Nebula Images: http://nebulaimages.com/
Astronomy articles: http://astronomyisawesome.com/
This video is a compilation of ultra-high definition time-lapses of the aurora shot from the space station. Auroras are a space weather phenomenon that occur when electrically-charged electrons and protons collide with neutral atoms in the upper atmosphere. The dancing lights of the aurora provide a spectacular show for those on the ground, but also capture the imaginations of scientists who study the aurora and the complex processes that create them.
Get a behind-the-scenes look at how test dummies at NASA's Langley Research Center contribute to making the planes we fly on safer and developing space exploration vehicles. Work ranges from next-generation aircraft to water-impact tests that evaluate the splashdown of Orion astronaut crew capsules returning from space.
Credit: NASA/Videographer: Gary Banziger; Writer and Co-Producer: Lily Daniels; Editor and Co-Producer: Kevin Anderson
Born February 9, 1960, Peggy A. Whitson (Ph.D.) flew on Expedition 50/51 and participated in four spacewalks, bringing her career total to ten. With a total of 665 days in space, Whitson holds the U.S. record, placing eighth on the all-time space endurance list. The Iowa native also completed two six-month tours of duty aboard the station for Expedition 5 in 2002, and as the station commander for Expedition 16 in 2008 where she accumulated 377 days in space between the two missions, the most for any U.S. woman at the time of her return to Earth.
Education: Graduated from Mt. Ayr Community High School, Mt. Ayr, Iowa, in 1978; received a Bachelor of Science in Biology/Chemistry from Iowa Wesleyan College in 1981 and a Doctorate in Biochemistry from Rice University in 1985.
Experience: From 1981 to 1985, Dr. Whitson conducted her graduate work in Biochemistry at Rice University, Houston, Texas, as a Robert A. Welch Predoctoral Fellow. Following completion of her graduate work, she continued at Rice University as a Robert A. Welch Postdoctoral Fellow until October 1986. Following this position, she began her studies at NASA Johnson Space Center (JSC), Houston, Texas, as a National Research Council Resident Research Associate. From April 1988 until September 1989, Whitson served as the Supervisor for the Biochemistry Research Group at KRUG International, a medical sciences contractor at NASA-JSC. From 1991 to 1997, Whitson was invited to be an Adjunct Assistant Professor in the Department of Internal Medicine and Department of Human Biological Chemistry and Genetics at University of Texas Medical Branch, Galveston, Texas. In 1997, Whitson began a position as Adjunct Assistant Professor at Rice University in the Maybee Laboratory for Biochemical and Genetic Engineering.
NASA Experience: From 1989 to 1993, Dr. Whitson worked as a Research Biochemist in the Biomedical Operations and Research Branch at NASA’s Johnson Space Center. From 1991 to 1993, she served as Technical Monitor of the Biochemistry Research Laboratories in the Biomedical Operations and Research Branch. From 1991 to 1992, she was the Payload Element Developer for the Bone Cell Research Experiment (E10) aboard SL-J (STS-47) and was a member of the U.S.-USSR Joint Working Group in Space Medicine and Biology. In 1992, she was named the Project Scientist of the Shuttle-Mir Program (STS-60, STS‑63, STS-71, Mir 18, Mir 19) and served in this capacity until the conclusion of the Phase 1A Program in 1995. From 1993 to 1996, Whitson held the additional responsibilities of the Deputy Division Chief of the Medical Sciences Division at Johnson Space Center. From 1995 to 1996, she served as Co-Chair of the U.S.-Russian Mission Science Working Group. In April 1996, she was selected as an Astronaut Candidate and started training in August 1996. Upon completing two years of training and evaluation, she was assigned technical duties in the Astronaut Office Operations Planning Branch and served as the lead for the Crew Test Support Team in Russia from 1998 to 1999. From November 2003 to March 2005, she served as Deputy Chief of the Astronaut Office. Also in 2003, she served as commander of the fifth NASA Extreme Environment Mission Operations (NEEMO) mission.
From March 2005 to November 2005, she served as Chief of the Station Operations Branch, Astronaut Office. Whitson trained as the backup ISS commander for Expedition 14 from November 2005 to September 2006. Whitson also was a member of the 2004 Astronaut Selection Board and chaired the Astronaut Selection Board in 2009.
Whitson completed two six-month tours of duty aboard the International Space Station, the second as the station commander for Expedition 16 in April 2008. This was Whitson’s second long-duration spaceflight. She has accumulated 377 days in space between the two missions, the most for any woman. Whitson has also performed a total of six career spacewalks, adding up to 39 hours and 46 minutes.
