Happy Birthday To NASA Astronaut Peggy Whitson!

NASA Weighs, Balances Orion for Ascent Abort Test

Researchers conducted mass property testing of the Orion crew module for the Ascent Abort Test-2 Friday, Feb. 16, at NASA's Langley Research Center in Hampton, Virginia. The crew module, built at Langley, was lifted and rotated on its side to determine its weight and center of gravity, known as balance. To get accurate results during the uncrewed flight test planned for April 2019 at Cape Canaveral Air Force Station in Florida, this simplified crew module needs to have the same outer shape and approximate mass distribution of the Orion crew module that astronauts will fly in on future missions to deep space. The markings on the sides and bottom of the capsule used for the test will allow cameras to follow the spacecraft’s trajectory as well as the orientation of the spacecraft relative to the direction of travel for data collection.

Next, it will be shipped to NASA’s Johnson Space Center in Houston where engineers will outfit it with the avionics, power, software, instrumentation and other elements needed to execute the flight test. This test will help ensure Orion’s launch abort system can carry astronauts to safety in the event of an emergency with its rocket during launch.

Image Credit: NASA/David C. Bowman

Maybe NASA Astronomer, @michellethaller , can spread some ‘light’ on this topic. She has spent years studying binary star systems!

Isn’t it beautiful two suns setting over the horizon. 

The NASA Aeronautics team is working to transform aviation by enabling a new commercial market for supersonic travel over land. The centerpiece of this effort is the X-59 QueSST (short for Quiet SuperSonic Technology), a new X-plane designed to produce sonic "thumps" that could open the door to new certification standards for commercial supersonic service. NASA and Lockheed Martin are working together to design and build the X-59. Beginning in 2023, NASA will use this X-plane to measure public response to sonic thumps. 

More at www.nasa.gov/lowboom

Seven Reasons Why Rover Challenge is Serious Business

Prizes, awards and a year’s worth of bragging rights are at stake during our annual Human Exploration Rover Challenge. Year after year, student teams from across the world design, build and race rovers against the clock and each other.

With a space-themed obstacle course, unique rovers, competitive racing, our exhibits and dozens of international teams… it’s everything cool about STEM (science, technology, engineering and mathematics) and space exploration. 

Here are the “must-know” details for this year’s event:

1. Bumps, Bruises and Battle Scars

Our space-themed obstacle course often brings racers to their knees, literally. This daunting three-quarter-mile long course is difficult to traverse and isn’t for the faint of heart. It uses both lunar and Mars-themed obstacles to simulate the types of terrain found on distant planets, asteroids or moons.

Plus, teams must race their rovers in, on and around full-scale rockets and space vehicle exhibits on display at the U.S. Space & Rocket Center – the official visitor center for NASA’s Marshall Space Flight Center, both in Huntsville, Alabama. See just how difficult and wild the course can be in our Flickr gallery.

2. Homemade Wheels Only

Rover teams must design and fabricate their own original, or “homemade” wheels. In-Situ Resource Utilization is an important component for our future missions to Mars, asteroids or other planets.

Astronauts can never simply purchase wheels at the store… and neither can our rover teams. Teams must not use any “off-the-shelf” wheels on their rover. By wheels, this means any component used for contact, traction or mobility on the surface of the obstacle course, including, but not limited to wheels, tracks, treads or belts.

And, as in years past, teams are not allowed to incorporate inflated (or un-inflated) pneumatic tires. Inflated tires would be considered an off-the-shelf product, not eligible under the current rules.

3. New “Sample Retrieval” Component Added

Teams may choose to compete in this optional challenge, collecting four samples (liquid, small pebbles, large rocks and soil) using a mechanical arm or a grabber they design and build. Teams must collect a soil sample and liquid sample while driving their rover, as well as collect rock samples (both large and small) while off the rover, all within a 25-minute time limit.  The “Sample Retrieval” challenge highlights our deep-space exploration goals. Teams competing are eligible for the $250 prize awarded to the winner of each high school and college/university division.

4. Caution: Real STEM @work

The sights and sounds of welding, grinding and computer programming are prevalent in this hands-on, experiential activity where students solve similar problems faced by our workforce. Rover Challenge provides a unique test-bed to get students involved in real-world research and development. Their progress and success may glean potential technologies for future exploration of Mars and beyond.

5. Draws Inspiration from Apollo and Journey to Mars

Rover Challenge was inspired by the historic success of the lunar rovers from the Apollo missions, each one built by engineers and scientists at NASA Marshall. While we continue to honor our past achievements, we now highlight future accomplishments on deep-space exploration missions to Mars, asteroids or other planets. The addition of the “Sample Return” component and the Martian obstacles emphasize our commitment toward space exploration.

