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STScI Astronomers Nancy Levenson and David Soderblom Elected AAAS Fellows
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By NASA
Four individuals with NASA affiliations have been named 2022 fellows by the American Association for the Advancement of Science (AAAS) in recognition of their scientifically and socially distinguished achievements in the scientific enterprise.
Election as a Fellow by the AAAS Council honors members whose efforts on behalf of the advancement of science or its applications in service to society have distinguished them among their peers and colleagues. The 2022 Fellows class includes 508 scientists, engineers, and innovators spanning 24 scientific disciplines.
Rita Sambruna from NASA’s Goddard Space Flight Center in Greenbelt, Maryland, was recognized in the AAAS Section on Astronomy, and Jennifer Wiseman, also from Goddard, was recognized in the AAAS Section on Physics. Dorothy Peteet of NASA’s Goddard Institute for Space Studies (GISS) in New York was honored in the AAAS section on Earth Science. Erik Conway of NASA’s Jet Propulsion Laboratory (JPL) in southern California was honored for distinguished contributions and public outreach to the history of science and understanding of contemporary science and science policy.
Dr. Rita Sambruna is the acting deputy director of the Science and Exploration Directorate and the deputy director of the Astrophysics Division at Goddard. She also promotes increased participation of underrepresented groups in science.Courtesy of Rita M. Sambruna Rita Sambruna
Dr. Rita Sambruna is the acting deputy director of the Science and Exploration Directorate and the deputy director of the Astrophysics Division at Goddard. She also promotes increased participation of underrepresented groups in science.
She worked with a team to position Goddard to lead the decadal top priority missions. She led a team to set into place a vision for a Multi-Messenger Astrophysics Science Support Center at Goddard, to lead the astrophysics community in reaping the most from NASA- and ground-based observations of celestial sources.
She came to Goddard in 2005 to work on multiwavelength observations of jets using the Fermi Gamma-ray Space Telescope and other NASA capabilities. From 2010 to 2020 she worked at NASA Headquarters, Washington, as a program scientist for astrophysics. Her research interests include relativistic jets, physics of compact objects, supermassive black holes in galaxies, and multiwavelength and multi-messenger astrophysics.
In December 2022, Sambruna was awarded the Honorary Fellowship of the Royal Astronomical Society (RAS) as an internationally acclaimed astrophysicist who embodies the RAS mission in promoting the advancement of science, the increased participation of historically underrepresented groups in astronomy, and a broad interest in astronomy. In 2019 she was awarded the NASA Extraordinary Achievement Medal for her leadership on the 2020 Astrophysics Decadal Survey studies. She was named Fellow of the American Physical Society in 2020 and a Fellow of the American Astronomical Society in 2021.
Dr. Jennifer Wiseman is a senior astrophysicist at Goddard and a Senior Fellow at Goddard, where she serves as the senior project scientist for the Hubble Space Telescope. Her primary responsibility is to ensure that the Hubble mission is as scientifically productive as possible.NASA Jennifer Wiseman
Dr. Jennifer Wiseman is a senior astrophysicist at Goddard and a Senior Fellow at Goddard, where she serves as the senior project scientist for the Hubble Space Telescope. Her primary responsibility is to ensure that the Hubble mission is as scientifically productive as possible. Previously, Wiseman headed Goddard’s Laboratory for Exoplanets and Stellar Astrophysics. She started her career at NASA in 2003 as the program scientist for Hubble and several other astrophysics missions at NASA Headquarters.
Wiseman’s scientific expertise is centered on the study of star-forming regions in our galaxy using a variety of tools, including radio, optical, and infrared telescopes. She has a particular interest in dense interstellar gas cloud cores, embedded protostars, and their related outflows as active ingredients of cosmic nurseries where stars and their planetary systems are born. In addition to research in astrophysics, Wiseman is also interested in science policy and public science outreach and engagement. She has served as a congressional science fellow of the American Physical Society, an elected councilor of the American Astronomical Society, and a public dialogue leader for AAAS. She enjoys giving talks on the excitement of astronomy and scientific discovery, and has appeared in many science and news venues, including The New York Times, The Washington Post, NOVA, and National Public Radio.
