm
    On Jan. 7, 2014, the sun unleashed a major solar flare and coronal mass ejection (the bright spot at center right), but the Earth’s magnetic field channeled the worst of the solar storm away from the planet, scientists say.
    Credit: Möstl et al., Nature Communications

    This article was originally published on The Conversation. The publication contributed this article to Space.com’s Expert Voices: Op-Ed & Insights.

    The Earth’s magnetic field – known as the “magnetosphere” – protects our atmosphere from the “solar wind.” That’s the constant stream of charged particles flowing outward from the sun. When the magnetosphere shields Earth from these solar particles, they get funneled toward the polar regions of our atmosphere.

    As the particles crash into the atmosphere’s ionospheric layer, light is given off, creating beautiful multicolored displays of aurora near both the North and South Poles. These are stunning visual representations of the complex interactions in the near-Earth space environment, which we collectively term “space weather.”

    The same space weather that generates these beautiful displays can cause havoc for a wide range of technologies. We’ve known for a while that space weather in high-latitude regions near the poles can cause power grid failures, sometimes causing heavy damage. The most famous instance was the March 1989 blackout in the Northeastern US and up through Quebec, Canada that left millions without power for 12 hours.

    But we haven’t thought of equatorial regions as being prime targets. Our new research shows that areas closer to the equator still experience bad space weather – and its disturbing effects on power grid infrastructure.

    Changing magnetic fields crank up electric currents

    High above the ground in the upper atmosphere are fluctuating electric currents driven by interactions in the magnetosphere and ionosphere. These atmospheric currents cause strong changes in the strength of the local magnetic field on the ground. We can’t feel the magnetic field ourselves, but researchers measure and track it at various points on the Earth’s surface.

    That’s all well and good. The problem comes in when these atmospheric currents cause swift changes in the magnetic field. When the magnetic field abruptly changes, it can generate electric currents in conductors at the Earth’s surface – for instance, long pipes or wires such as oil and gas pipelines or power transmission lines. This process of electric current generation is called magnetic induction.

    These electric currents are not-so-creatively called geomagnetically induced currents, or GICs for short. The high-latitude regions are most susceptible to GICs because of the intense electric currents flowing through the auroras, thanks to the way the solar wind gets diverted when it hits the Earth’s magnetosphere. However, the entire planet can be affected to varying degrees.

    When they occur, GICs effectively generate extra electric current in power grid infrastructure through magnetic induction. Power grids, during large events, can end up taking on more electricity than they can handle. These induced currents have caused numerous equipment failures that have led to power outages for large populations.

    Trouble at the equator too, not just near the poles

    Those same geomagnetically induced currents that happen in the high-latitude regions can happen around the equator of our planet too. There, they are caused not by the auroral electric current system we find near the poles, but by a weaker low-latitude counterpart called the equatorial electrojet. Like the high-latitude ionospheric current system, the equatorial electrojet’s electric current can be detected on the ground using magnetic field observations.

    Recently researchers reported that GIC activity is enhanced at the equator during severe geomagnetic storms – that’s when solar eruptions called “coronal mass ejections” trigger shock waves that hit the Earth. They pointed the finger at the equatorial electrojet as a suspected cause.

    In our new research article in Geophysical Research Letters, we show that countries near the magnetic equator are more vulnerable to space weather than previously thought.

    Rather than focusing on severe geomagnetic storms, such as the 2003 Halloween event that caused power grid problems in Sweden (among many other things), we took a different tack. Our analysis focused on the arrival of interplanetary shocks. These are abrupt pressure increases in the solar wind – that stream of plasma constantly flowing out of the sun. When these shocks hit the Earth’s magnetosphere, the impact causes a sudden magnetic field change that can be measured all over the world.

    Interplanetary shocks regularly announce the beginning of a geomagnetic storm. But many pass by relatively benignly without developing into a full-blown geomagnetic storm. We noticed that the magnetic response to these shock arrivals was sometimes significantly stronger at the magnetic equator when compared to locations only a few degrees away. Why?

    An analysis of how these equatorial responses differed throughout the day revealed they were strongest around noon and weakest at night. This daily contrast corresponds to the well-known variations in the equatorial electrojet. It’s strong evidence that the equatorial electrojet is amplifying the geomagnetically induced current activity during interplanetary shock arrivals in a way that hasn’t really been recognized until now.

    Aurora over Norway

    Aurora over Norway, visual of space weather.
    Credit: Alexa Halford, CC BY-ND

    Effects on equatorial power grids

    This result has significant implications for the many countries located beneath the equatorial electrojet that may be operating power infrastructure not initially designed to cope with space weather. These countries need to look into ways of protecting their infrastructure during geomagnetically quiet periods as well as during severe geomagnetic storms.

    One of our coauthors, Dr Endawoke Yizengaw from Boston College, grew up in Ethiopia, within the equatorial electrojet’s region of influence. He recalls regular unexplained power outages during his childhood and wonders whether interplanetary shocks may have played a role. We hope to be able to answer this question in the near future.

    Scientists around the world are conducting ongoing research to better understand the effects of these geomagnetically induced currents on power grids. It’s becoming increasingly clear that we need to investigate the effects of quiet periods, not just major events. What happens during these quiet times, and in regions often overlooked, can have a significant impact on our increasingly technology-dependent society.

    Brett Carter is Research Scientist in Space Weather and Ionospheric Physics at Boston College and Alexa Halford is Postdoctoral Research Associate in Physics and Astronomy at Dartmouth College

    This article was originally published on The Conversation. Read the original article. Follow all of the Expert Voices issues and debates — and become part of the discussion — on Facebook, Twitter and Google +. The views expressed are those of the author and do not necessarily reflect the views of the publisher. This version of the article was originally published on Space.com.

  • [Project Topics] KOUNOTORI5 launch rescheduled to 8:50:49 p.m. on August 19 (Wed.) 2015

    Topics List

    Aug. 17, 2015 Updated
    KOUNOTORI5 launch rescheduled to 8:50:49 p.m. on August 19 (Wed.) 2015

    The KOUNOTORI5(HTV5)/H-IIB F5 launch was postponed to 8:50:49 p.m. on August 19 due to adverse weather.
    Accordingly, the live launch report will begin at 8:00 p.m. on August 19 (Wed. , JST). The report will be broadcast through the Internet.
    Please send your support messages for the mission, or tweet it including the hashtag #HTV5.

    KOUNOTORI5 launch rescheduled to 8:50:49 p.m. on August 19 (Wed.) 2015

    Aug. 16, 2015 Updated
    KOUNOTORI5 launch postponed to Aug. 19 (Wed., JST)

    The launch date of the H-IIB Launch Vehicle No. 5 carrying the KOUNOTORI5 has been postponed as unfavorable weather is forecasted. The launch was originally scheduled for August 17. The live broadcast of the launch will also be put off accordingly.
    Your support messages are very much welcome through Twitter (Hashtag “#HTV5”) or via the following website.

    KOUNOTORI5 launch postponed to Aug. 19 (Wed., JST)

    Aug. 15, 2015 Updated
    New launch date and time of KOUNOTORI5/H-IIB F5 decided

    Aug. 14, 2015 Updated
    KOUNOTORI5 launch postponed to Aug. 17 (Mon., JST)

    The launch date of the H-IIB Launch Vehicle No. 5 carrying the KOUNOTORI5 has been postponed as unfavorable weather is forecasted. The launch was originally scheduled for August 16. The live broadcast of the launch will also be put off accordingly.
    Your support messages are very much welcome through Twitter (Hashtag “#HTV5”) or via the following website.

    KOUNOTORI5 launch postponed to Aug. 17 (Mon., JST)

    Jul. 21, 2015 Updated
    Dates set for capturing the KOUNOTORI5 and its berthing with ISS Astronaut Yui to be in charge of operation

    After international coordination, the dates for capturing the KOUNOTORI5, a cargo transporter to the International Space Station (ISS), and its berthing have been respectively set as August 20 (Thu.) and 21 (Fri.) The KOUNOTORI5 is scheduled to be launched on August 16 (Sun.) from the Tahegashima Space Center.
    It was also decided that Astronaut Kimiya Yui will manipulate the ISS robotic arm to capture the KOUNOTORI2.

