Tag: space.com

  • Alien Oceans' Glint Could Reveal Habitable Water Worlds

    Kepler-62f Exoplanet Image
    This artist’s concept shows Kepler-62f, an exoplanet in the habitable zone of its host star, which is located about 1,200 light-years from Earth in the constellation Lyra. Researchers think Kepler-62f may be a “water world.”
    Credit: NASA/Ames/JPL-Caltech

    The bright glint of alien oceans may be visible from afar, allowing astronomers to flag potentially habitable exoplanets.

    As Earth travels around the sun, it moves through phases much like the moon when seen from afar. The planet’s oceans reflect a great deal of light, especially during the crescent phase. The same principle should apply to exoplanets, researchers say.

    “Seeing excessive brightness at the crescent phases could be a telltale signal of ocean planets,” Tyler Robinson, of NASA’s Ames Research Center in Moffett Field, California, said at the Astrobiology Science Conference in Chicago in June. [‪10 Exoplanets That Could Host Alien Life]

    Although a host of satellites monitor Earth, few eye the planet as a whole. As a result, many exoplanet scientists turn to models to understand how Earth might appear if it were a distant alien world. However, the accuracy of these models can be difficult to gauge without observations to verify them.

    Scientists have made a few attempts to address this issue. In 1993, for example, Carl Sagan and other researchers used observations made by NASA’s Jupiter-studying Galileo spacecraft during a 1990 flyby of Earth to search for signs of life on our planet.

    Earth in Crescent View

    An image of Earth, taken by NASA’s LCROSS satellite, shows the planet in its crescent phase. The smaller light to the left is the moon.
    Credit: NASA

    And in 2009, NASA’s Lunar Crater Observation and Sensing Satellite(LCROSS) moon mission observed Earth at several phases, including near-full and crescent, in order to calibrate its instruments. Robinson and his colleagues analyzed these data, and found that the near-infrared and ultraviolet/visible light observations provided an approximation of how Earth might appear through extreme phases across various spectrums. Their study was published in 2014 in The Astrophysical Journal.

    “LCROSS looked at Earth for calibration, but its measurements were good for science,” Robinson said.

    The results showed that, although less of Earth’s surface was visible during its crescent phase, the brightness of the planet increased due to the light reflecting off its oceans. In visible light, the glint increased the planet’s brightness by as much as 40 percent; in the near-infrared, Earth shone nearly 80 percent more brightly, Robinson said.

    Robinson was also a co-author on a different paper that examined similar, though less detailed, observations of Earth using NASA’s Deep Impact spacecraft (which performed up-close examinations of two different comets, in 2005 and 2010).

    The observations performed by LCROSS — the first high-spectral-resolution observations of Earth in its crescent phases — lined up well with predictions based on existing models, Robinson said.

    Alien Planet Quiz: Are You an Exoplanet Expert?

    Astronomers have confirmed more than 800 planets beyond our own solar system, and the discoveries keep rolling in. How much do you know about these exotic worlds?

    Artist's conception of alien planets Kepler-36b and c

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    Alien Planet Quiz: Are You an Exoplanet Expert?

    Astronomers have confirmed more than 800 planets beyond our own solar system, and the discoveries keep rolling in. How much do you know about these exotic worlds?

    Start Quiz
    Artist's conception of alien planets Kepler-36b and c

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    However, similar results gained from observations of an exoplanet would not automatically be signs of an ocean, he cautioned; clouds and ice could also affect the brightness of a planet. Follow-up studies of the exoplanet’s atmospherecould reveal more about the world’s potential habitability.

    Still, an apparent glint from an exoplanet ocean would be an exciting find, Robinson said.

    “We conclude that the detection of such a feature would be intriguing, and would certainly indicate that a more detailed observational follow-up of the planet was warranted,” he and his colleagues wrote in their 2014 LCROSS paper.

    Follow Nola Taylor Redd on Twitter @NolaTRedd Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.

  • 'Cosmic Recycling' Seeds The Prawn Nebula | Observatory Zoom-In Video

    Credit: ESO/Nick Risinger (skysurvey.org)

  • US Military Launches Advanced Tactical Communications Satellite Into Orbit

    An unmanned Atlas V rocket carrying the U.S. Navy's Mobile User Objective System 4 satellite (MUOS-4) launches into space from Florida's Cape Canaveral Air Force Station in a pre-dawn liftoff on Sept. 2, 2015.
    An unmanned Atlas V rocket carrying the U.S. Navy’s Mobile User Objective System 4 satellite (MUOS-4) launches into space from Florida’s Cape Canaveral Air Force Station in a pre-dawn liftoff on Sept. 2, 2015.
    Credit: United Launch Alliance

    The United States Navy launched an advanced new tactical communications satellite into orbit today (Sept. 2) to join a growing network designed to aid U.S. military forces stationed around the world. 

