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NASA Ames Astrogram – March 2019

March 2019 issue of Ames' newsletter, the Astrogram

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Wendy Okolo Receives “Black Engineer’s Most Promising Engineer in Government Award”

Dr. Wendy Okolo, an aerospace engineer at NASA Ames, has received the “Black Engineer’s Most Promising Engineer in Government Award” at the BEYA STEM Conference in Washington D. C. Okolo is a Special Emphasis Programs Manager in the Intelligent Systems Division at Ames.

Okolo is working on the System-Wide Safety (SWS) project and a Space Technology Mission Directorate Early Career Initiative (STMD-ECI) project at Ames. For the SWS project, she led the task of predicting GPS faults in unmanned aerial systems commonly known as drones.

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Wendy Okolo, an aerospace research engineer at NASA Ames, is the recipient of the Black Engineer of the Year Award for the most promising engineer in government.
Credit: NASA

On the STMD-ECI project, she leads the controls team to develop unconventional control techniques for deployable vehicles, to enable precision landing and improve maneuverability during the entry, descent, and landing phases of spaceflight. The STMD-ECI project is a $2.5 million-dollar project that she proposed and won as part of a six-member early- career scientist team.

Her previous research has been recognized and funded by the Department of Defense through the National Defense Science and Engineering Graduate Fellowship; Zonta International, through the Amelia Earhart Fellowship; and the American Institute for Aeronautics and Astronautics through the John Leland Atwood Graduate Fellowship.

Okolo was only 26 years old when she became the first black woman to obtain a Ph.D. in aerospace engineering from the University of Texas at Arlington.  She earned both undergraduate and doctoral degrees in aerospace engineering from UT Arlington.

Okolo worked with Langley Research Center in Virginia to investigate flight data and facilitate data exchange across and within NASA centers.

All Hands Presented to Discuss Moon to Mars and Agency Budget Rollout

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The Center All Hands on March 11, 2019, began with Kimberly Ennico-Smith, (right photo), Code S, resident scientist in the Communication Office, Code DO, discussing Ames’ role in a presentation entitled, “Moon to Mars, A Pre-Game Perspective.” This was followed by the live broadcast Agency-wide Update by Administrator Jim Bridenstine. He provided information about the President’s proposed budget released earlier that morning and spoke about the Agency’s Moon to Mars program. After the Administrator’s update, Ames Center Director Eugene Tu provided Center-specific information and answered questions from the audience.
Credit: NASA Ames/Don Richey

For additional information about the Agency’s Moon to Mars program, visit: ExploreMoontoMars

Untouched Apollo Moon Rocks to be Studied at NASA Ames

by Frank Tavares

Pristinely preserved Moon rocks collected from the Apollo era are about to be released for study, and NASA has selected nine research teams for this special opportunity. One of these samples has never been in contact with Earth’s atmosphere, and some have been frozen or stored in helium since collection. Out of these nine teams, two are based at NASA Ames.

“These Moon rocks are a treasure, and the science we can do with them is a genuinely unique opportunity,” said Alexander Sehlke, a principal investigator for one of the selected research teams. “My group is using just a little vial with a bit of dust in it, but it’s really exciting.”

These preserved samples are a time capsule to the Moon’s past, containing information that NASA will need as we begin to prepare for permanently inhabiting the Moon in the coming years.

Astronaut on the Moon next to a bolder, with a rover in the foreground.
Apollo 17 geologist and astronaut Harrison Schmitt next to a large bolder on the sloping base of North Massif. This was the mission that brought back the samples now being opened up for use.
Credit: NASA/MSFC History Office

For full story, see: ApolloMoonRocks

Where’s the Water? Two Resource-Hunting Tools for the Moon’s Surface

On the Moon, scouting out water and mapping its whereabouts are important next steps toward humans living on the surface

by Abby Tabor

Launching one pound of any material into space costs thousands of dollars. Since a gallon of water weighs more than eight pounds, it’s easy to see that the ability to generate water, air and fuel in space could represent enormous cost savings for future deep-space missions. And that would make human exploration of the Moon, Mars and other destinations more affordable and sustainable.

But where will we find the raw materials to use? We already know that the Moon is a complex world full of familiar minerals and gases. It even holds reserves of water ice in some craters at its poles. Measurements from spacecraft orbiting the Moon tell us there is also material spread across the lunar surface that could be more water or a closely related resource, hydroxyl. What those orbiters found is actually the element hydrogen, which could turn out to be in the form of water – the familiar H2O – or hydroxyl, which is just one hydrogen and one oxygen atom, or OH.

