Check Out What Goes On At Our Hydro Impact Basin Facility At The NASA Langley Research Center! This

NASA Crash-Test Dummies Make A Splash Landing

Engineers drop a NASA’s Orion Spacecraft test capsule with crash-test dummies inside into 20-foot-deep Hydro Impact Basin to simulate what the spacecraft may experience when splashing down in the Pacific Ocean after deep-space missions.

More: http://www.nasa.gov/feature/langley/nasa-crash-test-dummies-suit-up-for-action

Hubble Finds a Lenticular Galaxy Standing Out in the Crowd

A lone source shines out brightly from the dark expanse of deep space, glowing softly against a picturesque backdrop of distant stars and colorful galaxies.

Captured by the NASA/ESA Hubble Space Telescope’s Advanced Camera for Surveys (ACS), this scene shows PGC 83677, a lenticular galaxy — a galaxy type that sits between the more familiar elliptical and spiral varieties.

It reveals both the relatively calm outskirts and intriguing core of PGC 83677. Here, studies have uncovered signs of a monstrous black hole that is spewing out high-energy X-rays and ultraviolet light.

Text Credit: ESA (European Space Agency)

Power of Pink Provides NASA with Pressure Pictures

They say you show your true colors when you’re under pressure.

Turns out the old saying works for models being tested in wind tunnels as well, specifically those coated with a unique Pressure-Sensitive Paint (PSP) that NASA engineers have used for more than 25 years.

Read more: https://www.nasa.gov/aero/power-of-pink-provides-nasa-with-pressure-pictures

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.

The Future of Monitoring Air Quality from Space

TEMPO’s measurements from geostationary orbit (GEO) will create a revolutionary dataset that provides understanding and improves prediction of air quality (AQ) and climate forcing.

The KORUS-AQ airborne science experiment taking to the field in South Korea this spring is part of a long-term, international project to take air quality observations from space to the next level and better inform decisions on how to protect the air we breathe.

Before a new generation of satellite sensors settle into orbit, field missions like KORUS-AQ provide opportunities to test and improve the instruments using simulators that measure above and below aircraft, while helping to infer what people breathe at the surface.

These geostationary instruments will make up a northern hemisphere air quality constellation to analyze their respective regions.Credits: Image Courtesy of Andreas Richter (University of Bremen) and Jhoon Kim (Yonsei University)

“We want to move beyond forecasting air pollution, we want to influence strategies to improve it,” said Jim Crawford, a lead scientist at NASA’s Langley Research Center in Hampton, Virginia. “This is where satellite observations can play an important role.”

Existing low Earth orbit (LEO) instruments have established the benefit of space-based views of air pollution. From space, large areas can be viewed consistently, whereas from the ground only discrete (often single) points can be measured. As Dave Flittner, TEMPO project scientist, explains, a geostationary (GEO) air-quality constellation can accurately track the import and export of air pollution as it is transported by large-scale weather patterns.

TEMPO, or Tropospheric Emissions: Monitoring of Pollution, is one instrument on the road to improving air quality from space. According to Flittner, hardware has recently begun development and TEMPO is on track to be finished no later than fall of 2017, and available for launch on a to be selected commercial communications satellite.

For the first time, TEMPO will make accurate hourly daytime measurements of tropospheric pollutants (specifically ozone, nitrogen dioxide, sulfur dioxide, formaldehyde, and aerosols) with high resolution over the U.S., Canada and Mexico. With help from related international missions, these observations provide a complete picture of pollution sources in the northern hemisphere and how they influence air quality from local to global scales.

These geostationary instruments will make up a northern hemisphere air quality constellation to analyze their respective regions.

Credits: Image Courtesy of Andreas Richter (University of Bremen) and Jhoon Kim (Yonsei University)

About 22,000 miles above the equator, the Korean Aerospace Research Institute’s GEMS (The Geostationary Environmental Monitoring Spectrometer), the European Space Agency’s Sentinel-4/UVN, and NASA’s TEMPO, will maintain their positions in orbit as the Earth rotates, covering a majority of the area from East Asia through greater North America and Europe. Together, these instruments will make up a northern hemisphere air quality constellation.. All three of these instruments analyze the same pollutant concentrations in their respective region, from the morning to evening.

Another critical part of the global air quality constellation are the LEO instruments, such as TROPOMI (a.k.a. Sentinel-5P), which will launch in late 2016 and provide a common reference for the three GEO sensors, allowing for a more accurate assessment of air quality within each region. 

Denise Lineberry

NASA Langley Research Center

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

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.

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NASA’s Transiting Exoplanet Survey Satellite (TESS) 

The Transiting Exoplanet Survey Satellite (TESS) is the next step in the search for planets outside of our solar system, including those that could support life. The mission will find exoplanets that periodically block part of the light from their host stars, events called transits. 

 TESS will survey 200,000 of the brightest stars near the sun to search for transiting exoplanets. The mission is scheduled to launch in 2018.  

The TESS launch date is NLT June 2018 (the current working launch date is April 2018).

