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By NASA
Hubble Space Telescope Home Hubble Observes a Peculiar… Missions Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Hubble News Archive Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts E-books Lithographs Fact Sheets Glossary Posters Hubble on the NASA App More Online Activities 2 min read
Hubble Observes a Peculiar Galaxy Shape
This NASA/ESA Hubble Space Telescope image features the galaxy, NGC 4694. ESA/Hubble & NASA, D. Thilker This NASA/ESA Hubble Space Telescope image reveals the galaxy, NGC 4694. Most galaxies fall into one of two basic types. Spiral galaxies are young and energetic, filled with the gas needed to form new stars and sporting spiral arms that host these hot, bright youths. Elliptical galaxies have a much more pedestrian look, and their light comes from a uniform population of older and redder stars. But some galaxies require in-depth study to classify their type: such is the case with NGC 4694, a galaxy located 54 million light-years from Earth in the Virgo galaxy cluster.
NGC 4694 has a smooth-looking, armless disk which — like an elliptical galaxy — is nearly devoid of star formation. Yet its stellar population is still relatively young and new stars are actively forming in its core, powering its bright center and giving it a markedly different stellar profile from that of a classic elliptical. Although elliptical galaxies often host significant quantities of dust, they generally do not hold the fuel needed to form new stars. NGC 4694 is filled with the hydrogen gas and dust normally seen in a young and sprightly spiral, and a huge cloud of invisible hydrogen gas surrounds the galaxy.
As this Hubble image reveals, NGC 4694’s dust forms chaotic structures that indicate some kind of disturbance. It turns out that the cloud of hydrogen gas around NGC 4694 forms a long bridge to a nearby, faint dwarf galaxy named VCC 2062. The two galaxies have undergone a violent collision, and the larger NGC 4694 is accreting gas from the smaller galaxy. This collision helped give NGC 4694 its peculiar shape and star-forming activity that classify it as a lenticular galaxy. Lenticular galaxies lack the unmistakable arms of a spiral, but still have a central bulge and disk. They also hold more star-forming gas than an elliptical galaxy. Some galaxies, like NGC 4694, aren’t as easy to categorize as one type or the other. It takes a bit more digging to reveal their true nature, and thanks to Hubble, we have the ability to uncover their secrets.
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Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
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Last Updated Oct 04, 2024 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Hubble Space Telescope Lenticular Galaxies Missions The Universe Keep Exploring Discover More Topics From Hubble
Hubble Space Telescope
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Hubble on the NASA App
Hubble’s Galaxies
Hubble by the Numbers
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By European Space Agency
In a final test before its shipping to its Indian launch site, ESA’s eclipse-making double-satellite Proba-3 mission has received commands from its science team and transmitted images back, exactly as it will operate in orbit.
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By NASA
During National Disability Employment Awareness Month, we celebrate the thousands of employees living with disabilities who contribute to NASA’s mission. By sharing their stories, we highlight the impact people with disabilities have on our organization and the vital role they play in fostering an inclusive workforce at NASA.
Meghan Daley sits in the Orbiter Processing Facility at NASA’s Kennedy Space Center in Florida during the final days of the Space Shuttle Program. Meghan Daley has spent nearly two decades blazing new trails in robotics. As a project manager in NASA’s Engineering, Software Robotics, and Simulation Division at Johnson Space Center in Houston, she is building simulations that will shape the future of space exploration.
From training astronauts with advanced robotic tools to collaborating with the Department of Defense on research simulations, Daley’s work is transforming how humans interact with space, ensuring that every mission is set up for success.
Daley oversees key programs at Johnson, including the Generic On-Orbit Robotic Trainer (GROOT), the Robotic OnBoard Trainer, and Dynamics Skills Trainers. These tools are vital to NASA’s mission and are used in both ground-based simulations and real-time space operations.
One of Daley’s proudest achievements is launching GROOT, a simulation system that trains astronauts in a variety of robotic operations. From handling the Canadarm2 for spacecraft docking to servicing satellites, GROOT prepares astronauts for tasks like performing maintenance, assembling structures in space, managing cargo, and even coordinating multiple robotic systems.
The tool also supports astronauts in mastering robotic inspections, autonomous operations, and emergency procedures, making it indispensable for missions to the Moon and Mars.
During a visit by Gen. John W. Raymond to the Systems Engineering Simulator, the general requested an outdated rendezvous and proximity operations simulation for the United States Space Force.
