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From space.com

  • Rocket Lab Sets New Window for Second Electron Launch

    Rocket Lab’s second Electron rocket stands on its New Zealand pad prior to a series of launch attempts in December 2017. A new window for the launch opens in late January 2018.

    WASHINGTON — Rocket Lab announced Jan. 11 it plans to make another attempt to launch its Electron small rocket on its second mission later this month.

    Rocket Lab said the nine-day launch window for the mission at its New Zealand launch site will open at 2:30 p.m. Jan. 20 local time (8:30 p.m. Jan. 19 Eastern time). There will be a four-hour window each day, opening at the same time, for the launch.

    The company, headquartered in the United States but with launch and other operations in New Zealand, attempted to carry out the launch during a 10-day window in December. However, several attempts were postponed by poor weather. The company came closest to launching Dec. 11, when computers aborted a launch attempt just two seconds before liftoff after sensors detected liquid oxygen temperatures above preset limits in one of the first stage’s nine engines. [Watch: Rocket Lab’s 1st Test Flight]

    In a Jan. 11 interview, Rocket Lab Chief Executive Peter Beck said the company stood down at the end of last month’s window, rather than attempt to extend it, to give employees a break over the Christmas holidays. “We were conscious to give our team a decent rest after a big year,” he said.

    There are no major changes planned for this launch opportunity versus last month’s attempt, he said. “The issues we had technically were minor,” he said. The high-altitude winds that scrubbed several attempts would likely have not been an issue for regular operations, he added, but the company wants “the best initial conditions” for this test flight.

    Rocket Lab launched the Electron, designed to place up to 150 kilograms into sun-synchronous orbit, for the first time last May. The rocket failed to reach orbit, which the company blamed on a telemetry problem that triggered range safety systems about four minutes after liftoff, and not a problem with the rocket itself.

    The rocket is carrying instrumentation as well as three cubesats, two from Spire and one from Planet. Should the launch be successful, Beck said Rocket Lab will move ahead with commercial missions. The next Electron will be at the pad as soon as February, although he did not disclose who the customer would be for that mission if it is a commercial flight.

    “Right now the focus is just to get through this test flight, and then we’ll start the commercial manifest for the year,” he said.

    This story was provided by SpaceNews, dedicated to covering all aspects of the space industry.

  • SpaceX Dragon Capsule Returns to Earth After Space Station Delivery

    A SpaceX Dragon capsule departs the International Space Station on Jan. 13, 2018 to return 4,100 lbs. (1,860 kilograms) of science gear to Earth and end a monthlong delivery mission.

    A SpaceX Dragon cargo ship left the International Space Station and returned to Earth Saturday (Jan. 13), wrapping up a nearly month-long delivery mission for NASA that also marked the spacecraft’s second trip to space.

    The uncrewed Dragon supply ship detached from the space station’s robotic arm at 4:58 a.m. EST (0958 GMT) and began firing thrusters for its return to Earth. The space capsule splashed down in the Pacific Ocean off the coast of Baja California to be retrieved by SpaceX, the company announced at 10:39 a.m. EST (1539 GMT). [See photos of the Dragon cargo ship’s mission]

    “Good splashdown of Dragon confirmed, completing the second resupply mission to and from the @Space_Station with a flight-proven commercial spacecraft,” SpaceX representatives said in a Twitter update

    Dragon is carrying nearly 4,100 lbs. (1,860 kilograms) of cargo to Earth, much of it science gear from human and animal research, and other experiments. That gear includes hardware from an experiment by space manufacturing company Made In Space to 3d-print ZBLAN glass fiber optic wire in space, and a group of live mice from NASA’s Rodent Research 6 study to develop medications that address muscle loss in space., NASA officials said.

    A SpaceX Falcon 9 rocket launched the Dragon mission on Dec. 15, with the capsule arriving at the International Space Station on Dec. 17. The mission, SpaceX’s 13th resupply flight for NASA, delivered 4,800 lbs. (2,177 kilograms) of supplies and gear for astronauts.

    In addition to delivering cargo, the mission marked a milestone for SpaceX’s rocket reusability program. Both the Dragon capsule and its Falcon 9 booster made their second trips to space on this flight. The Falcon 9 booster’s first stage previously launched a different Dragon capsule to the space station in June 2017. The Dragon capsule on this flight, meanwhile, previously visited the space station in April 2015. 

    Editor’s note: This story was updated at 10:49 a.m. EST to include the successful splashdown of the Dragon capsule. 

    Email Tariq Malik at tmalik@space.com or follow him @tariqjmalik and Google+. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.

  • Indian Rocket Launches 31 Satellites Into Orbit

    An Indian Polar Satellite Launch Vehicle has launched 31 new satellites into orbit, making a successful comeback after a launch failure last August.

    The PSLV rocket lifted off from the Indian Space Research Organisation’s Satish Dhawan Space Centre in Sriharikota on the country’s east coast carrying the agency’s Cartosat-2F Earth observation satellite and 30 smaller payloads. Liftoff occurred Thursday, Jan. 11, at 10:59 p.m. EST (0359 Jan. 12 GMT), though it was Friday morning local time at the launch site.

    The PSLV rocket launch was the first by ISRO since an Aug. 31 failure that doomed an Indian navigation satellite. That failure was traced to a malfunction with the booster’s payload fairing separation system, ISRO have said.

    A Polar Satellite Launch Vehicle launches the Cartosat-2F Earth observing satellite and 30 other smaller payloads into orbit from the Satish Dhawan Space Centre in Sriharikota for the Indian Space Research Organisation. Liftoff occurred on Jan. 12, 2018 local time.

    A Polar Satellite Launch Vehicle launches the Cartosat-2F Earth observing satellite and 30 other smaller payloads into orbit from the Satish Dhawan Space Centre in Sriharikota for the Indian Space Research Organisation. Liftoff occurred on Jan. 12, 2018 local time.

    Credit: Indian Space Research Organisation

    The Cartosat-2F satellite launched on the new mission is an Earth-mapping satellite designed to assist land and resource monitoring and management, according to a mission description. It is part of a growing series of Cartosat-2 satellites launched by ISRO. It was delivered successfully into orbit 313 miles (505 kilometers) above Earth.

    The 30 other satellites that hitched a ride to space with Cartosat-2F included a wide variety of craft from seven different countries, including the asteroid-hunting Arkyd-6 nanosatellite for the U.S. space mining company Planetary Resources.

    “The co-passenger satellites comprise one Microsatellite and one Nanosatellite from India as well as 3 Microsatellites and 25 Nanosatellites from six countries, namely, Canada, Finland, France, Republic of Korea, UK and USA,” ISRO officials wrote in a statement. 

    Email Tariq Malik at tmalik@space.com or follow him @tariqjmalik and Google+. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.

  • Wild 360-Degree Video Lets You See the Milky Way As a Giant Black Hole Would

    NATIONAL HARBOR, Md. — Ever wish you could see the galaxy from the perspective of a black hole? A new 360-degree simulation that uses data from NASA’s Chandra X-Ray Observatory is helping astronomers better understand more than 22 stellar giants found at the center of the Milky Way galaxy.