6. Our International Spirit is Alive and Well

Just like the International Space Station; we bring the best of several nations together to promote and celebrate space exploration. Nearly 80 teams are coming from as far away as Italy, Germany, India, Mexico, Columbia and Russia, as well as more “local” talent from the United States and Puerto Rico. View this year’s registered teams HERE.

7. Real-time Racing on Social Media

From start to finish, each racing rover team will be broadcast, live, on the Marshall Center’s Ustream channel. Plus, enjoy real-time race updates, results and awards by following Rover Challenge Twitter: @RoverChallenge

NASA’s Human Exploration Rover Challenge will take place at the U.S. Space & Rocket Center in Huntsville, Alabama, April 8-9. For event details, rules, course information and more, please visit: http://www.nasa.gov/roverchallenge

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

SAGE III Science Data Validation Efforts Begin

From its perch on the International Space Station, SAGE III is measuring stratospheric ozone as well as other gases and aerosols.

An orbiting science instrument whose legacy dates back 34 years continues to beam back data on Earth’s protective ozone layer – this time, from a perch on the hull of the International Space Station.

The Stratospheric Aerosol and Gas Experiment III (SAGE III), a NASA Langley Research Center-led mission, was launched on Feb. 19, 2017 and installed on the International Space Station during a 10-day robotic operation.

Since March 2017, the instrument has been measuring and collecting data on Earth’s sunscreen, stratospheric ozone, as well as other gases and aerosols, which are tiny particles in the atmosphere at all altitudes.

The SAGE III instrument makes these measurements through occultation, which involves looking at the light from the Sun or the Moon as it passes through Earth’s atmosphere at the edge, or limb, of the planet. The initial set of atmospheric data collected from the SAGE III instrument was released publicly in October 2017, and the first lunar data was released in January 2018.

Because the SAGE III instrument makes measurements through remote sensing - collecting data from some distance away - the science validation team cannot be sure if the data they are receiving is accurate without first validating it.

To do that, SAGE III science data must be compared to in-situ measurements, or measurements made by other instruments or systems that come in direct contact with the ozone, aerosol, or gas data being collected. These in-situ measurements are collected by the Network for Detection of Atmospheric Composition Change (NDACC), an international group, part of the National Oceanic and Atmospheric Administration, composed of research sites across the world collecting data on the Earth’s atmosphere.

“These sites have been vetted, validated, and have a long statistical history of making science measurements with their instruments,” said SAGE III Science Manager Marilee Roell.

The NDACC will collect these validated measurements through various methods, with two primary methods being through lidar - light detection and ranging - and sondes. Lidar is a ground-based measurement technique that uses a laser to shoot a beam into the Earth’s atmosphere, causing light to scatter by the atmospheric gases and particles. Being able to detect the distance to these gases and particles, the lidar can gather data on the Earth’s atmospheric composition.

Sondes are lightweight, balloon-borne instruments that are flown thousands of feet into the Earth’s atmosphere. As the instrument ascends, it transmits measurements of particle and gas concentrations by radio to a ground-based receiving station. Sondes are used daily across the globe to capture meteorological data, allowing people to check weather conditions each morning.

The science validation team is using NDACC ozone and aerosol lidar data, as well as ozone and water vapor sonde measurements, to validate science data collected from SAGE III.

“We want to match our vertical science product to an externally validated source. It helps the science community have confidence in our data set,” said Roell.

The team is working towards having an externally validated aerosol sonde to compare to the collected SAGE III data. This effort is in the preliminary stages of validating the aerosol balloon sonde against a suite of aerosol sounders, including lidar.

The team is working to validate science data with NDACC locations in Boulder, Colorado and Lauder, New Zealand, which fall within similar latitude bands in the northern and southern hemispheres. To be precise in validation efforts, the lidar or sonde measurement is taken at the same time and location that SAGE III is passing over and collecting equivalent data.

One of the most recent validation efforts took place in Table Mountain, California, and Haute Provence in France. Both locations include validated lidar systems, with lidar being operated by NASA’s Jet Propulsion Laboratory in Table Mountain, California.

Validation efforts were taken a step further by including a third source of measurements: NASA’s DC-8 aircraft. The aircraft, based out of NASA Armstrong Flight Research Center in Palmdale, California, operates as a flying science laboratory. It helps validate the accuracy of other remote-sensing satellite data, such as SAGE III, and can fly under the satellite’s path to collect the same measurements.

Validating the science data using this method required SAGE III, the NASA DC-8 aircraft, and the lidar system in California or France to be taking measurements at the same time and location. The science validation team worked to have all three systems line up while taking measurements and collected some coinciding science data.

