NASA Camera Shows Moon Crossing Face Of Earth For 2nd Time In A Year

Space Launch System (SLS) Core Stage 101

We need the biggest rocket stage ever built for the bold missions in deep space that NASA's Space Launch System rocket will give us the capability to achieve. This infographic sums up everything you need to know about the SLS core stage, the 212-foot-tall stage that serves as the backbone of the most powerful rocket in the world. The core stage includes the liquid hydrogen tank and liquid oxygen tank that hold 733,000 gallons of propellant to power the stage’s four RS-25 engines needed for liftoff and the journey to Mars. 

Image Credit: NASA/MSFC

A Wider Set of Eyes on the Universe

After years of preparatory studies, we are formally starting an astrophysics mission designed to help unlock the secrets of the universe. 

Introducing…

the Wide Field Infrared Survey Telescope, aka WFIRST.

With a view 100 times bigger than that of our Hubble Space Telescope, WFIRST will help unravel the secrets of dark energy and dark matter, and explore the evolution of the cosmos. It will also help us discover new worlds and advance the search for planets suitable for life.

WFIRST is slated to launch in the mid-2020s. The observatory will begin operations after traveling about one million miles from Earth, in a direction directly opposite the sun.

Telescopes usually come in two different “flavors” - you have really big, powerful telescopes, but those telescopes only see a tiny part of the sky. Or, telescopes are smaller and so they lack that power, but they can see big parts of the sky. WFIRST is the best of worlds.

No matter how good a telescope you build, it’s always going to have some residual errors. WFIRST will be the first time that we’re going to fly an instrument that contains special mirrors that will allow us to correct for errors in the telescope. This has never been done in space before!

Employing multiple techniques, astronomers will also use WFIRST to track how dark energy and dark matter have affected the evolution of our universe. Dark energy is a mysterious, negative pressure that has been speeding up the expansion of the universe. Dark matter is invisible material that makes up most of the matter in our universe.

Single WFIRST images will contain over a million galaxies! We can’t categorize and catalogue those galaxies on our own, which is where citizen science comes in. This allows interested people in the general public to solve scientific problems.

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Pluto ‘Paints’ its Largest Moon Red

In June 2015, when the cameras on NASA’s approaching New Horizons spacecraft first spotted the large reddish polar region on Pluto’s largest moon, Charon, mission scientists knew two things: they’d never seen anything like it elsewhere in our solar system, and they couldn’t wait to get the story behind it.

Over the past year, after analyzing the images and other data that New Horizons has sent back from its historic July 2015 flight through the Pluto system, the scientists think they’ve solved the mystery. As they detail this week in the international scientific journal Nature, Charon’s polar coloring comes from Pluto itself – as methane gas that escapes from Pluto’s atmosphere and becomes “trapped” by the moon’s gravity and freezes to the cold, icy surface at Charon’s pole. This is followed by chemical processing by ultraviolet light from the sun that transforms the methane into heavier hydrocarbons and eventually into reddish organic materials called tholins.

"Who would have thought that Pluto is a graffiti artist, spray-painting its companion with a reddish stain that covers an area the size of New Mexico?" asked Will Grundy, a New Horizons co-investigator from Lowell Observatory in Flagstaff, Arizona, and lead author of the paper. "Every time we explore, we find surprises. Nature is amazingly inventive in using the basic laws of physics and chemistry to create spectacular landscapes."

The team combined analyses from detailed Charon images obtained by New Horizons with computer models of how ice evolves on Charon’s poles. Mission scientists had previously speculated that methane from Pluto’s atmosphere was trapped in Charon’s north pole and slowly converted into the reddish material, but had no models to support that theory.

The New Horizons team dug into the data to determine whether conditions on the Texas-sized moon (with a diameter of 753 miles or 1,212 kilometers) could allow the capture and processing of methane gas. The models using Pluto and Charon’s 248-year orbit around the sun show some extreme weather at Charon’s poles, where 100 years of continuous sunlight alternate with another century of continuous darkness. Surface temperatures during these long winters dip to -430 Fahrenheit (-257 Celsius), cold enough to freeze methane gas into a solid.

“The methane molecules bounce around on Charon's surface until they either escape back into space or land on the cold pole, where they freeze solid, forming a thin coating of methane ice that lasts until sunlight comes back in the spring,” Grundy said. But while the methane ice quickly sublimates away, the heavier hydrocarbons created from it remain on the surface.

