Hubble Spots a Galaxy Shrouded by Stars

This NASA/ESA Hubble Space Telescope image shows a densely packed field of stars laid upon a background of dust, gas, and light from more distant celestial objects. There are so many stars in this image’s field of view that it may be a little tricky to discern that you are in fact looking at a galaxy. Known as ESO 245-5, this galaxy may be harder to recognize because of its apparent lack of structure, which contrasts sharply with Hubble’s spectacular images of spiral galaxies that hold seemingly ordered spiral arms of stars, gas, and dust.

ESO 245-5 is an IB(s)m type of galaxy under the De Vaucouleurs galaxy classification system. This designation means that the galaxy is irregular (I) with no ordered structure. It is also barred (B) meaning it holds a dense bar of stars that crosses through its center. The third term ((s)) indicates that it has a slight spiral structure, while the last term (m) means it is a type of galaxy similar to the Large and Small Magellanic Clouds that are irregular satellite galaxies of the Milky Way. ESO 245-5 is a relatively close neighbor of the Milky Way. It is located some of 15 million light-years from Earth in the constellation Phoenix.

Text credit: European Space Agency (ESA)

Media Contact:

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

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NASA Awards Inaugural Grants to Support Emerging Research Institutions

NASA has awarded $3.7 million to 11 teams to support new collaborations between the agency and United States institutions not historically part of the agency’s research enterprise. These are the first awards given through a new program from the agency’s Science Mission Directorate (SMD) to improve diversity, equity, inclusion, and accessibility in the science and engineering communities, as well as NASA’s workforce.

“As the agency continues to build relationships with under-resourced institutions through initiatives like the bridge program, we are intentionally increasing equitable access to NASA for the best and brightest talents in our nation,” said Shahra Lambert, NASA senior advisor for engagement. “These partnerships will help NASA develop a diverse and capable workforce to further our understanding of the cosmos.”

NASA’s SMD Bridge Program provides seed funding for research projects that will build strong foundations for long-lasting relationships with the agency. The projects offer hands-on training and mentorship for students, as well as new research opportunities for faculty, to help science and engineering students transition into graduate schools, employment by NASA, or science, technology, engineering, and math careers generally.

The teams are led by faculty at institutions that represent new collaborations for NASA. These include Hispanic-serving institutions, Historically Black Colleges and Universities, Asian American and Native American Pacific Islander-serving institutions, and primarily undergraduate institutions. The research projects connect these institutions to seven NASA centers and could impact more than 100 students.

“We applaud this inaugural cohort of grant recipients for their innovative research projects, which will make important connections between students, faculty, and NASA,” said Michael New, Science Mission Directorate deputy associate administrator for research at NASA Headquarters. “These awards are a first and important step for the SMD Bridge Program in supporting long-term relationships toward creating a more diverse and robust STEM workforce.”

There is an additional opportunity to apply for seed funding through the SMD Bridge Program. Applications are open until Friday, March 29.

The following projects were selected as the first cohort to receive seed funding:

“Diversifying Student Pipelines in STEM: Environmental Pollution Reduction Inspired by Planetary Science”

This project, a collaboration that brings California State University, Los Angeles, together with NASA’s Jet Propulsion Laboratory in Southern California, and California State Polytechnic University, Pomona, draws from the field of planetary science to address environmental pollution.

“FireSage: SJSU-NASA ARC Bridge Seed Program”

FireSage is a collaboration between San Jose State University’s Wildfire Interdisciplinary Research Center and the Earth Science Division at NASA’s Ames Research Center in California’s Silicon Valley. It engages students in a computing, artificial intelligence, and machine learning research project and training activities in wildfire science.

“Hampton University STEM Experience with NASA Langley Research Center Doppler Aerosol Wind Lidar”

This collaboration between Hampton University and NASA’s Langley Research Center in Hampton, Virginia, offers a foundation in the advancement of planetary boundary layer studies with Lidar remote sensing.

“Development of Antireflection Coatings for Future NASA Missions”

This project is a collaboration between Delaware State University and NASA Goddard, working with transparent, electrically conductive films to design and produce an environmentally durable anti-reflection coating for guidance, navigation, and control Lidar.