    An unmanned Atlas V rocket carrying the Navy’s fourth Mobile User Objective System satellite, or MUOS-4, lit up the pre-dawn sky in a dazzling display as it lifted off from a launchpad at Florida’s Cape Canaveral Air Force Station at 6:18 a.m. EDT (1018 GMT). It will eventually assume a geosynchronous orbit above Earth. The mission, which was overseen by the U.S. launch provider United Launch Alliance (ULA) was originally scheduled for Aug. 31, but delayed due to bad weather.

    The satellite is the fourth installment in the MUOS communications system, which is “designed to significantly improve ground communications for U.S. forces on the move,” according to a statement from Lockheed Martin, is building a total of five MUOS satellites for the U.S. military.

    The first two MUOS satellites launched in 2012 and 2013. The third MUOS satellite launched in January and is still undergoing testing before it becomes fully operational.

    A camera mounted to a United Launch Alliance Atlas V rocket captures an amazing view of the Earth from space while launching the U.S. Navy's Mobile User Objective System 4 satellite (MUOS-4) on Sept. 2, 2015.

    A camera mounted to a United Launch Alliance Atlas V rocket captures an amazing view of the Earth from space while launching the U.S. Navy’s Mobile User Objective System 4 satellite (MUOS-4) on Sept. 2, 2015.
    Credit: United Launch Alliance

    A United Launch Alliance Atlas V rocket carrying the MUOS-4 mission lifted off from Space Launch Complex 41 at the Cape Canaveral Air Force Station at 6:18 a.m. ET.

    A United Launch Alliance Atlas V rocket carrying the MUOS-4 satellite mission for the U.S. Navy lifted off from Space Launch Complex 41 at the Cape Canaveral Air Force Station at 6:18 a.m. ET.
    Credit: United Launch Alliance

    MUOS Communications Array

    Lockheed Martin, the company that built the MUOS satellites, created this graphic to show how the MUOS communications array benefits the U.S. military.
    Credit: Lockheed Martin

    “The MUOS works like a smartphone network in space, vastly improving secure satellite communications for mobile U.S. forces,” Navy Commander Paul Benishek said in a ULA webcast just after liftoff.

    MUOS is particularly helpful for troops in remote locations, because these soldiers can transmit and receive high-quality communications when the satellites are beyond the line of sight. All U.S. military services will be able to use the MUOS system, the statement said.

    “MUOS provides satellite communications in the narrowband spectrum,” Navy officials said in a statement. “Although narrowband communication is less than 2 percent of total Department of Defense [DoD] bandwidth, it represents more than 50 percent of all DoD satellite communication users. In addition to ad-hoc situations such as disaster response, narrowband represents the majority of communications for SEAL teams.”

    This is the 56th launch of an Atlas V rocket by ULA since the rocket’s debut in 2002. It is the sixth launch of an Atlas V rocket in the 551 configuration, which refers to the size of the payload capsule (5.4 meters or 17.7 feet wide), the number of solid rocket boosters (five) and the number of engines (one).

    The next MUOS satellite, MUOS-5, is expected to launch in 2016.

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

  • Russian Rocket Launches International Crew of 3 Toward Space Station

    Three new crewmembers launched toward the International Space Station early Wednesday morning, embarking on a mission that will boost the orbiting lab’s population to a level not seen in nearly two years.

    A Russian Soyuz spacecraft carrying cosmonaut Sergey Volkov, Andreas Mogensen from the European Space Agency and Kazakhstan’s Aidyn Aimbetov blasted off atop a Soyuz rocket Wednesday (Sept. 2) from Baikonur Cosmodrome in Kazakhstan at 12:37 a.m. EDT (0437 GMT). It was 10:37 a.m. local time in Baikonur at launch time. You can see a video of the flawless Soyuz launch here.

    “We’re doing great,” Volkov radioed down to Mission Control in Russia after the successful liftoff. “Everything is in order on board.”

    If all goes according to plan, the trio will reach the station on Friday morning (Sept. 4). The arrival will bring the number of crewmembers aboard the $100 billion orbiting complex to nine, a number last reached in November 2013, NASA officials said.

    But the abnormally dense population won’t last long. Mogensen and Aimbetov will return to Earth on Sept. 12 along with cosmonaut Gennady Padalka, who has been living on the International Space Station (ISS) since March.

    After that departure, six crewmembers will remain — Volkov and fellow cosmonauts Oleg Kononenko and Mikhail Kornienko, Japanese spaceflyer Kimiya Yui and NASA astronauts Scott Kelly and Kjell Lindgren.