    Dates set for capturing the KOUNOTORI5 and its berthing with ISS Astronaut Yui to be in charge of operation

    Jul. 10, 2015 Updated
    KOUNOTORI5 and operation simulation training opened to the press

    On July 1, the KOUNOTORI5, a cargo transporter to the ISS, was revealed to the media at the Tanegashima Space Center. The mission was also explained there.
    From the evening of July 9 to the morning of the 10th, simulation training for the KOUNOTORI5 operation and control was held in the KOUNOTORI operation room at the Tsukuba Space Center, and part of it was also open to the press. This training was a last opportunity for a joint session between JAXA and NASA before the KOUNOTORI5 launch. On the NASA side, Astronaut Wakata participated in the training as a CAPCOM (capsule/spacecraft communicator).

    KOUNOTORI5 and operation simulation training opened to the press

    Jun. 9, 2015 Updated
    Launch day set for KOUNOTORI5/H-IIB F5!

    The launch date and time for the H-IIB Launch Vehicle No. 5 (H-IIB F5) with the H-II Transfer Vehicle “KOUNOTORI5” (HTV5) onboard was set for around 10:01 p.m. on August 16 (Sun.), 2015 (Japan Standard Time).
    The H-IIB F5 has already been transported to the TNSC, and it is now being assembled there.
    * Launch time will be determined by the updated orbit of the ISS.

    Launch day set for KOUNOTORI5/H-IIB F5!

    Sep. 7, 2013 Updated
    KOUNOTORI4 completed its mission with re-entry!

    The KOUNOTORI4 (HTV4, a cargo transporter to the International Space Station) left the ISS on Sept. 5 and re-entered the atmosphere at 3:37 p.m. on Sept. 7 (Japan Standard Time.)
    The KOUNOTORI 4 successfully achieved its mission of taking cargo to the ISS, then completed all its tasks over about 36 days.
    We would like to send our sincere appreciation to all of you who have been supporting the KOUNOTORI project.

    KOUNOTORI4 completed its mission with re-entry!

    Sep. 3, 2013 Updated
    Re-entry date and time for KOUNOTORI4 decided

    Schedules of departure from the International Space Station (ISS) and of re-entry to the atmosphere for the H-II Transfer Vehicle “KOUNOTORI 4” (HTV4) are determined as follows.

    Departure from the ISS:
    September 5, 2013 / 1:00 a.m.(Japanese Standard Time, JST)*
    Re-entry to the atmosphere:
    September 7, 2013 / 3:36 p.m.(JST)*

    * The time may vary according to the actual operation.

    Aug. 10, 2013 Updated
    KOUNOTORI4 berthed at ISS!

    The KOUNOTORI4 (HTV4, a cargo transporter to the International Space Station) was captured by the ISS robotic arm at 8:22 p.m. on August 9 (Japan Standard Time) and berthed at the ISS at 3:38 a.m. on August 10 (JST). The KOUNOTORI4 was launched by the H-IIB Launch Vehicle No.4 on August 4. ISS astronauts will take cargo out from the Pressurized and Unpressurized Logistic Carriers into the ISS.

    Aug. 9, 2013 Updated
    Live broadcast of KOUNOTORI4 trip to ISS!

    The KOUNOTORI3 (HTV4, the cargo transporter to the International Space Station) launched on August 4 has been traveling to the ISS while adjusting its altitude. Between the evening on August 9 and early on the morning of August 10, the KOUNOTORI4 will make a final approach and berth at the ISS. JAXA will provide a live broadcast of its final access, capture, and berthing.
    The KOUNOTORI4’s approach and the ISS’s capture of the vehicle by the robotic arm is scheduled for about one hour from 7:40 p.m. on the 9th (Japan Standard Time.) Then the telecast of its berthing will last for about one hour from 22:00 p.m. on the 9th (JST.)
    Please don’t miss the broadcast!
    (Photo: The KOUNOTORI3 approaching the ISS, JAXA/NASA)

    Aug. 4, 2013 Updated
    Launch Success of KOUNOTORI4/H-IIB F4

    The H-IIB Launch Vehicle No. 4 with the KOUNOTORI4 (HTV4, a cargo transporter to the International Space Station) onboard lifted off from the Tanegashima Space Center at4:48:46 a.m. on August 4 (Sun., Japan Standard Time.)
    The launch vehicle flew smoothly, and at 14 minutes and 59 seconds after liftoff, the KOUNOTORI4 separation was confirmed.
    The KOUNOTORI4 will gradually go closer to the International Space Station, and it will be berthed at the ISS. We will broadcast the berthing on our website, so don’t miss it!

    Jun. 19, 2013 Updated
    KOUNOTORI4 revealed at TNSC

    On June 19, the H-II Transfer Vehicle (HTV, a cargo transporter to the International Space Station) “KOUNOTORI4” was shown to the media at the Tanegashima Space Center (TNSC.)
    The KOUNOTORI4 will be launched by the H-IIB Launch Vehicle No. 4 on Aug. 4 from the TNSC. It will carry various goods to the ISS including food and water for astronauts, as well as experiment devices and materials for the Japanese Experiment Module “Kibo.” Launch preparations continue for the KOUNOTORI4.

    May 21, 2013 Updated
    KOUNOTORI4/H-IIB F4 launch schedule decided!

    The H-IIB Launch Vehicle No. 4 (H-IIB F4) carrying the H-II Transfer Vehicle (HTV4, a cargo transporter to the International Space Station) will be launched on August 4 (Sunday, Japan Standard Time.) The launch time will be around 4:48 a.m. (JST.) It will be blasted off from the Yoshinobu Launch Complex at the Tanegahsima Space Center. Why don’t you take this opportunity to come to Tanegahima to witness the liftoff at hand!

    Sep. 14, 2012 Updated
    KOUNOTORI3 completed its mission with re-entry!

    The KOUNOTORI3 (HTV3, a cargo transporter to the International Space Station) left the ISS on Sept. 13 and re-entered the atmosphere at 2:27 p.m. on Sept. 14 (Japan Standard Time.)
    The KOUNOTORI 3 successfully achieved its mission of taking cargo to the ISS, then completed all its tasks over about 56 days.
    We would like to send our sincere appreciation to all of you who have been supporting the KOUNOTORI project.

    Sep. 11, 2012 Updated
    KOUNOTORI3 departure and re-entry live report!

    The H-II Transfer Vehicle “KOUNOTORI3” (HTV3,a cargo transporter to the International Space Station) will leave from the ISS at around 0:50 a.m. on Sept. 13 (Japan Standard Time, all the following dates and time are JST,) and will re-enter the atmosphere at around 2:24 p.m. on Sept. 14.
    JAXA will offer a live report of its departure from the ISS from 0:20 a.m. on the 13th (Thu.), then a live scene of the HTV operation room at the time of its re-entry from 1:45 p.m. on the 14th (Fri.) through the Internet. Please do not miss the footage!

    Sep. 7, 2012 Updated
    Re-entry date and time for KOUNOTORI3 decided

    The re-entry schedule for the KOUNOTORI3 was set as follows after extended mooring at the International Space Station due to an additional extravascular activity.

    Departure from the ISS:
    September 13, 2012 / 0:50 a.m.(Japanese Standard Time, JST)*
    Re-entry to the atmosphere:
    September 14, 2012 / 2:24 p.m.(JST)*

    * The time is subject to change due to actual operational status.

    The KOUNOTORI3 will carry a re-entry data recorder, the i-Ball, which was developed in cooperation between the public and private sectors to acquire atmosphere re-entry data as well as scenes of KOUNOTORI3’s destruction.

    Jul. 28, 2012 Updated
    KOUNOTORI3 berthed at ISS!