    The simulation, unveiled here Wednesday (Jan. 10) at the 231st meeting of the American Astronomical Society (AAS), allows you to view over 20 Wolf-Rayet stars, which are massive stars orbiting the center of the Milky Way from a distance of about 1.5 light-years. The 360-degree simulation, which you can see on YouTube here, starts 350 years in the past and moves forward 500 years, according to an accompanying statement. Check out the simulation below:

    In the simulation, viewers can stare outward from Sagittarius A*, the supermassive black hole that dominates the Milky Way’s galactic center. Though the video is available on YouTube, the best way to watch it is with virtual-reality (VR) systems, such as the Samsung Gear VR or Google Cardboard, according to NASA researchers. The video mimics the effect of VR goggles as you use a smartphone to pan around and see different parts of the simulation. [Best Samsung Gear VR Apps]

    “I have placed you, the viewer of the video, as Sagittarius A*, so you had a very good holiday season and gained 4 billion solar masses,” joked lead researcher Christopher Russell, of the Pontifical Catholic University of Chile, as he presented the video. “You now have stars that are orbiting you.”

    A labeled look at features of the Milky Way's galactic center in a new 360-degree tour of our galaxy's core.

    A labeled look at features of the Milky Way’s galactic center in a new 360-degree tour of our galaxy’s core.

    Credit: NASA/CXC/Pontifical Catholic Univ. of Chile /C.Russell et al.

    So how do astronomers get the data that makes this visualization possible?

    It turns out that the Wolf-Rayet stars release streams of gas into interstellar space, and when the former outer layer of one star comes into contact with that of another star, “sonic booms” are created. These shock waves then heat the gas to millions of degrees, causing a glow that Chandra can pick up as X-rays, according to NASA. The visualization is based off of fundamental infrared data on the Wolf-Rayet stars, detected with the European Southern Observatory’s Very Large Telescope, as well as data about the gas’s distribution and incredibly high temperatures taken by Chandra.

    Astronomers can watch the stellar gas coming off the Wolf-Rayet stars and can also watch a simulation in which the black hole interacts with the gas. In the second video, the gravity of Sagittarius A* pulls the gas inward. The black hole also produces outbursts that expel material, causing the “outburst” video to be darker at moments.

    The simulation also provides an opportunity to visualize other cosmic phenomena. As long as you have a large data set with enough variation, Russell said during a panel session at the AAS meeting, you can extend the simulation technology to model other worlds, too. He added that the next project may involve visualizing binary (double-star) systems.

    Follow Doris Elin Salazar on Twitter @salazar_elin. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.

  • Ames Research Center: R&D Lab for NASA

    Aerial image of NASA Ames Research Center.

    Ames Research Center is one of the oldest facilities currently operated by NASA. Lying just south of San Francisco, in the heart of Silicon Valley, Ames boasts a wealth of research projects. It is one of 10 NASA field centers.

    “Ames Research Center … contributes to virtually every major NASA mission and initiative,” the Ames website states. 

    Ames grew out of Moffett Field, which was originally conceived of as a base for the Navy’s rigid airships in 1931. Local communities donated 100 acres for the base, while the government purchased an additional 750 acres, according to Elizabeth Muenger in the book “Searching the Horizon: A History of Ames Research Center, 1940-1976.” At the time, the Navy had two such ships, the Akron and the Macon. 

    In 1939, Congress authorized a second laboratory for the National Advisory Committee for Aeronautics (NACA), the precursor to NASA, to be developed at Moffett. (The first was Langley Memorial Aeronautical Laboratory, which became Langley Research Center.) The Navy still hoped to develop rigid airships in the future, and requested that any NACA buildings be located outside the mooring circles. In December 1939, the Army gave NACA the use of 62 acres of land. The agency purchased another 40 acres from local farmers and began surveying building locations.

    Ground was broken at Moffett Field, California, in 1939, and operations began in early 1941. In 1944, NACA named the facility in honor of Joseph S. Ames, leading aerodynamicist, former president of Johns Hopkins University, and one of the founding members of NACA.

    From the start, Ames was bent toward urgent research in aircraft structures. Some of its original facilities include multiple wind tunnels used to test and refine aircraft and guided missiles; today, the facilities serve similar purposes for satellites. The Air Force passed Moffett Airfield to NASA in 1994, when the military base closed.

    “Wind tunnels are central to Ames’ history,” says Ames’ historical website. “Of particular note are three tunnels later designated key national resources.”

    The largest of the three, the Unitary Plan Wind tunnel, has tested almost all NASA crewed space vehicles, including the space shuttle, and is the only one still in use today. In 1985, the 11-acre wind tunnel was listed on the National Register of Historic Places.

    “The Ames Unitary Plan Wind Tunnel is significant because it represents the continual development of superior technical aeronautical research facilities after the end of the Second World War,” Harry Butowsky, then of the National Park Service, said on the nomination form.

    “These research facilities formed the foundation upon which the National Aeronautics and Space Administration would draw in 1958 to launch the American effort to land a man on the moon.”

    In 1958, Ames became part of the newly formed National Aeronautics and Space Administration (NASA). Ames provided input to the fledgling agency’s top priority, the lunar program, testing and refining the re-entry capsules and thermal protection in the Center’s new Arc Jet Complex and hypervelocity ranges. The arc jets later contributed to thermal protection for all of NASA’s crewed programs, including the space shuttle, as well as planetary missions like the Galileo satellite to Jupiter.

    “The complex will continue to be central to the research and development of materials suitable for heatshield applications,” the website says.

    In the 1950s, Moffitt Field’s Hangar One, one of the world’s largest freestanding structures, was designated a Historic American Engineering Record; in 2008, the 8-acre structure was listed as one of the most endangered historic places. In 2014, NASA leased the management of Hangar One and Moffett airfield to Planetary Ventures, a subsidiary of Google, for 60 years. Restoration of the hangar by Google is expected to be complete in 2025.

    “We’re looking to be as efficient as possible, but it’s hard to say (when we’ll be done). All our schedules are subject to change,” Anthony LaMarca told the Moffett Field Restoration Advisory Board in 2017, a local newspaper reported. LaMarca is the project manager for Planetary Ventures. “By the time we get through all these steps, the skin will be done by 2025. That’s quite a ways out.”

    The hangars were included as part of the U.S. Naval Air Station, Sunnyvale Historic District, also known as the Shenandoah Plaza, when the district was listed on the National Register of Historic Places in 1994.

    In 2017, several Ames facilities were listed on the National Register of Historic Places. These include the Ames Administration building, the Aviation Systems Division’s flight simulation and guidance laboratory, the Arc Jet Complex, and the NASA Ames Wind Tunnel Historic District.

    The team developing the landing system for NASA's Mars Science Laboratory tested the deployment of an early parachute design in mid-October 2007 inside the world's largest wind tunnel, at NASA Ames Research Center.

