Video: Orion Swing Drop At NASA Langley Research Center

Solar System: Things to Know This Week

Get the latest on women making history at NASA, our Juno mission, the Curiosity rover and move!

1. Women at NASA Making History, Creating the Future

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

2. Juno and the Giant

Our Juno spacecraft made its fifth close flyby over giant Jupiter’s mysterious cloud tops.

+ See the latest from the King of Planets

3. When the Road Gets Rough, the Tough Keep Rolling

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

4. What Do Mars and Dinosaurs Have in Common?

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

5. A Comet in Commotion

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

6. Next Generation Space Robot is Ingenious, Versatile–and Cute

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

7. Shadowy Dawn

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

8. On Orbit and Online

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

9. A Big Role for Small Sats in Deep Space Exploration

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

10. Rings Around the Red Planet?

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

Discover more lists of 10 things to know about our solar system HERE.

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

See Mercury Race Across The Sun On Monday

Skywatchers in the western hemisphere will see a rare sight on Monday: over the course of several hours, the silhouette of the planet Mercury will appear to cross the face of the Sun. The “transit” of Mercury results from the precise alignment of the orbits of Mercury and Earth that only happens either 13 or 14 times per century; usually the orbital alignment is weak, and as seen from our planet Mercury “misses” the Sun’s disk as it orbits once every 88 days. But on Monday, the view through a properly-shielded telescope will reveal the innermost planet as a dark, perfectly circular spot that moves completely across the Sun in exactly seven and a half hours.

Because of the specifics of our respective orbits, Mercury transits only happen in either the months of May or November, with average dates of 8th May and 10th November. May transits happen less frequently than November transits because during May, Mercury is closer to its largest distance from the Sun, while in November the opposite is true. As a result, the range of possible angles between the Sun and Mercury, as seen from Earth, is smaller in November than May. While the interval between successive November transits can be either 7, 13 or 33 years, May transits are less common, with successive appearances in either 13- or 33-year intervals.

Observations of Mercury transits reach back to at least the seventeenth century. Observations from earlier than this are unlikely because the apparent size of Mercury’s silhouette against the Sun is too small for the unaided eye to resolve. This is why the first recorded Mercury transit — by the French astronomer Pierre Gassendi on 7 November 1631 — dates to after Galileo Galilei’s invention of the telescope in about 1609. Johannes Kepler earlier understood that Mercury’s orbit should periodically take it in front of the Sun, but he died in 1630 before being able to observe a predicted transit. 

While these events once had great scientific interest, they are now mainly curiosities that delight astronomy aficionados. Rarer still are transits of Venus across the Sun, the last of which took place in 2012. These events come in pairs separated by 113 years, meaning that most people alive now will not be around to see the next one in December 2117.

Who can see Monday’s event? That depends on the hour of day and which side of the Earth faces the Sun at the time. The map below indicates which parts of the world see either all, some, or none of the transit: 

You’ll need at least a good pair of binoculars or a telescope — properly shielded with a heavy filer to prevent eye damage — to even sense Mercury during the transit. It will look like a small, perfectly round and completely opaque black dot against the bright solar photosphere. Mercury is distinguishable in this sense from sunspots, which are irregular in shape, can be partially transparent, and of much larger sizes. This image compares Mercury during a transit (bottom-center) with a sunspot near the solar limb (upper right).

NOTE: DO NOT LOOK AT THE SUN THROUGH A TELESCOPE WITHOUT A FULL-APERTURE SOLAR FILTER! Doing so can cause permanent blindness! Instead, try projecting the image of the sun from a telescope or binoculars onto white paper. This method avoids bringing dangerous, strongly-focused sunlight anywhere near one’s eyes. 

Better still: Watch the transit live online! Find live streaming coverage from Slooh, NASA TV, Celestron telescopes, Sky and Telescope magazine, and  the Virtual Telescope.

(Top image credit: Sky & Telescope magazine; map and transit image: Fred Espenak)

Retired Major General Finds Balance as NASA Engineer

In many ways, the military and NASA couldn’t be different. Frank Batts has managed to navigate both worlds with precision, grace and just a bit of humor. After serving as a major general in the Army National Guard, he made the transition to working on computers as an engineer at NASA’s Langley Research Center in Hampton, Virginia.

“They’re opposites, but that keeps me balanced,” Batts said. “In the Army, you’re out there blowing things up in the field. Here, you’re trying to build electronic computer components.”