    The KOUNOTORI3 (HTV3, a cargo transporter to the International Space Station) was captured by the ISS robotic arm at 9:23 p.m. on July 27 (Japan Standard Time) and berthed at the ISS at 2:31 a.m. on July 28. The KOUNOTORI3 was launched by the H-IIB Launch Vehicle No.3 on July 21. ISS astronauts will take cargo out from the Pressurized and Unpressurized Logistic Carriers into the ISS.
    (Photo: The KOUNOTORI3 to a Common Berthing Mechanism at the nadir port of Harmony, JAXA/NASA)

    Jul. 21, 2012 Updated
    Launch Success of KOUNOTORI3/H-IIB F3

    The H-IIB Launch Vehicle No. 3 with the KOUNOTORI3 (HTV3, a cargo transporter to the International Space Station) onboard lifted off from the Tanegashima Space Center at 11:06:18 on July 21 (Sat., Japan Standard Time.)
    The launch vehicle flew smoothly, and at 14 minutes and 53 seconds after liftoff, the KOUNOTORI3 separation was confirmed.
    The KOUNOTORI3 will gradually go closer to the International Space Station, and it will be berthed at the ISS. We will broadcast the berthing on our website, so don’t miss it!

    Jun. 21, 2012 Updated
    KOUNOTORI3/H-IIB F3 Special Site now open!

    JAXA will launch the KOUNOTORI3 (a cargo transporter to the International Space Station, ISS) by H-IIB Launch vehicle No.3 on July 21 from the Tanegashima Space Center. We have opened the KOUNOTORI3/H-IIB F3 Special Site to be ready for the launch.
    Please check the special site for more information. We have also started welcoming your support messages, so please send them to us!

    Jun. 7, 2012 Updated
    KOUNOTORI3 revealed to the media at TNSC

    On June 1 (Fri.), the H-II Transfer Vehicle “KOUNOTORI3” (HTV3, a cargo transporter to the International Space Station) was revealed to the media at the Spacecraft and Fairing Assembly Building 2 at the Tanegashima Space Center. The KOUNOTORI3 will be packed with food and daily necessities for astronauts aboard the ISS, test equipment for aquatic organisms, and other experiment devices including a small satellite, then will be launched by the H-IIB Launch Vehicle No. 3 at 11:18 a.m. on July 21, 2012 (Japan Standard Time.) The KOUNOTORI is currently under preparations for its journey to space.

    Mar. 21, 2012 Updated
    KOUNOTORI3/H-IIB F3 launch schedule decided!

    The launch date and time for the H-IIB Launch Vehicle No. 3 (H-IIB F3) with the H-II Transfer Vehicle “KOUNOTORI3” (HTV3), a cargo transporter to the International Space Station, has been set to be at around 11:18 a.m. on July 21 (Sat.), 2012 (Japan Standard Time.) The launch preparation operation for the KOUNOTORI is smoothly in progress at the Tanegashima Space Center.

    Mar. 30, 2011 Updated
    KOUNOTORI2 re-entered the atmosphere to complete its mission!

    The KOUNOTORI2 (HTV2, a cargo transporter to the International Space Station,) which left the ISS at around 0:46 a.m. on March 29 (Japan Standard Time,) re-entered the atmosphere at around 12:09 p.m. on March 30 (JST.)
    The KOUNOTORI2 successfully completed its role to transport materials to the ISS, then re-entered the Earth’s atmosphere to complete its mission of approximately 67 days.
    Thank you very much for supporting the KOUNOTORI2 and H-IIB Launch Vehicle No.2 missions.

    Mar. 29, 2011 Updated
    KOUNOTORI2 left ISS!

    The KOUNOTORI2 (HTV2, a cargo transporter to the ISS) was detached from the International Space Station (ISS) using the ISS robotic arm at 10:29 p.m. on March 28 (Japan Standard time,) and it emitted a jet to leave the ISS after being transported to the release point at 0:46 a.m. on the 30th.
    The KOUNOTORI2 will re-enter the Earth’s atmosphere at around 12:09 on March 30. From some areas, you can see the KOUNOTORI2 flying around the Earth between the 29th and the 30th. Also, please witness the scene of the HTV operation and control room when it re-enters the atmosphere through the live Internet broadcast, which will begin at 11:30 a.m. on the 30th.

    Mar. 25, 2011 Updated
    KOUNOTORI2 leaving ISS on the 29th! Live broadcast scheduled

    The KOUNOTORI2 (HTV2, a cargo transporter to the International Space Station) will depart from the ISS with used material loaded on March 29 (Japan Standard Time,) and will be slated for re-entry to the atmosphere on the 30th (JST.) JAXA will broadcast a live Internet report of the KOUNOTORI departure from the ISS from 0:00 a.m. on the 29th (JST,) then its re-entry to the atmosphere from 11:30 a.m. on the 30th (JST.) Please watch the events through the Internet!

    Mar. 22, 2011 Updated
    KOUNOTORI2 to leave ISS

    The departure date of the KOUNOTORI2 (HTV2, a cargo transporter to the ISS), which is loaded with used materials, from the International Space Station (ISS) has been decided.
    The KOUNOTORI2 will leave the ISS at around 0:45 a.m. on March 29 (Japan Standard Time) after completing its role at the ISS. After departure, it will be burned when it re-enters the atmosphere at around 12:10 p.m. on March 30. Following its combustion, its mission will be accomplished.
    We will broadcast a live report of the departure and re-entry of the KOUNOTORI2. More details will be posted on our website. (Photo by NASA)

    Mar. 11, 2011 Updated
    KOUNOTORI2 relocation to the earth-facing port completed

    At 8:49 p.m. on March 10 (Japan Standard Time), the KOUNOTORI2 (HTV2, a cargo transporter to the International Space Station) began to be moved from the zenith port to the earth-facing port using the robotic arm of the International Space Station. At 3:55 a.m. on the 11th (JST,) KOUNOTORI2’s electric and communication systems were connected to the ISS to complete the relocation. After being loaded with used items, the KOUNOTORI2 will re-enter the atmosphere to be burned.

    Mar. 9, 2011 Updated
    KOUNOTORI2 to return to earth-facing port from March 10

    The KOUNOTORI2 (HTV2, a cargo transporter to the International Space Station), will move back to the earth-facing port of the Harmony (Node 2) from its zenith port now that the Space Shuttle Discovery left the ISS to go home on March 7 (Japan Standard Time.) The relocation is scheduled to be performed on the 10th and 11th (JST.) More cargo will be taken out of the KOUNOTORI2, then, after being packed with used materials, the KOUNOTORI2 will re-enter the atmosphere.
    (Photo by NASA)

    Feb. 21, 2011 Updated
    KOUNOTORI2 relocation to the zenith port completed

    As part of preparations for the Space Shuttle Discovery’ s docking with the International Space Station (ISS,) the KOUNOTORI2 , or the HTV2, a cargo transporter to the ISS, was moved from the earth-facing port of the Harmony (Node 2) to its zenith port. This was the first time to perform such a relocation. The KOUNOTORI2 was successfully transported at 1:45 a.m. on Feb. 19 (Japan Standard Time,) and the electric cables were connected with the Harmony at 4:26 a.m. (JST) to complete its relocation.

    Jan. 28, 2011 Updated
    KOUNOTORI2 berthing at ISS

    The KOUNOTORI2, or the HTV2, a cargo transporter to the International Space Station (ISS) launched by the H-IIB Launch Vehicle No.2, was captured by the ISS robotic arm at around 8:41 p.m. on January 27 (Japan Standard Time,) and, at around 3:34 a.m. on the 28th (JST,) the KOUNOTORI berthed at the ISS. Cargo in the Pressurized Section will be transported to the ISS by the ISS astronauts followed by cargo in unpressurized areas.