The models also suggested that in Charon’s springtime the returning sunlight triggers conversion of the frozen methane back into gas. But while the methane ice quickly sublimates away, the heavier hydrocarbons created from this evaporative process remain on the surface.

Sunlight further irradiates those leftovers into reddish material – called tholins – that has slowly accumulated on Charon’s poles over millions of years. New Horizons’ observations of Charon’s other pole, currently in winter darkness – and seen by New Horizons only by light reflecting from Pluto, or “Pluto-shine” – confirmed that the same activity was occurring at both poles.

“This study solves one of the greatest mysteries we found on Charon, Pluto’s giant moon,” said Alan Stern, New Horizons principal investigator from the Southwest Research Institute, and a study co-author. “And it opens up the possibility that other small planets in the Kuiper Belt with moons may create similar, or even more extensive ‘atmospheric transfer’ features on their moons.”

Credits: NASA/JHUAPL/SwRI

Orion Launch Abort System Motor Gets Fired-up About the Journey to Mars

Applause resounded from NASA and its partners as they watched Orion’s jettison motor generate 40,000 pounds of thrust in just a blink of an eye, preparing the spacecraft for its first integrated mission with the Space Launch System rocket.  

Onlookers had just witnessed a 1.5-second jettison motor test firing at Aerojet Rocketdyne’s facility in Sacramento, California.

The Orion launch abort system (LAS) is designed to protect astronauts in the unlikely event there is an issue during launch by pulling the spacecraft away from the rocket during a mission. The jettison motor is activated during ascent to separate the launch abort system from the spacecraft after it is no longer needed during a mission.

“This test showed us that the jettison motor can quickly generate the amount of thrust needed to pull the LAS away during an Orion mission,” said Tim Larson, jettison motor principle engineer for Lockheed Martin who has been with the project since inception. “I’m very pleased with how the test went.”

The fifth firing

The jettison motor has now undergone five tests, including two test flights. Each test in the series builds upon each other, moving the nation forward on its journey to Mars.

The motor used for the fifth test was rebuilt from a previous test motor.

“We were able to recycle some of the parts from the second ground test and use it for this test,” said NASA LAS project manager Robert Decoursey. “We not only went green, but we also saved money.”

Inside and around the test motor were instruments that included strain gauges, accelerometers and pressure transducers, which feed engineers high-quality data that show whether the motor design is ready for upcoming flight tests and missions. This motor had more instruments and produced more data than any of the previous tests.

“There are many intricate details in the jettison motor design that are not obvious from the outside, and the consistent orchestration of those details are most important to obtain predictable performance,” said NASA LAS deputy project manager Deborah Crane. “Aerojet Rocketdyne has done an excellent job executing this test on schedule.”

The jettison motor bakery

Creating a jettison motor is like baking two big cakes and making enough batter for some leftover cupcakes, according to Tim Warner, NASA LAS business manager.

The jettison motor being tested in the photo above would be activated during ascent to separate the launch abort system from the spacecraft after it is no longer needed during a mission.Credits: Aerojet Rocketdyne

What’s most exciting for the team, besides the successful test, are the latest upgrades to their baking and mixing tools.

“We were using two mixing batches to make just one motor, but have recently upgraded to a larger mixing bowl, saving us time and money,” Decoursey said.

The new mixing bowl can hold up to 450 whopping gallons of cake batter, or in NASA terms, motor propellant.

The team mixes up the batter in this large mixing bowl and evenly splits the batter into two pots for a perfectly sculpted jettison motor.

Any leftover propellant is used to make small test motors. The smaller motors are used to check the propellant’s combustion capabilities before the motors are accepted for test or flight.

What’s next?

NASA and its partners are expected to perform the last flight test of the launch abort system in 2019 before they begin sending crew to deep space aboard Orion. During the final test, an uncrewed Orion capsule will launch from a modified Peacekeeper missile and demonstrate a successful abort under the highest aerodynamic loads it could experience during a mission.

The jettison motor will be used during Orion’s first integrated mission with SLS, known as Exploration Mission-1 (EM-1) in late 2018. The mission will be the second test flight for Orion, and the first for SLS. EM-1 will send Orion on a three-week journey approximately 40,000 miles beyond the moon. The test will demonstrate the integrated performance of the rocket and spacecraft before their second test flight together, Exploration Mission-2, which will carry crew.

The LAS is led out NASA’s Langley Research Center in Virginia in collaboration with NASA’s Marshall Space Flight Center in Alabama.

Sasha Ellis

NASA Langley Research Center

Happy Birthday to NASA Astronaut Peggy Whitson!

