Notícies d'astronomia

In 2023, NASA Langley’s workforce brought imagination to reality with innovative technological development and a continued commitment to tackling some of the tough challenges that both NASA and the nation face.

NASA

At NASA, we aspire to know more, dig deeper, climb higher and along the way we are asking, ‘What if?’,” said NASA Langley Center Director Clayton P. Turner in an introductory message to Langley’s 2023 Annual Report. “Our inquisitive nature propels us on our mission to reach for new heights and reveal the unknown for the benefit of humankind.”

All year, the Langley workforce pondered and planned for a future alongside self-flying drones, aircraft with reduced emissions, air travel that benefits from greater fuel efficiency and space exploration assisted by inflatable heat shields that could give us the ability to carry greater payloads than ever before.

“We invite you to explore all that NASA’s Langley Research Center has to offer — our amazing people, unique capabilities, and legacy of success,” Turner said in his introduction.

Use this link to explore the 2023 Annual Report for NASA’s Langley Research Center.

NASA

At NASA’s Langley Research Center, we are proud of our world-renowned role in innovating and improving the way we fly, explore, and understand our universe.” said NASA Langley leadership in an introductory message to Langley’s 2024 Annual Report. “The passion, dedication, and expertise of our workforce is bringing solutions to the nation’s toughest challenges in Aeronautics, Space Exploration, and Earth Science research.”

Featured achievements include work on NASA’s X-59 supersonic experimental aircraft, the largest air quality campaign to ever collaborate with countries across Asia and an autonomous robotic manipulation system that will one day provide NASA with a lunar moving crew.

Use this link to explore the 2024 Annual Report for NASA’s Langley Research Center.

NASA’s SPHEREx space observatory was photographed at BAE Systems in Boulder, Colorado, in November 2024 after completing environmental testing. The spacecraft’s three concentric cones help direct heat and light away from the telescope and other components, keeping them cool. Credit: BAE Systems

NASA will host a news conference at 12 p.m. EST Friday, Jan. 31, to discuss a new telescope that will improve our understanding of how the universe evolved and search for key ingredients for life in our galaxy.

Agency experts will preview NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) mission, which will help scientists better understand the structure of the universe, how galaxies form and evolve, and the origins and abundance of water. Launch is targeted for no earlier than Thursday, Feb. 27.

The news conference will be hosted at the agency’s Jet Propulsion Laboratory in Southern California. Watch live on NASA+, as well as JPL’s X and YouTube channels. Learn how to watch NASA content through a variety of platforms, including social media.

Laurie Leshin, director, NASA JPL, will provide opening remarks. Additional briefing participants include:

• Shawn Domagal-Goldman, acting director, Astrophysics Division, NASA Headquarters
• James Fanson, project manager, SPHEREx, NASA JPL
• Beth Fabinsky, deputy project manager, SPHEREx, NASA JPL  
• Jamie Bock, principal investigator, SPHEREx, Caltech
• Cesar Marin, SPHEREx integration engineer, Launch Services Program, NASA’s Kennedy Space Center in Florida

To ask questions by phone, members of the media must RSVP no later than two hours before the start of the event to: rexana.v.vizza@jpl.nasa.gov. NASA’s media accreditation policy is available online. Questions also can be asked on social media during the briefing using #AskNASA.

The SPHEREx observatory will survey the entire celestial sky in near-infrared light to help answer cosmic questions involving the birth of the universe, and the subsequent development of galaxies. It also will search for ices of water and organic molecules — essentials for life as we know it — in regions where stars are born from gas and dust, as well as disks around stars where new planets could be forming. Astronomers will use the mission to gather data on more than 450 million galaxies, as well as more than 100 million stars in our own Milky Way galaxy.

The space observatory will share its ride on a SpaceX Falcon 9 rocket with NASA’s PUNCH (Polarimeter to Unify the Corona and Heliosphere) mission, which will lift off from Launch Complex 4E at Vandenberg Space Force Base in Central California. 