    Jan. 22, 2011 Updated
    KOUNOTORI2/H-IIB F2 successfully launched

    The H-IIB Launch Vehicle No. 2 with the KOUNOTORI2 (HTV2, a cargo transporter to the International Space Station, ISS) onboard was launched from the Tanegashima Space Center at 2:37:57 p.m. on January 22 (Sat., Japan Standard Time.) The launch vehicle flew smoothly, and, at about 15 minutes and 13 seconds after liftoff, the separation of the KOUNOTORI2 was confirmed.
    The KOUNOTORI2 will fly to the ISS, then, on Jan. 28 (Fri., JST,) it is slated for berthing with the ISS.

    Dec. 14, 2010 Updated
    KOUNOTORI2 system checkup completed

    At the Tanegashima Space Center, all parts of the H-II Transfer Vehicle “KOUNOTORI2” (HTV2) were integrated electrically and mechanically in the end of October. Throughout November, the assembled KOUNOTORI2 has been checked as one system to confirm that no problem was found in the vehicle.
    After a thorough inspection, propellants were loaded onto the KOUNOTORI2 tanks, and currently the tank pressure is being adjusted. Preparation for launch is smoothly progressing.
    The final launch preparation including battery charge and loading onto the H-IIA Launch Vehicle No.2 will now be carried out for the KOUNOTORI2.

    Dec. 1, 2010 Updated
    KOUNOTORI2 control and operation simulation revealed to the press

    On November 30, JAXA showed part of the control and operation simulation of the KOUNOTORI2 to the media at the Tsukuba Space Center. The KOUNOTORI2 (HTV2) is a cargo transfer vehicle to the International Space Station (ISS.)
    The purpose of the simulation was to train and improve operators’ skills. It takes about 20 hours with NASA to simulate events, from the KOUNOTORI2’s arrival at around 12-km beneath the ISS, to its gradual approach to the ISS, to the capture of the KOUNOTORI2 by the ISS robotic arm, and then the docking of the KOUNOTORI2.

    Nov. 26, 2010 Updated
    KOUNOTORI2 shown to the Press at TNSC

    On Nov. 25, the H-II Transfer Vehicle “KOUNOTORI”2 (a cargo transporter to the International Space Station) was revealed to the media at the Spacecraft and Fairing Assembly Building No. 2 at the Tanegashima Space Center. We are engaging in preparation for the launch of the KOUNOTORI2 including propellant loading and mating with the launch vehicle.
    JAXA provides updated information about the KOUNOTORI2 and H-IIB Launch Vehicle No.2 at the special site. Your support messages are welcome there, too.

    Nov. 11, 2010 Updated
    HTV nickname selected & special site open!

    “KOUNOTORI” (meaning “a white stork” in English) was chosen as the nickname of the H-II Transfer Vehicle (HTV, a cargo transfer vehicle to the International Space Station.)
    During a month-long nickname campaign, we received 17,236 suggestions.
    Among them, “KOUNOTORI” was selected because a white stork carries an image of conveying an important thing (a baby, happiness, and other joyful things); therefore, it precisely expresses the mission to transport essential materials to the ISS.
    The KOUNOTORI2 is scheduled to be launched by the H-IIB Launch Vehicle No. 2 (H-IIB F2) at around 3:29 p.m. (Japan Standard Time) on January 20 (Thu.), 2011.
    Taking this opportunity of selecting the nickname, we would also like to open the “KOUNOTORI2/H-IIB F2 Special Site.” We will provide you with updated information about the project including a column by project personnel and launch related matters. Please enjoy the site!
    * Launch time will be determined by the updated orbit of the ISS.

    Nov. 10, 2010 Updated
    Launch day set for HTV2/H-IIB F2!

    The launch date and time for the H-IIB Launch Vehicle No. 2 (H-IIB F2) with the H-II Transfer Vehicle (HTV2) onboard was set for around 3:29 p.m. on January 20 (Thu.), 2011 (Japan Standard Time). The HTV2 is a cargo transporter to the International Space Station (ISS.) The integration of all modules of the HTV2 was completed at the Tanegashima Space Center (TNSC), and it will enter the final launch preparation phase. The H-IIB F2 has already been transported to the TNSC, and it is now being assembled there.
    * Launch time will be determined by the updated orbit of the ISS.

    Nov. 2, 2010 Updated
    HTV2: all modules connected, moved to final launch preparations

    (Left) All HTV2 modules are being connected (Center) Integrated HTV2 (front side) (Right) Integrated HTV2 (back side) (Images by JAXA)

    On Oct. 29, we completed connecting all modules of the second H-II Transfer Vehicle (HTV2, a cargo transporter to the International Space Station) electrically and mechanically at the Second Spacecraft and Fairing Assembly Building (SFA2) at the Tanegashima Space Center. The HTV2 is now in its configuration for launch.
    After a comprehensive check on the integrated HTV2, it will go through final launch preparations including propellant loading and fairing encapsulation. The HTV2 is scheduled to be launched in the winter launch period of Japan Fiscal Year 2010.

    Oct. 13, 2010 Updated
    Full assembly started for the second HTV

    The assembly operation for all modules of the second H-II Transfer Vehicle (HTV, the cargo transporter to the International Space Station) started on October 6 at the second Spacecraft and Fairing Assembly Building (SFA2) at the Tanegashima Space Center. Prior to full assembly, in mid September, cargo to the ISS was loaded onto the Pressurized and Unpressurized Carriers.

    Apr. 7, 2010 Updated
    Development of HTV/H-IIB received Japan industry technology/MEXT award

    JAXA was selected as one of 12 organizations to receive the Ministry of Education, Culture, Sports, Science and Technology award at the 39th Japan industry technology awards for its development of the HTV and H-IIB launch vehicle.
    The Japan industry technology awards are presented by Nikkan Kogyo Shimbun Ltd. (Business and Technology Daily News, Japan) to encourage development of original and unique technology that contributes to the promotion of industry. The news company bestows the awards to development projects of distinctive large-scale technological systems.

    Feb. 10, 2010 Updated
    HTV Project Team awarded for research

    Since 2005, the National Institute of Science Technology Policy (NISTEP) of the Ministry of Education, Culture, Sports, Science and Technology (MEXT) has been choosing researchers who have made significant contributions to science and technology every year to praise their efforts. In 2009, the demonstration flight of the H-II Transfer Vehicle (HTV, a cargo transporter to the International Space Station) was highly evaluated, and on February 9, Mr. Torano, HTV Project Manager, Mr. Koyari, Sub-project Manager, and Mr. Sasaki, Functional Manager, received a memento of the selection.

    Nov. 2, 2009 Updated
    HTV re-entered the atmosphere, mission completed

    The H-II Transfer Vehicle (HTV) Demonstration Flight, which departed from the International Space Station (ISS) on October 31, re-entered the atmosphere at around 6:26 a.m. on November 2.
    The HTV successfully completed its cargo transportation operations to the ISS, and accomplished all its missions in about 52 days following the re-entry today.

    Oct. 31, 2009 Updated
    HTV released from ISS

    The H-II Transfer Vehicle (HTV) Demonstration Flight, which completed its cargo transportation mission at the International Space Station (ISS), was unberthed from the ISS by its robotic arm (SSRMS) at 0:02 a.m. on October 31 (Japan Standard Time, the following dates and times are JST.) The HTV departed from the ISS at 2:32 a.m. on the 31st. The HTV will leave the ISS orbit, and is scheduled to re-enter the Earth’s atmosphere at around 6:25 a.m. on November 2 (Mon.)
    You may be able to see the HTV just prior to re-entry from Okinawa at around 6:13 a.m. on the 2nd if the deorbit process goes smoothly and the weather cooperates. (Photo by NASA)

    Oct. 27, 2009 Updated
    Internet Live Report: HTV leaving ISS on Oct. 31 (Sat)

    The H-II Transfer Vehicle (HTV) Demonstration Flight, which is currently berthed at the International Space Station (ISS), is scheduled to depart from the ISS at 2:30 a.m. on Oct. 31 (Sat) (Japan Standard Time, all the following days and times are in JST.) The HTV will be unberthed from the ISS by the ISS robotic arm (SSRMS) late at night on Oct. 30 (Fri) after its hatch to the ISS is closed at dawn of Oct. 30, then depart from the ISS. If everything goes smoothly, the HTV will re-enter the Earth’s atmosphere around 6:25 a.m. on Nov. 2 (Mon).