Dr. Dorothy M. Peteet is a senior research scientist at GISS and an adjunct professor at Columbia University. She directs the Paleoecology Division of the New Core Lab at Lamont Doherty Earth Observatory (LDEO) of Columbia.NASA Dorothy Peteet
Dr. Dorothy M. Peteet is a senior research scientist at GISS and an adjunct professor at Columbia University. She directs the Paleoecology Division of the New Core Lab at Lamont Doherty Earth Observatory (LDEO) of Columbia.
In collaboration with GISS climate modelers and LDEO geochemists, she is studying conditions of the Late Pleistocene and Holocene that are archived in sediments from lakes and wetlands. Peteet documents past changes in vegetation, derived from analyses of pollen and spores, plant and animal macrofossils, carbon, and charcoal embedded in sediments. Her research provides local and regional records of ancient vegetational and climate history. One recent focus has been the sequestration of carbon in northern peatlands and coastal marshes: ecosystems that are now vulnerable to climate change and potentially substantial releases of carbon back into the atmosphere.
Peteet also has performed climate modeling experiments to test hypotheses concerning the last glacial maximum and abrupt climate change. She is interested in climate sensitivity and in how past climate changes and ecological shifts might provide insights on future climate change.
Erik Conway has served as the historian at JPL since 2004. Prior to that, he was a contract historian at NASA’s Langley Research Center in Hampton, Virginia. He is a historian of science and technology, and has written histories of atmospheric science, supersonic transportation, aviation infrastructure, Mars exploration, and climate change denial.NASA Erik Conway
Erik Conway has served as the historian at JPL since 2004. Prior to that, he was a contract historian at NASA’s Langley Research Center in Hampton, Virginia. He is a historian of science and technology, and has written histories of atmospheric science, supersonic transportation, aviation infrastructure, Mars exploration, and climate change denial.
He is the author of nine books, most recently, “A History of Near-Earth Objects Research” (NASA, 2022), and “The Big Myth” (Bloomsbury, 2023). His book “Merchants of Doubt” with Naomi Oreskes was awarded the Helen Miles Davis and Watson Davis prize from the History of Science Society. He received a Guggenheim Fellowship in 2018 and the Athelstan Spilhaus Award from the American Geophysical Union in 2016.
AAAS noted that these honorees have gone above and beyond in their respective disciplines. They bring a broad diversity of perspectives, innovation, curiosity, and passion that will help sustain the scientific field today and into the future. Many of these individuals have broken barriers to achieve successes in their given disciplines.
AAAS is the world’s largest general scientific society and publisher of the Science family of journals.
For information about NASA and agency programs, visit: https://www.nasa.gov
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Last Updated Feb 10, 2025 EditorJamie Adkins Related Terms
Goddard Space Flight Center Goddard Institute for Space Studies People of Goddard View the full article
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By NASA
NASA has selected David Korth as deputy for Johnson Space Center’s Safety and Mission Assurance directorate. Korth previously served as deputy manager of the International Space Station Avionics and Software Office at Johnson Space Center prior to serving as acting deputy for Safety and Mission Assurance.
I’m excited to embark on my new role as deputy for Johnson’s Safety and Mission Assurance directorate,” Korth said. “Safety has been a priority for me throughout my NASA career. It is at the forefront of every decision I make.”
Korth brings more than 34 years’ experience to NASA human space flight programs. Prior to supporting the space station Avionics and Software Office, Mr. Korth served as deputy manager of the program’s Systems Engineering and Integration Office where he also led the agency Commercial Destination program’s procurement culminating in the selection of Axiom Space.
Mr. Korth began his NASA career as an engineer in the space station program’s operations planning group where he helped develop initial operational concepts and planning system requirements for the orbiting laboratory. He converted to civil servant in 1998 and was among the first three individuals to achieve front room certification as a space station ‘OPS PLAN’ front room operator. Korth also served as the lead operations planner for Expedition 1 – the first space station crewed expedition, was awarded two NASA fellowships, served as the operations division technical assistant in the Mission Operations Directorate, and was selected as a flight director in May 2007and served as lead space station flight director for Expeditions 21, 22, and 37, lead flight director for Japanese cargo ship mission HTV3, and lead flight director for US EVAs 22, 23,and 27.