“CUBES: Capacity Building Using CubeSats for Earth Science”

This collaboration between Tuskegee University, the Laboratory for Atmospheric Science and Physics at University of Colorado, and NASA Ames uses CubeSats to provide faculty and students with experience designing and executing science mission flight projects.

“Space Materials and Microbiome Research: A Bridge to Future JSC Workforce”

In this project, the University of Houston-Clear Lake collaborates with NASA’s Johnson Space Center in Houston. The project’s Composite Materials track will develop a protective nanocomposite shield for spacecraft materials, while the Microbiome track will create a comprehensive library of draft bacterial genomes.

“The HALOQUEST: Halobacterium Astrobiological Laboratory for Observing and Questioning Extraterrestrial Signatures and Traits Project”

This collaboration between California State University, Northridge, and NASA JPL will study Halobacterium salinarum NRC-1 grown under simulated stressful environmental conditions, which could help understand possibilities for life on other planets.

“Observations of Ice-Water and Isotopes Using Mid-Infrared Laser Heterodyne Radiometer LIDAR”

In collaboration with NASA Goddard, Delaware State University will develop Earth science, planetary exploration, and sensing technologies, including a lunar rover payload with instruments to simultaneously detect and correlate water isotopes with other trace gas species.

“Application of Remote Sensing for Predicting Mosquito-Borne Disease Outbreaks”

This project is a collaboration between Southern Nazarene University and NASA JPL to identify areas at risk for mosquito-borne disease outbreaks using remote sensing data.

“Building a Diverse, Sustainable, and Robust Undergraduate-to-Graduate STEM Network through Inter-Institutional, Interdisciplinary Research Collaborations in Complex Fluids/Soft Matter”

This project is a collaboration between Colorado Mesa University and NASA’s Glenn Research Center in Cleveland to strengthen and grow a research, education, and training network centered around problems in complex fluids and soft matter, with initial emphasis on heat transfer and multiphase flows.

“Additive Manufacturing of Electronics for NASA Applications”

This project, a collaboration between Florida A&M University and NASA’s Marshall Space Flight Center in Huntsville, Alabama, and NASA Goddard, will explore technology solutions through additive manufacturing approaches to manufacture strain and gas sensors.

Learn more about the SMD Bridge Program at:

https://science.nasa.gov/researchers/smd-bridge-program/

-end-

Alise Fisher
Headquarters, Washington
202-358-2546a
alise.m.fisher@nasa.gov

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Roxana Bardan

Skylab 4 Recovery Ends Program

The crewmen of the third and final manned Skylab mission relax on the USS New Orleans, prime recovery ship for their mission, about an hour after their Command Module splashed down at 10:17 a.m. (CDT), Feb. 8, 1974. The splashdown, which occurred 176 statute miles from San Diego, ended 84 record-setting days of flight activity aboard the Skylab space station cluster in Earth orbit.

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Gary Daines

NASA’s New Experimental Antenna Tracks Deep Space Laser

Capable of receiving both radio frequency and optical signals, the DSN’s hybrid antenna has tracked and decoded the downlink laser from DSOC, aboard NASA’s Psyche mission.

An experimental antenna has received both radio frequency and near-infrared laser signals from NASA’s Psyche spacecraft as it travels through deep space. This shows it’s possible for the giant dish antennas of NASA’s Deep Space Network (DSN), which communicate with spacecraft via radio waves, to be retrofitted for optical, or laser, communications.

By packing more data into transmissions, optical communication will enable new space exploration capabilities while supporting the DSN as demand on the network grows.

The 34-meter (112-foot) radio-frequency-optical-hybrid antenna, called Deep Space Station 13, has tracked the downlink laser from NASA’s Deep Space Optical Communications (DSOC) technology demonstration since November 2023. The tech demo’s flight laser transceiver is riding with the agency’s Psyche spacecraft, which launched on Oct. 13, 2023.

