NASA Researcher Honored by Goddard Tech Office for Earth Science Work

Earth science researcher Dr. Antonia Gambacorta earned the 2023 Goddard IRAD Technology Leadership award for pioneering new ways to measure lower layers of Earth’s atmosphere from space.

The award from the chief technologist of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, recognizes Gambacorta’s work demonstrating how hyperspectral microwave sounding, the measurement of hundreds of thousands of wavelengths of microwave light, could dissect Earth’s atmospheric planetary boundary layer (PBL). She also conceptualized a microwave photonics radiometer instrument to reveal these measurements.

The part of Earth’s atmosphere people live in, and have the most experience studying, is the hardest to measure from space due to the volume and complex behavior of the air above it, Gambacorta said. Developing the ability to probe and measure the boundary layer on a global, routine basis is important to better understanding its connections to the rest of our atmosphere, the land surface, and the oceans.

“The unique challenge of the PBL requires a novel path forward that will bring together traditionally disparate observing system components in order to enable transformative scientific advances in Earth system science,” said fellow researcher Joseph Santanello. “To that end, Dr. Gambacorta’s efforts extend beyond individual technology developments, and are represented in her aspirational vision of PBL sounding as ‘the tie that binds.’ Just as notably, Dr. Gambacorta’s passion, enthusiasm, and respect for her colleagues has been evident through each of stage of the project’s development.”

In seeking solutions to measure the boundary layer, Gambacorta stepped up to lead Goddard’s hyperspectral microwave projects and became the face of the center’s Decadal Survey Incubation (DSI) efforts. Through multiple Internal Research and Development, or IRAD grants, she and her team performed fundamental research to show the effectiveness of hyperspectral microwave sounding, conceptualized a microwave photonics radiometer instrument, and more recently began developing a framework to integrate data from multiple sensors for boundary layer science observations.

“Antonia’s innovation rises above her individual successes as a capable and creative innovator,” said Goddard Chief Technologist Peter Hughes. “She capitalized on multiple programs to incubate new technology while engaging expertise from across agencies and around the world to connect to other resources.”

Her cutting-edge innovations and research earned support from NASA’s Earth Science Technology Office and from the National Oceanic and Atmospheric Administration.

Specifically, Gambacorta built on her IRAD successes to secure an Earth Science Technology Office Instrument Incubator Program (IIP) project award to further develop her team’s microwave photonics radiometer concept and DSI funding to advance the multi-sensor fusion framework. Additionally, her momentum enabled a DSI-funded airborne instrument project attempting to transform CoSMIR, Goddard’s Conical Scanning Millimeter-wave Radiometer, into a hyperspectral sensor. That project is led by up-and-coming instrument scientist Rachael Kroodsma.

This entire portfolio that Gambacorta now manages also culminated in a successful NOAA Broad Agency Announcement proposal to demonstrate hyperspectral microwave radiometry. Through her engagement with colleagues in ESTO, NOAA, and the European Organisation for the Exploitation of Meteorological Satellites, Hughes said Goddard’s hyperspectral microwave and PBL initiatives are regarded globally as the trusted strategy for understanding the planetary boundary layer. Goddard is widely viewed as a pioneer in the use of integrated photonics for Earth remote sensing due to Gambacorta’s leadership, he added.

“Antonia serves as a true inspiration to the technologists and scientists on her teams,” her colleague Santanello added. “Her innovation and contribution to Goddard and the larger community can also be measured in each of these ways.”

By Karl B. Hille

NASA’s Goddard Space Flight Center, Greenbelt, Md.

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NASA Wallops Supports Hypersonic Rocket Launches

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The Heat is On! NASA’s “Flawless” Heat Shield Demo Passes the Test

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The Heat is On! NASA’s “Flawless” Heat Shield Demo Passes the Test

A little more than a year ago, a NASA flight test article came screaming back from space at more than 18,000 mph, reaching temperatures of nearly 2,700 degrees Fahrenheit before gently splashing down in the Pacific Ocean. At that moment, it became the largest blunt body — a type of reentry vehicle that creates a heat-deflecting shockwave — ever to reenter Earth’s atmosphere.