    European Space Agency astronaut Andreas Mogensen (top) gives a thumb's up sign as he launched into space aboard a Russian Soyuz TMA-18M spacecraft with cosmonaut Sergei Volkov (bottom) and Kazakh Space Agency cosmonaut Aidyn Aimbetov from Baikonur Cosmodr

    European Space Agency astronaut Andreas Mogensen (top) gives a thumb’s up sign as he launched into space aboard a Russian Soyuz TMA-18M spacecraft with cosmonaut Sergei Volkov (bottom) and Kazakh Space Agency cosmonaut Aidyn Aimbetov (out of frame) from Baikonur Cosmodrome, Kazakhstan on Sept. 2, 2015. The trio is headed for the International Space Station.
    Credit: NASA TV

    Kelly and Kornienko are about halfway through the first-ever yearlong mission aboard the space station. Researchers are studying how they adapt physiologically and psychologically to long-duration spaceflight; the results should help pave the way for future human missions to Mars, NASA officials have said.

    (L to R) Aidyn Aimbetov of the Kazakh Space Agency, Sergei Volkov of the Russian Federal Space Agency and Andreas Mogensen of ESA (European Space Agency) will launch from the Baikonur Cosmodrome in Kazakhstan Wednesday, Sept. 2, 2015, and head to the Inte

    (L to R) Aidyn Aimbetov of the Kazakh Space Agency, Sergei Volkov of the Russian Federal Space Agency and Andreas Mogensen of the European Space Agency (ESA) will launch from the Baikonur Cosmodrome in Kazakhstan Wednesday, Sept. 2, 2015, and head to the International Space Station.
    Credit: NASA

    Kelly’s identical twin brother Mark, who is a former NASA astronaut, is participating in the experiment from the ground, serving as a control against which to compare the data gathered about Scott.

    Most crewmembers spend 5 to 6 months aboard the orbiting lab. Mogensen and Aimbetov are flying their brief 10-day mission because Soyuz spacecraft are certified to stay in space for just six months. So Kelly and Kornienko cannot return to Earth in the Soyuz that brought them up; instead, they will come down in the vehicle that is carrying Mogensen, Aimbetov and Volkov to the station.

    Aimbetov was a late addition to this “taxi flight.” His seat was supposed to be filled by English singer Sarah Brightman, who was reportedly set to pay about $50 milllion for her orbital experience. But Brightman backed out in May, citing “personal family reasons.”

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

  • Blast Off! New Crew Launch Will Make It 9 On Space Station | Video

    Credit: NASA

  • New Space Station Crew Will Launch Into Orbit Tonight: Watch Live

    A Russian Soyuz rocket stands poised atop its launchpad at Baikonur Cosmodrome, Kazakhstan ahead of the Sept. 2 launch of a new three-man crew to the International Space Station. The rocket will launch Russian cosmonaut Sergei Volkov, Danish astronaut And
    A Russian Soyuz rocket stands poised atop its launchpad at Baikonur Cosmodrome, Kazakhstan ahead of the Sept. 2 launch of a new three-man crew to the International Space Station. The rocket will launch Russian cosmonaut Sergei Volkov, Danish astronaut Andreas Mogensen and Kazakh astronaut Aidyn Aimbetov into orbit on a Soyuz TMA-18M spacecraft.
    Credit: RSC Energia

    Three new crewmembers will blast off toward the International Space Station late tonight (Sept. 1) and you can watch the liftoff live online.

    (L to R) Aidyn Aimbetov of the Kazakh Space Agency, Sergei Volkov of the Russian Federal Space Agency and Andreas Mogensen of ESA (European Space Agency) will launch from the Baikonur Cosmodrome in Kazakhstan Wednesday, Sept. 2, 2015, and head to the Inte

    (L to R) Aidyn Aimbetov of the Kazakh Space Agency, Sergei Volkov of the Russian Federal Space Agency and Andreas Mogensen of the European Space Agency (ESA) will launch from the Baikonur Cosmodrome in Kazakhstan Wednesday, Sept. 2, 2015, and head to the International Space Station.
    Credit: NASA

    Cosmonaut Sergei Volkov of the Russian Federal Space Agency, Andreas Mogensen of the European Space Agency and Aidyn Aimbetov of the Kazakh Space Agency are scheduled to blast off from the Baikonur Cosmodrome in Kazakhstan early Wednesday, Sept. 2, at 12:37 a.m. EDT (0437 GMT/10:37 a.m. Baikonur time). 

    NASA will begin live coverage of the launch at 11:45 p.m. EDT (0345 GMT) and you can watch the broadcast on Space.com, courtesy of NASA TV.

    The astronauts are scheduled to arrive at the station on Friday, Sept. 4, at 3:24 a.m. EDT (0724 GMT). NASA will also provide live coverage of that event.

    Cosmic Quiz: Do You Know the International Space St…

    The International Space Station is the largest structure in space ever built by humans. Let’s see how much you know about the basics of this science laboratory in the sky.

    Sunlight glints off the International Space Station.

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    Cosmic Quiz: Do You Know the International Space St…

    The International Space Station is the largest structure in space ever built by humans. Let’s see how much you know about the basics of this science laboratory in the sky.

