Robotic Arm Gets A Workout

Langley Research Center Centennial Event

NASA Administrator Charles Bolden, right, and Langley Research Center Director, Dr. David E. Bowles, left, poses for a photo with staff dressed in space suits on Langley Research Center's Centennial float on Thursday, Dec. 1, 2016, at Langley Research Center in Hampton, VA.

Photo Credit: NASA Langley Research Center

NASA Astronomy Picture of the Day 2016 April 6 

Auroras and the Magnetosphere of Jupiter 

Jupiter has auroras. Like near the Earth, the magnetic field of our Solar System’s largest planet compresses when impacted by a gust of charged particles from the Sun. This magnetic compression funnels charged particles towards Jupiter’s poles and down into the atmosphere. There, electrons are temporarily excited or knocked away from atmospheric gases, after which, when de-exciting or recombining with atmospheric ions, auroral light is emitted. The featured illustration portrays the magnificent magnetosphere around Jupiter in action. In the inset image released last month, the Earth-orbiting Chandra X-ray Observatory shows unexpectedly powerful X-ray light emitted by Jovian auroras, depicted in false-colored purple. That Chandra inset is superposed over an optical image taken at a different time by the Hubble Space Telescope. This aurora on Jupiter was seen in October 2011, several days after the Sun emitted a powerful Coronal Mass Ejection (CME).

Pan (moon of Saturn) - March 07 2017

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

NASA’s Hubble Spots Possible Water Plumes Erupting on Jupiter's Moon Europa

This composite image shows suspected plumes of water vapor erupting at the 7 o’clock position off the limb of Jupiter’s moon Europa. The plumes, photographed by NASA’s Hubble’s Space Telescope Imaging Spectrograph, were seen in silhouette as the moon passed in front of Jupiter. Hubble’s ultraviolet sensitivity allowed for the features -- rising over 100 miles (160 kilometers) above Europa’s icy surface -- to be discerned. The water is believed to come from a subsurface ocean on Europa. The Hubble data were taken on January 26, 2014. The image of Europa, superimposed on the Hubble data, is assembled from data from the Galileo and Voyager missions.Credits: NASA/ESA/W. Sparks (STScI)/USGS Astrogeology Science Center

Astronomers using NASA's Hubble Space Telescope have imaged what may be water vapor plumes erupting off the surface of Jupiter's moon Europa. This finding bolsters other Hubble observations suggesting the icy moon erupts with high altitude water vapor plumes.

The observation increases the possibility that missions to Europa may be able to sample Europa’s ocean without having to drill through miles of ice.

“Europa’s ocean is considered to be one of the most promising places that could potentially harbor life in the solar system,” said Geoff Yoder, acting associate administrator for NASA’s Science Mission Directorate in Washington. “These plumes, if they do indeed exist, may provide another way to sample Europa’s subsurface.”

The plumes are estimated to rise about 125 miles (200 kilometers) before, presumably, raining material back down onto Europa's surface. Europa has a huge global ocean containing twice as much water as Earth’s oceans, but it is protected by a layer of extremely cold and hard ice of unknown thickness. The plumes provide a tantalizing opportunity to gather samples originating from under the surface without having to land or drill through the ice.

The team, led by William Sparks of the Space Telescope Science Institute (STScI) in Baltimore observed these finger-like projections while viewing Europa's limb as the moon passed in front of Jupiter.

The original goal of the team's observing proposal was to determine whether Europa has a thin, extended atmosphere, or exosphere. Using the same observing method that detects atmospheres around planets orbiting other stars, the team realized if there was water vapor venting from Europa’s surface, this observation would be an excellent way to see it.

"The atmosphere of an extrasolar planet blocks some of the starlight that is behind it," Sparks explained. "If there is a thin atmosphere around Europa, it has the potential to block some of the light of Jupiter, and we could see it as a silhouette. And so we were looking for absorption features around the limb of Europa as it transited the smooth face of Jupiter."

In 10 separate occurrences spanning 15 months, the team observed Europa passing in front of Jupiter. They saw what could be plumes erupting on three of these occasions.

This work provides supporting evidence for water plumes on Europa. In 2012, a team led by Lorenz Roth of the Southwest Research Institute in San Antonio, detected evidence of water vapor erupting from the frigid south polar region of Europa and reaching more than 100 miles (160 kilometers) into space. Although both teams used Hubble's Space Telescope Imaging Spectrograph instrument, each used a totally independent method to arrive at the same conclusion.

"When we calculate in a completely different way the amount of material that would be needed to create these absorption features, it's pretty similar to what Roth and his team found," Sparks said. "The estimates for the mass are similar, the estimates for the height of the plumes are similar. The latitude of two of the plume candidates we see corresponds to their earlier work."

But as of yet, the two teams have not simultaneously detected the plumes using their independent techniques. Observations thus far have suggested the plumes could be highly variable, meaning that they may sporadically erupt for some time and then die down. For example, observations by Roth’s team within a week of one of the detections by Sparks’ team failed to detect any plumes.

If confirmed, Europa would be the second moon in the solar system known to have water vapor plumes. In 2005, NASA's Cassini orbiter detected jets of water vapor and dust spewing off the surface of Saturn's moon Enceladus.