From October 2009 to July 2012, Whitson served as Chief of the Astronaut Corps and was responsible for the mission preparation activities and on-orbit support of all International Space Station crews and their support personnel. She was also responsible for organizing the crew interface support for future heavy launch and commercially-provided transport vehicles. Whitson was the first female, nonmilitary Chief of the Astronaut Office.
Spaceflight Experience: Expedition 5 (June 5 through December 7, 2002). The Expedition 5 crew launched on June 5, 2002, aboard STS-111 and docked with the International Space Station on June 7, 2002. During her six-month stay aboard the space station, Dr. Whitson installed the Mobile Base System, the S1 truss segment and the P1 truss segment, using the Space Station Remote Manipulator System; performed a four hour and 25-minute Orlan spacewalk to install micrometeoroid shielding on the Zvezda Service Module and activated and checked out the Microgravity Sciences Glovebox, a facility class payload rack. She was named the first NASA Science Officer during her stay, and she conducted 21 investigations in human life sciences and microgravity sciences as well as commercial payloads. The Expedition 5 crew (one American astronaut and two Russian cosmonauts) returned to Earth aboard STS-113 on December 7, 2002. Completing her first flight, Dr. Whitson logged 184 days, 22 hours and 14 minutes in space.
Expedition 16 (October 10 through April 19, 2008). The Expedition 16 crew of Whitson and Cosmonaut Yuri Malenchenko launched on October 10, 2007, aboard a Soyuz TMA-11 spacecraft and docked with the International Space Station on October 12, 2007. The third crew member position for this expedition was filled by astronauts rotating in and out via shuttle flights and included Clay Anderson, Dan Tani, Leo Eyharts and Garrett Reisman. As commander, Whitson oversaw the first expansion of the station’s living and working space in more than six years. The station and visiting space shuttle crews added the Harmony connecting node, the European Space Agency’s Columbus laboratory, the Japan Aerospace Exploration Agency’s Kibo logistics pressurized module and the Canadian Space Agency’s Dextre robot. Whitson performed five spacewalks to conduct assembly and maintenance tasks outside the complex. She and Malenchenko undocked from the station and returned to Earth on April 19, 2008, aboard the Soyuz TMA-11 spacecraft. Whitson logged 192 days in space.
Whitson launched on November 17, 2016, as part of Expedition 50/51 and returned safely on Earth on September 3, 2017. She contributed to hundreds of experiments in biology, biotechnology, physical science and Earth science, welcomed several cargo spacecraft delivering tons of supplies and research experiments, and conducted a combined six spacewalks to perform maintenance and upgrades to the station. Whitson participated in four spacewalks, bringing her career total to ten. With a total of 665 days in space, Whitson holds the U.S. record, placing eighth on the all-time space endurance list.
Awards/Honors: Inducted into Iowa Aviation Hall of Fame (2011); BioHouston Women in Science Award (2011); Houston’s 50 Most Influential Women of 2011; Russian Medal of Merit for Space (2011); Texas Women on the Move award recipient (2010); Distinguished Alumni Award, Rice University (2010); NASA Space Flight Medal (2002, 2008); First Lady of Iowa Award presented by the Iowa High School Girls’ Athletic Union (2010); Iowa Transportation Museum, Hero of Valor (2009); Lion’s Club Mount Ayr Elementary Science Lab dedication, Peggy Whitson Science Center (2008); NASA Outstanding Leadership Medal (2006); Distinguished Alumni Award, Iowa Wesleyan College (2002); two patents approved (1997, 1998); Group Achievement Award for Shuttle-Mir Program (1996); American Astronautical Society Randolph Lovelace II Award (1995); NASA Tech Brief Award (1995); NASA Space Act Board Award (1995, 1998); NASA Silver Snoopy Award (1995); NASA Exceptional Service Medal (1995, 2003, 2006, 2008); NASA Space Act Award for Patent Application; NASA Certificate of Commendation (1994); Selected for Space Station Redesign Team (March to June 1993); NASA Sustained Superior Performance Award (1990); Krug International Merit Award (1989); NASA JSC National Research Council Resident Research Associate (1986 to 1988); Summa Cum Laude from Iowa Wesleyan College (1981); President’s Honor Roll (1978 to 1981); Orange van Calhoun Scholarship (1980); State of Iowa Scholar (1979); Academic Excellence Award (1978).