Recognizing the limitations of the old system and knowing her team’s capabilities, Daley proposed building a new simulation from scratch to meet their needs. In 2019, GROOT was born and continues to be a critical asset in NASA’s training toolkit.
United States Space Force Vice Chief of Space Operations Gen. David D. Thompson observes a demonstration of the Generic On-Orbit Robotic Trainer alongside NASA astronauts and crew members. For Daley, celebrating her identity and culture in the workplace is about advocacy and education. She is passionate about using her voice to promote awareness and understanding, not just for her own experience, but for the benefit of all.
“Being a woman in engineering is extremely difficult. However, being a woman with a disability in engineering is even harder,” Daley said. “I have learned how important it is to communicate your ideas, questions, and concerns.”
When reflecting on her career, Daley says she cannot pick a favorite project. Each one—from Orion to Gateway to the International Space Station and space shuttle—has deepened her understanding of NASA’s vision.
The Robotic OnBoard Trainer onboard the International Space Station in the U.S. Destiny Laboratory. As Daley looks to the future of robotics and human spaceflight, she remains optimistic and passionate about inspiring the next generation of explorers.
“Keep your hope and don’t be afraid to ask questions because that is how you learn and become a leader!” she said.
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By NASA
An artist’s concept of NASA’s Europa Clipper spacecraft. Credits: NASA/JPL-Caltech Lee esta nota de prensa en español aquí.
NASA will provide live coverage of prelaunch and launch activities for Europa Clipper, the agency’s mission to explore Jupiter’s icy moon Europa. NASA is targeting launch at 12:31 p.m. EDT Thursday, Oct. 10, on a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Beyond Earth, Jupiter’s moon Europa is considered one of the solar system’s most promising potentially habitable environments. After an approximately 1.8-billion-mile journey, Europa Clipper will enter orbit around Jupiter in April 2030, where the spacecraft will conduct a detailed survey of Europa to determine whether the icy world could have conditions suitable for life. Europa Clipper is the largest spacecraft NASA has ever developed for a planetary mission. It carries a suite of nine instruments along with a gravity experiment that will investigate an ocean beneath Europa’s surface, which scientists believe contains twice as much liquid water as Earth’s oceans.
For a schedule of live events and the platforms they’ll stream on, visit:
https://go.nasa.gov/europaclipperlive
The deadline for media accreditation for in-person coverage of this launch has passed. NASA’s media credentialing policy is available online. For questions about media accreditation, please email: ksc-media-accreditat@mail.nasa.gov.
NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations):
Tuesday, Oct. 8
1 p.m. – In-person, one-on-one interviews, open to media credentialed for this launch.
3:30 p.m. – NASA’s Europa Clipper science briefing with the following participants:
Gina DiBraccio, acting director, Planetary Science Division, NASA Headquarters Robert Pappalardo, project scientist, Europa Clipper, NASA JPL Haje Korth, deputy project scientist, Europa Clipper, Applied Physics Laboratory (APL) Cynthia Phillips, project staff scientist, Europa Clipper, NASA JPL Coverage of the science news conference will stream live on NASA+ and the agency’s website, Learn how to stream NASA content through a variety of platforms, including social media.
Media may ask questions in person and via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the start of the event at: ksc-newsroom@mail.nasa.gov.
Wednesday, Oct. 9
2 p.m. – NASA Social panel at NASA Kennedy with the following participants:
Kate Calvin, chief scientist and senior climate advisor, NASA Headquarters Caley Burke, Flight Design Analyst, NASA’s Launch Services Program Erin Leonard, project staff scientist, Europa Clipper, NASA JPL Juan Pablo León, systems testbed engineer, Europa Clipper, NASA JPL Elizabeth Turtle, principal investigator, Europa Imaging System instrument, Europa Clipper, APL The panel will stream live on NASA Kennedy’s YouTube, X, and Facebook accounts. Members of the public may ask questions online by posting to the YouTube, X, and Facebook live streams or using #AskNASA.
3:30 p.m. – NASA’s Europa Clipper prelaunch news conference (following completion of the Launch Readiness Review), with the following participants:
NASA Associate Administrator Jim Free Sandra Connelly, deputy associate administrator, Science Mission Directorate, NASA Headquarters Tim Dunn, launch director, NASA’s Launch Services Program Julianna Scheiman, director, NASA Science Missions, SpaceX Jordan Evans, project manager, Europa Clipper, NASA JPL Mike McAleenan, launch weather officer, 45th Weather Squadron, U.S. Space Force Coverage of the prelaunch news conference will stream live on NASA+, the agency’s website, the NASA app, and YouTube.