The SPHEREx mission is managed by NASA JPL for the agency’s Astrophysics Division within the Science Mission Directorate at NASA Headquarters in Washington. The principal investigator is based at Caltech in Pasadena, California, which manages NASA JPL for the agency. 

The spacecraft is supplied by BAE Systems. The Korea Astronomy and Space Science Institute contributed the non-flight cryogenic test chamber. Mission data will be publicly available through IPAC at Caltech.

For more information about the mission, visit:

https://nasa.gov/spherex

-end-

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

Val Gratias / Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-6215 / 626-808-2469
valerie.m.gratias@jpl.nasa.gov / calla.e.cofield@jpl.nasa.gov

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Details Last Updated Jan 27, 2025 EditorJessica TaveauLocationNASA Headquarters Related Terms

• SPHEREx (Spectro-Photometer for the History of the Universe and Ices Explorer)
• Astrophysics Division
• Jet Propulsion Laboratory
• Kennedy Space Center
• Launch Services Program
• Polarimeter to Unify the Corona and Heliosphere (PUNCH)
• Science Mission Directorate

Reducing reliance on resupply missions

Resupply of life support elements such as air, water, food, clothing, and hygiene items will be impractical on missions to the Moon and beyond. This research assessed current use and resupply of these elements on the International Space Station and outlines technologies needed for sustained human presence in space, such as 3D printing maintenance parts, systems for laundering clothes, and improved recovery and recycling of elements.

Researchers analyzed the types and mass of elements supplied from Earth to the station and astronaut feedback from various studies and interviews. The paper also used data from ISS Internal Environments, a wide-ranging investigation that samples various aspects of the space station environment in support of many types of research.

Japan Aerospace Exploration Agency astronaut Satoshi Furukawa exercises on the station’s treadmill. Astronauts currently have no way to launder clothes in space.NASA

Verifying a technique for analyzing emulsions

This paper presents a review of examining the behavior of emulsions (suspensions of particles in a liquid) in microgravity using a technique called diffusing wave spectroscopy. Results offer insights that could support development of technologies to improve living environments and foods for crew members on future missions.

FSL Soft Matter Dynamics – PASTA studied the dynamics of droplets in emulsions. Accurate study and characterization of the effects of additives on emulsion stability is possible in microgravity. Emulsions have applications in foods, cosmetics, pharmaceuticals, fuels, paints and coatings, chemical processing, and materials.

European Space Agency astronaut Samantha Cristoforetti exchanges samples for the FSL Soft Matter Dynamics-PASTA investigation.NASA

EEG measurements and predicting cognitive changes in spaceflight

Researchers used an electroencephalogram (EEG) to measure brainwave activity during a relaxed, wakeful state in crew members and found no significant differences before, during, and after flight. These types of measurements could serve as biomarkers of brain health status, helping to predict changes in cognitive performance and the need for prevention and countermeasure strategies during future missions.

Studies have shown that spaceflight can affect key cognitive and motor skills such as task management, attention, and movement speed and accuracy. Neurowellness in Space Ax-1 tested using a portable, easy to use EEG headset to measure ongoing and task-related brain activity in microgravity. The data could help predict and monitor neural changes on future space missions.

The 11-person crew aboard the station in April 2022 included Axiom Mission 1 astronauts (center row from left) Mark Pathy, Eytan Stibbe, Larry Conner, and Michael Lopez-Alegria.NASA

An inquisitive sandhill crane approaches the photographer near the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on March 24, 2021. Kennedy shares space with the Merritt Island National Wildlife refuge, which is home to more than 1,000 species of plants, 117 species of fish, 68 amphibians and reptiles, 330 birds, and 31 different mammals. The refuge provides a favorable environment for sandhill cranes as it contains shallow freshwater habitats for nesting, along with a variety of vegetation and prey to feed on.

NASA/Ben Smegelsky

A NASA photographer took this portrait of a curious sandhill crane on March 24, 2021, near the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida. Sandhill cranes are just one of the hundreds of types of birds that call the Merritt Island National Wildlife Refuge, which shares space with NASA Kennedy, their home.

See more photos of birds at NASA Kennedy.