Batts is a senior data-systems engineer with the Advanced Measurement and Data Systems Branch at NASA’s Langley Research Center in Hampton, Virginia. He has been at Langley for 34 years and has seen the tools of the job change.

“Technology has changed tremendously,” said the 63-year-old Batts. “When we started out in the eighties, we were all using proprietary operating systems on real-time computers that were not widely used or understood. Now we’re pretty much using PCs for our work.”

In addition to his NASA career, Batts served his country with distinction in the armed forces – and made history along the way. He retired from the Army National Guard in 2012 as a major general and commander of the 29th Infantry Division in Fort Belvoir, Virginia - the first African-American to hold that post. He also served in the West Virginia and Tennessee national guards.

The adventure begins

Batts’ journey started in 1976, when he was accepted at North Carolina Agricultural and Technical State University in Greensboro and joined the Army Reserve Officer Training Corps (ROTC) there.

While at the university, Batts entered a cooperative program with the Union Carbide Corp., working in a gaseous diffusion plant in the nuclear division. After graduating from North Carolina A&T, Batts worked fulltime as an electrical engineer with Union Carbide, and as an engineering officer in the West Virginia National Guard.

“Initially when you get out of college, you’re competing with engineers from other schools,” Batts said. “I found out pretty soon that regardless of what school you came from, it got down to who can really deliver projects on time and on budget.”

Batts was pursuing a master’s degree in electronics engineering at North Carolina A&T around the time IBM introduced personal computers. He was told PCs were a fad and not worth investing in, but he glimpsed the future and got on board.

“It looked like to me it was the way to go,” he said.

But then in 1979, the Three Mile Island nuclear power plant in Pennsylvania experienced a partial core meltdown, releasing radioactive gas into the atmosphere.

The incident changed his professional trajectory, as the Union Carbide-run K-25 facility in Oak Ridge, Tennessee, where Batts was working, enriched uranium for nuclear power plants.

“Prior to Three Mile Island there were plans to construct nuclear plants all over the country, and K-25’s future was secure,” Batts said. “After Three Mile Island, all of those plans were dropped; we had more enriched uranium than was needed and K-25 was slated for closure.”

That meant he needed another job. While looking to move on, Batts found that NASA Langley was using a computing system similar to the one he used while he was with Union Carbide. He sets his sights on Langley, and has been on center as an electronic engineer since 1984 .

Two worlds in one

Batts’ military and NASA worlds were peacefully cohabitating until the Sept. 11, 2001, terrorist attacks. Batts was soon activated and from May 2004 through April 2005, served with the 54th Field Artillery Brigade Headquarters as the mobile liaison team chief in Kabul, Afghanistan as part of Operation Enduring Freedom.

“With the Army comes the leadership responsibilities. I managed a few thousand troops, and that’s no fun. I make an effort in my career at NASA to stay on the technical side rather than on the administrative side of things,” he said with a laugh.

What is fun for Batts, besides getting in more rounds at the golf course in his spare time, is serving as an example for engineering students though NASA’s outreach programs.

Batts, as the first engineer in his family, said he realizes the importance of recognizing those who blazed the trail for others.

“I have to pay homage to the people who came before me,” he said. “Before I was able to command a battalion, there was some else who commanded one, and did a credible enough job so that I had an opportunity.”

Batts also enjoys the reaction of people when they learn he works for NASA.

“There’s a lot of prestige that goes with working at NASA,” he said. “When people find out you work at NASA, they seem to look at you a bit differently.”

Eric Gillard NASA Langley Research Center

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.

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

NASA Begins Work to Build a Quieter Supersonic Passenger Jet

The return of supersonic passenger air travel is one step closer to reality with NASA's award of a contract for the preliminary design of a "low boom" flight demonstration aircraft. This is the first in a series of 'X-planes' in NASA's New Aviation Horizons initiative, introduced in the agency's Fiscal Year 2017 budget.

NASA Administrator Charles Bolden announced the award at an event Monday at Ronald Reagan Washington National Airport in Arlington, Virginia.

The return of supersonic passenger travel is one step closer to reality with NASA's award of a contract for the preliminary design of a low boom flight demonstrator aircraft. This is the first in a series of X-planes in NASA's New Aviation Horizons initiative, introduced in the agency’s Fiscal Year 2017 budget.Credits: NASA

"NASA is working hard to make flight cleaner, greener, safer and quieter – all while developing aircraft that travel faster, and building an aviation system that operates more efficiently," said Bolden. "To that end, it's worth noting that it's been almost 70 years since Chuck Yeager broke the sound barrier in the Bell X-1 as part of our predecessor agency's high speed research. Now we're continuing that supersonic X-plane legacy with this preliminary design award for a quieter jet that may break the barrier to accessible, affordable supersonic passenger flight."