Media may ask questions in person and via phone. Limited auditorium space will be available for in-person participation. For the dial-in number and passcode, media should contact the NASA Kennedy newsroom no later than one hour before the start of the event at ksc-newsroom@mail.nasa.gov.
5:30 p.m. – NASA’s Europa Clipper rollout show. Coverage will stream live on NASA+, the agency’s website, the NASA app, and YouTube.
Thursday, Oct. 10
11:30 a.m. – NASA launch coverage in English begins on NASA+ and the agency’s website.
11:30 a.m. – NASA launch coverage in Spanish begins on NASA+, the agency’s website and NASA’s Spanish YouTube channel.
12:31 p.m. – Launch
Audio Only Coverage
Audio only of the news conferences and launch coverage will be carried on the NASA “V” circuits, which may be accessed by dialing 321-867-1220, -1240 or -7135. On launch day, “mission audio,” countdown activities without NASA+ media launch commentary, is carried on 321-867-7135.
Live Video Coverage Prior to Launch
NASA will provide a live video feed of Launch Complex 39A approximately 18 hours prior to the planned liftoff of the mission on the NASA Kennedy newsroom YouTube channel. The feed will be uninterrupted until the launch broadcast begins on NASA+.
NASA Website Launch Coverage
Launch day coverage of the mission will be available on the agency’s website. Coverage will include links to live streaming and blog updates beginning no earlier than 10 a.m., Oct. 10, as the countdown milestones occur. On-demand streaming video and photos of the launch will be available shortly after liftoff.
Follow countdown coverage on the Europa Clipper blog. For questions about countdown coverage, contact the Kennedy newsroom at 321-867-2468.
Para obtener información sobre cobertura en español en el Centro Espacial Kennedy o si desea solicitar entrevistas en español, comuníquese con Antonia Jaramillo: antonia.jaramillobotero@nasa.gov o Messod Bendayan: messod.c.bendayan@nasa.gov
Attend the Launch Virtually
Members of the public can register to attend this launch virtually. NASA’s virtual guest program for this mission also includes curated launch resources, notifications about related opportunities or changes, and a stamp for the NASA virtual guest passport following launch.
Watch, Engage on Social Media
Let people know you’re following the mission on X, Facebook, and Instagram by using the hashtags #EuropaClipper and #NASASocial. You can also stay connected by following and tagging these accounts:
X: @NASA, @EuropaClipper, @NASASolarSystem, @NASAJPL, @NASAKennedy, @NASA_LSP
Facebook: NASA, NASA’s Europa Clipper, NASA’s JPL, NASA’s Launch Services Program
Instagram: @NASA, @nasasolarsystem, @NASAKennedy, @NASAJPL
For more information about the mission, visit:
https://science.nasa.gov/mission/europa-clipper
-end-
Karen Fox / Molly Wasser
Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser.nasa.gov
Leejay Lockhart
Kennedy Space Center, Florida
321-747-8310
leejay.lockhart@nasa.gov
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Last Updated Oct 03, 2024 LocationKennedy Space Center Related Terms
Europa Clipper Europa Jupiter Jupiter Moons Missions View the full article
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By NASA
5 min read
NASA’s LRO: Lunar Ice Deposits are Widespread
Deposits of ice in lunar dust and rock (regolith) are more extensive than previously thought, according to a new analysis of data from NASA’s LRO (Lunar Reconnaissance Orbiter) mission. Ice would be a valuable resource for future lunar expeditions. Water could be used for radiation protection and supporting human explorers, or broken into its hydrogen and oxygen components to make rocket fuel, energy, and breathable air.
Prior studies found signs of ice in the larger permanently shadowed regions (PSRs) near the lunar South Pole, including areas within Cabeus, Haworth, Shoemaker and Faustini craters. In the new work, “We find that there is widespread evidence of water ice within PSRs outside the South Pole, towards at least 77 degrees south latitude,” said Dr. Timothy P. McClanahan of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and lead author of a paper on this research published October 2 in the Planetary Science Journal.