    The team developing the landing system for NASA’s Mars Science Laboratory tested the deployment of an early parachute design in mid-October 2007 inside the world’s largest wind tunnel, at NASA Ames Research Center.

    Credit: NASA

    NASA Ames Research Center has grown over the past seven decades. Today, it has approximately 2,500 on-site employees and contractors spread across 500 acres.

    Ames emerged as the leading builder of flight simulators in the 1960s, with a wide range of simulators, equipment and facilities developed by the park to improve pilot workloads, cockpit design and safety. In particular, the Vertical Motion Simulator still enables testing of a variety of aircraft.

    Ames also has a life science program. The agency boasts various centrifuges, two of which are unique to the agency, as well as genome facilities. Future Flight Central remains a sophisticated facility for basic research on movement into and around airports.

    In the 1990s, Ames expanded its research to new realms. Nanotechnology laboratories aim to help reduce mass in space while increasing capability, while astrobiology facilities include a world-renowned astrochemistry laboratory to simulate deep space, a bio-mat greenhouse laboratory to study Earth’s earliest living organisms, and bio-signature labs.

    Ames is also investigating exoplanets. The center provides scientific and management leadership of NASA’s Kepler mission, which has discovered over 6,500 exoplanets and exoplanet candidates. The Ames Coronagraph Experiment (ACE) is a laboratory testbed for potential instruments to help NASA directly image exoplanets in the future.

    The agency lists eight core competencies on its website that it says helps it to contribute to virtually every NASA mission. They are:

    • Entry systems
    • Advanced computing & IT systems
    • Aerosciences
    • Air Traffic Management
    • Astrobiology and Life Sciences
    • Cost-Effective Space Missions
    • Intelligent/Adaptive Systems
    • Space and Earth Science

    Ames is active on several NASA missions. It serves as a partner for NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA), the world’s largest airborne astronomical observatory, as well as for the International Space Station and Mars Science Laboratory and the Curiosity rover currently operating on the Red Planet. It is also a partner on the New Horizons mission, which flew by Pluto in 2015 and is on its way to rendezvous with a distant Kuiper-belt object.

    While the massive research center itself is closed to the public, the nearby visitor center is open to all. With an exterior resembling a melting marshmallow, the visitor center has a self-guided walkthrough that discusses the research at Ames.

    Current exhibits include Science on a Sphere, Ames Spacecraft missions, a moon rock, a Mercury Redstone 1a capsule used in the last unmanned test flight before Mercury 7, a wind-tunnel model of SOFIA, a Kepler display, and a walk-through model of the International Space Center on Living and Working in Space. The center offers videos of varying lengths.

    While individuals and small groups are welcome to drop in, groups of ten or more require reservations.

    The centers hours are: 10 a.m. – 4 p.m., Tuesday – Friday; noon – 4 p.m., Saturday and Sunday. The visitor center is closed Mondays and federal holidays. To contact the visitor center, call (650) 604-6497.

    Additional resources

    Follow Nola Taylor Redd at @NolaTRedd, Facebook, or Google+. Follow us at @Spacedotcom, Facebook or Google+.

  • Whirlpool Galaxy: Exploding With Supernovas

    One of the first images taken by the Discovery Channel Telescope was of the Whirlpool Galaxy, M51. The image was obtained April-May 2012.

    The Whirlpool Galaxy is a spiral galaxy that is relatively close to Earth — about 30 million light-years away. It is visible in the northern constellation Canes Venatici, just southeast of the Big Dipper.

    More properly known as M51 or NGC 5194, the galaxy is noted as “one of the brightest and most picturesque” ones that Earthlings can see, according to NASA. The Space Telescope Science Institute (STScI) calls it one of “astronomy’s galactic darlings.”

    Among astrophysicists, one of the Whirlpool’s highlights is the abundance of supernovas (star explosions) that have been recorded there in recent years. It also is noted for its closeness to companion galaxy NGC 5195, which may be affecting the structure of the Whirlpool itself.

    M51 was first catalogued by Charles Messier in 1773 while the astronomer was plotting objects in the sky that could confuse comet-hunters. “M51” is a reference to “Messier 51,” one of about 110 entries now plotted in his Catalogue of Nebulas and Star Clusters. (The companion NGC 5195 was discovered in 1781 by Pierre Méchain, who the University of Manitoba describes as a close friend to Messier.)

    It would take about 70 years to learn more about the fuzzy object’s structure, however. It was first discerned by William Parsons, using a 72-inch reflector telescope in 1845. “His drawing of the spiral galaxy M51 is a classic work of mid-19th-century astronomy,” said Encyclopedia Britannica of Parsons’ observations.

    Parsons’ discovery was the first so-called “spiral nebula” ever discovered, and in the five years following he found 14 more of these objects, according to the STScI. It was unclear for decades if these objects were a part of the Milky Way Galaxy or things that were independent of that.

    It wasn’t until Edwin Hubble used Cepheid variable stars to chart cosmic distances in M31 (the Andromeda Galaxy) in the 1920s that astronomers understood they were actually distant galaxies.

    The Whirlpool galaxy (M51) before (left) and after (right) the eruption of supernova SN 2011dh in May 2011. The image on the left was taken in 2009, and on the right July 8th, 2011.

    The Whirlpool galaxy (M51) before (left) and after (right) the eruption of supernova SN 2011dh in May 2011. The image on the left was taken in 2009, and on the right July 8th, 2011.

    Credit: Conrad Jung

    There’s been a veritable cornucopia of supernovas in the Whirlpool in recent years. Skywatchers recorded supernovas in 1994, 2005 and 2011.

    “Three supernovas in 17 years is a lot for single galaxy, and reasons for the supernova surge in M51 are being debated,” noted the NASA website Astronomy Picture of the Day in 2011, without elaborating on the possible explanations.

    The latest supernova, called SN 2011dh, was at its brightest in June 2011 before slipping back into obscurity. After the event, astronomers scoured older pictures to see if they could find the source of the explosion. They narrowed their search to a yellow supergiant star (visible in Hubble Space Telescope pictures) that was there before the explosion, and appears to be missing afterwards.

    While most yellow supergiants aren’t expected to go supernova when they finish out their lives, the team said it’s possible that the star was actually a binary star. The other star would have been a bluer, hotter star that was close enough to pull some of the yellow supergiant’s mass away. Given enough time, this would have destabilized the star and caused the explosion, astronomers said.

    The blue star wasn’t spotted in Hubble photos, but astronomers added that it is likely best visible in ultraviolet light — a band of light that Hubble does not look at.

    “The present results reveal the necessity and importance of further studying the evolution and explosion of binary stars,” said Melina Bersten of the Kavli Institute for the Physics and Mathematics of the Universe in Japan, who led the team, in a statement. “I look forward to the observation that will confirm our prediction.”

    The Whirlpool’s arms are one of the more prominent observed in spiral galaxies, STScI noted. The group said this could be because of what they termed a “close encounter” with its companion galaxy, NGC 5195.

