NASA’s Hubble Examines Cloud-9, First of New Type of Object

NASA’s Hubble Examines Cloud-9, First of New Type of Object

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NASA’s Hubble Examines Cloud-9, First of New Type of Object

A region of space mostly filled with background galaxies, with one prominent star at upper left. A large blob of purple haze occupies much of the field. Within the purple region, an unremarkable area is outlined with a dashed white circle.
Magenta is radio data from the ground-based Very Large Array showing the presence of Cloud-9. The dashed circle marks the peak of radio emission, which is where researchers focused their search for stars. Hubble found no stars within Cloud-9. The few objects within its boundaries are background galaxies.
Credits:
NASA, ESA, VLA, Gagandeep Anand (STScI), Alejandro Benitez-Llambay (University of Milano-Bicocca); Image Processing: Joseph DePasquale (STScI)

A team using NASA’s Hubble Space Telescope has uncovered a new type of astronomical object — a starless, gas-rich, dark-matter cloud considered a “relic” or remnant of early galaxy formation. Nicknamed “Cloud-9,” this is the first confirmed detection of such an object in the universe — a finding that furthers the understanding of galaxy formation, the early universe, and the nature of dark matter itself.

“This is a tale of a failed galaxy,” said the program’s principal investigator, Alejandro Benitez-Llambay of the Milano-Bicocca University in Milan, Italy. “In science, we usually learn more from the failures than from the successes. In this case, seeing no stars is what proves the theory right. It tells us that we have found in the local universe a primordial building block of a galaxy that hasn’t formed.”

The results, published in The Astrophysical Journal Letters, were presented at a press conference Monday at the 247th meeting of the American Astronomical Society in Phoenix.

“This cloud is a window into the dark universe,” said team member Andrew Fox of the Association of Universities for Research in Astronomy/Space Telescope Science Institute (AURA/STScI) for the European Space Agency. “We know from theory that most of the mass in the universe is expected to be dark matter, but it’s difficult to detect this dark material because it doesn’t emit light. Cloud-9 gives us a rare look at a dark-matter-dominated cloud.”

A region of space mostly filled with background galaxies, with one prominent star at upper left. A large blob of purple haze occupies much of the field. Within the purple region, an unremarkable area is outlined with a dashed white circle.
This image shows the location of Cloud-9, which is 14 million light-years from Earth. The diffuse magenta is radio data from the ground-based Very Large Array (VLA) showing the presence of the cloud. The dashed circle marks the peak of radio emission, which is where researchers focused their search for stars. Follow-up observations by the Hubble Space Telescope’s Advanced Camera for Surveys found no stars within the cloud. The few objects that appear within its boundaries are background galaxies. Before the Hubble observations, scientists could argue that Cloud-9 is a faint dwarf galaxy whose stars could not be seen with ground-based telescopes due to the lack of sensitivity. Hubble’s Advanced Camera for Surveys shows that, in reality, the failed galaxy contains no stars.
Science: NASA, ESA, VLA, Gagandeep Anand (STScI), Alejandro Benitez-Llambay (University of Milano-Bicocca); Image Processing: Joseph DePasquale (STScI)

The object is called a Reionization-Limited H I Cloud, or “RELHIC.” The term “H I” refers to neutral hydrogen, and “RELHIC” describes a natal hydrogen cloud from the universe’s early days, a fossil leftover that has not formed stars. For years, scientists have looked for evidence of such a theoretical phantom object. It wasn’t until they turned Hubble toward the cloud, confirming that it is indeed starless, that they found support for the theory.

“Before we used Hubble, you could argue that this is a faint dwarf galaxy that we could not see with ground-based telescopes. They just didn’t go deep enough in sensitivity to uncover stars,” said lead author Gagandeep Anand of STScI. “But with Hubble’s Advanced Camera for Surveys, we’re able to nail down that there’s nothing there.”

The discovery of this relic cloud was a surprise. “Among our galactic neighbors, there might be a few abandoned houses out there,” said STScI’s Rachael Beaton, who is also on the research team.

Astronomers think RELHICs are dark matter clouds that couldn’t accumulate enough gas to form stars. They represent a window into the early stages of galaxy formation. Cloud-9 suggests the existence of many other small, dark matter-dominated structures in the universe — other failed galaxies. This discovery provides new insights into the dark components of the universe that are difficult to study through traditional observations, which focus on bright objects like stars and galaxies.

Scientists have studied hydrogen clouds near the Milky Way for many years, but these clouds tend to be much bigger and more irregular than Cloud-9. Compared with other observed hydrogen clouds, Cloud-9 is smaller, more compact, and highly spherical, making it look very different from the others.

The core of this object is composed of neutral hydrogen and is about 4,900 light-years in diameter. Researchers measured the hydrogen gas in Cloud-9 by the radio waves it emits, measuring it to be approximately one million times the mass of the Sun. Assuming that the gas pressure is balancing the dark matter cloud’s gravity, which appears to be the case, researchers calculated Cloud-9’s dark matter must be about five billion solar masses.