Two tools from NASA Ames will be delivered to the Moon, perhaps as soon as 2020, to find out more. Through the Commercial Lunar Payload Services contract, commercial partners are building lunar landers to carry NASA experiments like these to the surface. The measurements taken on the lunar surface will help researchers understand what form the Moon’s hydrogen takes and how it behaves in the lunar environment.  

The Near Infrared Volatile Spectrometer Subsystem (NIRVSS)
The Near-Infrared Volatiles Spectrometer System, or NIRVSS, looks at light emitted or absorbed by materials to help identify their composition. When it is delivered to the Moon, NIRVSS will detect the different types of minerals and ices present in the soil, including water.
Credit: NASA

For full story, see: MoonWater

NASA Deputy Administrator James Morhard Tours Ames, Meets with Students

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NASA Deputy Administrator James Morhard visited Ames on Feb. 25, 2019. He is seen here (second person from left with red tie facing the camera, accompanied by Ames Center Director Eugene Tu, first from left). He also went on a tour of the center visiting the 80-foot-by-120-foot windtunnel (center photo) and FutureFlight Center (lower photo).
Credit: NASA Ames/Dominic Hart

Carlos Quesada, President of Costa Rica, Visits Ames to Discuss Future Collaborations

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Carlos Alvarado Quesada, President of Costa Rica and several of his high-ranking ministers visited Ames on March 14, 2019, to meet with Ames Center Director Eugene Tu and his executive staff (top left photo). The two-hour visit included discussions on possible future collaborations to enhance the current NASA-Costa Rica partnership. The president also went on a tour of the Ames, visiting the Hyperwall (top right photo), the Intelligent Robotics Laboratory (botton left photo) and the NASA Advanced Supercomputer Facility (bottom right photo), where we showed our work in science, exploration and aeronautics. Ames partnered with Costa Rica in 2013, when Ames’ UAVs flew over Turrialba volcano to monitor the ash plume from an eruption. This last summer, Ames hosted engineering students from Costa Rica as interns in support of the Astrobee project, which is launching to the International Space Station next month.
Credit: NASA Ames/Dominic Hart

What is LCROSS, the Lunar Crater Observation and Sensing Satellite?

Smashing into the Moon for science, LCROSS found water ice in a dark, cold lunar crater

by Abby Tabor

In the late 1990s, scientists studying the Moon had their appetites whet by the possibility that the Moon might, in fact, be wet. The orbiting spacecraft Lunar Prospector had sensed large amounts of hydrogen at the Moon’s poles. Could this hydrogen be in the form of water molecules – H2O? NASA would have to send a spacecraft that would really get its hands dirty and find out.

In the span of just two years, NASA’s Ames Research Center, in California’s Silicon Valley, developed a mission that reached out and touched the hydrogen detected on the Moon. It was called LCROSS, the Lunar Crater Observation and Sensing Satellite. Their clever design involved two parts: a projectile that would slam into a crater to kick up a giant plume of debris and a spacecraft that would fly through the plume to identify what it was made of.

Artist's rendering of the LCROSS spacecraft and Centaur separation, with the Moon beyond.
Artist’s rendering of the LCROSS spacecraft and Centaur separation.
Credit: NASA

For full story, see: LCROSS

Former AA for Education Donald James Speaks at Black History Month Celebration

The African American Advisory Group (AAAG) welcomed former Associate Administrator for Education Donald James as the keynote speaker on Feb. 28, 2019 to present, “Living the Dream,” in observance of Black History Month. February 1 marked the beginning of Black History Month. It is not only a time when people of African ancestry can come together in memory of their rich past and learn about the many contributions and accomplishments made to our nation’s history, but allows every American the opportunity to celebrate the traditions of African Americans and those aspects of their own culture and positive contributions made to society.

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Donald James, left photo, speaking at Ames on Feb. 28, 2019. He presented a talk entitled, “Living the Dream,” in observance of Black History Month. Tyler Gordon, top right photo seen here with Donald James, presented his artwork at Ames.
Credit: NASA Ames/Dominic Hart

Black History Month originally began as Negro History Week in 1926. It took place during the second week of February because it coincided with the birthdates of Frederick Douglass and Abraham Lincoln. Harvard-trained historian, Carter G. Woodson, is credited with the creation of Negro History Week. In 1976, the bicentennial of the United States, President Gerald R. Ford expanded the week into a full month. He said, “Our country needed to seize the opportunity to honor the too-often neglected accomplishments of black Americans in every area of endeavor throughout our history.”

Donald James was appointed NASA’s Associate Administrator for the Office of Education in Sept. 8, 2014. He was responsible for developing and implementing NASA’s education programs to strengthen student involvement and public awareness pertaining to the agency scientific goals and missions. James earned a bachelor of arts degree in international relations from the University of Southern California in Los Angeles; a master of arts degree in international economic development from the American University in Washington, D.C. and a graduate fellowship from the National Science Foundation. James also studied economics at Cambridge University, England in 1975 and attended Harvard’s Senior Executive Fellows program in 2004.