NASA also created a validation website for other NDACC sites to use. The site displays SAGE III overpasses of NDACC sites that are three weeks out or less. These sites can choose to make lidar or sonde measurements at the same time as the instrument overpass, and compare them to SAGE III data collected to see if the two sets coincide. The validation team is pursuing additional NDACC sites to coordinate overpass timeframes when the sites may be taking lidar and sonde measurements.

The SAGE III team will present initial science validation data at the European Geosciences Union conference in Vienna, Austria this April.

SAGE III is the latest in a legacy of Langley instruments that go back to the Stratospheric Aerosol Measurement (SAM), which flew on the 1975 Apollo-Soyuz mission. SAGE II, operational from 1984 to 2005, measured global declines in stratospheric ozone that were later shown to be caused by human-induced increases in atmospheric chlorine. Data from it and other sources led to the development of the Montreal Protocol on Substances that Deplete the Ozone Layer.

After the passage of the protocol, SAGE II data also provided key evidence that the ozone layer was showing signs of recovery.

SAGE III, which launched to the station Feb. 19 from Kennedy Space Center in Florida, will continue to monitor that recovery, but with more of Earth’s atmosphere in its sights. SAGE II monitored only the stratosphere. SAGE III is monitoring both the stratosphere and the mesosphere, which is the layer directly above the stratosphere.

Ozone in the upper atmosphere acts as Earth’s sunscreen, protecting the surface from cancer-causing, crop-damaging ultraviolet rays. Atmospheric aerosols contribute to variability in the climate record.

Allison Leybold NASA Langley Research Center

Thanks for the shoutout!

I will be taking a short photography break to attend to a few long-neglected projects. I’ll be back with bone-yard pictures in time for Halloween, or sooner if something interesting crops up first.

Until then, here’s a completely irrelevant parting shot of the vacuum chambers on a hypersonic aeroelasticity wind tunnel at NASA’s Langley Research Center in Hampton, Virginia. Later, y'all. 

The State of Our NASA is Strong

~*~

“When you experience all of the work that is going on here at Langley today, tell people how you feel.” – Charles Bolden, Jr. (Maj. Gen. USMC-Ret), NASA Administrator

~*~

On February 9, 2016 I was offered the opportunity to tour NASA’s Langley Research Center (LRC) facilities and attend the State of NASA Address as a social media press correspondent with NASA Social.

Keep reading

New Gravity Map Gives Best View Yet Inside Mars

A new map of Mars' gravity made with three NASA spacecraft is the most detailed to date, providing a revealing glimpse into the hidden interior of the Red Planet.

"Gravity maps allow us to see inside a planet, just as a doctor uses an X-ray to see inside a patient," said Antonio Genova of the Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts. "The new gravity map will be helpful for future Mars exploration, because better knowledge of the planet's gravity anomalies helps mission controllers insert spacecraft more precisely into orbit about Mars. Furthermore, the improved resolution of our gravity map will help us understand the still-mysterious formation of specific regions of the planet." Genova, who is affiliated with MIT but is located at NASA's Goddard Space Flight Center in Greenbelt, Maryland, is the lead author of a paper on this research published online March 5 in the journal Icarus.

The improved resolution of the new gravity map suggests a new explanation for how some features formed across the boundary that divides the relatively smooth northern lowlands from heavily cratered southern highlands. Also, the team confirmed that Mars has a liquid outer core of molten rock by analyzing tides in the Martian crust and mantle caused by the gravitational pull of the sun and the two moons of Mars. Finally, by observing how Mars' gravity changed over 11 years – the period of an entire cycle of solar activity -- the team inferred the massive amount of carbon dioxide that freezes out of the atmosphere onto a Martian polar ice cap when it experiences winter. They also observed how that mass moves between the south pole and the north pole with the change of season in each hemisphere.

The map was derived using Doppler and range tracking data collected by NASA's Deep Space Network from three NASA spacecraft in orbit around Mars: Mars Global Surveyor (MGS), Mars Odyssey (ODY), and the Mars Reconnaissance Orbiter (MRO). Like all planets, Mars is lumpy, which causes the gravitational pull felt by spacecraft in orbit around it to change. For example, the pull will be a bit stronger over a mountain, and slightly weaker over a canyon.

Slight differences in Mars' gravity changed the trajectory of the NASA spacecraft orbiting the planet, which altered the signal being sent from the spacecraft to the Deep Space Network. These small fluctuations in the orbital data were used to build a map of the Martian gravity field.

The gravity field was recovered using about 16 years of data that were continuously collected in orbit around Mars. However, orbital changes from uneven gravity are tiny, and other forces that can perturb the motion of the spacecraft had to be carefully accounted for, such as the force of sunlight on the spacecraft's solar panels and drag from the Red Planet's thin upper atmosphere. It took two years of analysis and computer modeling to remove the motion not caused by gravity.