This is an artist’s concept of a possible Low Boom Flight Demonstration Quiet Supersonic Transport (QueSST) X-plane design. The award of a preliminary design contract is the first step towards the possible return of supersonic passenger travel – but this time quieter and more affordable.Credits: Lockheed Martin

NASA selected a team led by Lockheed Martin Aeronautics Company of Palmdale, California, to complete a preliminary design for Quiet Supersonic Technology (QueSST). The work will be conducted under a task order against the Basic and Applied Aerospace Research and Technology (BAART) contract at NASA's Langley Research Center in Hampton, Virginia.

After conducting feasibility studies and working to better understand acceptable sound levels across the country, NASA's Commercial Supersonic Technology Project asked industry teams to submit design concepts for a piloted test aircraft that can fly at supersonic speeds, creating a supersonic "heartbeat" – a soft thump rather than the disruptive boom currently associated with supersonic flight.

"Developing, building and flight testing a quiet supersonic X-plane is the next logical step in our path to enabling the industry's decision to open supersonic travel for the flying public," said Jaiwon Shin, associate administrator for NASA's Aeronautics Research Mission.

Lockheed Martin will receive about $20 million over 17 months for QueSST preliminary design work. The Lockheed Martin team includes subcontractors GE Aviation of Cincinnati and Tri Models Inc. of Huntington Beach, California.

The company will develop baseline aircraft requirements and a preliminary aircraft design with specifications, and provide supporting documentation for concept formulation and planning. This documentation would be used to prepare for the detailed design, building and testing of the QueSST jet. Performance of this preliminary design also must undergo analytical and wind tunnel validation.

The detailed design and building of the QueSST aircraft, conducted under the NASA Aeronautics Research Mission Directorate's Integrated Aviation Systems Program, will fall under a future contract competition. In addition to design and building, this Low Boom Flight Demonstration (LBFD) phase of the project also will include validation of community response to the new, quieter supersonic design.

NASA's 10-year New Aviation Horizons initiative has the ambitious goals of reducing fuel use, emissions and noise through innovations in aircraft design, ground operations and the national air transportation system.

The New Aviation Horizons X-planes will typically be about half-scale of a production aircraft and likely are to be piloted. Design-and-build will take several years with aircraft starting their flight campaign around 2020, depending on funding.

For more information about NASA's aeronautics research, visit:

www.nasa.gov/aero

NASA Langley researchers are experts in modeling and simulations for entry, descent and landing, working on missions since the Viking lander in 1976. In this episode, we explore the challenges of guiding landers like Mars InSight through the Martian atmosphere for a safe landing. 

NASA InSight launched on March 5, 2018.

For more, visit https://mars.nasa.gov/insight/

This Day in NASA History: February 10, 1959

On this day, 1959, wind tunnel tests of Project Mercury configuration models were started.

By the end of the year, over 70 different models had been tested by facilities at the Air Force's Arnold Engineering Development Center and the NASA Langley, Ames, and Lewis Research Centers.

Here at NASA Langley Research Center, a lot of those tests took place in our 7 X 10-Foot High Speed Tunnel (pictured above).

Some tests also took place in our 20-Foot Vertical Spin Tunnel.

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

The Hunt for New Worlds Continues with TESS

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!

Watch the Launch + More!

Sunday, April 15 11 a.m. EDT - NASA Social Mission Overview

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.

Watch HERE. 

1 p.m. EDT - Prelaunch News Conference

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.

Watch HERE.

3 p.m. EDT - Science News Conference

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. 

Watch HERE.

4 p.m. EDT - TESS Facebook Live

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. 

Watch HERE. 

Monday, April 16 10 a.m. EDT - NASA EDGE: TESS Facebook Live

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.

Watch HERE.

1 p.m. EDT - Reddit AMA

Join us live on Reddit for a Science AMA to discuss the hunt for exoplanets and the upcoming launch of TESS!

Join in HERE.

6 p.m. EDT - Launch Coverage!

TESS is slated to launch at 6:32 p.m. EDT on a SpaceX Falcon 9 rocket from our Kennedy Space Center in Florida.

Watch HERE.

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

See what goes on behind the gates of the NASA Langley Research Center (LaRC)!