    “As NGC 5195 drifts by, its gravitational muscle pumps up waves within the Whirlpool’s pancake-shaped disk. The waves are like ripples in a pond generated when a rock is thrown in the water,” STScI stated.

    “When the waves pass through orbiting gas clouds within the disk, they squeeze the gaseous material along each arm’s inner edge. The dark dusty material looks like gathering storm clouds. These dense clouds collapse, creating a wake of star birth.”

    Over time, the biggest stars would then radiate away the surrounding gas, leaving behind blue star clusters that are easily visible in the Whirlpool’s arms, STScI added. More generally, the fact that the galaxy is so close by allows astronomers to look at its structure and way it forms stars, with the aim of extrapolating that understanding to other galaxies.

    In 2015, NASA released an image of the Whirlpool galaxy that the Chandra X-Ray Observatory captured over 250 hours of observation time. The space telescope observed 500 X-ray sources in the galaxy’s region, racking up about five times the number of sources observed in previous studies. At least 10 of these sources are believed to come from black holes.

    With the rise of inexpensive and powerful camera equipment, the Whirlpool is becoming a popular target for amateur astronomers. Space.com has examples of photos taken by amateurs in 2011 and 2015.

  • In Photos: NROL-47 Spy Satellite Launches Into Space on Delta IV Rocket

    On Jan. 12, 2018, the U.S. spy satellite NROL-47 launched into space atop a United Launch Alliance Delta IV rocket from Vandenberg Air Force Base in California. See video of the launch here! See photos from the stunning launch here. This Photo: The liftoff moment for NROL-47 as a secret mission is born.

  • Zoom Through the Famous Orion Nebula with NASA's Incredible 3D Video

    Take a tour of one of the most famous star-forming gas clouds in the night sky, the Orion Nebula, with a new, 3D visualization released by NASA. 

    In this short video, viewers slip through the colorful clouds, bright stars and detailed structures of the popular nebula. The visualization was created using real data from the Hubble and Spitzer space telescopes, combined with “Hollywood techniques,” according to a statement from the Space Telescope Science Institute (STScI), which co-produced the video. 

    The creators of the video said in the statement that they hope the visualization will give viewers a better idea of the 3D structure of the star-forming region. For example, the Trapezium star cluster in the heart of the nebula includes a bowl-shaped valley carved out by intense ultraviolet radiation and “winds” from new stars. The complete topology of that region isn’t visible in 2D images. [The Splendor of the Orion Nebula (Photos)]

    “Astronomers and visualizers worked together to make a three-dimensional model of the depths of this cavernous region, like plotting mountains and valleys on the ocean floor,” according to the statement. “Colorful Hubble and Spitzer images were then overlaid on the terrain.”

    The movie occasionally switches between images taken by the two separate telescopes. The Hubble space telescope captures light in the visible range seen by humans, as well as longer and shorter wavelengths in the ultraviolet and near-infrared ranges. The Spitzer space telescope captures light in the mid-infrared to far-infrared range, capturing objects and structures that are lower in temperature than what Hubble sees. But scientists can create visible representations of the data, revealing structures that would otherwise be invisible to humans.

     

    “Looking at the universe in infrared light gives striking context for the more familiar visible-light views,” Robert Hurt, a lead visualization scientist at the Infrared Processing and Analysis Center (IPAC) at the California Institute of Technology (Caltech), said in the statement. “This movie provides a uniquely immersive chance to see how new features appear as we shift to wavelengths of light normally invisible to our eyes.”

    The two telescopes provide 2D images of cosmic objects, so the creators had to rely on both “scientific knowledge and scientific intuition” to create the 3D tour. Summer and Hurt “worked with experts to analyze the structure inside the nebula,” using visible light to create the surfaces, and infrared light to construct much of the nebula’s structure. 

    “Being able to fly through the nebula’s tapestry in three dimensions gives people a much better sense of what the universe is really like,” Frank Summers, the STScI visualization scientist who led the team that developed the movie, said in the statement. 

    The visualization was created by scientists at STScI and Caltech/IPAC as part of NASA’s Universe of Learning program. The program uses a “direct connection” to NASA science and scientists, to create content that “[enables] youth, families, and lifelong learners to explore fundamental questions in science, experience how science is done, and discover the universe for themselves.”

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

  • What Does It Take to Be an Astrophysicist?

    An ultraviolet portrait of our galactic neighbor, Andromeda, taken with NASA’s Swift satellite.

    Paul Sutter is an astrophysicist at The Ohio State University and the chief scientist at COSI science center. Sutter is also host of Ask a Spaceman and Space Radio, and leads AstroTours around the world. Sutter contributed this article to Space.com’s Expert Voices: Op-Ed & Insights.

    Jumping into the world of astronomy and physics as a career can seem daunting, especially for precocious high schoolers with a passion for the field.

    It’s relatively easy to get interested in astronomy, especially as a kid — after all, what’s cooler than monster black holes, stars and planets galore, swirling nebulas and galaxies? And what can’t be accessed through online videos or books can be enjoyed through the simple and visceral pleasure of a clear, dark night. [Astronomy Gear Guide: Tools, Tips and Tricks to Stargaze Like a Boss]

    There are all sorts of awesome sights in the sky. What’s not to love? But as soon as curious youngsters dip their toes past the pretty pictures, they’re bound to find that the world of the professional astronomer is full of complicated theories, mountains of data to painstakingly analyze, and whiteboards full of tedious calculations.

    It turns out that nature does not reveal its secrets willingly or easily. It takes countless hours of work by armies of dedicated professionals to understand the deepest workings of our cosmos.

    So how does one make the jump? How do you go from a basic interest in the field to a full-fledged independent scientific research track? What are the skills you’ll need? If you’re considering a college degree in astronomy or physics, or know someone in your life who is, read on.

    The key message I try to convey about an astro-career is that it takes time. Lots of time. You’ll need four to six years just for a bachelor’s degree, which is true of many other professions. Then comes graduate school, which can take anywhere from five years for theorists up to seven or eight for experimentalists and observers. Then comes a postdoctoral research appointment, where your on-the-job training continues outside of your Ph.D. institution. In astronomy and physics, you typically have two or three of these two-to-five-year stints before you’re considered ready for a faculty job at a major research university.

    So by the time you’re middle-age, congrats: You now officially have a stable career in science!

    Part of the delay in going from pursuing a degree to getting a dedicated job is the general lack of funding in astronomy and physics, and I’ll talk about that more in another article. But another part is that it simply takes time to bring someone up to speed in academic research. You need your base knowledge, which is hundreds of years of accomplishments and accumulated wisdom compacted into a few short classes. Classical physics, statistical mechanics, relativity, electromagnetism and quantum mechanics form the backbone of a physics degree, with some more work on optics and common astrophysical processes added to extend to an astronomy degree. [The Weirdest Jobs In Science]

    Classes usually peter out once you’re a couple of years into graduate school. The remainder of your time is spent working on your dissertation research under the guidance of your adviser, and that’s where the real training comes in. That’s when you learn how to be an actual scientist, not just have science facts and methods shoved into your cranium day after day.