In addition to this talk, the AAAG featured a young African American student who is “living the dream.” Tyler Gordon is an inspiring artist who has overcome many obstacles in his life, but refuses to allow them to hinder his dream. This talk was hosted by the AAAG and the Office of Diversity and Equal Opportunity (ODEO) in recognition of the many contributions made by African Americans in this country. For more information, please contact Denise Snow, mailto:Denise.R.Snow@nasa.gov

Actor Anthony Rapp Discusses His Efforts in Shaping Social Movements

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Ames employees were invited to hear actor Anthony Rapp for a forum discussion and Q&A on March 12, 2019 (left photo). Rapp is perhaps best known to science fiction fans for playing “Lieutenant Commander Paul Stamets,” a Starfleet science officer, astromycologist and spore drive specialist/navigator in the CBS All Access show Star Trek: Discovery. Stamets is the first regular LGBT character on a Star Trek television series. He also is well known for originating the role of “Mark Cohen” in Jonathan Larson’s Tony Award-winning rock opera Rent. Rapp spoke about his history in working on efforts that impact social movements and answered questions following the presentation. He also went on a tour of Ames’ facilities, including FutureFlight Central (bottom right photo) and the flight simulator (top right photo).
Credit: NASA Ames/Dominic Hart

Fluid Lensing – Mapping the Closest Frontier, Our Oceans

by Frank Tavares

Whenever you look through a substance, whether it’s the water in a pool or a pane of old, rippled glass, the objects you see look distorted. For centuries, astronomers have been mapping the sky through the distortions caused by our atmosphere, however, inn recent years, they’ve developed techniques to counter these effects, clearing our view of the stars. If we turn to look at the Earth instead of the skies, distorted visuals are a challenge too: Earth scientists who want to map the oceans or study underwater features struggle to see through the distortions caused by waves at the surface.

Researchers at NASA’s Ames Research Center, in California’s Silicon Valley, are focused on solving this problem with fluid lensing, a technique for imaging through the ocean’s surface. While we’ve mapped the surfaces of the Moon and Mars in great detail, only 4% of the ocean floor is currently mapped. Getting accurate depth measurements and clear images is difficult in part, due to how light is absorbed and intensified by the water and distorted by its surface. By running complex calculations, the algorithm at the heart of fluid lensing technology is largely able to correct for these troublesome effects.

FluidCam instrument floating above a shallow and clear ocean.
The FluidCam instrument on deployment in Puerto Rico for testing.
Credit: NASA

For full story, see: fluidlensing

Adrienne Mayor Presents, "Gods & Robots – Myths, Machines & Ancient Dreams of Technology"

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On March 14, 2019, in honor of Women’s History Month, Stanford research scholar in classics and history of science Adrienne Mayor, presented at Ames the talk, “Gods and Robots – Myths, Machines and Ancient Dreams of Technology.” The presentation was sponsored by the Ames Women’s Influence Network and the Office of the Chief Scientist. In her talk, Mayor presented the fascinating story of how the ancient Greeks imagined robots and self-moving devices and invented sophisticated machines in the ancient city of learning, Alexandria (the original Silicon Valley). Greek myths refer to the creation of automatons and grappled with ethical concerns about biotechne, “life through craft” and foreshadowed some of today’s most advanced innovations in robotics, AI and human enhancements.
Credit: NASA Ames/Don Richey

Freund Discusses Identifying Pre-Earthquake Signals Using Non-mechanical Approaches

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On March 20, 2019, an Early Career Network Seminar at Ames was held with Dr. Friedemann Freund, a National Research Council Fellow. During his presentation, “Earthquakes – Most Feared and Least Understood,” he discussed his work identifying pre-earthquake signals using non-mechanical approaches. Major earthquakes are monstrous mechanical events. Magnitude 9 quakes release the energy equivalent to the simultaneous explosion of more than 2,000.000 Hiroshima-class atomic bombs. For more than 100 years, mainstream seismology has tried and failed to predict earthquakes using a mechanical physics approach. Yet, there are many signals that can be detected before large earthquakes, which are not mechanical. These signals come (1) from deep within the Earth, (2) from the Earth surface, (3) from the atmosphere and ionosphere. Most are subtle, but a few are distinct. How they are generated has been a mystery, but this mystery is now being solved. Freund studied proton conductivity using semiconductor concepts with proton valence and conduction bands, which allows for H+ transport against proton concentration gradients. He is credited with the discovery of the near-universal presence of oxygen in the 1- valence state in the mineral world, forming highly mobile positive hole charge carriers that are equivalent to the Reactive Oxygen Species (ROS) in biological systems.
Credit: NASA Ames/Dominic Hart

BASALT – Designing Future Human Space Exploration on Hawaii’s Lava Fields

by Abby Tabor

NASA’s BASALT project is designing and developing elements of future missions that could send humans to conduct science and exploration on Mars. Many of the lessons they learn can also be applied to human exploration of the Moon, the moons of Mars and near-Earth asteroids.