    Start Quiz
    Sunlight glints off the International Space Station.

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    The arrival of the three new crewmembers will bring the total crew count on the station to nine. This is the first time nine crewmembers have been on board the orbiting laboratory simultaneously since November 2013, according to a statement from NASA.

    Mogensen and Aimbetov will serve short-duration stints, returning to Earth on Sept. 12, along with Russian cosmonaut Gennady Padalka, who is already on the station. Volkov will stay on the station for six months, joining American astronaut Scott Kelly and Russian cosmonaut Mikhail Kornienko in the second half of their yearlong mission, the longest mission ever completed aboard the International Space Station.

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

  • Stunning Web Comic 'Brassens in Space' Takes Readers on Cosmic Journey

    'Brassens in Space' Comic
    An image from the Web comic “Brassens in Space,” by French cartoonist Boulet. In the comic, the artist takes the songwriter Georges Brassens on a tour of the solar system, to show him the wonder and awe made possible by science.
    Credit: Boulet/bouletcorp.com

    Does science kill the poetry of nature, or does it write new volumes of wonder and awe?

    A French cartoonist who goes by the name Boulet says it’s the latter, and he expressed his opinion in a gorgeous Web comic called “Brassens in Space,” which you can find here. Boulet’s comic takes readers on a journey through the cosmos, pointing out just a few of the awe-inspiring landscapes made visible by science.

    'Brassens in Space' Comic Panel

    An image from the Web comic “Brassens in Space,” by the French cartoonist Boulet.
    Credit: Boulet/bouletcorp.com

    Boulet’s inspiration for the comic was a song by the French singer Georges Brassens. The song laments that science has taken away humanity’s belief in ancient gods. “The song always bothered me…” Boulet tells the songwriter. “It sounds like … Like you’re blaming science for killing poetry. And I strongly disagree!” [Fly Through Real Space Photos in Amazing Video]

    The comic is Boulet’s attempt to convey that, rather than killing poetry and passion, science has provided new things to be passionate about, by revealing the wonders of the universe that were once hidden.

    The Web comic shows a young Boulet looking at the night sky through a telescope in his backyard. From there, he could see some of those incredible cosmic locations, and dreamed of visiting them. He takes Brassens on a tour of the solar system, visiting places like the gas giant Jupiter.

    “It’s Hell there, an entire world made of storms so violent that would make a nuclear blast look like a mosquito’s fart,” the comic said. “And it’s just … THERE. Floating in the sky, visible from your garden!”

    Throughout their illustrated journey, Boulet tries to show Brassens how knowledge of the universe has opened up more opportunities to be awestruck, humbled, passionate and poetic.

    “I see in the night sky a sort of opposite Plat[o]’s Cave: when you shut down the blinding light, you can see billions of things hiding in the dark,” Boulet wrote in the comic. “So many wonders in this ocean, like the lights of the Pleiades, shining like little diamonds…And the emotion you feel the first time you see Saturn and its rings, so tiny in the telescope!”

    To get the full experience, go read the entire comic (and thanks to The Planetary Society blog for pointing it out to us). If you’re already a lover of the cosmos, you’ll know exactly what Boulet is talking about. And if you aren’t totally awed by what astronomy has revealed about the universe, this comic might just convince you.  

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

  • This Photo of Saturn's Moon Dione Crossing the Planet Is Simply Jaw-Dropping

    Dione Transit of Saturn
    Saturn’s moon Dione crosses the face of the ringed planet in an image obtained on May 21, 2015.
    Credit: NASA/JPL-Caltech/Space Science Institute

    An icy moon of Saturn hangs against the face of its giant parent planet in a breathtaking new image captured by NASA’s Cassini spacecraft.

    The photo, which Cassini took on May 21, shows the moon Dione crossing Saturn’s disk. Careful study of such “transits” can help astronomers better understand the orbits of Dione and other moons in the solar system, NASA officials said.

    Furthermore, NASA’s Kepler space telescope and some other instruments hunt for exoplanets by looking for tiny dips in a star’s brightness caused by transiting alien worlds. Studying the light coming from such extrasolar systems can also reveal details about the composition of these exoplanets’ atmospheres.

    At 696 miles (1,120 kilometers) in diameter, Dione is the fourth-largest of Saturn’s sixty-odd moons; only Titan, Rhea and Iapetus are bigger. Parts of Dione are heavily cratered, and the satellite’s trailing side features mysterious ice cliffs and fractures that run for tens or hundreds of kilometers. Cassini has also detected a wispy oxygen atmosphere surrounding the frigid moon.

    Cassini snapped the new photo, which was released today (Aug. 31), when the probe was about 1.4 million miles (2.3 million km) from Saturn. The image’s resolution is 9 miles (14 km) per pixel.

    Saturn Quiz: How Well Do You Know the Ringed Planet?