Image credit: NASA/Ben Smegelsky

Perseus Cluster: X-ray: NASA/CXC/SAO/V. Olivares et al.; Optical/IR: DSS; H-alpha: CFHT/SITELLE; Centaurus Cluster: X-ray: NASA/CXC/SAO/V. Olivaresi et al.; Optical/IR: NASA/ESA/STScI; H-alpha: ESO/VLT/MUSE; Image Processing: NASA/CXC/SAO/N. Wolk

Astronomers have taken a crucial step in showing that the most massive black holes in the universe can create their own meals. Data from NASA’s Chandra X-ray Observatory and the Very Large Telescope (VLT) provide new evidence that outbursts from black holes can help cool down gas to feed themselves.

This study was based on observations of seven clusters of galaxies. The centers of galaxy clusters contain the universe’s most massive galaxies, which harbor huge black holes with masses ranging from millions to tens of billions of times that of the Sun. Jets from these black holes are driven by the black holes feasting on gas.

These images show two of the galaxy clusters in the study, the Perseus Cluster and the Centaurus Cluster. Chandra data represented in blue reveals X-rays from filaments of hot gas, and data from the VLT, an optical telescope in Chile, shows cooler filaments in red.

The results support a model where outbursts from the black holes trigger hot gas to cool and form narrow filaments of warm gas. Turbulence in the gas also plays an important role in this triggering process.

According to this model, some of the warm gas in these filaments should then flow into the centers of the galaxies to feed the black holes, causing an outburst. The outburst causes more gas to cool and feed the black holes, leading to further outbursts.

This model predicts there will be a relationship between the brightness of filaments of hot and warm gas in the centers of galaxy clusters. More specifically, in regions where the hot gas is brighter, the warm gas should also be brighter. The team of astronomers has, for the first time, discovered such a relationship, giving critical support for the model.

This result also provides new understanding of these gas-filled filaments, which are important not just for feeding black holes but also for causing new stars to form. This advance was made possible by an innovative technique that isolates the hot filaments in the Chandra X-ray data from other structures, including large cavities in the hot gas created by the black hole’s jets.

The newly found relationship for these filaments shows remarkable similarity to the one found in the tails of jellyfish galaxies, which have had gas stripped away from them as they travel through surrounding gas, forming long tails. This similarity reveals an unexpected cosmic connection between the two objects and implies a similar process is occurring in these objects.

This work was led by Valeria Olivares from the University of Santiago de Chile, and was published Monday in Nature Astronomy. The study brought together international experts in optical and X-ray observations and simulations from the United States, Chile, Australia, Canada, and Italy. The work relied on the capabilities of the MUSE (Multi Unit Spectroscopic Explorer) instrument on the VLT, which generates 3D views of the universe.

NASA’s Marshall Space Flight Center in Huntsville, Alabama, 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.

Learn more about the Chandra X-ray Observatory and its mission here:

https://www.nasa.gov/chandra

https://chandra.si.edu

Visual Description

This release features composite images shown side-by-side of two different galaxy clusters, each with a central black hole surrounded by patches and filaments of gas. The galaxy clusters, known as Perseus and Centaurus, are two of seven galaxy clusters observed as part of an international study led by the University of Santiago de Chile.

In each image, a patch of purple with neon pink veins floats in the blackness of space, surrounded by flecks of light. At the center of each patch is a glowing, bright white dot. The bright white dots are black holes. The purple patches represent hot X-ray gas, and the neon pink veins represent filaments of warm gas. According to the model published in the study, jets from the black holes impact the hot X-ray gas. This gas cools into warm filaments, with some warm gas flowing back into the black hole. The return flow of warm gas causes jets to again cool the hot gas, triggering the cycle once again.

While the images of the two galaxy clusters are broadly similar, there are significant visual differences. In the image of the Perseus Cluster on the left, the surrounding flecks of light are larger and brighter, making the individual galaxies they represent easier to discern. Here, the purple gas has a blue tint, and the hot pink filaments appear solid, as if rendered with quivering strokes of a paintbrush. In the image of the Centaurus Cluster on the right, the purple gas appears softer, with a more diffuse quality. The filaments are rendered in more detail, with feathery edges, and gradation in color ranging from pale pink to neon red.