"With this new map, we've been able to see gravity anomalies as small as about 100 kilometers (about 62 miles) across, and we've determined the crustal thickness of Mars with a resolution of around 120 kilometers (almost 75 miles)," said Genova. "The better resolution of the new map helps interpret how the crust of the planet changed over Mars' history in many regions."

For example, an area of lower gravity between Acidalia Planitia and Tempe Terra was interpreted before as a system of buried channels that delivered water and sediments from Mars' southern highlands into the northern lowlands billions of years ago when the Martian climate was wetter than it is today. The new map reveals that this low gravity anomaly is definitely larger and follows the boundary between the highlands and the lowlands. This system of gravity troughs is unlikely to be only due to buried channels because in places the region is elevated above the surrounding plains. The new gravity map shows that some of these features run perpendicular to the local topography slope, against what would have been the natural downhill flow of water.

An alternative explanation is that this anomaly may be a consequence of a flexure or bending of the lithosphere -- the strong, outermost layer of the planet -- due to the formation of the Tharsis region. Tharsis is a volcanic plateau on Mars thousands of miles across with the largest volcanoes in the solar system. As the Tharsis volcanoes grew, the surrounding lithosphere buckled under their immense weight.

The new gravity field also allowed the team to confirm indications from previous gravity solutions that Mars has a liquid outer core of molten rock. The new gravity solution improved the measurement of the Martian tides, which will be used by geophysicists to improve the model of Mars' interior.

Changes in Martian gravity over time have been previously measured using the MGS and ODY missions to monitor the polar ice caps. For the first time, the team used MRO data to continue monitoring their mass. The team has determined that when one hemisphere experiences winter, approximately 3 trillion to 4 trillion tons of carbon dioxide freezes out of the atmosphere onto the northern and southern polar caps, respectively. This is about 12 to 16 percent of the mass of the entire Martian atmosphere. NASA's Viking missions first observed this massive seasonal precipitation of carbon dioxide. The new observation confirms numerical predictions from the Mars Global Reference Atmospheric Model – 2010.

The research was funded by grants from NASA's Mars Reconnaissance Orbiter mission and NASA's Mars Data Analysis Program.

Bill Steigerwald

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. 

Museum Exhibit Reveals the NASA Langley Human Computers from "Hidden Figures"

Sam McDonald NASA Langley Research Center

A new display at the Hampton History Museum offers another view of African-American women whose mathematical skills helped the nation’s early space program soar.

“When the Computer Wore a Skirt: NASA’s Human Computers” opens to the public Saturday, Jan. 21, and focuses on three women — Dorothy Vaughan, Mary Jackson and Katherine Johnson — who were illuminated in Margot Lee Shetterly’s book “Hidden Figures” and the major motion picture of the same name. Located in the museum's 20th century gallery, it was created with support from the Hampton Convention and Visitor Bureau and assistance from NASA's Langley Research Center.

“Langley’s West Computers were helping America dominate aeronautics, space research, and computer technology, carving out a place for themselves as female mathematicians who were also black, black mathematicians who were also female,” Shetterly wrote.

The modestly sized exhibit is comprised of four panels with photos and text along with one display case containing artifacts, including a 1957 model Friden mechanical calculator. That piece of equipment represented state-of-the-art technology when then original human computers were crunching numbers. A three-minute video profiling Johnson —a Presidential Medal of Freedom winner — is also part of the exhibit.

A display case at left contains a 1957 Friden STW-10 mechanical calculator, the type used by NASA human computers including Katherine Johnson. "If you were doing complicated computations during that time, this is what you used," said Hampton History Museum Curator Allen Hoilman. The machine weighs 40 pounds.

Credits: NASA/David C. Bowman

Museum curator Allen Hoilman said his favorite artifact is a May 5, 1958 memo from Associate Director Floyd Thompson dissolving the West Area Computers Unit and reassigning its staff members to other jobs around the center.

“It meant that the segregated work environment was coming to an end,” Hoilman said. “That’s why this is a significant document. It’s one of the bookends.”

That document, along with several others, was loaned to the museum by Ann Vaughan Hammond, daughter of Dorothy Vaughan. Hoilman said family members of other human computers have been contacted about contributing artifacts as well.

Ann Vaughan Hammond worked hard to find meaningful items for the display. “She really had to do some digging through the family papers,” Hoilman said, explaining that the women who worked as human computers were typically humble about their contributions. They didn’t save many mementos.

“They never would have guessed they would be movie stars,” Hoilman said.

For more information on Katherine Johnson, click here.

Credits:

Sam McDonald NASA Langley Research Center