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

NASA Touches Down in Virginia to Tout Missions at AeroSpace Days

Leaders from NASA’s Langley Research Center in Hampton, Virginia, and Wallops Flight Facility on Wallops Island, Virginia, described their accomplishments and future missions at NASA’s AeroSpace Days on Feb. 6 and 7 in Richmond.

NASA Langley Director Dave Bowles, left, meets with Virginia Secretary of Education Atif Qarni at NASA AeroSpace Days Feb. 6 in Richmond, Virginia.Credits: NASA/David C. Bowman

NASA officials and representatives from the aerospace industry met with all 140 members of the General Assembly or their staffs, as well as Gov. Ralph Northam, Lt. Gov. Justin Fairfax, and  cabinet members.

One of those lawmakers was newly elected Del. Kathy Convirs-Fowler. When she finished getting autographed pictures of Lindgren for her two children, she asked officials how aerospace initiatives can be advanced to students.

“As a former teacher, I’m very big on the programs we can implement,” she said, adding that a goal of hers is to increase the number of women and girls in science, technology, engineering, art and math (STEAM) public school programs.

It’s not every day you get to shake hands with an astronaut. Kjell Lindgren, who flew on the International Space Station, was a popular face in the group of NASA representatives on an annual journey to bring the agency’s message to Virginia lawmakers.

Sen. John Consgrove was so fired up to talk with Lindgren that he apologized for it.

“I’m sorry I’m ignoring everybody else, but I don’t get to speak to an astronaut every day,” he said.

Lindgren is used to the outsized attention, and welcomed it as an opportunity to talk about NASA’s contributions to Virginia.

“It’s one of my favorite parts of the job,” he said. “You can see that they’re very enthusiastic, very interested and excited.”

Leaders from NASA’s Langley Research Center in Hampton, Virginia, and Wallops Flight Facility on Wallops Island, Virginia, described their accomplishments and future missions at NASA’s AeroSpace Days on Feb. 6 and 7 in Richmond.

NASA officials and representatives from the aerospace industry met with all 140 members of the General Assembly or their staffs, as well as Gov. Ralph Northam, Lt. Gov. Justin Fairfax, and  cabinet members.

One of those lawmakers was newly elected Del. Kathy Convirs-Fowler. When she finished getting autographed pictures of Lindgren for her two children, she asked officials how aerospace initiatives can be advanced to students.

“As a former teacher, I’m very big on the programs we can implement,” she said, adding that a goal of hers is to increase the number of women and girls in science, technology, engineering, art and math (STEAM) public school programs.

“We want to excite the next generation,” Langley Deputy Director Clayton Turner told her. “That’s part of what we do.”

NASA Langley and Wallops have strong partnerships with private industry, including numerous technology transfer, commercialization and licensing success stories. In 2017, the two NASA centers brought a combined economic impact of $1.3 billion to Virginia and supported more than 10,000 jobs, according to an analysis by a private-sector company contracted by Langley.

“The collaboration has been really helpful,” Turner said.

Also, the state has assets that offer potential for growing the aerospace sector, including multiple universities, more than 285 aerospace firms, 66 public-use airports and a spaceport with access to orbit – one of only four in the U.S.

“By having two NASA centers here in Virginia, it also gives our students something to aim for,” Lindgren said. “The state is very fortunate and unique in that respect to have all those resources.”

AeroSpace Days, held for the past 13 years, aims to leverage those resources to recruit the next generation of explorers. That imperative drives Del. Marcia Price.

“If there’s anything I can do to help, especially in my community, to help with the outreach efforts so that they know about programs so my kids can be a part of the excellent things that are going on, let me know,” she said.

Those thoughts were echoed by Secretary of Education Atif Qarni, who offered to sponsor field trips to Langley and Wallops, speaking engagements, and support of science, technology, engineering and math (STEM)-related legislation.

“We’re here to help any way we can,” he said.

In addition to meeting lawmakers and their staffs, NASA was formally recognized on the floor of the Virginia Senate by Sen. Mamie Locke during session. Locke praised Langley’s contributions over the last 100 years and asked the group of NASA employees participating in AeroSpace Days to stand up and be recognized.

“That was a cool moment,” said Langley spokesman Michael Finneran.” It’s very satisfying to realize that we’re helping improve people’s lives through what we and our partners do. We felt like rock stars for a few minutes.”

To view a photo gallery of 2018 AeroSpace Days, click here.