    With more than 60 known moons to go along with its famous rings, Saturn is as intriguing as it is beautiful. How much do you know about the sixth planet from the sun?

    Spectacular New Images Showcase Saturn's Rings

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    Saturn Quiz: How Well Do You Know the Ringed Planet?

    With more than 60 known moons to go along with its famous rings, Saturn is as intriguing as it is beautiful. How much do you know about the sixth planet from the sun?

    Start Quiz
    Spectacular New Images Showcase Saturn's Rings

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    But Cassini has gotten much closer looks at Dione, thanks to a handful of flybys over the years. During the most recent one, which occurred Aug. 17, the spacecraft zoomed within just 295 miles (474 km) of the moon’s surface, returning a set of amazing images.

    The Aug. 17 maneuver was the last scheduled up-close look at Dione, however; no more close flybys are planned before Cassini ends its mission with an intentional death dive into Saturn’s thick atmosphere in September 2017.

    The $3.2 billion Cassini mission, which launched in 1997 and arrived in the Saturn system in 2004, is a joint operation involving NASA, the European Space Agency and the Italian Space Agency.

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

  • Unearthing NASA's 'Worm': Reissue of Manual Celebrates Retired NASA Logo

    NASA Graphics Standards Manual
    The NASA Graphics Standards Manual, which in 1976 defined the use of now-retired NASA “worm” logo, is getting a limited reissue through Kickstarter.
    Credit: Hamish Smyth

    A 40-year-old book that gave rise to one of NASA’s most iconic logos is being relaunched as a limited edition reprint on Kickstarter.

    The NASA Graphics Standards Manual, first published in January 1976, defined a new graphic identity for the U.S. space agency. As designed by Richard Danne and Bruce Blackburn, the guide introduced a stark logotype, on which the letters “N-A-S-A” were “reduced to their simplest form, replacing the red, white and blue circular emblem with the white block letters,” as Danne’s original introduction to the book described.

    The manual debuted the planned deployment of the NASA “worm,” an affectionate or derogatory unofficial nickname, depending on the viewer’s perspective, taking the place of the “meatball,” the space agency’s first insignia. The red-letter, stylized logotype was front and center for the first decade of the space shuttle program, emblazoned on the wings of the orbiters, the astronauts’ spacesuits, and even the body of the Hubble Space Telescope. [Photos: NASA’s Offbeat Mission Posters]

    And then in 1992, at the singular order of the then-head of NASA, the worm was rejected and the meatball restored.

    Now, two designers who grew up knowing the worm as the only symbol that represented NASA are seeking to reprint the Graphics Standards Manual, to honor what Danne and Blackburn achieved and to ensure that the legacy of the worm is preserved.

    “We’re really looking at this as an archival project to really preserve this document so that it can be seen by graphic designers, space enthusiasts and by people who can learn from the manual,” remarked Jesse Reed, who with fellow designer Hamish Smyth is behind the crowd-funding effort that began on Tuesday morning (Sept. 1).

    The pair’s 34-day Kickstarter campaignis offering a hard-bound copy of the original manual, supplemented with files from Danne’s own archives, for $79. For the project to go into print, Reed and Smyth need pledges for 2,000 copies of the book, raising at least $158,000.

    “We’re really only offering the book as a reward in support of the campaign,” Reed said. “We are not doing packages of items or collectibles. It is really just about the book.”

    Reed and Smyth, who work as associate partners for the design firm Pentagram, have experience reissuing a style guide through Kickstarter. Last year, their first campaign rocketed to more than $800,000 — eight times more than what they had set as their goal — for a new reprint of the 1970 New York City Transit Authority Graphics Standards Manual, the design reference that solved how to find the way around on the city’s underground subway. [Related: How Crowdfunding is Helping Space Projects]

    Like the NYCTA book, the NASA manual has become one of the world’s classic examples of modern design.

    “From a graphic designer’s perspective, this document is a very good example of systematic design and the way to take what was a mess of graphic identity and really strip that all away, creating this very analytical system on how to communicate what type of agency NASA is,” described Reed.

    Reed and Smyth plan to reproduce the manual in full-scale within the 200 pages of the limited edition reissue.

    “Every page of the manual will be completely included. It’ll appear exactly as it appeared in the manual,” Reed said. “Nothing about the design will be altered in any way.”

    The most noticeable difference between the 1976 manual and the reissue will be the binding. The original, like most graphics standards manuals of its day, was held together in a ring binder so pages could be taken out and replaced as updates were made.

    The new hardcover reissue will include 10 fold-out pages (gatefolds) and will be packaged in a static shield pouch (“like space hardware or computer parts use,” Reed said).

    The new edition will also include extra content before and after the pages of the vintage manual.

    “What we are doing is including an essay at the beginning of the book written by Christopher Bananos, who writes for New York Magazine. He’ll be doing a historical introduction to NASA, the culture of the administration and the socio-economic view within the country during that period,” Reed told collectSPACE.com.