The Low-Earth Orbit Flight Test of an Inflatable Decelerator (LOFTID) launched on Nov. 10, 2022, aboard a United Launch Alliance (ULA) Atlas V rocket and successfully demonstrated an inflatable heat shield. Also known as a Hypersonic Inflatable Aerodynamic Decelerator (HIAD) aeroshell, this technology could allow larger spacecraft to safely descend through the atmospheres of celestial bodies like Mars, Venus, and even Saturn’s moon, Titan.

“Large-diameter aeroshells allow us to deliver critical support hardware, and potentially even crew, to the surface of planets with atmospheres. This capability is crucial for the nation’s ambition of expanding human and robotic exploration across our solar system,” said Trudy Kortes, director of the Technology Demonstrations Missions (TDM) program within the agency’s Space Technology Mission Directorate (STMD) at NASA Headquarters in Washington.

NASA has been developing HIAD technologies for over a decade, including two smaller scale suborbital flight tests before LOFTID. In addition to this successful tech demo, NASA is investigating future applications, including partnering with commercial companies to develop technologies for small satellite reentry, aerocapture, and cislunar payloads.

“This was a keystone event for us, and the short answer is: It was highly successful,” said LOFTID Project Manager Joe Del Corso. “Our assessment of LOFTID concluded with the promise of what this technology may do to empower the exploration of deep space.”

Due to the success of the LOFTID tech demo, NASA announced under its Tipping Point program that it would partner with ULA to develop and deliver the “next size up,” a larger 12-meter HIAD aeroshell for recovering the company’s Vulcan engines from low Earth orbit for reuse.

A Successful Test in the Books, A Video Recap

The LOFTID team recently held a post-flight analysis assessment of the flight test at NASA’s Langley Research Center in Hampton, Virginia. Their verdict?

Upon recovery, the team discovered LOFTID appeared pristine, with minimal damage, meaning its performance was, as Del Corso puts it, “Just flawless.”

Here are some interesting visual highlights from LOFTID’s flight test.

To get to atmospheric reentry, LOFTID had to go through an intricate sequence of events. Del Corso compared it to a Rube Goldberg device, a complex machine designed to carry out simple tasks through a series of chain reactions.

Video captured the moment LOFTID deployed the HIAD (on the left), compared to a preflight animation developed by NASA Langley’s Advanced Concepts Lab (on the right). Inflation happens at the bottom of the video as LOFTID flies over the African continent.

As it flew over the Mediterranean Sea, LOFTID separated from the ULA Centaur upper stage. On the left, LOFTID is seen from Centaur’s forward-facing camera. The composite image on the right is from cameras around LOFTID’s center body, looking forward and outboard at the orange inflatable HIAD structure. In the center, looking back at Centaur, LOFTID is seen from an aft-facing camera.

As LOFTID reentered Earth’s atmosphere and reached nearly 2,700 degrees Fahrenheit, the extreme heat caused gases around it to ionize and form plasma. On the right, the images from the center body cameras became extremely bright in the visible spectrum, while the Earth is visible on infrared cameras  as the vehicle rotated.

The camera captured footage of the plasma quickly changing colors from orange to purple. Why the color change? “We’re still investigating exactly what causes that,” said John DiNonno, LOFTID chief engineer. The animation on the left shows an artist’s concept of what the front side may have looked like.

This video, captured by NASA Langley’s Scientifically Calibrated In-Flight Imagery  team, shows LOFTID during peak deceleration as the plasma recedes. On the left, LOFTID streaks through the night sky over the Pacific Ocean. On the right, the purple coloration flares up on the back side of LOFTID.

In the second part of the video, the left shifts to one of the cameras looking at the back of the aeroshell, with the receding plasma streaking at its edge.

After slowing down from more than 18,000 mph to less than 80 mph, LOFTID deployed its parachutes. 

From an infrared camera aboard the recovery ship, this video shows the parachute deployment and splashdown just over the horizon. The preflight animation is provided on the right for comparison.