Eric Gillard NASA Langley Research Center

Landing and Impact Research Facility

From enabling astronauts to practice moon landings to aircraft crash testing to drop tests for Orion, NASA's gantry has come full circle.

The gantry, a 240-foot high, 400-foot-long, 265-foot-wide A-frame steel structure located at Langley Research Center in Hampton, Va., was built in 1963 and was used to model lunar gravity. Originally named the Lunar Landing Research Facility (LLRF), the gantry became operational in 1965 and allowed astronauts like Neil Armstrong and Edwin "Buzz" Aldrin to train for Apollo 11's final 150 feet before landing on the moon.

Because the moon's gravity is only 1/6 as strong as Earth's, the gantry had a suspension system that supported 5/6 of the total weight of the Lunar Excursion Module Simulator (LEMS), the device the astronauts used to perform the tests. This supportive suspension system imitated the moon's gravitational environment. Additionally, many of the tests were conducted at night to recreate lighting conditions on the moon.

Neil Armstrong with the LEMS at the Lunar Landing Research Facility. This picture (below) was taken in February 1969 - just five months before Armstrong would become the first person to set foot on the surface of the moon.

Aircraft Crash Test Research

After the Apollo program concluded, a new purpose emerged for the gantry – aircraft crash testing. In 1972, the gantry was converted into the Impact Dynamics Research Facility (IDRF) and was used to investigate the crashworthiness of General Aviation (GA) aircraft and rotorcraft. The facility performed full-scale crash tests of GA aircraft and helicopters, system qualification tests of Army helicopters, vertical drop tests of Boeing 707 and composite fuselage sections and drop tests of the F-111 crew escape capsule.

The gantry was even used to complete a number of component tests in support of the Mars Sample Return Earth Entry Vehicle.

With features including a bridge and a 72-foot vertical drop tower, the gantry was able to support planes that weighed up to 30,000 pounds. Engineers lifted aircraft as high as 200 feet in the air and released them to determine how well the craft endured the crash. Data from the crash tests were used to define a typical acceleration for survivable crashes as well as to establish impact criteria for aircraft seats. The impact criteria are still used today as the Federal Aviation Administration standard for certification.

In 1985, the structure was named a National Historic Landmark based on its considerable contributions to the Apollo program.

Revitalized Space Mission

The gantry provides engineers and astronauts a means to prepare for Orion's return to Earth from such missions. With its new mission, the gantry also received a new name – the Landing and Impact Research (LandIR) Facility.

Although originally capable of supporting only 30,000 pounds, the new bridge can bear up to 64,000 pounds after the summer 2007 renovations. Other renovations include a new elevator, floor repairs and a parallel winch capability that allows an accurate adjustment of the pitch of the test article. The new parallel winch system increases the ability to accurately control impact pitch and pitching rotational rate. The gantry can also perform pendulum swings from as high as 200 feet with resultant velocities of over 70 miles per hour.

The gantry makes researching for the optimal landing alternative for NASA's first attempted, manned dry landing on Earth possible. Orion's return on land rather than water will facilitate reuse of the capsule. A water landing would make reuse difficult due to the corrosiveness of salt water.

The testing process involves lifting the test article by steel cables to a height between 40 and 60 feet and swinging it back to Earth. Although the airbags appear most promising, the gantry has the capability to perform different kinds of tests, including a retro rocket landing system and a scale-model, water landing test using a four-foot-deep circular pool. So far, three types of tests have been conducted in support of the Orion program, each progressing from the previous to more realistic features.

The first test consisted of dropping a boilerplate test article that was half the diameter of what Orion will be. For the second round of testing, engineers added a welded structure to the top, with a shape more comparable to Orion to examine the article's tendency to flip or remain upright.

Hydro-Impact

The on-going tests for Orion continue with impacts on water. This is to ensure astronaut safety during a return to Earth mission. Similar to the Apollo program, Orion will re-enter Earth’s atmosphere at very high speeds and after slowing down, deploy parachutes to further slow the descent into the ocean. At NASA Langley Research Center, engineers use the hydro-impact research to determine the stresses on the vehicle and examine its behavior during a mock splashdown. 