    “Additionally, Richard [Danne] has given us all of his other supplementary material, including the original presentation that he gave to NASA to propose this new identity,” Reed said. “We also have all of these amazing photographs of the shuttle, space food, of [the worm] actually being used in space, that will be included in the book as well.”

    Reed and Hamish, as self-described “design nerds,” hold the original NASA graphics manual in high regard as “a beautiful example of rational, systematic design.” Initially, after the success of their NYCTA reprint in 2014, they had no plans to take on a similar project but were attracted by what the worm represented.

    Danne & Blackburn Graphics Standards Manual

    The Danne & Blackburn Graphics Standards Manual provided a reference for how the NASA logo was to be applied across the space agency.
    Credit: Hamish Smyth

    “I think what is great about the worm logo is that it visually communicates what NASA does. It really communicates the idea of streamlining and interconnectivity without any frivolous or extra components that are not necessary to do the job,” said Reed. “I think that is what the worm does.”

    “When you look at it, the reason I think that most people like it from a subconscious point of view, is that it actually look likes space,” he said.

    Watch a video about the NASA Graphics Standards Manual, its history and legacy, at collectSPACE.

    Follow collectSPACE.com on Facebook and on Twitter at @collectSPACE. Copyright 2015 collectSPACE.com. All rights reserved.

  • Best Night Sky Events of September 2015 (Stargazing Maps)

    Sunday, Sept. 27, evening. There will be a triple treat for observers in eastern North America as sun, Earth, and moon align: a total lunar eclipse, the…Read More » moon at its closest, and a full moon, all in one evening. At 8:12 p.m. EDT, the lunar eclipse will begin with the first faint lunar shadow creeping onto the moon. At 9:48, the moon reaches an extreme perigee, the closest it will get to Earth in all of 2015: 221,753 miles (356,877 km). Total phase of the eclipse will begin at 10:11 p.m. and mid eclipse will be at 10:47. At 10:51 it will be the instant of full moon, the largest full moon in 2015. At 11:23, the total phase of the eclipse will end, and at 1:23 a.m. the last of the Earth’s shadow will leave the moon. In western North America, the moon will already be in eclipse when the moon rises. Observers in South America, Europe, and Africa will also see most of this eclipse. The illustration shows the moon just entering the umbral shadow of Earth at 9:12 p.m. EDT.   Less «

  • Ride Along on New Horizons Probe's Epic Pluto Flyby (Video)

    An amazing new video takes viewers along for the ride during a NASA spacecraft’s epic July flyby of Pluto.

    The Pluto flyby video gives a probe’s-eye view of the historic July 14 encounter, during which the New Horizons spacecraft zoomed within just 7,800 miles (12,550 kilometers) of the dwarf planet’s frigid surface.

    The short video stitches together real images captured by New Horizons, showing a dramatically sped-up depiction of the probe’s approach and close Pluto flyby, as well as its passage out into the dark depths of the faraway Kuiper Belt. It was assembled by Stuart Robbins, who was a post-doc student at the Southwest Research Institute who worked on the New Horizons mission.

    New Horizons kept its eyes trained on Pluto for a spell after the flyby, watching the dwarf planet pass in front of the sun to learn more about the icy object’s wispy but far-reaching atmosphere.

    The New Horizons team has received only a tiny fraction of the flyby data; it will likely take the probe until the end of 2016 to beam all of the images and measurements captured during the event back to Earth, mission officials have said.

    But the observations that have made it down to mission control have already revolutionized researchers’ understanding of Pluto, showing a complex world with towering ice mountains and vast ice plains. New Horizons’ images show that large areas of Pluto are completely or largely crater-free, suggesting that the dwarf planet remained geologically active until the recent past — and may even still be active today.

    Pluto Quiz: How Well Do You Know the Dwarf Planet?

    Pluto, the most famous dwarf planet in our solar system, underwent a well-publicized (and somewhat controversial) reclassification that took away its title as the ninth and most distant planet from the sun. So, how well do you know this fascinating world?

    Hubble Space Telescope photo of Pluto is most detailed ever seen.

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    Pluto Quiz: How Well Do You Know the Dwarf Planet?

    Pluto, the most famous dwarf planet in our solar system, underwent a well-publicized (and somewhat controversial) reclassification that took away its title as the ninth and most distant planet from the sun. So, how well do you know this fascinating world?

    Start Quiz
    Hubble Space Telescope photo of Pluto is most detailed ever seen.

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    New Horizons’ photos have also revealed huge canyon systems on Charon, the largest of Pluto’s five moons, and given scientists their first decent looks at small satellites in the system, such as Nix and Hydra.

    The $720 million New Horizons mission launched in January 2006 to lift the veil on Pluto. But the probe’s science work is probably not done: Mission team members announced last week that they plan to target a small Kuiper Belt object known as 2014 MU69 for a close flyby that would take place in January 2019.