    It’s over the years of your thesis research that you learn how to prepare a poster or presentation at a conference without looking like an idiot, how to handle questions from competing researchers who are trying to poke holes in your work, how to take naps during conference calls, how to shove all the right introductory fluff and jargon into a paper, how to read a paper while looking for clues of what to work on next, how to ask intelligent-sounding and relevant questions during a seminar, how to beat the analysis software into submission, how to properly format a figure for publication, and on and on.

    During those years, you’re also brought up to speed on the true state of the art in the field, and you learn things that the classes, with curricula probably designed two decades ago, simply haven’t caught up on. You learn what people are working on right now, and where you can push to advance the current limits of human understanding.

    In these roles, your adviser is crucial. This person is not only your mentor but also your colleague and co-worker. Initially, they guide you and help shape your research directions, but very quickly, they’ll be learning from you about your latest discoveries and newest methods. That is why they hire you, after all — to train you at first, but with the aim of making you useful.

    While physics and astronomy require a healthy dose of mathematics (either in theoretical calculations or observational analysis), almost all of it is learned over the course of your graduate career. Even advanced undergraduate classes teach you only the basic outlines of the actual math you will employ throughout your career. 

    So if the math seems overwhelming, don’t fret. You’re never expected to jump into a full-time research gig fully equipped with all the mathematical tools at your disposal. They’re taught to you, fed to you, slowly and steadily, over the course of years. Techniques that seem like straight-up wizardry become, after sufficient practice, as second nature as blinking. Not up to speed with the latest computer programming techniques? That will come too, whether you like it or not.

    The truth is that you’re not expected to be an expert at the most difficult parts of being a scientist. That’s the entire point of the long, drawn-out training process. What you are expected to have is something far simpler: pure determination. It’s only through grit and sheer force of will that you’ll be able to handle the workload, the long hours, the blind alleys, the outright failures, the critiques and the wrestling with nature.

    If you have a healthy dose of perseverance and a lot of curiosity, you have what it takes to be a scientist.

    Learn more by listening to the episode “How does one become an astrophysicist?” on the Ask A Spaceman podcast, available on iTunes and on the Web at askaspaceman.com. Thanks to @92Rufino and Vicki K. for the questions that led to this piece! Ask your own question on Twitter using #AskASpaceman or by following Paul @PaulMattSutter and facebook.com/PaulMattSutter.

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

  • Previewing the Blue Blood Supermoon Eclipse of January 2018 Using Mobile Apps

    Mobile astronomy apps such as SkySafari 6 are an ideal tool to preview celestial events. The total lunar eclipse on the morning of Jan. 31, 2018 features an enlarged supermoon. It’s also a Blue Moon, the second full moon in January — a combination that hasn’t occurred in many years. In the eastern US and Canada, the moon will set mid-eclipse. But skywatchers in the west will be able to watch the entire eclipse, as shown here near the end of the eclipse at 6:15 a.m. PST in San Francisco, CA. By telling you where in the sky it will occur, your astronomy app can help you plan to observe or photograph any eclipse.

    In 2018, the world will experience three partial solar eclipses and two total lunar eclipses — but whether you can see them depends on where you live. The first event is a total lunar eclipse that happens on the morning of Jan. 31. This eclipse will be special! The moon will be both “super” and “blue,” and if skies are clear, skywatchers in North America will be able to see all or part of the eclipse.

    In this edition of Mobile Astronomy, we’ll highlight the rare “Blue Blood Supermoon” total lunar eclipse and tell you how to use your favorite astronomy app to preview it. We’ll also help you use your app to explore how lunar eclipses work. [Super Blue Blood Moon 2018: When, Where and How to See It]

    On Jan. 31, 2018, skywatchers across much of the world will receive a postholiday gift: the total lunar eclipse of a full supermoon that is also a Blue Moon! Unlike last summer’s Great American Total Solar Eclipse, lunar eclipses are completely safe to look at because the sun is below the horizon. Any sunlight that reaches the eclipsed moon has to pass over the Earth’s horizon, panting the moon with reddish light — hence the nickname “blood moon” for eclipsed moons. 

    Due to the moon's elliptical orbit, its distance from Earth varies by about 12 percent, bringing it closer (perigee) and farther (apogee) during every 27.3 day circuit of Earth. The moon runs through its phases on a separate cycle of 29.5 days. From time to time, the two cycles synchronize for a few months, allowing the moon to be full while near perigee, causing it to be up to 30 percent brighter and 7 percent larger than average. The three full moons in December 2017 and January 2018 are all supermoons.

    Due to the moon’s elliptical orbit, its distance from Earth varies by about 12 percent, bringing it closer (perigee) and farther (apogee) during every 27.3 day circuit of Earth. The moon runs through its phases on a separate cycle of 29.5 days. From time to time, the two cycles synchronize for a few months, allowing the moon to be full while near perigee, causing it to be up to 30 percent brighter and 7 percent larger than average. The three full moons in December 2017 and January 2018 are all supermoons.

    Credit: NASA/JPL-Caltech

    This total lunar eclipse occurs only 1.2 days after perigee (the moon’s closest approach to Earth), so the moon’s diameter will appear about 7 percent larger than average, making it a “supermoon.” The full moon will also be a Blue Moon — the second full moon to occur within the calendar month. Eclipsed supermoons aren’t all that rare, but the total eclipse of a Blue Moon hasn’t occurred since March 31, 1866. That’s 152 years! Don’t let the nickname mislead you, though — the moon won’t look blue at all.

    The entire eclipse will be visible from northwestern North America, across the Pacific Ocean, and as far as eastern Siberia and Asia. Most of North America will see a portion of the eclipse before the moon sets and morning twilight arrives, while Eastern Europe and Central Asia will see the eclipse already in progress when the moon rises. During totality, when the moon is fully in shadow, the moon’s northern limb will pass just south of the center of the Earth’s shadow, darkening the moon’s northern half more than its southern half. 

    To find out whether the eclipse will be visible where you live and to preview what it will look like, use an astronomy app such as SkySafari 6, Star Walk 2 or Stellarium Mobile.. Open the app, and then search for and center the moon — don’t worry if it’s below the horizon for now. Next, set the app’s date to Jan. 31, 2018, and the app’s time to about 1 a.m. in your local time zone. For locations in North America, the app will show the moon high in the night sky. Zoom in on the display until the moon shows as a good-sized disk. 

    The free Solar System Scope app features a 3D model of the solar system that you can manipulate to better understand the motions of the moon and planets. You can select a specific date and time, or allow time to flow forwards and watch things move. Here, the Jan. 31, 2018 total lunar eclipse is modeled. The software is available in both browser and mobile versions, and includes a sky chart mode for night-time skywatchers.

    The free Solar System Scope app features a 3D model of the solar system that you can manipulate to better understand the motions of the moon and planets. You can select a specific date and time, or allow time to flow forwards and watch things move. Here, the Jan. 31, 2018 total lunar eclipse is modeled. The software is available in both browser and mobile versions, and includes a sky chart mode for night-time skywatchers.