Scientists may use the infrared vision of NASA’s James Webb Space Telescope, which is scheduled to launch in 2018, to confirm venting or plume activity on Europa. NASA also is formulating a mission to Europa with a payload that could confirm the presence of plumes and study them from close range during multiple flybys.

“Hubble’s unique capabilities enabled it to capture these plumes, once again demonstrating Hubble’s ability to make observations it was never designed to make,” said Paul Hertz, director of the Astrophysics Division at NASA Headquarters in Washington. “This observation opens up a world of possibilities, and we look forward to future missions -- such as the James Webb Space Telescope -- to follow up on this exciting discovery.”

The work by Sparks and his colleagues will be published in the Sept. 29 issue of the Astrophysical Journal.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA (the European Space Agency.) NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. STScI, which is operated for NASA by the Association of Universities for Research in Astronomy in Washington, conducts Hubble science operations.

For images and more information about Europa and Hubble, visit:

http://www.nasa.gov/hubble & http://hubblesite.org/news/2016/33

Sean Potter / Laurie Cantillo Headquarters, Washington 202-358-1536 / 202-358-1077 sean.potter@nasa.gov / laura.l.cantillo@nasa.gov

Ann Jenkins / Ray Villard Space Telescope Science Institute, Baltimore 410-338-4488 / 410-338-4514 ​jenkins@stsci.edu / villard@stsci.edu

RELEASE 16-096

It’s incredible what humans can do on and off of our planet. Here is a view from the International Space Station taken by Engineer and NASA Astronaut, Colonel Tim Kopra.

Doha, Bahrain – manmade EarthArt.

February 7, 2016.

Credit: NASA Astronaut Tim Kopra’s Twitter Account

We do the coolest tests here! Check out the Boeing Commercial Crew CST-100 Starliner drop:

Engineers from NASA’s Langley Research Center in Hampton, Va., and Boeing dropped a full-scale test article of the company’s CST-100 Starliner into Langley’s 20-foot-deep Hydro Impact Basin at the Landing and Impact Research Facility. Although the spacecraft is designed to land on land, Boeing is testing the Starliner’s systems in water to ensure astronaut safety in the unlikely event of an emergency. This test happened Feb. 9, 2016.

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

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)

Feb. 12 'State of NASA' Events Highlight Agency Goals for Space Exploration

NASA centers across the country, including the Langley Research Center in Hampton, Virginia, are opening their doors Monday, Feb. 12, to media and social media for 'State of NASA' events.

Activities include a speech from acting NASA Administrator Robert Lightfoot, and unique opportunities for a behind-the-scenes look at the agency's work. These events follow President Trump's Fiscal Year 2019 budget proposal delivery to the U.S. Congress.

Events at NASA centers will include media tours and presentations on the agency's exploration goals for the Moon, Mars and worlds beyond, the innovative technologies developed and under development, as well as the scientific discoveries made as NASA explores and studies Earth and our universe, and advancements toward next-generation air travel.

Lightfoot will provide a 'State of NASA' address to the agency's workforce at 1 p.m. EST from Marshall Space Flight Center in Huntsville, Alabama. His remarks will air live on NASA Television and the agency's website, https://www.nasa.gov/live. Following the presentation, NASA centers will host tours of their facilities for media and social media guests.

At Langley, the news and social media event will run from 1 to 5 p.m. and include:

A look at the SAGE III flight control center. SAGE III is the Stratospheric Aerosol and Gas Experiment III studying Earth's atmosphere from the International Space Station.

A visit to the research aircraft hangar to see aircraft that are used in support of airborne research campaigns, as well as an inflatable heat shield that will enable landing on distant worlds.

A view of the labs where sonic-boom testing is being done to lower their impact so that commercial aircraft can be developed to fly supersonically over land.

A tour in a lab where inflatable space structures are being developed.

Follow the hashtag #StateOfNASA for more!

New NASA X-Plane Construction Begins Now

NASA’s aeronautical innovators are ready to take things supersonic, but with a quiet twist.

For the first time in decades, NASA aeronautics is moving forward with the construction of a piloted X-plane, designed from scratch to fly faster than sound with the latest in quiet supersonic technologies.

The new X-plane’s mission: provide crucial data that could enable commercial supersonic passenger air travel over land.

To that end, NASA on April 2 awarded a $247.5 million contract to Lockheed Martin Aeronautics Company of Palmdale, Calif., to build the X-plane and deliver it to the agency’s Armstrong Flight Research Center in California by the end of 2021.

“It is super exciting to be back designing and flying X-planes at this scale,” said Jaiwon Shin, NASA’s associate administrator for aeronautics. “Our long tradition of solving the technical barriers of supersonic flight to benefit everyone continues.”

The key to success for this mission – known as the Low-Boom Flight Demonstrator – will be to demonstrate the ability to fly supersonic, yet generate sonic booms so quiet, people on the ground will hardly notice them, if they hear them at all.

Current regulations, which are based on aircraft speed, ban supersonic flight over land. With the low-boom flights, NASA intends to gather data on how effective the quiet supersonic technology is in terms of public acceptance by flying over a handful of U.S. cities, which have yet to be selected.