Katherine Johnson Biography

https://www.nasa.gov/content/katherine-johnson-biography

Date of Birth: August 26, 1918 Hometown: White Sulphur Springs, WV Education: B.S., Mathematics and French, West Virginia State College, 1937 Hired by NACA: June 1953 Retired from NASA: 1986 Actress Playing Role in Hidden Figures: Taraji P. Henson

Being handpicked to be one of three black students to integrate West Virginia’s graduate schools is something that many people would consider one of their life’s most notable moments, but it’s just one of several breakthroughs that have marked Katherine Johnson’s long and remarkable life. Born in White Sulphur Springs, West Virginia in 1918, Katherine Johnson’s intense curiosity and brilliance with numbers vaulted her ahead several grades in school. By thirteen, she was attending the high school on the campus of historically black West Virginia State College. At eighteen, she enrolled in the college itself, where she made quick work of the school’s math curriculum and found a mentor in math professor W. W. Schieffelin Claytor, the third African American to earn a PhD in Mathematics. Katherine graduated with highest honors in 1937 and took a job teaching at a black public school in Virginia.  

When West Virginia decided to quietly integrate its graduate schools in 1939, West Virginia State’s president Dr. John W. Davis selected Katherine and two male students as the first black students to be offered spots at the state’s flagship school, West Virginia University. Katherine left her teaching job, and enrolled in the graduate math program. At the end of the first session, however, she decided to leave school to start a family with her husband.  She returned to teaching when her three daughters got older, but it wasn’t until 1952 that a relative told her about open positions at the all-black West Area Computing section at the National Advisory Committee for Aeronautics’ (NACA’s) Langley laboratory, headed by fellow West Virginian Dorothy Vaughan. Katherine and her husband, James Goble, decided to move the family to Newport News to pursue the opportunity, and Katherine began work at Langley in the summer of 1953. Just two weeks into Katherine’s tenure in the office, Dorothy Vaughan assigned her to a project in the Maneuver Loads Branch of the Flight Research Division, and Katherine’s temporary position soon became permanent. She spent the next four years analyzing data from flight test, and worked on the investigation of a plane crash caused by wake turbulence. As she was wrapping up this work her husband died of cancer in December 1956.

The 1957 launch of the Soviet satellite Sputnik changed history—and Katherine Johnson’s life. In 1957, Katherine provided some of the math for the 1958 document Notes on Space Technology, a compendium of a series of 1958 lectures given by engineers in the Flight Research Division and the Pilotless Aircraft Research Division (PARD). Engineers from those groups formed the core of the Space Task Group, the NACA’s first official foray into space travel, and Katherine, who had worked with many of them since coming to Langley, “came along with the program” as the NACA became NASA later that year. She did trajectory analysis for Alan Shepard’s May 1961 mission Freedom 7, America’s first human spaceflight. In 1960, she and engineer Ted Skopinski coauthored Determination of Azimuth Angle at Burnout for Placing a Satellite Over a Selected Earth Position, a report laying out the equations describing an orbital spaceflight in which the landing position of the spacecraft is specified. It was the first time a woman in the Flight Research Division had received credit as an author of a research report.

In 1962, as NASA prepared for the orbital mission of John Glenn, Katherine Johnson was called upon to do the work that she would become most known for. The complexity of the orbital flight had required the construction of a worldwide communications network, linking tracking stations around the world to IBM computers in Washington, DC, Cape Canaveral, and Bermuda. The computers had been programmed with the orbital equations that would control the trajectory of the capsule in Glenn’s Friendship 7 mission, from blast off to splashdown, but the astronauts were wary of putting their lives in the care of the electronic calculating machines, which were prone to hiccups and blackouts. As a part of the preflight checklist, Glenn asked engineers to “get the girl”—Katherine Johnson—to run the same numbers through the same equations that had been programmed into the computer, but by hand, on her desktop mechanical calculating machine.  “If she says they’re good,’” Katherine Johnson remembers the astronaut saying, “then I’m ready to go.” Glenn’s flight was a success, and marked a turning point in the competition between the United States and the Soviet Union in space.

When asked to name her greatest contribution to space exploration, Katherine Johnson talks about the calculations that helped synch Project Apollo’s Lunar Lander with the moon-orbiting Command and Service Module. She also worked on the Space Shuttle and the Earth Resources Satellite, and authored or coauthored 26 research reports. She retired in 1986, after thirty-three years at Langley. “I loved going to work every single day,” she says. In 2015, at age 97, Katherine Johnson added another extraordinary achievement to her long list: President Obama awarded her the Presidential Medal of Freedom, America’s highest civilian honor.

Biography by Margot Lee Shetterly

https://www.nasa.gov/content/katherine-johnson-biography

Life at the Lab: Dummies Crash Planes!

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

Congratulations to SpaceX for successfully launching the Falcon Heavy Rocket 🚀

Image Credits: SpaceX; Brady Kenniston/NASAspaceflight.com