Music: "Prototype" and "Trial" both from Killer Tracks. Credit: NASA’s Goddard Space Flight Center

NASA Goddard Space Flight Center

Tiny NASA Cameras to Watch Commercial Lander form Craters on Moon

Footage from vibration and thermal vacuum testing of the SCALPSS cameras and data storage unit.

Credits: NASA/Gary Banziger

This little black camera looks like something out of a spy movie — the kind of device one might use to snap discrete photos of confidential documents.

It's about half the size of a computer mouse.

The SCALPSS cameras, one of which is pictured here prior to thermal vacuum testing, are about the size of a computer mouse. Credits: NASA

But the only spying this camera — four of them, actually — will do is for NASA researchers wondering what happens under a spacecraft as it lands on the Moon.

It's a tiny technology with a big name — Stereo Camera for Lunar Plume-Surface Studies, or SCALPSS for short — and it will journey to the Moon in 2021 as a payload aboard an Intuitive Machines Nova-C lunar lander spacecraft. Intuitive Machines is one of two U.S. companies delivering technology and science experiments to the lunar surface later this year as part of NASA's Commercial Lunar Payload Services (CLPS) initiative. SCALPSS will provide important data about the crater formed by the rocket plume of the lander as it makes its final descent and landing on the Moon's surface.

As part of the Artemis program, NASA will send robots and humans to study more of the Moon than ever before. The agency plans to establish sustainable lunar exploration by the end of the decade, and has outlined its Artemis Base Camp concept for the lunar South Pole. Landers may deliver multiple payloads very near one another. Data such as that from SCALPSS will prove aid in computer models that inform subsequent landings.

SCALPSS team members prepare the cameras and data storage unit for vibration testing. Credits: NASA/David C. Bowman

"As we send bigger, heavier payloads and we try to land things in close proximity to each other, first at the Moon then at Mars, this ability to predict landing impacts is very important," said Michelle Munk, principal investigator for SCALPSS at NASA's Langley Research Center in Hampton, Virginia.

The four SCALPSS cameras, which will be placed around the base of the commercial lander, will begin monitoring crater formation from the precise moment a lander's hot engine plume begins to interact with the Moon's surface.

"If you don't see the crater when it starts to form, you can't really model it," said Munk. "You've got to have the start point and the end point and then you can figure out what happened, in between."

The cameras will continue capturing images until after the landing is complete. Those final stereo images, which will be stored on a small onboard data storage unit before being sent to the lander for downlink back to Earth, will allow researchers to reconstruct the crater's ultimate shape and volume.

The SCALPSS data storage unit will store the imagery the cameras collect as the Intuitive Machines Nova-C lunar lander spacecraft makes its final descent and lands on the Moon's surface. Credits: NASA

Testing to characterize the SCALPSS camera and lens took place last year at NASA's Marshall Space Flight Center in Huntsville, Alabama. Researchers conducted radial distortion, field-of-view and depth-of-focus tests among others. They also ran analytical models to better characterize how the cameras will perform. Development of the actual SCALPSS payload took place at Langley. And over the summer, researchers were able to enter the lab to assemble the payload and conduct thermal vacuum and vibration tests.

That lab access involves special approval from officials at Langley, which is currently only giving access to essential employees and high-priority projects to keep employees safe during the ongoing COVID-19 pandemic. SCALPSS was one of the first projects to return to the center. Before they could do that, facilities had to pass safety and hazard assessments. And while on center, the team had to follow strict COVID-19 safety measures, such as wearing masks and limiting the number of people who could be in a room at one time. The center also provided ample access to personal protective equipment and hand sanitizer.

The SCALPSS hardware was completed in late October and will be delivered to Intuitive Machines in February.

"Development and testing for the project moved at a pretty brisk pace with very limited funds," said Robert Maddock, SCALPSS project manager. "This was likely one of the most challenging projects anyone on the team has ever worked on."

But Munk, Maddock and the entire project team have embraced these challenges because they know the images these little cameras collect may have big ripple effects as NASA prepares for a human return to the Moon as part of the Artemis program.

"To be able to get flight data and update models and influence other designs — it's really motivating and rewarding," said Munk.

Hot off the heels of this project, the SCALPSS team has already begun development of a second payload called SCALPSS 1.1. It will be flown by another CLPS commercial lander provider to a non-polar region of the Moon in 2023 and collect data similar to its predecessor. It will also carry two additional cameras to get higher resolution stereo images of the landing area before engine plume interactions begin, which is critical for the analytic models in establishing the initial conditions for the interactions.

NASA’s Artemis program includes sending a suite of new science instruments and technology demonstrations to study the Moon, landing the first woman and next man on the lunar surface in 2024, and establishing a sustained presence by the end of the decade. The agency will leverage its Artemis experience and technologies to prepare for humanity’s the next giant leap – sending astronauts to Mars as early as the 2030s.

Joe Atkinson NASA Langley Research Center

Pan (moon of Saturn) - March 07 2017

NASA/JPL-Caltech/SSI/Kevin M. Gill