“David did an excellent job supporting Johnson’s many programs and institutional safety needs while serving as acting deputy manager,” said Willie Lyles, director of the Safety and Mission Assurance directorate. “He successfully weighed in on several critical risk-based decisions with the technical authority community. David’s program and flight operations experience is unique and is an asset to this role.”
Throughout his career, Korth has been recognized for outstanding technical achievements and leadership, receiving a Rotary National Award for Space Achievement, a Silver Snoopy award, two Superior Achievement awards, two NASA Outstanding Leadership medals, and a NASA Exceptional Achievement medal.
“David is an outstanding leader and engineer who truly understands NASA’s safety environment and protocols,” said Vanessa Wyche, director of NASA’s Johnson Space Center. “His leadership will ensure the center continues its ‘safety first’ ideology. I am extremely pleased to announce his selection for this position.”
Mr. Korth earned his bachelor’s degree in aerospace engineering from Texas A&M University, and a master’s degree in statistics from the University of Houston-Clear Lake.
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By NASA
International teams of astronomers monitoring a supermassive black hole in the heart of a distant galaxy have detected features never seen before using data from NASA missions and other facilities. The features include the launch of a plasma jet moving at nearly one-third the speed of light and unusual, rapid X-ray fluctuations likely arising from near the very edge of the black hole.
Radio images of 1ES 1927+654 reveal emerging structures that appear to be jets of plasma erupting from both sides of the galaxy’s central black hole following a strong radio flare. The first image, taken in June 2023, shows no sign of the jet, possibly because hot gas screened it from view. Then, starting in February 2024, the features emerge and expand away from the galaxy’s center, covering a total distance of about half a light-year as measured from the center of each structure. NSF/AUI/NSF NRAO/Meyer at al. 2025 The source is 1ES 1927+654, a galaxy located about 270 million light-years away in the constellation Draco. It harbors a central black hole with a mass equivalent to about 1.4 million Suns.
“In 2018, the black hole began changing its properties right before our eyes, with a major optical, ultraviolet, and X-ray outburst,” said Eileen Meyer, an associate professor at UMBC (University of Maryland Baltimore County). “Many teams have been keeping a close eye on it ever since.”
She presented her team’s findings at the 245th meeting of the American Astronomical Society in National Harbor, Maryland. A paper led by Meyer describing the radio results was published Jan. 13 in The Astrophysical Journal Letters.
After the outburst, the black hole appeared to return to a quiet state, with a lull in activity for nearly a year. But by April 2023, a team led by Sibasish Laha at UMBC and NASA’s Goddard Space Flight Center in Greenbelt, Maryland, had noted a steady, months-long increase in low-energy X-rays in measurements by NASA’s Neil Gehrels Swift Observatory and NICER (Neutron star Interior Composition Explorer) telescope on the International Space Station. This monitoring program, which also includes observations from NASA’s NuSTAR (Nuclear Spectroscopic Telescope Array) and ESA’s (European Space Agency) XMM-Newton mission, continues.
The increase in X-rays triggered the UMBC team to make new radio observations, which indicated a strong and highly unusual radio flare was underway. The scientists then began intensive observations using the NRAO’s (National Radio Astronomy Observatory) VLBA (Very Long Baseline Array) and other facilities. The VLBA, a network of radio telescopes spread across the U.S., combines signals from individual dishes to create what amounts to a powerful, high-resolution radio camera. This allows the VLBA to detect features less than a light-year across at 1ES 1927+654’s distance.
Active galaxy 1ES 1927+654, circled, has exhibited extraordinary changes since 2018, when a major outburst occurred in visible, ultraviolet, and X-ray light. The galaxy harbors a central black hole weighing about 1.4 million solar masses and is located 270 million light-years away. Pan-STARRS Radio data from February, April, and May 2024 reveals what appear to be jets of ionized gas, or plasma, extending from either side of the black hole, with a total size of about half a light-year. Astronomers have long puzzled over why only a fraction of monster black holes produce powerful plasma jets, and these observations may provide critical clues.
“The launch of a black hole jet has never been observed before in real time,” Meyer noted. “We think the outflow began earlier, when the X-rays increased prior to the radio flare, and the jet was screened from our view by hot gas until it broke out early last year.”
A paper exploring that possibility, led by Laha, is under review at The Astrophysical Journal. Both Meyer and Megan Masterson, a doctoral candidate at the Massachusetts Institute of Technology in Cambridge who also presented at the meeting, are co-authors.
