The Orion crew module for the Ascent Abort Test 2 (AA-2) was transported from NASA's Langley Research Center in Hampton, Virginia, to the Joint Base Langley-Eustis Friday, Jan. 26, for a fresh coat of paint before final testing and shipment to NASA’s Johnson Space Center in Houston. Specific flight test markings are being painted on the crew module to allow for attitude and trajectory data collection during launch. Next, it will be tested to determine the module's mass and weight, and also its center of gravity or balance, and then delivered to Johnson for integration and additional testing.
The crew module to be used for the test, fabricated at Langley, is a simplified representation designed to match the outer shape and approximate mass distribution of the Orion crew module that astronauts will fly in. During the test, planned for April 2019, the launch abort system will be activated during challenging ascent conditions at NASA's Kennedy Space Center in Florida.
Image credit: NASA/David C. Bowman
Jacob Earley, left, Frank Jones and his mother, Maria Jones, learned about the effects of gravity on other planets from NASA intern Jessica Hathaway during Homeschool Appreciation Day, which took place May 6 at the Virginia Air & Space Center (VASC) in Hampton, Virginia. Hathaway was one of several volunteers from NASA's Langley Research Center in Hampton who taught homeschooled children and their parents interactive lessons about everything from ultraviolet radiation to engineering satellites to navigating a rover on Mars. Approximately 300 people registered for the event, which has a focus on activities involving science, technology, engineering and math (STEM). The VASC is the official visitor center for NASA Langley.
Joe Atkinson NASA Langley Research Center
Engineers at NASA’s Langley Research Center in Hampton, Virginia, are developing inflatable heat shield technology called a Hypersonic Inflatable Aerodynamic Decelerator that could be vacuum packed into a rocket, then expanded in space to allow more cargo or even humans to land on distant planets, like Mars. Here they are testing the packing of a 9-foot diameter donut-shaped test article to simulate what would happen before a space mission.
The Vehicle Assembly Building (VAB) is one of the largest buildings in the world (525 ft 10 in tall, 716 ft long, and 518 ft wide) . It was originally built for assembly of Apollo/Saturn vehicles and was later modified to support Space Shuttle operations and now, Space Launch System rocket and Orion spacecraft for Exploration Mission 1.
In this view looking up from the floor of the VAB at NASA’s Kennedy Space Center in Florida, four levels of new work platforms are now installed on the north and south sides of High Bay 3. The G-level work platforms were most recently installed, at about the 14th floor level. Below them are the H, J and K level platforms.
The G-level work platforms are the fourth of 10 levels of work platforms that will surround and provide access to SLS. The Ground Systems Development and Operations Program is overseeing upgrades and modifications to VAB High Bay 3, including installation of the new work platforms, to prepare for NASA’s journey to Mars.
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.
Throughout Women’s History Month, we’ve been presenting profiles of the women who are leading the way in deep space exploration.
+ Meet some of them
Our Juno spacecraft made its fifth close flyby over giant Jupiter’s mysterious cloud tops.
+ See the latest from the King of Planets
A routine check of the aluminum wheels on our Curiosity Mars rover has found two small breaks on the rover’s left middle wheel tread–the latest sign of wear and tear as the rover continues its journey, now approaching the 10-mile (16 kilometer) mark. But there’s no sign the robotic geologist won’t keep roving right through its ongoing mission.
+ Get the full report
Our research reveals that volcanic activity at the giant Martian volcano Arsia Mons ceased about 50 million years ago, around the time of Earth’s Cretaceous-Paleogene extinction, when large numbers of plant and animal species (including dinosaurs) went extinct. However, there’s no reason to think the two events were more than a cosmic coincidence.
+ Learn how scientists pieced together the past
Images returned from the European Space Agency’s Rosetta mission indicate that during its most recent trip through the inner solar system, the surface of comet 67P/Churyumov-Gerasimenko was a very active place – full of growing fractures, collapsing cliffs and massive rolling boulders.
+ See the many faces of Comet #67P
The next rovers to explore another planet might bring along a scout. The Pop-Up Flat Folding Explorer Robot (PUFFER) in development at the Jet Propulsion Laboratory was inspired by origami. Its lightweight design is capable of flattening itself, tucking in its wheels and crawling into places rovers can’t fit.
+ Meet PUFFER
According to data from our Dawn mission to Ceres, shadowed craters on the dwarf planet may be linked to the history of how the small world has been tilted over time by the gravity of planets like Jupiter.