The complete set of community response data is targeted for delivery in 2025 to the Federal Aviation Administration (FAA) and the International Civil Aviation Organization (ICAO) from which they can develop and adopt new rules based on perceived sound levels to allow commercial supersonic flight over land.

Years of sonic boom research, beginning with the X-1 first breaking the sound barrier in 1947 – when NASA was the National Advisory Committee for Aeronautics – paved the way for the Low-Boom Flight Demonstration X-plane’s nearly silent treatment of supersonic flight.

The answer to how the X-plane's design makes a quiet sonic boom is in the way its uniquely-shaped hull generates supersonic shockwaves. Shockwaves from a conventional aircraft design coalesce as they expand away from the airplane’s nose and tail, resulting in two distinct and thunderous sonic booms.

But the design’s shape sends those shockwaves away from the aircraft in a way that prevents them from coming together in two loud booms. Instead, the much weaker shockwaves reach the ground still separated, which will be heard as a quick series of soft thumps – again, if anyone standing outside notices them at all.

It’s an idea first theorized during the 1960s and tested by NASA and others during the years since, including flying from 2003-2004 an F-5E Tiger fighter jetmodified with a uniquely-shaped nose, which proved the boom-reducing theory was sound.

NASA’s confidence in the Low-Boom Flight Demonstration design is buoyed by its more recent research using results from the latest in wind-tunnel testing, and advanced computer simulation tools, and actual flight testing.

Recent studies have investigated methods to improve the aerodynamic efficiency of supersonic aircraft wings, and sought to better understand sonic boom propagation through the atmosphere.

Even a 150-year-old photographic technique has helped unlock the modern mysteries of supersonic shockwave behavior during the past few years.

“We’ve reached this important milestone only because of the work NASA has led with its many partners from other government agencies, the aerospace industry and forward-thinking academic institutions everywhere,” said Peter Coen, NASA’s Commercial Supersonic Technology project manager.

So now it’s time to cut metal and begin construction.

The X-plane’s configuration will be based on a preliminary design developed by Lockheed Martin under a contract awarded in 2016. The proposed aircraft will be 94 feet long with a wingspan of 29.5 feet and have a fully-fueled takeoff weight of 32,300 pounds.

The design research speed of the X-plane at a cruising altitude of 55,000 feet is Mach 1.42, or 940 mph. Its top speed will be Mach 1.5, or 990 mph. The jet will be propelled by a single General Electric F414 engine, the powerplant used by F/A-18E/F fighters.

A single pilot will be in the cockpit, which will be based on the design of the rear cockpit seat of the T-38 training jet famously used for years by NASA’s astronauts to stay proficient in high-performance aircraft.

Jim Less is one of the two primary NASA pilots at Armstrong who will fly the X-plane after Lockheed Martin’s pilots have completed initial test flights to make sure the design is safe to fly.

“A supersonic manned X-plane!” Less said, already eager to get his hands on the controls. “This is probably going to be a once-in-a-lifetime opportunity for me. We’re all pretty excited.”

Less is the deputy chief pilot for Low-Boom Flight Demonstration. He and his boss, chief pilot Nils Larson, have already provided some input into things like cockpit design and the development of the simulators they will use for flight training while the aircraft is under construction.

“It’s pretty rare in a test pilot’s career that he can be involved in everything from the design phase to the flight phase, and really the whole life of the program,” Less said.

The program is divided into three phases and the tentative schedule looks like this:

2019 – NASA conducts a critical design review of the low-boom X-plane configuration, which, if successful, allows final construction and assembly to be completed.

2021 – Construction of the aircraft at Lockheed Martin’s Skunk Works facility in Palmdale is completed, to be followed by a series of test flights to demonstrate the aircraft is safe to fly and meets all of NASA’s performance requirements. The aircraft is then officially delivered to NASA, completing Phase One.

2022 – Phase Two will see NASA fly the X-plane in the supersonic test range over Edwards to prove the quiet supersonic technology works as designed, its performance is robust, and it is safe for operations in the National Airspace System.

2023 to 2025 – Phase Three begins with the first community response test flights, which will be staged from Armstrong. Further community response activity will take place in four to six cities around the U.S.

All of NASA’s aeronautics research centers play a part in the Low-Boom Flight Demonstration mission, which includes construction of the demonstrator and the community overflight campaign. For the low-boom flight demonstrator itself, these are their roles:

Ames Research Center, California — configuration assessment and systems engineering.

Armstrong Flight Research Center, California — airworthiness, systems engineering, safety and mission assurance, flight/ground operations, flight systems, project management, and community response testing.

Glenn Research Center, Cleveland — configuration assessment and propulsion performance.

Langley Research Center, Virginia — systems engineering, configuration assessment and research data, flight systems, project management, and community response testing.

“There are so many people at NASA who have put in their very best efforts to get us to this point,” said Shin. “Thanks to their work so far and the work to come, we will be able to use this X-plane to generate the scientifically collected community response data critical to changing the current rules to transforming aviation!”

Jim Banke Aeronautics Research Mission Directorate