LOFTID splashed down in the Pacific Ocean several hundred miles off the east coast of Hawaii and only about eight miles from the recovery ship’s bow — almost exactly as modeled. A crew got on a small boat and retrieved and hoisted LOFTID onto the recovery ship. Here is an image from the first contact with LOFTID after it splashed down.

“The LOFTID mission was important because it proved the cutting-edge HIAD design functioned successfully at an appropriate scale and in a relevant environment,” said Tawnya Laughinghouse, manager of the TDM program office at NASA’s Marshall Space Flight Center in Huntsville, Alabama.

The LOFTID demonstration was a public private-partnership with ULA funded by STMD and managed by the Technology Demonstration Mission Program, executed by NASA Langley with contributions from across NASA centers. Multiple U.S. small businesses contributed to the hardware. NASA’s Launch Services Program  was responsible for NASA’s oversight of launch operations.

For more information on LOFTID, click here.

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Hubble Images Galaxy with an Explosive Past

This image from NASA’s Hubble Space Telescope features the spiral galaxy NGC 941, which lies about 55 million light-years from Earth. Hubble’s Advanced Camera for Surveys (ACS) collected the data that created this image. Beautiful NGC 941 is undoubtedly the main attraction in this view; however, the hazy-looking galaxy was not the motivation for collecting the data. That distinction belongs to an astronomical event that took place in the galaxy years before: the supernova SN 2005ad. The location of this faded supernova was observed as part of a study of multiple hydrogen-rich supernovae, also known as type II supernovae, to better understand the environments in which certain types of supernovae take place. While the study was conducted by professional astronomers, SN 2005ad itself owes its discovery to a distinguished amateur astronomer named Kōichi Itagaki, who has discovered over 170 supernovae.

This might raise the question of how an amateur astronomer could spot something like a supernova event before professional astronomers who have access to telescopes such as Hubble. The detection of supernovae is a mixture of skill, facilities, and luck. Most astronomical events happen over time spans that dwarf human lifetimes, but supernova explosions are extraordinarily fast, appearing very suddenly and then brightening and dimming over a period of days or weeks. Another aspect is time – data from a few hours of observations with telescopes like Hubble might take weeks, months, or sometimes even years to process and analyze. Amateur astronomers can spend much more time actively observing the skies, and sometimes have extremely impressive systems of telescopes, computers, and software they can use. 

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Text credit: European Space Agency

Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov

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NASA’s Deep Space Optical Comm Demo Sends, Receives First Data

DSOC, an experiment that could transform how spacecraft communicate, has achieved ‘first light,’ sending data via laser to and from far beyond the Moon for the first time.

NASA’s Deep Space Optical Communications (DSOC) experiment has beamed a near-infrared laser encoded with test data fromnearly 10 million miles (16 million kilometers) away – about 40 times farther than the Moon is from Earth – to the Hale Telescope at Caltech’s Palomar Observatory in San Diego County, California. This is the farthest-ever demonstration of optical communications.

Riding aboard the recently launched Psyche spacecraft, DSOC is configured to send high-bandwidth test data to Earth during its two-year technology demonstration as Psyche travels to the main asteroid belt between Mars and Jupiter. NASA’s Jet Propulsion Laboratory in Southern California manages both DSOC and Psyche.

The tech demo achieved “first light” in the early hours of Nov. 14 after its flight laser transceiver – a cutting-edge instrument aboard Psyche capable of sending and receiving near-infrared signals – locked onto a powerful uplink laser beacon transmitted from the Optical Communications Telescope Laboratory at JPL’s Table Mountain Facility near Wrightwood, California. The uplink beacon helped the transceiver aim its downlink laser back to Palomar (which is 100 miles, or 130 kilometers, south of Table Mountain) while automated systems on the transceiver and ground stations fine-tuned its pointing.

“Achieving first light is one of many critical DSOC milestones in the coming months, paving the way toward higher-data-rate communications capable of sending scientific information, high-definition imagery, and streaming video in support of humanity’s next giant leap: sending humans to Mars,” said Trudy Kortes, director of Technology Demonstrations at NASA Headquarters in Washington.