+ Find out how understanding “cycles of obliquity” might solve solar system mysteries
We’re developing a long-term technology demonstration project of what could become the high-speed internet of the sky. The Laser Communications Relay Demonstration (LCRD) will help engineers understand the best ways to operate laser communications systems, which could enable much higher data rates for connections between spacecraft and Earth, such as scientific data downlink and astronaut communications.
+ See how it will work
We selected 10 studies to develop mission concepts using CubeSats and other kinds of very small satellites to investigate Venus, Earth’s moon, asteroids, Mars and the outer planets. “These small but mighty satellites have the potential to enable transformational science,” said Jim Green, director of NASA’s Planetary Science Division.
+ Get the small details
It’s possible that one of our closest neighbors had rings at one point – and may have them again someday. At least, that’s the theory put forth by NASA-funded scientists at Purdue University.
+ See more details about the once and future rings of Mars
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We’re getting ready to start our next mission to find new worlds! The Transiting Exoplanet Survey Satellite (TESS) will find thousands of planets beyond our solar system for us to study in more detail. It’s preparing to launch from our Kennedy Space Center at Cape Canaveral in Florida.
Once it launches, TESS will look for new planets that orbit bright stars relatively close to Earth. We’re expecting to find giant planets, like Jupiter, but we’re also predicting we’ll find Earth-sized planets. Most of those planets will be within 300 light-years of Earth, which will make follow-up studies easier for other observatories.
TESS will find these new exoplanets by looking for their transits. A transit is a temporary dip in a star’s brightness that happens with predictable timing when a planet crosses between us and the star. The information we get from transits can tell us about the size of the planet relative to the size of its star. We’ve found nearly 3,000 planets using the transit method, many with our Kepler space telescope. That’s over 75% of all the exoplanets we’ve found so far!
TESS will look at nearly the entire sky (about 85%) over two years. The mission divides the sky into 26 sectors. TESS will look at 13 of them in the southern sky during its first year before scanning the northern sky the year after.
What makes TESS different from the other planet-hunting missions that have come before it? The Kepler mission (yellow) looked continually at one small patch of sky, spotting dim stars and their planets that are between 300 and 3,000 light-years away. TESS (blue) will look at almost the whole sky in sections, finding bright stars and their planets that are between 30 and 300 light-years away.
TESS will also have a brand new kind of orbit (visualized below). Once it reaches its final trajectory, TESS will finish one pass around Earth every 13.7 days (blue), which is half the time it takes for the Moon (gray) to orbit. This position maximizes the amount of time TESS can stare at each sector, and the satellite will transmit its data back to us each time its orbit takes it closest to Earth (orange).
Kepler’s goal was to figure out how common Earth-size planets might be. TESS’s mission is to find exoplanets around bright, nearby stars so future missions, like our James Webb Space Telescope, and ground-based observatories can learn what they’re made of and potentially even study their atmospheres. TESS will provide a catalog of thousands of new subjects for us to learn about and explore.
The TESS mission is led by MIT and came together with the help of many different partners. Learn more about TESS and how it will further our knowledge of exoplanets, or check out some more awesome images and videos of the spacecraft. And stay tuned for more exciting TESS news as the spacecraft launches!
Join mission experts to learn more about TESS, how it will search for worlds beyond our solar system and what scientists hope to find! Have questions? Use #askNASA to have them answered live during the broadcast.
Get an update on the spacecraft, the rocket and the liftoff operations ahead of the April 16 launch! Have questions? Use #askNASA to have them answered live during the broadcast.
Hear from mission scientists and experts about the science behind the TESS mission. Have questions? Use #askNASA to have them answered live during the broadcast.
This live show will dive into the science behind the TESS spacecraft, explain how we search for planets outside our solar system and will allow you to ask your questions to members of the TESS team.
This half-hour live show will discuss the TESS spacecraft, the science of searching for planets outside our solar system, and the launch from Cape Canaveral.
Join us live on Reddit for a Science AMA to discuss the hunt for exoplanets and the upcoming launch of TESS!
TESS is slated to launch at 6:32 p.m. EDT on a SpaceX Falcon 9 rocket from our Kennedy Space Center in Florida.
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On 2/18/1930, 86 years ago, Clyde Tombaugh discovered #Pluto. Happy Anniversary, buddy, we should have sent flowers. Hope you’re happy with #NewHorizons instead!
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
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.
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.