As rain poured down, the “astronauts” suited up for a day of exploration on Hawaii’s Kilauea volcano. A NASA research group had come here to study the geology and biology of the area’s lava fields in the same ways future explorers might study the surface of the Moon or Mars. While traversing the barren landscape, taking measurements and rock samples, they were also testing their software, communication systems, methods and NASA’s very ideas about how such extreme exploration will work.

This high-fidelity simulation of a human-led space exploration mission belonged to a project called Biologic Analog Science Associated with Lava Terrains, or BASALT. Using the volcanic activity of Hawaii Island as a good stand-in for the conditions that existed on ancient Mars, the project created a unique blend of science, mission operations and technology research.

A team sets off across the lava field near Keanakakoi crater on Hawaiis Kilauea volcano.
A team sets off across the lava field near Keanakako’i crater on Hawaii’s Kilauea volcano. Their goal is to locate and evaluate sites of scientific interest, and collect geological and biological samples for the BASALT project’s science team. In a realistic simulation of a mission to the surface of Mars, the team includes two people acting as astronauts, testing navigation and data transmission tools, and operating with communications delays and bandwidth limitations that future space travelers will really experience on Mars. Remaining members of the team provide logistical field support during the test.
Credit: NASA

For full story, see:  BASALTlavafields

Weighing Galactic Wind Provides Clues to Evolution of Galaxies

by Kassandra Bell

The Cigar Galaxy (M82) is famous for its extraordinary speed in making new stars, with stars being born 10 times faster than in the Milky Way. Now, data from the Stratospheric Observatory for Infrared Astronomy, SOFIA, have been used to study this galaxy in further detail, revealing how material that affects the evolution of galaxies may get into intergalactic space.

Researchers found, for the first time, that the galactic wind flowing from the center of the Cigar Galaxy (M82) is aligned along a magnetic field and transports a very large mass of gas and dust — the equivalent mass of 50 to 60 million Suns.

Image of Cigar Galaxy with its magnetic field shown as streamlines over red outflow, yellow dust, and black and white stars
Composite image of the Cigar Galaxy (also called M82), a starburst galaxy about 12 million light-years away in the constellation Ursa Major. The magnetic field detected by SOFIA, shown as streamlines, appears to follow the bipolar outflows (red) generated by the intense nuclear starburst. The image combines visible starlight (gray) and a tracing of hydrogen gas (red) from the Kitt Peak Observatory, with near-infrared and mid-infrared starlight and dust (yellow) from SOFIA and the Spitzer Space Telescope.
Credit: NASA/SOFIA/E. Lopez-Rodriguez; NASA/Spitzer/J. Moustakas et al.

For full story, see: SOFIACigarGalaxy

Lissauer Discusses Discovery of Kepler-11’s Planetary System at H. Julian Allen Award Seminar

The H. Julian Allen Award Seminar “Discovery, Updated Analysis and Legacy of the Supercalifragilisticexpialidocious Six-Planet Kepler-11 System” was presented by Dr. Jack J. Lissauer on Feb. 28, 2019 at Ames. The H. Julian Allen Award is truly one of NASA Ames’ highest honors. It was established in 1969 to annually recognize a scientific or engineering paper of outstanding technical merit and significance.

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Jack Lissauer, NASA Ames space scientist, discusses Kepler-11’s planet system at recent H. Julian Allen Award Seminar.
Credit: NASA Ames/Dominic Hart

In 2018, the H. Julian Allen Award was awarded to Dr. Jack J. Lissauer for the paper entitled, “A Closely Packed System of Low-mass, Low-density Planets Transiting Kepler-11” published in Nature 470, 53-58, (February 2011). This paper described new classes of planetary systems and planets. It is the first system discovered to have more than three tightly concentrated, transiting planets orbiting in the same plane. It also contains planets that are less massive than Neptune with much of their volumes occupied by hydrogen and/or helium gas.

Dr. Jack J. Lissauer is a space scientist in the Planetary Systems Branch at NASA Ames, where he conducts research on planet formation, planetary dynamics and exoplanets. For more information on the H. Julian Allen Award, please visit: https://www.nasa.gov/ames/ocs/hjulianallen

Statistical Summary of Activities of the Protective Service Division’s Security/Law Enforcement and Fire Protection Services Units for Period Ending February 2019

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