The hybrid antenna is located at the DSN’s Goldstone Deep Space Communications Complex, near Barstow, California, and isn’t part of the DSOC experiment. The DSN, DSOC, and Psyche are managed by NASA’s Jet Propulsion Laboratory in Southern California.

“Our hybrid antenna has been able to successfully and reliably lock onto and track the DSOC downlink since shortly after the tech demo launched,” said Amy Smith, DSN deputy manager at JPL. “It also received Psyche’s radio frequency signal, so we have demonstrated synchronous radio and optical frequency deep space communications for the first time.”

In late 2023, the hybrid antenna downlinked data from 20 million miles (32 million kilometers) away at a rate of 15.63 megabits per second – about 40 times faster than radio frequency communications at that distance. On Jan. 1, 2024, the antenna downlinked a team photograph that had been uploaded to DSOC before Psyche’s launch.

Two for One

In order to detect the laser’s photons (quantum particles of light), seven ultra-precise segmented mirrors were attached to the inside of the hybrid antenna’s curved surface. Resembling the hexagonal mirrors of NASA’s James Webb Space Telescope, these segments mimic the light-collecting aperture of a 3.3-foot (1-meter) aperture telescope. As the laser photons arrive at the antenna, each mirror reflects the photons and precisely redirects them into a high-exposure camera attached to the antenna’s subreflector suspended above the center of the dish.

The laser signal collected by the camera is then transmitted through optical fiber that feeds into a cryogenically cooled semiconducting nanowire single photon detector. Designed and built by JPL’s Microdevices Laboratory, the detector is identical to the one used at Caltech’s Palomar Observatory, in San Diego County, California, which acts as DSOC’s downlink ground station.

“It’s a high-tolerance optical system built on a 34-meter flexible structure,” said Barzia Tehrani, communications ground systems deputy manager and delivery manager for the hybrid antenna at JPL. “We use a system of mirrors, precise sensors, and cameras to actively align and direct laser from deep space into a fiber reaching the detector.”

Tehrani hopes the antenna will be sensitive enough to detect the laser signal sent from Mars at its farthest point from Earth (2 ½ times the distance from the Sun to Earth). Psyche will be at that distance in June on its way to the main asteroid belt between Mars and Jupiter to investigate the metal-rich asteroid Psyche.

The seven-segment reflector on the antenna is a proof of concept for a scaled-up and more powerful version with 64 segments – the equivalent of a 26-foot (8-meter) aperture telescope – that could be used in the future.

An Infrastructure Solution

DSOC is paving the way for higher-data-rate communications capable of transmitting complex scientific information, video, and high-definition imagery in support of humanity’s next giant leap: sending humans to Mars. The tech demo recently streamed the first ultra-high-definition video from deep space at record-setting bitrates.

Retrofitting radio frequency antennas with optical terminals and constructing purpose-built hybrid antennas could be a solution to the current lack of a dedicated optical ground infrastructure. The DSN has 14 dishes distributed across facilities in California, Madrid, and Canberra, Australia. Hybrid antennas could rely on optical communications to receive high volumes of data and use radio frequencies for less bandwidth-intensive data, such as telemetry (health and positional information).

“For decades, we have been adding new radio frequencies to the DSN’s giant antennas located around the globe, so the most feasible next step is to include optical frequencies,” said Tehrani. “We can have one asset doing two things at the same time; converting our communication roads into highways and saving time, money, and resources.”

More About the Mission

DSOC is the latest in a series of optical communication demonstrations funded by NASA’s Technology Demonstration Missions (TDM) program and the agency’s Space Communications and Navigation (SCaN) program. JPL, a division of Caltech in Pasadena, California, manages DSOC for TDM within NASA’s Space Technology Mission Directorate and SCaN within the agency’s Space Operations Mission Directorate.

For more about NASA’s optical communications projects, visit:

https://www.nasa.gov/lasercomms/

News Media Contact

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

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Telescopes Show the Milky Way’s Black Hole is Ready for a Kick

This artist’s illustration depicts the findings of a new study about the supermassive black hole at the center of our galaxy called Sagittarius A* (abbreviated as Sgr A*). As reported in our latest press release, this result found that Sgr A* is spinning so quickly that it is warping spacetime — that is, time and the three dimensions of space — so that it can look more like a football.