    We will broadcast a live report of the HTV unberthing and departure from the ISS through the Internet from 11:45 p.m. on Oct. 30 (Fri) and from 2:15 a.m. on Oct. 31 (Sat) respectively. (Sorry, the live reports are broadcasted only in the Japanese language.) Please enjoy the HTV live reports over the weekend!
    The live broadcast time schedule has changed due to the delay of the HTV departure.

    Oct. 21, 2009 Updated
    The HTV PLC unloading operations completed, trash loading continues

    HTV-1, being berthed to the ISS, is operating nominally. The Small Fine Arm (SFA) of the Kibo Remote Manipulator System (JEMRMS), packed in a Cargo Transfer Bag (CTB) and delivered to the ISS, was transferred from the HTV Pressurized Logistics Carrier (PLC) to Kibo on October 4. The Pressurized Stowage Resupply Rack (PSRR), also delivered on the HTV-1, was transferred to Kibo’s Experiment Logistics Module-Pressurized Section (ELM-PS) on October 14. All the cargo transfer operation from the HTV PLC to the ISS was completed on October 20.
    Aboard the ISS, trash loading into the HTV PLC is currently underway. With this trash stow activity completed, the HTV-1 will depart from the ISS, and enter the atmosphere early next month.
    Photo (provided by NASA): Astronaut Robert Thirsk taking cargo out from the HTV Pressurized Carrier.

    Oct. 14, 2009 Updated
    HTV operations running smoothly, cargo unloading continues

    Cargo unloading operations continued from the Pressurized Logistics Carrier of the H-II Transfer Vehicle (HTV) Demonstration Flight berthed at the International Space Station (ISS). On Oct. 4, the Small Fine Arm (SFA) of the Kibo’s Robotic Arm was moved to the ISS. The SFA was transported to the ISS as it was still packed in the Cargo Transfer Bag. One unit of the Pressurized Stowage Resupply Rack will be transferred to the ISS on the 14th.
    Photo (provided by NASA): Astronaut Nicole Stott taking cargo out from the HTV Pressurized Carrier.

    Sep. 26, 2009 Updated
    Exposed Pallet stored back in HTV

    The Exposed Pallet of the H-II Transfer Vehicle (HTV) Demonstration Flight was retrieved and stored back in the HTV Unpressurized Carrier at 10:20 p.m. on Sept. 25 (Japan Standard Time) by the robotic arms of the Kibo and the International Space Station (SSRMS) after its two cargoes, the experiment devices in the unpressurized environment, had been installed in the Kibo’s Exposed Facility.
    Cargo in the HTV Pressurized Carrier will now be unloaded by the astronauts aboard the ISS. After the unloading, used material and equipment on the ISS will be packed into the Pressurized Carrier. The HTV will depart from the ISS in mid-November to re-enter the atmosphere. (The detailed schedule will be decided based on the ISS/HTV operational status.) (Photo by NASA)

    Sep. 25, 2009 Updated
    Two experiment devices installed onto Kibo Exposed Facility

    On Sept. 24 and 25 (Japan Standard Time), two experiment devices that were shipped by the H-II Transfer Vehicle (HTV) Demonstration Flight were unloaded from the HTV Exposed Pallet and installed onto the Exposed Facility of the Japanese Experiment Module “Kibo.”
    The two devices are the “Superconducting Submilimeter-Wave Limb-Emission Sounder (SMILES)” and the “Hyperspectral Imager for the Coastal Ocean (HICO) & Remote Atmospheric & Ionospheric Detection System (RAIDS) Experimental Payload (HREP.)” The HREP and the SMILES were mounted at 8:15 p.m. on the 24th and 1:12 a.m on the 25th respectively. (Photo by NASA)

    Sep. 24, 2009 Updated
    HTV Exposed Pallet attached to the Kibo Exposed Facility

    At 6:06 p.m. on Sept. 23rd (Japan Standard Time, JST), the Exposed Pallet was taken out from the H-II Transfer Vehicle (HTV) Demonstration Flight, which is now berthed at the International Space Station (ISS). The Pallet was then attached onto the Exposed Facility of the Japanese Experiment Module “Kibo” at 11:33 p.m. (JST). The experiment devices on the Pallet will be moved to be installed onto the Kibo’s Exposed Facility. (Photo by NASA)

    Sep. 18, 2009 Updated
    HTV Demonstration Flight successfully berthed at ISS

    The H-II Transfer Vehicle (HTV) Demonstration Flight, launched by the H-IIB Launch Vehicle Test Flight at 2:01 a.m. on Sept. 11 (Japan Standard Time, JST,) took almost one week to approach the International Space Station (ISS) and arrived at the Berthing Point 10 meters below the ISS at 4:27 a.m. on the 18th (JST, following times are all JST.) At 4:51 a.m., the HTV was captured by the ISS robotic arm (Space Station Remote Manipulator System, SSRMS) manipulated by the ISS crew, and it was installed onto the Common Berthing Mechanism (CBM) on the lower side (earth side) of the Harmony (Node 2) at 7:26 a.m. At 10:49 a.m., electric and communication lines were connected, and the HTV was successfully berthed at the ISS.

    Sep. 15, 2009 Updated
    Live reports of the HTV final approach to the ISS on Sept. 18 (Fri.)

    The H-II Transfer Vehicle (HTV) Demonstration Flight, which was launched by the H-IIB Launch Vehicle at 2:01:46 a.m. on September 11 (Fri.) has been smoothly flying on its scheduled course. Its final approach to the International Space Station (ISS) was approved at the ISS Mission Management Team (IMMT) meeting on Sept. 15, thus, from the 16th, the altitude of the HTV will be maneuvered to gradually approach the ISS. The HTV is scheduled to be berthed at the ISS on Sept. 18 (Fri.)
    JAXA will broadcast the live reports of the ISS robotic arm capturing the HTV from 4:00 a.m., and the berthing of the HTV at the ISS from 7:00 a.m. They are early in the morning, but don’t miss them!

    Sep. 11, 2009 Updated
    HTV/H-IIB Successfully Launched!!

    The Japan Aerospace Exploration Agency (JAXA) launched the H-II Transfer Vehicle (HTV) Demonstration Flight aboard the H-IIB Launch Vehicle Test Flight (H-IIB TF1) at 2:01:46 a.m. on September 11, 2009 (Japan Standard Time, JST) from the Tanegashima Space Center. The launch vehicle flew smoothly, and, at about 15 minutes and 6 seconds after liftoff, the separation of the HTV Demonstration Flight was confirmed.

    The HTV will gradually approach the International Space Station (ISS) and berth at the ISS on the 18th (Friday, JST.)

    Aug. 31, 2009 Updated
    HTV moved to the VAB! Final launch preparation phase

    On August 30, the encapsulated HTV Demonstration Flight was transported to the Vehicle Assembly Building (VAB.) It will be loaded onto the H-IIB Launch Vehicle to be ready for the launch on September 11. We published a promotion movie of the HTV/H-IIB mission. Please watch it before witnessing the actual launch!

    Aug. 24, 2009 Updated
    HTV encapsulated

    On August 21, the H-II Transfer Vehicle (HTV) Demonstration Flight was mated with the Payload Attach Fitting (PAF) at the Spacecraft and Fairing Assembly Building #2.
    On the 23rd, the HTV on the PAF was encapsulated by the payload fairing, which covers the payload to protect it from air resistance, friction and the acoustic vibrations of launch. The fairing for the HTV is a 5S-H type and is about 5 meters in diameter and about 15 meters in length. It was developed for the HTV launch.
    The encapsulated HTV Demonstration Flight will be transported to the Vehicle Assembly Building (VAB) and loaded onto the H-IIB Launch Vehicle Test Flight.