    Credit: Solar System Scope

    By running time forward, or by stepping hour by hour, you can watch the moon become eclipsed and then lighten again as it leaves the Earth’s shadow. The moon’s edge will start to darken at 6:48 a.m. EST (1148 GMT). Maximum eclipse occurs at 8:30 a.m. EST (1330 GMT), and the eclipse ends at 10:11 a.m. EST (1511 GMT). For skywatchers in the eastern United States, the moon will set before maximum eclipse, but you can see the entire eclipse by removing the horizon and turning off daylight using the app’s settings.

    If you plan to view the actual eclipse, or photograph it, use your app to note the direction and how high above the horizon the moon will be during the event. That way, you can scout out a viewing spot where the moon will be visible throughout the eclipse duration.

    Understanding how lunar eclipses work is easy if your app allows you to display the invisible circles representing the full and partial shadows that Earth casts into space. In the SkySafari 6 app, the setting is located under Settings > Solar System > Orbits, Paths & Shadows. Enable the Earth & Moon Shadow Circles, and exit Settings. The smallest circle is the zone, or umbra, where the sun is completely blocked by the Earth. The larger circle is the penumbra, the region where some of the sun is still shining on objects passing through it. 

    Sunlight shining on the solid globe of Earth casts a circular shadow, or umbra, into space. The shadow is always opposite the sun and near the ecliptic (yellow line), which defines the plane of Earth's orbit around the sun. The moon's orbit (gray line) is tilted 5 degrees away from the ecliptic. Whenever full moons occur close to the point in space where the moon's orbit and ecliptic intersect, a lunar eclipse can occur. While the moon is passing through the smaller white circle, only sunlight that has been reddened as it refracts over the Earth's horizon reaches it — painting it a blood red color. The larger circle, or penumbra, represents the region where some direct sunlight still reaches the moon.

    Sunlight shining on the solid globe of Earth casts a circular shadow, or umbra, into space. The shadow is always opposite the sun and near the ecliptic (yellow line), which defines the plane of Earth’s orbit around the sun. The moon’s orbit (gray line) is tilted 5 degrees away from the ecliptic. Whenever full moons occur close to the point in space where the moon’s orbit and ecliptic intersect, a lunar eclipse can occur. While the moon is passing through the smaller white circle, only sunlight that has been reddened as it refracts over the Earth’s horizon reaches it — painting it a blood red color. The larger circle, or penumbra, represents the region where some direct sunlight still reaches the moon.

    Credit: SkySafari App

    Even though the moon is relatively small compared with the size of Earth’s shadow, the moon usually misses it. That shadow always lies near the ecliptic, which defines the plane of Earth’s orbit around the sun. The moon’s orbit is tilted about 5 degrees from the ecliptic. Lunar eclipses can occur only if the moon is full while it is near the point in space where the moon’s orbit crosses the ecliptic.

    If you flow time forward, you can watch how, during this lunar eclipse, the moon’s orbit carries it eastward through the penumbra and umbra, and out the opposite side. During partial lunar eclipses, the moon never fully enters the umbra. [How to Photograph a Total Lunar Eclipse (A Moon Photo Guide)]

    A second total lunar eclipse occurs on July 27. This one is only 0.6 days after apogee (the moon’s farthest distance from Earth), so the moon’s apparent diameter will be near its minimum. The moon will cross just north of the center of Earth’s umbral shadow, setting up conditions for a very dark eclipsed moon. At greatest eclipse, the moon will be among the stars of Capricorn, sitting 6 degrees north of Mars, which will be close to maximum brightness. The eclipsed moon will also be positioned within 10 degrees of three deep sky objects, Messiers 75, 72, and 73. They should be visible in binoculars during maximum eclipse.

    Using Astronomy apps to preview lunar eclipses allow you to discover additional interesting aspects of the events. The total lunar eclipse of July 27, 2018 coincides with the opposition of Mars. The blood moon and the very bright Red Planet will make a wonderful sight and photo opportunity for observers where the eclipse is visible. When fully immersed in the Earth's shadow, the darkened full moon will also allow fainter deep sky objects to appear, such as the nearby Messier objects shown here. For skywatchers in Madagascar, the maximum eclipsed moon will be high in the sky, close to the Zenith (green cross).

    Using Astronomy apps to preview lunar eclipses allow you to discover additional interesting aspects of the events. The total lunar eclipse of July 27, 2018 coincides with the opposition of Mars. The blood moon and the very bright Red Planet will make a wonderful sight and photo opportunity for observers where the eclipse is visible. When fully immersed in the Earth’s shadow, the darkened full moon will also allow fainter deep sky objects to appear, such as the nearby Messier objects shown here. For skywatchers in Madagascar, the maximum eclipsed moon will be high in the sky, close to the Zenith (green cross).

    Credit: SkySafari App

    If you’re observing from North America, you will not see any of this eclipse, but you can preview it on your app anytime and then watch the event livestreamed over the internet. The entire eclipse will be visible from Africa, the Middle East, India and western Australia. Observers in eastern Australia and Southeast Asia will see a portion of the eclipse before the moon sets and morning twilight arrives, while for Europe and eastern South America, the eclipse will be already in progress when the moon rises. The partial eclipse begins at 1824 GMT, the greatest eclipse is at 2022 GMT and the partial eclipse ends at 2219 GMT. To use your app, either hide the ground and turn off daylight, or change your app’s location settings to somewhere the eclipse is visible. It’s fun! 

    You can safely preview solar eclipses with mobile apps, too. This year’s two partial solar eclipses occur on Feb. 15, July 13, and August 11. The first two are best visible from Antarctica, and the third one peaks over the North Pole, so using your app will be much less trouble!

    In future editions of Mobile Astronomy, we’ll preview more 2018 highlights, including opportunities to see Mercury, the dance of Jupiter’s moons and some possible naked-eye comets at year’s end. We’ll also cover how to measure stars’ distances, and some whimsical asterisms — star groupings that are not constellations. Until then, keep looking up!

    Editor’s note: Chris Vaughan is an astronomy public outreach and education specialist at AstroGeo, a member of the Royal Astronomical Society of Canada, and an operator of the historic 74″ (1.88-meter) David Dunlap Observatory telescope. You can reach him via email, and follow him on Twitter @astrogeoguy, as well as on Facebook and Tumblr.

    This article was provided by Simulation Curriculum, the leader in space science curriculum solutions and the makers of the SkySafari app for Android and iOS. Follow SkySafari on Twitter @SkySafariAstro. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.

  • Puerto Rico Blackout Looked Striking from Space, Astronaut Tells Students in Q&A

    Astronaut Joe Acaba says it was very difficult to see the island of Puerto Rico from space after Hurricane Maria swept through the region on Sept. 20.