Image Credits: NASA
Voyager 2 Photograph of Jupiter
A photo of Jupiter. Took by Voyager with VGISS on July 02, 1979 at 06:01:35. Detail page on OPUS database.
Skywatchers in the western hemisphere will see a rare sight on Monday: over the course of several hours, the silhouette of the planet Mercury will appear to cross the face of the Sun. The “transit” of Mercury results from the precise alignment of the orbits of Mercury and Earth that only happens either 13 or 14 times per century; usually the orbital alignment is weak, and as seen from our planet Mercury “misses” the Sun’s disk as it orbits once every 88 days. But on Monday, the view through a properly-shielded telescope will reveal the innermost planet as a dark, perfectly circular spot that moves completely across the Sun in exactly seven and a half hours.
Because of the specifics of our respective orbits, Mercury transits only happen in either the months of May or November, with average dates of 8th May and 10th November. May transits happen less frequently than November transits because during May, Mercury is closer to its largest distance from the Sun, while in November the opposite is true. As a result, the range of possible angles between the Sun and Mercury, as seen from Earth, is smaller in November than May. While the interval between successive November transits can be either 7, 13 or 33 years, May transits are less common, with successive appearances in either 13- or 33-year intervals.
Observations of Mercury transits reach back to at least the seventeenth century. Observations from earlier than this are unlikely because the apparent size of Mercury’s silhouette against the Sun is too small for the unaided eye to resolve. This is why the first recorded Mercury transit — by the French astronomer Pierre Gassendi on 7 November 1631 — dates to after Galileo Galilei’s invention of the telescope in about 1609. Johannes Kepler earlier understood that Mercury’s orbit should periodically take it in front of the Sun, but he died in 1630 before being able to observe a predicted transit.
While these events once had great scientific interest, they are now mainly curiosities that delight astronomy aficionados. Rarer still are transits of Venus across the Sun, the last of which took place in 2012. These events come in pairs separated by 113 years, meaning that most people alive now will not be around to see the next one in December 2117.
Who can see Monday’s event? That depends on the hour of day and which side of the Earth faces the Sun at the time. The map below indicates which parts of the world see either all, some, or none of the transit:
You’ll need at least a good pair of binoculars or a telescope — properly shielded with a heavy filer to prevent eye damage — to even sense Mercury during the transit. It will look like a small, perfectly round and completely opaque black dot against the bright solar photosphere. Mercury is distinguishable in this sense from sunspots, which are irregular in shape, can be partially transparent, and of much larger sizes. This image compares Mercury during a transit (bottom-center) with a sunspot near the solar limb (upper right).
NOTE: DO NOT LOOK AT THE SUN THROUGH A TELESCOPE WITHOUT A FULL-APERTURE SOLAR FILTER! Doing so can cause permanent blindness! Instead, try projecting the image of the sun from a telescope or binoculars onto white paper. This method avoids bringing dangerous, strongly-focused sunlight anywhere near one’s eyes.
Better still: Watch the transit live online! Find live streaming coverage from Slooh, NASA TV, Celestron telescopes, Sky and Telescope magazine, and the Virtual Telescope.
(Top image credit: Sky & Telescope magazine; map and transit image: Fred Espenak)
As Tropical Storm Hermine charged up the East Coast Sept. 2, 2016, Langley Air Force Base reached out to the Research Services Directorate and NASA Langley Research Center hangar manager Dale Bowser to see if NASA Langley could store a few F-22 Raptors. Even though the hangar in Hampton, Virginia, already had a large visitor — a C-130 from the Wallops Flight Facility on Virginia’s Eastern Shore — the hangar was able to carefully sandwich in more than a dozen Air Force fighters and offer them protection from the wind. NASA Langley photographer David C. Bowman captured the image using a fish-eye lens and shooting down from the hangar's catwalk some 70 feet above the building's floor.
The hangar provides 85,200 square feet (7,915 square meters) of open space and large door dimensions that allow for entry of big aircraft such as Boeing 757s and other commercial or military transport-class planes. The hangar normally is home to 13 of NASA Langley's own research aircraft, when they are not out doing atmospheric science or aeronautics research. Still, there is enough space to share with neighboring Langley Air Force Base during emergencies. The facility is rated for at least a Category 2 hurricane. Built in the early 1950s, it was designed to fit a B-36. It can also accommodate the Super Guppy, which visited NASA Langley in 2014.