    Jul. 9, 2009 Updated
    HTV opened to the press at TNSC

    On July 9, the H-II Transfer Vehicle (HTV, a cargo transporter to the International Space Station) was opened to the press at the Spacecraft and Fairing Assembly Building #2 (SFA2) at the Tanegashima Space Center (TNSC.)
    We are providing updated information on the HTV and H-IIB at the HTV/H-IIB Special Site.

    Jul. 8, 2009 Updated
    HTV/H-IIB launch date decided! Special site opened

    The H-IIB Launch Vehicle Test Flight with the H-II Transfer Vehicle (HTV, a cargo transporter to the International Space Station) will be launched at 2:04 a.m. on September 11 (Fri.). (*)
    The HTV has been fully assembled at the Tanegashima Space Center, and it will be under final launch preparations including comprehensive checkout and propellant loading to be ready for launch.
    The ground comprehensive test for the H-IIB Launch Vehicle using the Ground Test Vehicle (the GTV test) is scheduled on the 11th.
    Please check the updated information on the HTV and H-IIB at the “HTV/H-IIB Special Site,” which was opened today. We hope you enjoy the site.
    (*) Time will be determined by the updated orbit of the International Space Station (ISS.)

    Jun. 30, 2009 Updated
    Preparations for the HTV Demonstration Flight going smoothly at TNSC

    Preparations for the Demonstration Flight of the H-II Transfer Vehicle (HTV) are underway at the Tanegashima Space Center (TNSC).
    At dawn on April 23, the HTV arrived at the TNSC and was moved into the Spacecraft and Fairing Assembly Building #2 for a post-transportation inspection on each element of the vehicle.
    Payloads to be shipped to the International Space Station (ISS) by the HTV were then loaded onto the HTV’s Pressurized Logistic Carrier and Unpressurized Logistic Carrier.

    In the Pressurized Logistic Carrier, life-related supplies, such as food and clothes, which were packed in the Cargo Transfer Bag (CTB) and other experiment materials were stored on the HTV Re-supply Rack (HRR) of the Carrier. In the Unpressurized Logistic Carrier, the Superconducting Submilimeter-Wave Limb-Emission Sounder (SMILES,) which is an experiment device for the Kibo’s Exposed Facility, and NASA experimental equipment were loaded onto the Exposed Pallet of the Carrier.

    After completing the payload loading, the two carriers were mated.
    On June 24, all HTV modules including the Avionics Module and Propulsion Module were connected.
    The HTV demonstration flight is now fully assembled, and will start final launch preparations such as a comprehensive vehicle inspection and propellant loading.

    Apr. 24, 2009 Updated
    HTV arrives at TNSC

    At dawn on April 23, the First H-II Transfer Vehicle (HTV) was transported from Shimama Port at Tanegashima to the Tanegashima Space Center (TNSC.) The HTV left the Tsukuba Space Center on April 17. The Pressurized Logistic Carrier, Unpressurized Logistic Carrier, the Avionics Module, and the Propulsion Module were detached for the transportation, thus they will be assembled after arrival. A final functional checkup will be held prior to the launch.

    Apr. 17, 2009 Updated
    HTV left for the TNSC

    The first H-II Transfer Vehicle (HTV), or the HTV Technology Demonstrator, left the Tsukuba Space Center at dawn on April 17, 2009, for the Tanegashima Space Center (TNSC.) After arrival, the HTV will be assembled and checked for launch by the H-IIB Launch Vehicle, which is now under testing.


    The first HTV leaving the TKSC (Unpressurized Logistics Carrier, Avionics Module, and Plopulsion Module)

    The first HTV arrived at Tsuchiura Port
    (Unpressurized Logistics Carrier)

    Dec. 26, 2008 Updated
    HTV open to the press

    On Dec. 25, 2008, JAXA revealed the maiden H-II Transfer Vehicle (HTV), an unmanned supply transfer vehicle that will fly to the International Space Station (ISS), to the press at the Tsukuba Space Center (TKSC.) It was the first press conference since assembling all the modules of the first HTV.

    At the press conference, the HTV and its launch by the H-IIB Launch Vehicle were explained by HTV Project Manager Yoshihiko Torano and H-IIB Launch Vehicle Project Manger Tomihisa Nakamura. The Superconducting Submilimeter-Wave Limb-Emission Sounder (SMILES,) which will be transported to the ISS by the first HTV, was also introduced by Professor Masato Shiotani of the Research Institute for Sustainable Humanosphere of Kyoto University. The SMILES is one of the experiment devices that will be installed onto the Exposed Facility of the Japanese Experiment Module “Kibo.”

    Also at the press conference, the first HTV and the SMILES undergoing an all-vehicle functional test were shown to the media at the Spacecraft Integration and Test Building at the TKSC. The modules of the cargo section (“Pressurized Carrier” and “Unpressurized Carrier,”) “Avionics Module” and “Propulsion Module” were assembled for the test. The “Exposed Pallet” loaded with a dummy cargo for the test and the SMILES were also displayed.

    We will conduct comprehensive functional tests with the mechanically and electrically integrated HTV, such as conductivity verification of the pipes and electric system, and other compatibility tests. The HTV is then scheduled to be transported to the Tanegashima Space Center in April, 2009, at the earliest, and be launched by the H-IIB Launch Vehicle in the summer launch season of 2009 or later.

    Dec. 18, 2008 Updated
    All flight modules assembled for first time for inaugural HTV flight

    On Dec. 12, all the parts of the H-II Transfer Vehicle (HTV,) the supply transfer vehicle to the International Space Station, were assembled for an all-vehicle functional test ahead of its first flight. They are the “Logistic Carrier Pressurized Section,” the cargo section of the “Un-pressurized Carrier,” the “Exposed Pallet,” the “Avionics Module” and the “Propellant Module.” This was the first time that all the modules were assembled. The size of the assembled HTV was about the same size as the Pressurized Module of the Japanese Experiment Module “Kibo.” The HTV will be the largest payload that JAXA has ever launched.

    During the all-vehicle functional test, all the modules are mechanically and electrically connected to verify their function as one piece of the vehicle such as proper pipe routing and electric conductivity.

    The first HTV is scheduled to be launched by the H-IIB Launch Vehicle in September 2009 at the earliest.

    Aug. 28, 2008 Updated
    Thermal Vacuum Test for first flight of HTV

    A thermal vacuum test on the first flight vehicle of the H-II Transfer Vehicle (HTV) has been carried out at the Spacecraft Integration and Test Building at the Tsukuba Space Center.
    The purpose of the test is to evaluate the thermal design of the structure and to verify its endurance in the harsh environment of space by simulating the vacuum and thermal environment in space.
    Thermal vacuum tests for the Pressurized Carrier and Unpressurized Carrier have already been completed, and the main part with the Avionics Module and Propulsion Module combined is now in the 13-meter diameter space chamber for testing.
    The test will be completed in early September before the acoustic test and functional test are performed. After all the test results are reviewed to make sure that no problem is left unsolved, the vehicle will be transported to the Tanegashima Space Center for final launch preparations.

    (Photo: The main part of the HTV (Avionics Module and Propulsion Module) moved into the 13-meter diameter space chamber)

    Apr. 18, 2008 Updated
    The first model HTV (Technology Demonstration Model) was shown to the press

    On April 17, 2008, a press review was held for the first model H-II Transfer Vehicle (HTV) (Technology Demonstration Model), which is an unmanned cargo transfer spacecraft to the International Space Station. On display separately were the Pressurized Logistics Carrier for supply transportation, the Avionics Module for vehicle body control and the Propulsion Module which carries the propulsion system. When the HTV is completed and fully equipped, it will be the largest spacecraft in Japan with a length of 10 meters and a weight of 16.5 tons. After going through performance tests like the Thermal Vacuum Test and Acoustic Test, the first model HTV is scheduled for launch from Tanegashima on the H-IIB Launch Vehicle No. 1 (Test Model) in the summer of 2009.