    In comments during a space-to-ground question-and-answer session with hundreds of Puerto Rican students today (Jan. 12), Acaba said the Caribbean island is usually easy to spot because of its lights. That changed quickly after the hurricane came through as a Category 4 storm, devastating the island’s infrastructure. Acaba is the first astronaut of Puerto Rican heritage — both of his parents were born there, although he is from California. 

    “The first thing I noticed was the lack of electricity,” Acaba said in both Spanish and English. Continuing in English, he said, “Usually when you fly over Puerto Rico at night, you can identify the island, and it was almost impossible to see it at night.” [In Photos: Hurricane Maria Seen from Space]

    In Spanish, Acaba added that his thoughts are with Puerto Rico, and he understands that it was difficult after the hurricane swept through — and that life remains difficult today. “I’m thinking about you,” he said in Spanish.

    Another student asked Acaba if it was difficult to adjust to a limited menu in space, adding that many Puerto Ricans needed to eat a limited menu themselves after the hurricane.

    “It’s a pretty good menu. It repeats itself every seven to 14 days. The food is pretty good, but it does get a little monotonous,” Acaba responded in English. He added that he can’t wait to get home and have a “great meal.”

    Puerto Rico continues to recover from the storm. As of yesterday (Jan. 11) — nearly four months after Maria hit — approximately 40 percent of the island’s public utility customers still do not have electricity, according to NPR and status.pr, a website that tracks how infrastructure repairs are progressing in Puerto Rico.

    Acaba spoke with more than 500 students in Manatí, which is 40 minutes west of San Juan, the capital. The students represent 30 school districts in 12 cities, and participated as part of the Puerto Rico Institute of Robotics’ (PRIOR) network. 

    The students asked many questions, ranging from daily life on the space station, to Acaba’s background and work in space. When asked about how his training as an educator helps with astronaut work, Acaba said communication is key in both professions. He added in Spanish that being a teacher is one of the “most difficult and most important professions in the world.”

    Another student asked how Acaba felt during a spacewalk in October, compared to his past missions — specifically, whether Acaba felt more comfortable or more anxious. Acaba responded in Spanish that while he felt comfortable, he still maintained focus to avoid any problems. 

    Other insights Acaba shared with students included the challenges of fixing the space toilet (one of the station’s toilets just broke again, he said), and the ease of flowing between different nations’ modules on the International Space Station without using a passport.

    The event started a few minutes late due to an audio issue on the Puerto Rican side of the communications link, according to NASA. Acaba passed some of the time by doing a lazy somersault and jumping to an adjacent wall in the Japanese Kibo laboratory, where he held the conversation with students.

    Acaba arrived at the space station on Sept. 12, about a week before Maria battered Puerto Rico. Later in September, Acaba sent a tweet expressing support and prayers for everyone affected by the storm

    “From @Space_Station, thinking and praying for all families and friends in Puerto Rico,” Acaba wrote on Sept. 24. Acaba’s tweet was accompanied by a photo of himself with a Puerto Rican baseball shirt and holding the Puerto Rican flag; behind him were the windows of the space station’s Cupola observatory.

    Acaba was selected as an astronaut in 2004 This is his third space voyage. On his first trip — space shuttle mission STS-119, in 2009 — Acaba brought a Puerto Rican flag with him and asked that one of the wake-up songs be the Puerto Rican folklore song “Qué Bonita Bandera,” which translates to “What a Beautiful Flag.”

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

  • US Launches New Spy Satellite on Secret Mission

    The fleet of U.S. spy satellites has just welcomed a new member.

    The NROL-47 spacecraft soared into Earth orbit today (Jan. 12), riding atop a United Launch Alliance (ULA) Delta IV Medium rocket that lifted off from California’s Vandenberg Air Force Base at 5:11 p.m. EST (2211 GMT, 2:11 p.m. local California time).

    NROL-47 will be operated by the National Reconnaissance Office (NRO), which builds and manages the United States’ spy satellites. NRO missions tend to be hush-hush, and NROL-47 is no exception; no details have been released about the satellite’s planned activities. [The Secret NROL-47 Spy Satellite Launch in Photos]

    A United Launch Alliance Delta IV rocket carrying the classified NROL-47 spy satellite launches from Space Launch Complex-6 at Vandenberg Air Force Base in California on Jan. 12, 2018.

    A United Launch Alliance Delta IV rocket carrying the classified NROL-47 spy satellite launches from Space Launch Complex-6 at Vandenberg Air Force Base in California on Jan. 12, 2018.

    Credit: United Launch Alliance/Jeff Spotts

    However, we can make a few inferences. Today’s launch employed the “5,2” variant of the Delta IV — meaning the rocket featured a 5-meter-wide (16.5 feet) payload fairing and two solid rocket boosters strapped to the core stage.

    “That version of the Delta IV has flown only twice before, and analysts who track space activities believe both launches — in 2012 and 2016 — hauled so-called Topaz radar reconnaissance satellites into orbit,” Spaceflight Now’s Stephen Clark wrote in late December.

    The Delta IV carrying NROL-47 rises into the California sky on Jan. 12, 2018.

    The Delta IV carrying NROL-47 rises into the California sky on Jan. 12, 2018.

    Credit: ULA

    Today’s launch was the first of the year for ULA, which is a partnership between aerospace giants Boeing and Lockheed Martin. ULA has now launched 27 satellites for the NRO, including three last year, all of which lifted off atop Atlas V rockets.

    The two-stage, 217-foot-tall (66 m) Delta IV now has a total of 36 space missions under its belt, ULA representatives said. The rocket has been flying since 2002, when it was solely a Boeing vehicle. (ULA formed in December 2006.)

    This afternoon’s liftoff was delayed two days, first by strong winds and then by an issue with a ground-system valve. NROL-47 ended up taking to the skies five days after another national-security launch, that of the mysterious Zuma payload by a SpaceX Falcon 9 rocket. The Zuma mission appears to be a failure, though what exactly happened is unclear at the moment. SpaceX representatives have said the Falcon 9’s performance met expectations; speculation is currently centering on a possible problem with the satellite’s separation from the rocket’s upper stage.

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

  • Winter Skywatching: See Taurus, the Angry Bull

    Taurus is the first of the bright winter constellations to rise, carried high in the southern sky by late evening every December. The bull is tilted over as if charging nearby Gemini and Orion. His triangular face features the bright-orange star Aldebaran and many easy-to-observe double stars.

    Manuel Laureano Rodríguez Sánchez (1917-1947), better known as Manolete, is considered by some to be the greatest bullfighter of all time. Of course, Manolete faced down his bovine opponents in a bullfighting ring with a large crowd looking on. It is a bit of a different scenario in our current night sky, where we can see another form of bullfight, this one between a charging bull and a mighty hunter.  

    Our Manolete of the sky is none other than Orion, the most prominent constellation. And he is certainly doing battle with a “bullish” competitor: Taurus, the Bull. 