News Media Contact

Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
mwatzke@cfa.harvard.edu

Lane Figueroa
Marshall Space Flight Center, Huntsville, Alabama
256-544-0034
lane.e.figueroa@nasa.gov

This NASA/ESA Hubble Space Telescope image features a dusty yet sparkling scene from one of the Milky Way’s satellite galaxies, the Large Magellanic Cloud. The Large Magellanic Cloud is a dwarf galaxy situated about 160,000 light-years away in the constellations Dorado and Mensa.

This is an artist's concept of a two-person Gemini spacecraft in flight, showing a cutaway view. The Gemini program was designed as a bridge between the Mercury and Apollo programs.

NASA astronaut and Expedition 72 commander Suni Williams is pictured during a spacewalk outside the International Space Station where she replaced a rate gyro assembly that helps maintain the orientation of the orbital outpost.

The Martin Luther King, Jr. Memorial is seen in the foreground with the Washington Monument in the background, Sunday, Jan. 5, 2025, in Washington. The memorial covers four acres and includes the Stone of Hope, a granite statue of civil rights movement leader Martin Luther King Jr. carved by sculptor Lei Yixin.

Released on Nov. 3, 2023, in honor of Jupiter reaching opposition, which occurs when the planet and the Sun are in opposite sides of the sky, this view of the gas giant planet includes the iconic, massive storm called the “Great Red Spot.”

Chief of aerodynamics Elton W. Miller ponders the future of the Sperry M-1 Messenger, the first full-scale airplane tested in the Propeller Research Tunnel. Miller was one of the designers of the Propeller Research Tunnel.

A visitor takes a picture of a sculpture of an adult Alamosaurus wearing solar glasses outside of The Children’s Museum of Indianapolis, Saturday, April 6, 2024, in Indianapolis, Ind. On Monday, April 8, 2024, a total solar eclipse swept across a narrow portion of the North American continent from Mexico’s Pacific coast to the Atlantic coast of Newfoundland, Canada.

A color enhancement of a far-ultraviolet photo of Earth taken by astronaut John W. Young, commander, with the ultraviolet camera on April 21, 1972. The original black-and-white photo was printed on Agfacontour film three times, each exposure recording only one light level. The three light levels were then colored blue (dimmest), green (next brightest), and red (brightest).

On Jan. 10, 2025, NASA astronaut Don Pettit posted two images of the Los Angeles fires from the International Space Station.

"As a young college student, it was the first time I ever faced [this situation], and it buckled me. It set me back until I realized that I could do it and that my worth wasn't based on what someone else thought of me or my abilities…If I had pulled myself out of that STEM major, I would never have been managing a technology demonstration program for NASA that launched ten technologies into space.” – Tawnya Plummer Laughinghouse, Director of the Materials and Processes Laboratory, Engineering Directorate, NASA’s Marshall Space Flight Center

The New York-based artist team Geraluz, left, and WERC, right, and their son Amaru Alvarez, 5, pose for picture with the mural “To the Moon, and Back” by the artist team that was created as part of the reimagined NASA Art Program, Tuesday, September 24, 2024, at 350 Hudson Street in New York City. The murals use geometrical patterns to invite deeper reflection on the exploration, creativity, and connection with the cosmos.

A test subject being suited up for studies on the Reduced Gravity Walking Simulator located in the hangar at Langley Research Center. The initial version of this simulator was located inside the hangar. Later a larger version would be located at the Lunar Landing Facility.

From left, CSA (Canadian Space Agency) astronaut Jenni Gibbons, NASA astronaut Andre Douglas, CSA astronaut Jeremy Hansen, and NASA astronauts Christina Koch, Victor Glover, and Reid Wiseman participate in a media day event on Monday, Dec. 16, 2024, inside the Vehicle Assembly Building at the agency’s Kennedy Space Center in Florida.