    Jul. 2, 2007 Updated
    Proximity Communication System (PROX) undergoes testing

    Tests are currently being performed on the Proximity Communication System (PROX) at NASA’s Kennedy Space Center (KSC).

    The PROX system will be installed in the Japanese Experiment Module “Kibo” to communicate between the H-II Transfer Vehicle (HTV) and transmit and receive data between the International Space Station (ISS). It will also measure the relative distance and speed between the ISS and the HTV in order to support the HTV’s rendezvous with the ISS.

    Since last year, tests on the PROX and a compatibility test for the PROX/rack had been carried out before it went through a pre-shipping examination and was shipped out to the U.S. in January 2007. After performing several tests like the JEM/PROX compatibility test, it will be installed in the Experiment Logistics Module Pressurized Section (ELM-PS) and is scheduled for launch on Assembly Flight 1J/A at the end of February 2008.

    Photo1 : A general view of the PROX (Bottom right is the PROX before shipping at Tsukuba Space Center).
    Photo2 : A scene from a test on the PROX at the Kennedy Space Center.
    Photo3 : A crew review scene performed by astronaut Furukawa (taken from behind the PROX rack.)

    Jun. 26, 2006 Updated
    Prototype HTV unveiled to press at Tsukuba Space Center

    On June 23, a prototype of the H-II Transfer Vehicle (HTV) was unveiled to the press at the Tsukuba Space Center (TKSC.) The HTV is an unmanned orbital carrier to the International Space Station (ISS.) It is equipped with both the function of a “manned cargo carrier” for ISS crews to actually embark and carry out supportive work on it and the function of an “inter-orbital carrier” to perform “inter-orbit transportation to a selected attitude,” “rendezvous flights to the ISS,” and “re-entry” to aim to acquire the necessary technology for autonomous activities in space.

    The prototype will be used for various environment tests to make sure it can bear the extreme temperatures in space and acoustic and vibration environment at the time of launch. Through the tests, the project team will verify basic design data, and incorporate test results into future development.

    Outline of the HTV project

    Length about 10 m (including thruster)
    Diameter about 4.4 m
    Mass about 10.5 ton (excluding cargo)
    Loading capacity (for supply) about 6 tons
    Loading capacity (for waste) about 6 tons
    • Target orbit: ISS orbit
      Altitude: 350 to 460 km
      Inclination: about 51.6 degrees
    • Mission hours
      Solo flight: about 100 hours
      Stand-by: more than a week
      Docked with the ISS: about 30 days

    May 28, 2004 Updated
    Debris protection function was verified by shooting aluminum balls at the HTV at 6 km per second.

    Each module of the Space Station including the Japan Experiment Module has a “debris bumper” for protecting itself from losing its functions by colliding with space debris.
    The level of protection depends on the location (position) of each module and the probability of collision. Many technological ideas are incorporated to achieve the required protection effect, such as making the distance between the debris bumper and the pressurized wall longer.
    Solar array panels around the HTV have been considered to be part of the protective walls, but they needed to be verified.
    The verification was performed by a high-speed collision test using a HTV mockup. Aluminum balls of various sizes were shot at the protective walls at a speed of 6 km per second. After the test, the pressurized wall behind the protective walls was checked for holes. As a result, the solar array panels and the panel structure (an aluminum honeycomb structure) were verified to be effective for protection, and necessary data were also acquired for the further debris protection design assessment for the HTV.

    Upper Photo: A mockup for the verification (The thick wall on the right is a solar array panel.)
    Lower Photo:A solar panel from the back after the verification.

    Upper Photo: A mockup for the verification (The thick wall on the right is a solar array panel.)/Lower Photo:A solar panel from the back after the verification.;

    Mar. 28, 2003 Updated
    Manufacturing “Thermal Structural Test Models ” for Tests in the Next Fiscal Year

    HTV is about four meters in diameter and a bit shorter than 10 meters in length. In other words, its size can be explained as a container that could accommodate a sightseeing bus. In the process of developing HTV, therefore, it is divided into four modules namely Logistic Carrier Pressurized section, Logistic Carrier Un-Pressurized section, Avionics module, and Propulsion module. Thermal structural test models are being manufactured for each module. A thermal structural test model is a mimic model to test it in simulated harsh launch and space environments for checking acoustic condition, vibration, shock at separation and endurance in the space.

    The main structure is in conical semi-monocoque structure based on a launch vehicle design, and four modules will be assembled at the final fabrication phase and be tested for evaluating comprehensive strength and stiffness.

    Furthermore, tests for evaluating strength, pressure, acoustic data, shock, and heat balance, and acquisition of resonance frequency will be carried out to collect data for specifying environmental conditions of onboard loads and to find environmental characteristics data. The series of these tests will start in the next fiscal year.

    Upper Photo: Structural Thermal Test Model for Main Structure
    Lower Photo: Thermal Structural Test Model for Propulsion System “Helium Gas Supply Sub-Module”

    Oct. 5, 2001 Updated

    After HTV’s arrival to International Space Station (ISS), Exposed Pallet is taken out of HTV, and cargoes are replaced by robotic arm. This Exposed Pallet has rollers on its sides to minimize the friction and to keep the position accurately when it is brought back to HTV.
    A series of roller rotation slip tests was conducted from August to September 2001. The rollers are made of plastic to reduce the weight and they have solid lubricant on their surfaces. This combination of plastic and solid lubricant is rare. The purpose of this test is to confirm the manufacturing process and to collect the basic data of friction in the various environments (hot, cold, vacuum, air) and the wearing life.
    In addition, by conducting the test with the full-size model, the friction data closer to the actual operation were collected. The data will be applied not only for the HTV design and robotics analysis but also the future satellite programs and space equipment.

    Upper Photo: Setup for the rotation test in vacuum heat chamber
    Lower Photo: Setup for the full-size roller test

    Jun. 29, 2001 Updated

    Post Development Review of HTV Pressurized Carrier Aft Dome
    NASDA conducted additional preliminary design review (delta-PDR) with lots of participant from NASA and CSA (including ISS program manager) at Tsukuba Space Center as following schedule.
    Pre-Board Meeting : May 15th and 16th, 2001
    Board Meeting : May 18th, 2001
    We focused on two kinds of items in this review panel. One was a kind of additional items which were not reviewed in PDR held in 1999 (e.g.Un-pressurized carrier / Exposed pallet, GPS receivers in JEM, Crew operation panel, etc.) and another was a kind of items which had been changed the design from PDR (e.g. Solar power generation system, Approaching trajectory, etc.).
    Prior to holding the review panel, NASDA delivered review documents toward NASA, CSA and ESA and received a thousand of “Review Item Disposition Sheets (RID)” on these documents. We determined all dispositions for these RIDs after the discussions within three weeks. NASDA/NASA/CSA founded a few issues related to the ISS safety in this review panel and we determined to give high priority to these issues.

    Photo: HTV Delta-PDR Pre-Board Panel

    Feb. 19, 2001 Updated

    Post Development Review of HTV Pressurized Carrier Aft Dome A pressurized carrier equipped in HTV was designed based on the JEM Experiment Logistics Module Pressurized Section (ELM-PS). NASDA determined to use a newly designed integral molded structure for the Aft Dome of pressurized carrier to reduce the weight of 260 kg and the similar structure has already been used by the propellant tanks of Launch vehicles. Similar to H-IIA rocket, MAN-Technologie in Germany took the charge of the development under the supervision of Mitsubishi Heavy Industries LTD. Through this development, MAN-Technologie cleared the manufacturing problems such as thickness, welding, strength, etc., and completed them successfully. The photo shows a manufacturing sample that will be used for following engineering tests in Japan. After this review, NASDA will start manufacturing of the Flight Model and mass production.