    In a modern bullfight, the matador uses a special lance (a pica) and banderillas (little flags), as well as his emblematic cape. But Orion is equipped with a club, a sword and a lion’s skin for a shield. [Constellations of the Night Sky: Famous Star Patterns Explained (Images)]

    Taurus appears to be descended from a mythical heavenly Sumerian bull, an animal that used its great horns to open up the year and usher in spring, to plough the long furrow of the sky that was the zodiac. 

    This association with springtime came about because the stars of Taurus became prominent in the sky around the vernal (spring) equinox from about 4500 B.C. to 2000 B.C. During this time, the equinox was the most important date in the year. For the Sumerians, it was a time of rejoicing, their equivalent of New Year’s Day, when the dark and cold winter season was ending and there was a feeling of new life in the air. Thus, for a long time, Taurus was the first and most powerful of the zodiacal constellations

    This week, the constellation Taurus is positioned at its highest point in the south and nearly overhead at around 9 p.m. local time. When I give shows under the sky of the “pretend universe” of a planetarium or conduct star-identification sessions under the real sky, I always identify Taurus as an angry bull.  

    But why is he so angry?

    Last month, I wrote a column about how, at this time of year, stargazers seem to concentrate solely on Orion, while all the other constellations surrounding him are seemingly nothing more than celestial second-stringers or part of a supporting cast. 

    I used the analogy of a house spangled with Christmas lights while nearby homes are more modestly decorated. 

    Perhaps Taurus is angry because he feels he shouldn’t be considered a mere second banana to Orion (and consequently wants to take his frustration out on the hunter). Indeed, that anger at second billing is justified; our Heavenly Bull contains a wealth of interesting objects to see, and among all the star patterns, should certainly be categorized as first-rate.

    Hubble Space Telescope image of bright and beautiful cosmic clumps in the constellation Taurus, the Bull.

    Hubble Space Telescope image of bright and beautiful cosmic clumps in the constellation Taurus, the Bull.

    Credit: ESA/Hubble and NASA

    Probably the most noteworthy feature of Taurus is a small, concentrated group of stars called the Pleiades, or Seven Sisters. Few star figures are as familiar as the Pleiades. If you have difficulty in recognizing various stars and constellations, you should start with the Pleiades, because there is really nothing else like them in the sky, and nobody can look at the sky on a frosty winter night very long without noticing these sisters and wondering what they are. 

    To the average eye, this group looks at first like a little, luminous cloud. But further examination, aided by good eyesight, will reveal a tight cluster of six or seven stars, though some observers have recorded a dozen or more stars under excellent conditions. I know one gentleman blessed with such acute vision that he has claimed to see as many as 19 Pleiades stars from under exceptionally dark skies in Arizona. 

    The Pleiades grouping might be one of the first astronomical subjects recorded. It was known to the Greek poet Hesiod nearly 3,000 years ago, and a reference to it has been found in Chinese annals dated to around 2357 B.C. It is also mentioned three times in the Bible.  

    So apparent is the group that almost all cultures concerned with the sky have told tales of these stars’ significance. For cultures of Central and South America, an important time of year began when the Pleiades appeared at their highest point at midnight. The ancient Greek astronomer Hipparchus dated the starts of seasons according to certain risings and settings of this group. 

    Several stars in the cluster seem to be enveloped in clouds of dust, perhaps left over from the stuff from which they formed. At 410 light-years away from us, and some 20 light-years across, the group may be no older than 20 million years. It contains a total of perhaps 250 stars.  

    And just subjectively, I believe the Pleiades are worth the cost of any good pair of binoculars. In fact, they just might be the most beautiful binocular object you can view in the sky. [The Best Binoculars for Earth and Sky]

    The Bull’s face is plainly marked by yet another cluster of stars in the shape of a V, known as the Hyades. Notice the bright orange star at the end of the lower arm of the V, which represents the Bull’s fiery eye. That’s Aldebaran, “the follower”; it rises soon after the Pleiades and pursues them across the sky.  

    The Hyades are among the nearest of the star clusters, which explains why so many of the separate stars in that grouping are visible. At a distance of 130 light-years, the Hyades are moving in the general direction of the star Betelgeuse in Orion while receding from us at the rate of 100,000 mph (160,000 km/h). 

    Aldebaran, on the other hand, is just an innocent bystander — not part of the Hyades at all. Instead, it is moving toward the south, almost at a right angle to the cluster’s motion, and twice as fast. Taurus’s V-shaped head is, therefore, going to pieces. For another 25,000 years or more it will pass for a V, but after 50,000 years, it will be nothing more than a random jumble of stars. 

    A composite view of the famous Crab Nebula, from the Herschel Space Observatory and the Hubble Space Telescope.

    A composite view of the famous Crab Nebula, from the Herschel Space Observatory and the Hubble Space Telescope.

    Credit: ESA/Herschel/PACS/MESS Key Programme Supernova Remnant Team; NASA, ESA and Allison Loll/Jeff Hester (Arizona State University)

    Back in the year A.D. 1054, an explosion of mammoth proportions took place: a supernova. A star at least 10 times more massive than our own sun suddenly blew apart; the bursting star likely blazed as brilliantly as our entire galaxy, the equivalent of 400 billion normal stars!  

    In the aftermath, nothing remained, except the intensely hot, newly revealed core of the star and an expanding cloud of gaseous debris. Fortunately, inhabitants of China, Japan and what is now the American Southwest were careful to note the position in the sky of this cosmic outburst: about two breadths of a full moon northwest of the star we know as Zeta Tauri, which marks the southern horn of Taurus.  

    The “guest star” that suddenly appeared there could easily be seen in daylight for more than three weeks. It finally faded completely from view after 653 days. The gas cloud that remained from the explosion is popularly known as the Crab Nebula and is still expanding outward in all directions at nearly 4 million mph (6.4 million km/h). [Photos: Amazing Views of the Famous Crab Nebula]

    In November 1968, the core of the exploded star was discovered to be a pulsar, a rapidly rotating neutron star, which was spinning at an incredible rate of some 30 times per second! Apparently, there is a “hotspot” on the star’s surface, which emits energy in virtually every part of the electromagnetic spectrum. Hence, as the star whirls on its axis, it appears to “pulse” from our earthly perspective.  

    This pulsar is extremely dense, packing about the mass of our sun into a volume measuring just 30 miles (50 kilometers) or so in diameter. Were it somehow possible to transport just a teaspoon of this material to Earth, it would weigh many hundreds of tons! 

    It was the Crab Nebula’s resemblance to a telescopic comet that prompted astronomer Charles Messier to compile his celebrated catalogue of such fuzzy objects so that they might not deceive other comet hunters. The Crab Nebula is first on his list and is therefore known as M1. 

    Taurus is one of the 12 zodiacal constellations. This means that, periodically, the moon and one or more of the bright planets pass through this part of the sky, adding to the interest and luster of this beautiful, starry backdrop. 

    For instance, during the final days of April, the brilliant planet Venus will pass near the Pleiades, making an already-beautiful scene even more spectacular.

    An “admirabull” sight, to say the least!

    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 Verizon Fios1 News, based in Rye Brook, N.Y. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.