The study further aids lunar mission planners by providing maps and identifying the surface characteristics that show where ice is likely and less likely to be found, with evidence for why that should be. “Our model and analysis show that greatest ice concentrations are expected to occur near the PSRs’ coldest locations below 75 Kelvin (-198°C or -325°F) and near the base of the PSRs’ poleward-facing slopes,” said McClanahan.
This illustration shows the distribution of permanently shadowed regions (in blue) on the Moon poleward of 80 degrees South latitude. They are superimposed on a digital elevation map of the lunar surface (grey) from the Lunar Orbiter Laser Altimeter instrument on board NASA’s Lunar Reconnaissance Orbiter spacecraft. NASA/GSFC/Timothy P. McClanahan “We can’t accurately determine the volume of the PSRs’ ice deposits or identify if they might be buried under a dry layer of regolith. However, we expect that for each surface 1.2 square yards (square meter) residing over these deposits there should be at least about five more quarts (five more liters) of ice within the surface top 3.3 feet (meter), as compared to their surrounding areas,” said McClanahan. The study also mapped where fewer, smaller, or lower-concentration ice deposits would be expected, occurring primarily towards warmer, periodically illuminated areas.
Ice could become implanted in lunar regolith through comet and meteor impacts, released as vapor (gas) from the lunar interior, or be formed by chemical reactions between hydrogen in the solar wind and oxygen in the regolith. PSRs typically occur in topographic depressions near the lunar poles. Because of the low Sun angle, these areas haven’t seen sunlight for up to billions of years, so are perpetually in extreme cold. Ice molecules are thought to be repeatedly dislodged from the regolith by meteorites, space radiation, or sunlight and travel across the lunar surface until they land in a PSR where they are entrapped by extreme cold. The PSR’s continuously cold surfaces can preserve ice molecules near the surface for perhaps billions of years, where they may accumulate into a deposit that is rich enough to mine. Ice is thought to be quickly lost on surfaces that are exposed to direct sunlight, which precludes their accumulations.
The team used LRO’s Lunar Exploration Neutron Detector (LEND) instrument to detect signs of ice deposits by measuring moderate-energy, “epithermal” neutrons. Specifically, the team used LEND’s Collimated Sensor for Epithermal Neutrons (CSETN) that has a fixed 18.6-mile (30-kilometer) diameter field-of-view. Neutrons are created by high-energy galactic cosmic rays that come from powerful deep-space events such as exploding stars, that impact the lunar surface, break up regolith atoms, and scatter subatomic particles called neutrons. The neutrons, which can originate from up to about a 3.3-foot (meter’s) depth, ping-pong their way through the regolith, running into other atoms. Some get directed into space, where they can be detected by LEND. Since hydrogen is about the same mass as a neutron, a collision with hydrogen causes the neutron to lose relatively more energy than a collision with most common regolith elements. So, where hydrogen is present in regolith, its concentration creates a corresponding reduction in the observed number of moderate-energy neutrons.
“We hypothesized that if all PSRs have the same hydrogen concentration, then CSETN should proportionally detect their hydrogen concentrations as a function of their areas. So, more hydrogen should be observed towards the larger-area PSRs,” said McClanahan.
The model was developed from a theoretical study that demonstrated how similarly hydrogen-enhanced PSRs would be detected by CSETNs fixed-area field-of-view. The correlation was demonstrated using the neutron emissions from 502 PSRs with areas ranging from 1.5 square miles (4 km2) to 417 square miles (1079 km2) that contrasted against their surrounding less hydrogen-enhanced areas. The correlation was expectedly weak for the small PSRs but increased towards the larger-area PSRs.
The research was sponsored by the LRO project science team, NASA’s Goddard Space Flight Center’s Artificial Intelligence Working Group, and NASA grant award number 80GSFC21M0002. The study was conducted using NASA’s LRO Diviner radiometer and Lunar Orbiter Laser Altimeter instruments. The LEND instrument was developed by the Russian Space Agency, Roscosmos by its Space Research Institute (IKI). LEND was integrated to the LRO spacecraft at the NASA Goddard Space Flight Center. LRO is managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for the Science Mission Directorate at NASA Headquarters in Washington.
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Last Updated Oct 03, 2024 Editor wasteigerwald Contact wasteigerwald william.a.steigerwald@nasa.gov Location Goddard Space Flight Center Related Terms
Earth’s Moon Lunar Reconnaissance Orbiter (LRO) Uncategorized Explore More
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