Image credit: NASA/David C. Bowman
Engineers at NASA’s Langley Research Center in Hampton, Virginia, kicked off a series of nine drop tests of a representative Orion crew capsule withcrash test dummies inside to understand what the spacecraft and astronauts may experience when landing in the Pacific Ocean after deep-space missions. The high-fidelity capsule, coupled with the heat shield from Orion’s first flight in space, was hoisted approximately 16 feet above the water and vertically dropped into Langley’s 20-foot-deep Hydro Impact Basin. The crash test dummies were instrumented to provide data and secured inside the capsule to help provide information engineers need to ensure astronauts will be protected from injury during splashdown. Each test in the series simulates different scenarios for Orion’s parachute-assisted landings, wind conditions, velocities and wave heights the spacecraft may experience when touching down in the ocean.
It’s incredible what humans can do on and off of our planet. Here is a view from the International Space Station taken by Engineer and NASA Astronaut, Colonel Tim Kopra.
Doha, Bahrain – manmade EarthArt.
February 7, 2016.
Credit: NASA Astronaut Tim Kopra’s Twitter Account
A new robotic arm for assembling spacecraft and exploration platforms in space flexed its muscle in a successful ground demonstration Jan. 19.
The device, called the Tension Actuated in Space MANipulator (TALISMAN) was tested in the Structures and Materials Test Laboratory at NASA’s Langley Research Center in Hampton, Virginia.
TALISMAN is just one component of the Commercial Infrastructure for Robotic Assembly and Servicing (CIRAS). In this demonstration, the team manipulated the newer, longer arm back and forth from folded to extended positions to demonstrate that it is fully operational and ready for more comprehensive testing.
“The demonstration we accomplished last week was the rough equivalent of what the Navy calls a “shakedown cruise,” said John Dorsey, NASA principal investigator for CIRAS.
The tests will get progressively more difficult over the coming months as more detailed tasks are demanded of the robots. Future tests include not only a series of demonstrations exercising TALISMAN’s ability to move and manipulate objects along a truss, but also a demonstration of the NASA Intelligent Jigging and Assembly Robot (NINJAR) and the Strut Assembly, Manufacturing, Utility & Robotic Aid (SAMURAI) building two truss bays from pieces.
CIRAS is a collaboration with industry partner Orbital ATK of Dulles, Virginia, aimed at developing a “toolbox” of capabilities for use in servicing, refueling, and ultimately the construction of assets on orbit.
Advanced in-space assembly technologies will provide a more cost-effective way to build spacecraft and future human exploration platforms in space, such as the tended spaceport between the Earth and the Moon the agency is looking to build that would serve as a gateway to deep space and the lunar surface.
One of the biggest benefits of in-space assembly is the ability to launch the necessary material and components in tightly packed envelopes, given rockets have limited capacity with strict requirements on the size and shape of pre-assembled items being launched into orbit.
“It’s the difference between taking your new bedroom suite home in a box from IKEA using your Honda Civic and hiring a large box truck to deliver the same thing that was fully assembled at a factory. Space is a premium on launches,” said Chuck Taylor, CIRAS project manager at Langley.
Being able to build and assemble components in space will allow more affordable and more frequent science and discovery missions in Earth orbit, across the solar system and beyond.
CIRAS is made up of several components. TALISMAN, the long-reach robotic arm technology, was developed and patented at Langley. TALISMAN moves SAMURAI, which is like the hand that brings truss segments to NINJAR, the robotic jig that holds the truss segments in place perfectly at 90 degrees while they are permanently fastened using electron beam welding to join together 3D printed titanium truss corner joints to titanium fittings at the strut ends. NINJAR was built almost entirely by interns in the lab. The students have done incredible things, Taylor said.
“We couldn't have done what we’ve done without them,” he added.
CIRAS is a part of the In-Space Robotic Manufacturing and Assembly project portfolio, managed by NASA’s Technology Demonstration Missions Program and sponsored by NASA’s Space Technology Mission Directorate.
The CIRAS team includes prime contractor Orbital ATK, supported by its wholly-owned subsidiary, Space Logistics, LLC; along with NASA Langley; NASA’s Glenn Research Center in Cleveland, Ohio; NASA’s Goddard Space Flight Center in Greenbelt, Maryland; and the U.S. Naval Research Laboratory in Washington, D.C. If Orbital and Langley are successful in this spring’s series of demonstrations, they may be awarded a second contract to demonstrate these same capabilities on orbit.
To learn more about NASA's Space Technology Mission Directorate, visit:
https://www.nasa.gov/spacetech
Kristyn Damadeo NASA Langley Research Center