    Photo: Aft Dome Structure for HTV Pressurized Carrier Engineering Test

    Dec. 8, 2000 Updated

    Succeeding to the previous tests conducted from April 18 to 20, 2000, NASDA/NASA/CSA conducted a series of real-time HTV capturing operation tests with expanded SSRMS conditions, evaluators, and facility by following schedule.
    Date: Nov. 8th to Nov. 10th, 2000
    Place: Canadian Space Agency Headquarter in Saint-Hubert, Quebec, CANADA
    In this series of tests, Astronaut Doi and other four astronauts executed total of up to 120 simulation- run cases with MOTS (MSS Operations and Training Simulator) in CSA, the facility with more complicated and numerous equipments. Just like previous tests, Astronauts evaluated the operability, by controlling SSRMS and executing capturing operation with free drifting HTV within predefined time. Though the results are still under investigation, the operation time was improved by re-designed operation sequence based on the experience in last tests.
    Photo (Upper): Astronaut Doi trying to capture Photo (Lower): CSA members supporting

    Nov. 9, 2000 Updated

    When crew enters HTV pressurized carrier berthed to ISS, it is necessary to circulate atmosphere in pressured cabin. The fan system for air circulation should meet several requirements such as large flow rate, low noise, lightweight, compact size, and high durability for severe environment during launch. Because each HTV mission period is relatively short, NASDA plans to develop a new air circulation fan system that is appropriate to HTV requirements.
    NASDA is conducting a series of development tests with this new fan system in Shinko-Denki Co. The purpose of tests is to ensure the silent and low vibration design with multi-stage/coaxial concept and new blade/housing shape. NASDA will then review the test results and reflect them to the final fan design.

    Photo: Test Setup

    Oct. 6, 2000 Updated

    The Pre-Shipping Review (PSR) for 28 R-1E thrusters, that will be used for HTV attitude control was held by Primex Space Systems Co. in the United States. These thrusters will be delivered to Ishikawajima-Harima Heavy Industries Co. Then after used in System Firing Test (SFT) in which NASDA confirms the Propulsion-system performance, they will be installed to the first HTV.
    The same thrusters have been used in Space Shuttle for attitude control and they will be installed in Propulsion Module of International Space Station.

    Photo: 28 sets of R-1E thruster (Offered by Primex Space Systems Co.)

    Jul. 7, 2000 Updated

    HTV has two carrier sections, one is a pressurized section which carries the logistics to ISS pressurized section and another is an un-pressurized section which carries experiment devices in ISS exposed section. The exposed experiment devices will be taken out from un-pressurized section with exposed pallet by ISS manipulator (SSRMS).
    From April 10 to June 8, NASDA had conducted Breadboard test in Mizuho facility of Ishikawajima-Harima Heavy Industries Ltd. for Paraffin Actuator that will be used for separation mechanism between exposed pallet and experiment devices. The Paraffin Actuator drives the output pin using phenomena of increasing of volume when paraffin changes its phases from solid to liquid and this attracts attention as a shock-less separation mechanism. In this series of tests, NASDA conducted a nominal driving test, environmental (vacuum/high temperature/low temperature) driving tests and a data-gathering test. NASDA obtained several data and the results will be used to improve the design of HCAM (HTV Cargo Attachment Mechanism).

    May 26, 2000 Updated

    HTV will perform autonomous rendezvous flight to the ISS, however, in the final operation, HTV will be captured by ISS manipulator system (SSRMS) controlled by ISS crew and be berthed to the ISS. Such operation is a peculiar requirement for HTV and we must confirm that it can be certainly captured by ISS crew within the limited time.
    To investigate the feasibility of this operation, a series of SSRMS capturing simulation test was conducted at MD-R (MacDonald Dettwiler Space and Advanced Robotics Limited) in Brampton City, Ontario, Canada from April 18 through 20. Besides four astronauts including Mr. Takao Doi, engineers from NASDA, CSA, and NASA had joined this test.
    In this simulation test, astronauts evaluated by controlling SSRMS and executing capturing operation in computer simulator: MDSF-RT (Manipulator Development and Simulation Facility in Real-Time) which HTV dynamics data from NASDA had been already input. Though details of the result are still under investigation, astronauts judged that this operation is feasible difficulty and it seemed that there are not any critical issues.

    Photo: HTV Capture Real-Time Crew Evaluation (offered by MD-R)

    Apr. 21, 2000 Updated

    In this month, NASA held the following safety review panel toconfirm the HTV safeness regarding to the International Space Station.
    HTV Safety Review Panel (Phase 1): March 13th to March 17th at Johnson Space Center in Houston.
    NASA holds the Safety Review Panel to all segments that compose the ISS and all approaching vehicles in rendezvousing to the ISS. Especially, HTV, which is the first newly designed transfer vehicle, turned out to be reviewed first in this panel. In this review panel, NASA and NASDA members had an animated discussion focused not only upon the hardware safety for the transfer vehicles such as logistics carrier and propulsion system but also upon the safety of flight-plan for rendezvous to the ISS. As a result, NASA confirmed the feasible of the HTV safety design and approved NASDA to progress the next design phase.

    Photo: Safety Review Panel Members

    Jan. 31, 2000 Updated

    PDR (Preliminary Design Review) for SIGI (Space Integrated GPSR/IMU) which is most important sensor of HTV Guidance and Navigation System was conducted at Honeywell co. in Tampa, Florida in United States from Dec. 9 to 10.
    In addition to accelerometers and ring laser gyros for control of HTV attitude/maneuver, this sensor unifies GPS receiver for navigation into one package.
    SIGI is also used in International Space Station to measure the attitude, and H764, the base of SIGI, are used in many aircraft.

    Figure: HTV Guidance and Control Schematic

    Dec. 17, 1999 Updated

    PDR (Preliminary Design Review) for Rendezvous Sensor which to be used during the HTV final approach was conducted at Daimler Chrysler Jena-Optronik in Jena, Germany from Nov.15 to 18. This sensor will also be used for ATV(Autonomous Transfer Vehicle) being developed by ESA.
    We expect a cost reduction / risk decrease become possible by this joint supply of NASDA-ESA.

    The figure: rendezous sensor function during final approach

    Nov. 19, 1999 Updated

    NASDA conducted the Approach/Release (Rendezvous) Flight Technology Test on the ETS-VII, which has close relation to the HTV rendezvous technology from Oct. 26 to 27.
    During the test, ETS-VII tried the R-bar approach which simulates the HTV final approach trajectory to the ISS. HIKOBOSHI satellite regarded as HTV, approached to the virtual R-bar formed by ORIHIME, using the algorithm developed for HTV. As a result, HIKOBOSHI raised the appropriate orbit within the expected corridor determined for rendezvous sensor and successfully finished at the 114 meters close.
    We are now analyzing the data obtained from this experiment. It will greatly contribute to the establishment of all HTV flight algorithm.

    Sep. 17, 1999 Updated

    NASDA held two major review meetings. One was the HTV Phase 1 Safety Review, which examined the HTV design from the point of safety. The another was HTV Preliminary Design Review (PDR), which examined the HTV design from the point of technique.
    The safety review meeting was held from August 18 to 20. The safety design of HTV was generally confirmed. After some additional study, HTV project will take a NASA safety review.
    The HTV PDR meeting was held by NASDA from August 23 to September 3. Approximately forty NASA, European Space Agency (ESA), and Canadian Space Agency (CSA) people attended the meeting and examined the HTV design. As the result of review, design of HTV was confirmed to be adequate. Therefore, the production of HTV Engineering Model (EM) and the progress to detailed design phase were admitted.

    Jul. 26, 1999 Updated

    The documents for PDR (Preliminary Design Review), which will be conducted from July 15th to September 3rd have been released. These documents have also been sent to NASA, CSA, and ESA in the end of June.
    We will continue to coordinate with reviewers of both NASDA and other organizations on matters which they point out until PDR Main Board.
    At the same time, the documents for Phase 1 Safety Review have been released.

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