    New Horizons’ handlers plan to perform several engine burns in October and November to put them on a course for 2014 MU69. But for the future flyby to occur, NASA must officially approve a New Horizons mission extension, which the team will apply for next year. 

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

  • Rare 'Supermoon' Total Lunar Eclipse Coming This Month

    The first “supermoon” lunar eclipse in more than three decades will grace Earth’s skies this month, as will a partial solar eclipse that most of the world will miss.

    The supermoon total lunar eclipse, which occurs on Sept. 27, features a full moon that looks significantly larger and brighter than usual. It will be the first supermoon eclipse since 1982, and the last until 2033, NASA officials said in a newly released video.

    The total lunar eclipse will be visible to observers throughout the Americas, Europe, Africa, western Asia and the eastern Pacific Ocean region. [‪How Lunar Eclipses Work (Infographic)]

    A partial solar eclipse will take place two weeks before this special supermoon, on Sept. 13, but the earlier event will be visible only to skywatchers in southern Africa (as well as penguins, leopard seals and the other wildlife of Antarctica).

    Supermoons” occur because the moon’s orbit around Earth is elliptical rather than circular. While the moon’s average distance from our planet is about 239,000 miles (384,600 kilometers), the natural satelite roams as far away as 252,000 miles (405,600 km) at “apogee” and gets as close as 226,000 miles (363,700 km) at “perigee.”

    A supermoon is a full moon that occurs at, or very near, perigee and appears abnormally big in the sky as a result. In fact, supermoons appear about 14 percent larger and 30 brighter than apogee full moons, which are also known as “minimoons.”

    Supermoon eclipses are special; they’ve occurred just five times since 1900 (in 1910, 1928, 1946, 1964 and 1982), NASA officials said in the new video. “Normal” lunar eclipses are much more common. In fact, an observer at any particular location around the globe can expect to see a total lunar eclipse about once every 2.5 years on average.

    Total Lunar Eclipse of April 2015

    Photographer Dean Hooper captured this spectacular view of the April 4, 2015 total lunar eclipse from Melbourne, Australia. This image was shared by the Virtual Telescope Project in Italy.
    Credit: Dean Hooper via Virtual Telescope Project

    Lunar and solar eclipses are both caused by alignments of the moon, Earth and sun. In the case of a lunar eclipse, the Earth is the middle of this line and the moon passes into the planet’s shadow. But the moon doesn’t go completely dark during total eclipses; rather, it often turns a reddish hue because it’s hit by sunlight bent by Earth’s atmosphere. For this reason, total lunar eclipses are often referred to as “blood moons.”

    With a solar eclipse, the moon is in the middle of the Earth-moon-sun line and blots out all or part of the solar disk from an Earth observer’s perspective.

    If you live in southern Africa or plan to travel to the region to view the Sept. 13 partial solar eclipse, a word of warning: NEVER look at the sun without proper eye protection, even during an eclipse; serious and permanent eye damage can result.

    You can learn about safe eclipse-viewing strategies in this Space.com infographic.

    Editor’s note: If you capture an amazing view of the supermoon lunar eclipse or any other night sky view that you would like to share with Space.com for a possible story or gallery, send images and comments in to managing editor Tariq Malik at: spacephotos@space.com.

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

  • How 'Starshades' Could Aid Search for Alien Life

    1/100th-Scale Starshade
    Nineteen different subscale versions of a light-blocking “starshade” were tested recently in the Nevada desert.
    Credit: Northrop Grumman Corporation

    The next step in the exoplanet revolution may be an in-space “starshade” that lets alien worlds step out of a blinding glare.

    Researchers are testing designs for a starshade, which would fly in formation with a future space-based telescope. The starshade, also known as an “external occulter,” would block the light from a star while allowing the scope to spot emissions from much dimmer orbiting planets.

    Scientists are conducting desert tests of the technology on Earth. They’re using the McMath-Pierce Solar Telescope at Kitt Peak National Observatory in Arizona to model a starshade’s ability to help future instruments find and characterize rocky, Earth-like alien worlds. [10 Exoplanets That Could Host Alien Life]

    A starshade may be used on NASA’s potential Wide-Field Infrared Survey Telescope (WFIRST), a space-based instrument that would feature a primary mirror 8 feet (2.4 meters) wide, the same size as that of the agency’s iconic Hubble Space Telescope.

    Several years ago, the U.S. National Reconnaissance Office (NRO) donated two space telescopes to NASA. In 2013, the space agency announced it hoped to use one of these scopes for WFIRST. That move spurred anticipation in the U.S. astronomical community for Hubble-quality imaging over an area of sky 100 times larger than that viewed by Hubble. This version of the mission is called WFIRST-AFTA (for “Astrophysics-Focused Telescope Assets”).