These results were made with NASA’s Chandra X-ray Observatory and the NSF’s Karl G. Jansky Very Large Array (VLA). A team of researchers applied a new method that uses X-ray and radio data to determine how quickly Sgr A* is spinning based on how material is flowing towards and away from the black hole. They found Sgr A* is spinning with an angular velocity that is about 60% of the maximum possible value, and with an angular momentum of about 90% of the maximum possible value.

Black holes have two fundamental properties: their mass (how much they weigh) and their spin (how quickly they rotate). Determining either of these two values tells scientists a great deal about any black hole and how it behaves. In the past, astronomers made several other estimates of Sgr A*’s rotation speed using different techniques, with results ranging from Sgr A* not spinning at all to it spinning at almost the maximum rate.

The new study suggests that Sgr A* is, in fact, spinning very rapidly, which causes the spacetime around it to be squashed down. The illustration shows a cross-section of Sgr A* and material swirling around it in a disk. The black sphere in the center represents the so-called event horizon of the black hole, the point of no return from which nothing, not even light, can escape.

Looking at the spinning black hole from the side, as depicted in this illustration, the surrounding spacetime is shaped like a football. The faster the spin the flatter the football.

The yellow-orange material to either side represents gas swirling around Sgr A*. This material inevitably plunges towards the black hole and crosses the event horizon once it falls inside the football shape. The area inside the football shape but outside the event horizon is therefore depicted as a cavity. The blue blobs show jets firing away from the poles of the spinning black hole. Looking down on the black hole from the top, along the barrel of the jet, spacetime is a circular shape.

A black hole’s spin can act as an important source of energy. Spinning supermassive black holes produce collimated outflows such as jets when their spin energy is extracted, which requires that there is at least some matter in the vicinity of the black hole. Because of limited fuel around Sgr A*, this black hole has been relatively quiet in recent millennia with relatively weak jets. This work, however, shows that this could change if the amount of material in the vicinity of Sgr A* increases.

To determine the spin of Sgr A*, the authors used an empirically based technique referred to as the “outflow method” that details the relationship between the spin of the black hole and its mass, the properties of the matter near the black hole, and the outflow properties. The collimated outflow produces the radio waves, while the disk of gas surrounding the black hole is responsible for the X-ray emission. Using this method, the researchers combined data from Chandra and the VLA with an independent estimate of the black hole’s mass from other telescopes to constrain the black hole’s spin.

The paper describing these results led by Ruth Daly (Penn State University) is published in the January 2024 issue of the Monthly Notices of the Royal Astronomical Society and appears online at https://ui.adsabs.harvard.edu/abs/2024MNRAS.527..428D/abstract. The other authors are Biny Sebastian (University of Manitoba, Canada), Megan Donahue (Michigan State University), Christopher O’Dea (University of Manitoba), Daryl Haggard (McGill University) and Anan Lu (McGill University).

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.

Read more from NASA’s Chandra X-ray Observatory.

For more Chandra images, multimedia and related materials, visit:

https://www.nasa.gov/mission/chandra-x-ray-observatory/

Visual Description:

This artist’s illustration shows a cross-section of Sagittarius A*, pronounced as “SAJ-ee-TARE-ee-us A-star”, the supermassive black hole near the center of our Milky Way galaxy.

In the middle of the image, the spinning, circular black hole is presented from the side in black. The shape of the surrounding spacetime, pictured in shades of dark yellow, looks as though it has been squashed down, thus resembling the shape of an American football. The swirling gas that surrounds Sagittarius A* is presented on either side of the black hole, within a rectangular-shaped dotted line, indicating the representation is a cross-section view.

The background of the image contains a multitude of faint stars, peeking out from within brooding, dark red, indistinct clouds.

News Media Contact

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998

Jonathan Deal
Marshall Space Flight Center
Huntsville, Ala.
256-544-0034

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Lee Mohon