Using XMM-Newton observations, Masterson found that the black hole exhibited extremely rapid X-ray variations between July 2022 and March 2024. During this period, the X-ray brightness repeatedly rose and fell by 10% every few minutes. Such changes, called millihertz quasiperiodic oscillations, are difficult to detect around supermassive black holes and have been observed in only a handful of systems to date.
“One way to produce these oscillations is with an object orbiting within the black hole’s accretion disk. In this scenario, each rise and fall of the X-rays represents one orbital cycle,” Masterson said.
If the fluctuations were caused by an orbiting mass, then the period would shorten as the object fell ever closer to the black hole’s event horizon, the point of no return. Orbiting masses generate ripples in space-time called gravitational waves. These waves drain away orbital energy, bringing the object closer to the black hole, increasing its speed, and shortening its orbital period.
Over two years, the fluctuation period dropped from 18 minutes to just 7 — the first-ever measurement of its kind around a supermassive black hole. If this represented an orbiting object, it was now moving at half the speed of light. Then something unexpected happened — the fluctuation period stabilized.
In this artist’s concept, matter is stripped from a white dwarf (sphere at lower right) orbiting within the innermost accretion disk surrounding 1ES 1927+654’s supermassive black hole. Astronomers developed this scenario to explain the evolution of rapid X-ray oscillations detected by ESA’s (European Space Agency) XMM-Newton satellite. ESA’s LISA (Laser Interferometer Space Antenna) mission, due to launch in the next decade, should be able to confirm the presence of an orbiting white dwarf by detecting the gravitational waves it produces. NASA/Aurore Simonnet, Sonoma State University “We were shocked by this at first,” Masterson explained. “But we realized that as the object moved closer to the black hole, its strong gravitational pull could begin to strip matter from the companion. This mass loss could offset the energy removed by gravitational waves, halting the companion’s inward motion.”
So what could this companion be? A small black hole would plunge straight in, and a normal star would quickly be torn apart by the tidal forces near the monster black hole. But the team found that a low-mass white dwarf — a stellar remnant about as large as Earth — could remain intact close to the black hole’s event horizon while shedding some of its matter. A paper led by Masterson summarizing these results will appear in the Feb. 13 edition of the journal Nature.
This model makes a key prediction, Masterson notes. If the black hole does have a white dwarf companion, the gravitational waves it produces will be detectable by LISA (Laser Interferometer Space Antenna), an ESA mission in partnership with NASA that is expected to launch in the next decade.
Download high-resolution images from NASA’s Scientific Visualization Studio
By Francis Reddy
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Media Contacts:
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Last Updated Jan 13, 2025 Related Terms
Active Galaxies Astrophysics Black Holes Galaxies, Stars, & Black Holes Goddard Space Flight Center Jet Propulsion Laboratory Neil Gehrels Swift Observatory NICER (Neutron star Interior Composition Explorer) NuSTAR (Nuclear Spectroscopic Telescope Array) Radio Astronomy Supermassive Black Holes The Universe White Dwarfs X-ray Astronomy XMM-Newton (X-ray Multi-Mirror Newton) View the full article
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By NASA
This illustration shows a red, early-universe dwarf galaxy that hosts a rapidly feeding black hole at its center. Using data from NASA’s James Webb Space Telescope and Chandra X-ray Observatory, a team of astronomers have discovered this low-mass supermassive black hole at the center of a galaxy just 1.5 billion years after the Big Bang. It is pulling in matter at a phenomenal rate — over 40 times the theoretical limit. While short lived, this black hole’s “feast” could help astronomers explain how supermassive black holes grew so quickly in the early universe.NOIRLab/NSF/AURA/J. da Silva/M. Zamani A rapidly feeding black hole at the center of a dwarf galaxy in the early universe, shown in this artist’s concept, may hold important clues to the evolution of supermassive black holes in general.
Using data from NASA’s James Webb Space Telescope and Chandra X-ray Observatory, a team of astronomers discovered this low-mass supermassive black hole just 1.5 billion years after the big bang. The black hole is pulling in matter at a phenomenal rate — over 40 times the theoretical limit. While short lived, this black hole’s “feast” could help astronomers explain how supermassive black holes grew so quickly in the early universe.