    The WFIRST-AFTA mission would carry out exoplanet exploration, dark energy research, and galactic and extragalactic surveys.

    Desert and mountaintop testing

    Small-scale versions of starshades have undergone nighttime desert testing in Nevada and California and, more recently, at the McMath-Pierce Solar Telescope site.

    Starshade Concept Northrop Grumman

    How a starshade works. The concept is telescope-agnostic and could find use on NASA’s Wide-Field Infrared Survey Telescope (WFIRST) project.
    Credit: Northrop Grumman

    The sites selected for evaluating starshade designs each have pros and cons, but collectively the evaluations are complementary and help to validate optical modeling of the idea, said Steve Warwick, Starshade program manager at Northrop Grumman Aerospace Systems.

    “We can’t do everything we can do in space on the ground in terms of optics, but the tests add a lot of confidence to how the starshade will work on orbit,” Warwick told Space.com.

    McMath operators said testing sharshades with the telescope, which was dedicated in 1962, was the craziest way that anyone had used the facility to date, Warwick said.

    “They were extremely helpful and excited to see what we could do with their facility,” Warwick said of the McMath team. Starshade testing at the Arizona site has been done twice so far, in late March and then in June.

    The hope is to return to that location in the November-December time period; the exact timing will depend partly on other McMath users’ schedules, Warwick said.

    A mix of NASA funding and Northrop Grumman funding has enabled the starshade test program to move forward.

    Planet light

    So what’s the big deal about starshades?

    The technology — a flower-shaped screen that flies at a considerable distance from a space telescope —blocks starlight to create a high-contrast shadow. This shadow is so dark that only planet light enters a space telescope for examination by onboard instruments.

    Artist's Rendition of Proposed WFIRST-AFTA Mission from NRO Image

    NASA’s proposed Wide-Field Infrared Survey Telescope (WFIRST) is an orbiting telescope with a 2.4-meter primary mirror — the same size as the Hubble Space Telescope mirror. Work is underway to fly a starshade in concert with WFIRST to enable exoplanet studies.
    Credit: NASA/Goddard Space Flight Center

    You can think of it as your big thumb blocking out blazing beams of light from the sun.

    Tackling technology gaps

    But a starshade in space has never seen the light of day, so to speak. While starshade engineers are drawing upon a successful track record of fielding large, deployable antennas in space, they must also beat back what are called “key technology gaps,” Warwick said.

    “For there to be a starshade launch with any telescope,” Warwick said, “we obviously need a lot of confidence that we’re going to get the science that we want to get.”

    Both the desert trials and McMath mountaintop testing address a key technology gap — “that the optical models are trustworthy … that the models agree with what we measure,” said Warwick. He added that he thinks these gaps can be filled relatively soon.

    “For me, where I sit, what excites me is the idea of being able to fly along with WFIRST,” he added.

    McMath-Pierce Solar Telescope

    Technicians have made use of the McMath-Pierce Solar Telescope at Kitt Peak National Observatory in Arizona to assess and validate optical models of starshade designs.
    Credit: Northrop Grumman/Robert Brown

    Given the potential 2024-2025 launch of that instrument, a decision about whether to include a starshade on the mission could come in the next two to three years, Warwick said.

    There are other possibilities beyond WFIRST as well. For example, the proposed 33-foot (10 m) Large Ultraviolet Optical Infrared (LUVOIR) telescope and the projected Habitable Planet Explorer, or HabEx for short, could also incorporate starshades, Warwick said. [Next-Generation Space Telescopes Could Look for Aliens (Video)]

    Snagging spectra

    There is growing general support for WFIRST to include technology demonstrations of both a coronagraph (a light-blocking instrument that’s built into the space telescope) and a starshade (which flies separately), Warwick said.

    “From our point of view, that’s a very exciting opportunity,” Warwick said. Such technology may enable spectra to be examined of some planets located in the “habitable zone” around their stars, where liquid water could exist on a world’s surface.

    “A starshade with WFIRST could give us indications about habitable planets … but there’s a huge difference between ‘habitable’ and ‘inhabited,’” Warwick cautioned.

    A larger telescope with a larger starshade could inform scientists about biosignatures from exoplanets, Warwick said, “and that would give us an indication of inhabited planets.”

    But again, Warwick said, any biosignatures detected would not necessarily identify intelligent alien life. Rather, such signs would indicate some type of biological activity that has changed the planet’s atmosphere.

    In pondering the larger cosmic picture, Warwick said he sees a starshade or something similar revealing that Earth life is not alone in the universe.

    “I’ll take a bet that we will find signs of life outside of our solar system before we find it inside our solar system,” Warwick concluded.

    Leonard David has been reporting on the space industry for more than five decades. He is former director of research for the National Commission on Space and is co-author of Buzz Aldrin’s 2013 book “Mission to Mars – My Vision for Space Exploration” published by National Geographic with a new updated paperback version released in May 2015. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.