Cloud-9 is an example of structures and mysteries that don’t involve stars. Just looking at stars doesn’t give the full picture. Studying the gas and dark matter helps provide a more complete understanding of what’s going on in these systems that would otherwise be unknown.

Observationally, identifying these failed galaxies is challenging because nearby objects outshine them. Such systems are also vulnerable to environmental effects like ram-pressure stripping, which can remove gas as the cloud moves through intergalactic space. These factors further reduce their expected numbers.

The starless relic was discovered three years ago as part of a radio survey by the Five-hundred-meter Aperture Spherical Telescope (FAST) in Guizhou, China, a finding later confirmed by the Green Bank Telescope and the Very Large Array facilities in the United States. But only with Hubble could researchers definitively determine that the failed galaxy contains no stars.

Cloud-9 was simply named sequentially, having been the ninth gas cloud identified on the outskirts of a nearby spiral galaxy, Messier 94 (M94). The cloud is close to M94 and appears to have a physical association with the galaxy. High-resolution radio data shows slight gas distortions, possibly indicating interaction between the cloud and galaxy.

The cloud may eventually form a galaxy in the future, provided it grows more massive — although how that would occur is under speculation. If it were much bigger, say, more than 5 billion times the mass of our Sun, it would have collapsed, formed stars, and become a galaxy that would be no different than any other galaxy we see. If it were much smaller than that, the gas could have been dispersed and ionized and there wouldn’t be much left. But it’s in a sweet spot where it could remain as a RELHIC.

The lack of stars in this object provides a unique window into the intrinsic properties of dark matter clouds. The rarity of such objects and the potential for future surveys is expected to enhance the discovery of more of these “failed galaxies” or “relics,” resulting in insights into the early universe and the physics of dark matter.  

The Hubble Space Telescope has been operating for more than three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

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Last Updated
Jan 05, 2026
Editor
Andrea Gianopoulos
Contact
Media

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

Ann Jenkins, Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

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5 Tips to Craft a Standout NASA Internship Application

5 Tips to Craft a Standout NASA Internship Application

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Four NASA interns pose in front of the NASA Pavilion at the EAA AirVenture Oshkosh, an annual airshow in Oshkosh, Wisconsin.
Four NASA interns pose in front of the NASA Pavilion at the EAA AirVenture Oshkosh, an annual airshow in Oshkosh, Wisconsin.
NASA

A NASA internship provides a stellar opportunity to launch your future as part of America’s aerospace workforce. NASA interns take on meaningful work and contribute to exciting agency projects with the guidance of a supportive mentor. The agency’s internship program regularly ranks as the nation’s most prestigious and competition is steep: in fiscal year 2025, NASA’s Office of STEM Engagement received about 250,000 internship applications for its roughly 1,800 internship opportunities.

To give you the best shot at a NASA internship, we’ve compiled a list of tips mentors say can make an application stand out from the crowd. It is NASA’s mentors who create internship project descriptions, review applications, and take the lead in choosing candidates to work on their specific internship projects. Here’s what they had to say:

1. Your personal statement is your chance to make a lasting impression.

Mentors pay close attention to personal statements to identify the best candidate for their project and team. A powerful personal statement shares personal background, experience, and goals, and how they relate to the needs of the project.

NASA mentors are looking for interns who will enjoy the work and fit in with the team culture. Beyond your academic background, grades, and interests, this is your chance to share your curiosity, enthusiasm, passion, or resilience. Show us who you are and what you can do!

2. Show off your academic achievements.

Mentors love to see what academic expertise and hands-on experience you can bring to the internship project. Your transcripts, grade point average, coursework, research, academic projects, awards, and accomplishments are valuable highlights in your application.

3. Tell us about your extracurriculars, too!

Who are you outside the classroom?

Mentors like to see well-rounded candidates whose interests take them beyond their chosen academic and career path. Include any extracurricular activities you participate in, such as a club or team at school or an organization in your community. Whether you’re involved in a local rocketry club, a school athletic team, or a musical ensemble, these pursuits may demonstrate academic skills or soft skills such as collaboration. Shared hobbies can also be a great point of personal connection with a future mentor.

4. Include as many of your skills as possible.

Share the valuable skills that you can bring to an internship project. These could be technical skills, such as experience with specific tools or computer programming languages, and non-technical skills, which may include communications skills or leadership experience. Mentors search for skills that meet their project requirements and, match with the role, but also for unique skills that might be an added asset.

5. Give yourself a chance.

Don’t count yourself out before you get started! If you have a passion for spaceflight or aviation, it’s worth applying for a NASA internship – even if you’re not a math, science, engineering, or technology major. That’s because NASA achieves its exploration goals with the support of a nationwide team with a wide variety of skills: communicators, creatives, business specialists, legal experts, and so many more. Take a look at NASA’s internship opportunities and you’ll find projects in a wide range of fields.