Supermassive black holes exist at the center of most galaxies, and modern telescopes continue to observe them at surprisingly early times in the universe’s evolution. It’s difficult to understand how these black holes were able to grow so big so rapidly. But with the discovery of a low-mass supermassive black hole feasting on material at an extreme rate so soon after the birth of the universe, astronomers now have valuable new insights into the mechanisms of rapidly growing black holes in the early universe.
The black hole, called LID-568, was hidden among thousands of objects in the Chandra X-ray Observatory’s COSMOS legacy survey, a catalog resulting from some 4.6 million Chandra observations. This population of galaxies is very bright in the X-ray light, but invisible in optical and previous near-infrared observations. By following up with Webb, astronomers could use the observatory’s unique infrared sensitivity to detect these faint counterpart emissions, which led to the discovery of the black hole.
The speed and size of these outflows led the team to infer that a substantial fraction of the mass growth of LID-568 may have occurred in a single episode of rapid accretion.
LID-568 appears to be feeding on matter at a rate 40 times its Eddington limit. This limit relates to the maximum amount of light that material surrounding a black hole can emit, as well as how fast it can absorb matter, such that its inward gravitational force and outward pressure generated from the heat of the compressed, infalling matter remain in balance.
These results provide new insights into the formation of supermassive black holes from smaller black hole “seeds,” which current theories suggest arise either from the death of the universe’s first stars (light seeds) or the direct collapse of gas clouds (heavy seeds). Until now, these theories lacked observational confirmation.
The new discovery suggests that “a significant portion of mass growth can occur during a single episode of rapid feeding, regardless of whether the black hole originated from a light or heavy seed,” said International Gemini Observatory/NSF NOIRLab astronomer Hyewon Suh, who led the research team.
A paper describing these results (“A super-Eddington-accreting black hole ~1.5 Gyr after the Big Bang observed with JWST”) appears in the journal Nature Astronomy.
About the Missions
NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
Read more from NASA’s Chandra X-ray Observatory.
Learn more about the Chandra X-ray Observatory and its mission here:
https://www.nasa.gov/chandra
https://chandra.si.edu
News Media Contact
Elizabeth Laundau
NASA Headquarters
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Lane Figueroa
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lane.e.figueroa@nasa.gov
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By NASA
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The American Institute of Aeronautics and Astronautics (AIAA) has named two distinguished engineers at NASA’s Glenn Research Center in Cleveland AIAA Associate Fellows.
The grade of Associate Fellow recognizes individuals who have accomplished or overseen important engineering or scientific work, done original work of outstanding merit, or have otherwise made outstanding contributions to the arts, sciences, or technology of aeronautics or astronautics. To be selected as an Associate Fellow, an individual must be an AIAA Senior Member in good standing, with at least 12 years of professional experience, and be recommended by three AIAA members.
L. Danielle KochCredit: NASA L. Danielle Koch, aerospace engineer, performs research and educational outreach at NASA Glenn. Her 34-year career at NASA has been dedicated to conducting research for safer, cleaner, and quieter aircraft engines; high-performance ventilation systems for spacecraft; and bio-inspired broadband acoustic absorbers. She has authored over 50 technical publications and has been granted three patents. Koch has been recognized for excellence in engineering and educational outreach with many awards, most recently named as one of the 2024 Women of Distinction by the Girl Scouts of Northeast Ohio.
Dr. Sam LeeCredit: NASA Dr. Sam Lee, a research engineer supporting the Aircraft Icing Branch, conducts research in NASA Glenn’s Icing Research Tunnel to study how ice builds up, or accretes, on aircraft surfaces. The results from the experiments are used to understand the physics of how ice accretes on aircraft during flight and to provide the validation data to develop computational tools to predict ice accretion. He also performs research on the effects of ice accretion on aircraft performance in aerodynamic wind tunnels. Lee has authored 17 conference papers and journal papers. He has contributed to the development of many future engineers and scientists as a mentor for NASA’s Explorer Scouts program and various college internship programs. Lee has been part of the Aircraft Icing Branch since 2002.
AIAA will formally honor and induct the class at the AIAA Associate Fellows Induction Ceremony and Dinner on Jan. 8, 2025, during the 2025 AIAA SciTech Forum in Orlando.
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