Test data also was sent simultaneously via the uplink and downlink lasers, a procedure known as “closing the link” that is a primary objective for the experiment. While the technology demonstration isn’t transmitting Psyche mission data, it works closely with the Psyche mission-support team to ensure DSOC operations don’t interfere with those of the spacecraft.

“Tuesday morning’stest was the first to fully incorporate the ground assets and flight transceiver, requiring the DSOC and Psyche operations teams to work in tandem,” said Meera Srinivasan, operations lead for DSOC at JPL. “It was a formidable challenge, and we have a lot more work to do, but for a short time, we were able to transmit, receive, and decode some data.”

Before this achievement, the project needed to check the boxes on several other milestones, from removing the protective cover for the flight laser transceiver to powering up the instrument. Meanwhile, the Psyche spacecraft is carrying out its own checkouts, including powering up its propulsion systems and testing instruments that will be used to study the asteroid Psyche when it arrives there in 2028.

First Light and First Bits

With successful first light, the DSOC team will now work on refining the systems that control the pointing of the downlink laser aboard the transceiver. Once achieved, the project can begin its demonstration of maintaining high-bandwidth data transmission from the transceiver to Palomar at various distances from Earth. This data takes the form of bits (the smallest units of data a computer can process) encoded in the laser’s photons – quantum particles of light. After a special superconducting high-efficiency detector array detects the photons, new signal-processing techniques are used to extract the data from the single photons that arrive at the Hale Telescope.

The DSOC experiment aims to demonstrate data transmission rates 10 to 100 times greater than the state-of-the-art radio frequency systems used by spacecraft today. Both radio and near-infrared laser communications utilize electromagnetic waves to transmit data, but near-infrared light packs the data into significantly tighter waves, enabling ground stations to receive more data. This will help future human and robotic exploration missions and support higher-resolution science instruments.

“Optical communication is a boon for scientists and researchers who always want more from their space missions, and will enable human exploration of deep space,” said Dr. Jason Mitchell, director of the Advanced Communications and Navigation Technologies Division within NASA’s Space Communications and Navigation (SCaN) program. “More data means more discoveries.”

While optical communication has been demonstrated in low Earth orbit and out to the Moon, DSOC is the first test in deep space. Like using a laser pointer to track a moving dime from a mile away, aiming a laser beam over millions of miles requires extremely precise “pointing.”

The demonstration also needs to compensate for the time it takes for light to travel from the spacecraft to Earth over vast distances: At Psyche’s farthest distance from our planet, DSOC’s near-infrared photons will take about 20 minutes to travel back (they took about 50 seconds to travel from Psyche to Earth during the Nov. 14 test). In that time, both spacecraft and planet will have moved, so the uplink and downlink lasers need to adjust for the change in location.

“Achieving first light is a tremendous achievement. The ground systems successfully detected the deep space laser photons from DSOC’s flight transceiver aboard Psyche,” said Abi Biswas, project technologist for DSOC at JPL. “And we were also able to send some data, meaning we were able to exchange ‘bits of light’ from and to deep space.”

More About the Mission

DSOC is the latest in a series of optical communication demonstrations funded by NASA’s Space Technology Mission Directorate and the Space Communications and Navigation (SCaN) program within the agency’s Space Operations Mission Directorate.

The Psyche mission is led by Arizona State University. JPL is responsible for the mission’s overall management, system engineering, integration and test, and mission operations. Psyche is the 14th mission selected as part of NASA’s Discovery Program under the Science Mission Directorate, managed by the agency’s Marshall Space Flight Center in Huntsville, Alabama. NASA’s Launch Services Program, based at the agency’s Kennedy Space Center, managed the launch service. Maxar Technologies in Palo Alto, California, provided the high-power solar electric propulsion spacecraft chassis.

For more information about DSOC, visit:

https://www.jpl.nasa.gov/missions/dsoc

News Media Contact

Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov

2023-171

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