Yes, competition is fierce. But someone is going to land that internship – and that person could be you!

Learn More

Check eligibility requirements, see current deadlines, and launch your internship journey at https://intern.nasa.gov.

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Sandra May

Scientific Balloon Begins Antarctic Ascent

Scientific Balloon Begins Antarctic Ascent

A white scientific balloon rises into the bright blue sky above snowy Antarctica. The sky and the balloon take up most of the image, with the ground only being a small white stripe at the bottom of the photo. The balloon has a long white "tail" with orange and black portions.
NASA/Scott Battaion

A scientific balloon starts its ascent into the air as it prepares to launch carrying NASA’s Payload for Ultrahigh Energy Observations (PUEO) mission. The mission lifted off from Antarctica at 5:56 a.m. NZST, Saturday, Dec. 20 (11:56 a.m., Friday, Dec. 19 in U.S. Eastern Time).

The PUEO mission is designed to detect radio signals created when highly energetic particles called neutrinos from space hit the ice. The PUEO payload will collect data that give us insight into events like the creation of black holes and neutron star mergers. Alongside the PUEO mission are two other balloons carrying calibration equipment sending test signals to help scientists make sure the payload equipment is working correctly when it tries to detect real signals from space. 

Track the balloons in realtime.

Image credit: NASA/Scott Battaion

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Monika Luabeya

An Amphitheater of Rock at Cedar Breaks

An Amphitheater of Rock at Cedar Breaks

A Landsat image is centered on an orange, amphitheater-shaped escarpment cutting into darker green, forested terrain at Cedar Breaks National Monument in southwestern Utah. Light-colored and orange cliffs and ridges form a semicircular rim, with deeply eroded drainages radiating westward. A black lava flow with little vegetation is visible east of the escarpment. Trails from Brian Head, a nearby mountain and ski area, are visible to the north.
June 18, 2025

When people stand at the rim of the amphitheater in Utah’s Cedar Breaks National Monument and look down on an otherworldly landscape of multicolored rock spires, pinnacles, and other geologic oddities, they’re looking across tens of millions of years of Earth’s history. The same can be said when viewing the bowl-shaped escarpment from space.

The OLI-2 (Operational Land Imager-2) on Landsat 9 captured this view of the amphitheater’s semicircular rim and deeply eroded drainages on June 18, 2025. The erosive power of water from Ashdown Creek and several tributaries, along with relentless physical and chemical weathering, is evident in the many channels, cliffs, and canyons that radiate outward from the rim and define the escarpment and amphitheater.

The feature’s striking rock formations are composed of sedimentary rock layers laid down roughly 50 to 25 million years ago within a basin that, at times, held a large body of water called Lake Claron. Many of the amphitheater’s limestone layers began as sediments that settled on its lakebed as carbonate-rich muds.

Differences in rock type and color, evident in the layering seen in ground photographs and to a degree in Landsat images, reflect differences in environmental conditions during deposition. Lake Claron, for instance, was sometimes quite deep, but during dry periods it was shallow or nonexistent. In wet conditions, iron in muddy sediments was scarce or had too little exposure to oxygen to oxidize, or rust, leaving the resulting rock white or gray. During drier periods, iron in sediments had greater exposure to oxygen, forming minerals that turned layers red and orange. 

After deposition, slow-moving tectonic forces lifted all these rock layers upward, ultimately putting them at the top of the Grand Staircase—an immense sedimentary sequence that stretches south from Cedar Breaks and Bryce Canyon, through Grand Staircase-Escalante National Monument and Zion Canyon, and finally into the Grand Canyon. Younger rock layers are found at the top of the sequence and older layers at the bottom.

The rim at Cedar Breaks, the top of the staircase, sits about 10,000 feet (3,000 meters) above sea level, roughly 7,000 feet above the Colorado River in the Grand Canyon. The high elevation influences everything from the weather to the plants and animals that live there. Winters are long, cold, and snowy, with nearby Brian Head seeing 30 feet (10 meters) of snowfall each year on average.

While the cool temperatures and short growing season are an impediment to many types of vegetation, the slow-growing and notoriously long-lived bristlecone pines found along the escarpment’s rim use the harsh conditions to their advantage. Slow growth makes their wood unusually dense, which protects the trees from disease and insects. Likewise, their ability to survive in thin soils, on mostly barren limestone outcrops where little else can grow, protects them from wildfires. Some of the oldest bristlecones in the monument are more than 1,700 years old.

Sitting atop the sedimentary layers, signs of a more volcanically active period also appear in the image. The dark basaltic lava flows visible to the east of the amphitheater formed between 5 million and 10,000 years ago, when several volcanoes on the Markagunt Plateau erupted regularly. Areas of soft, gray rock around the summit of Brian Head—now the site of a ski resort—formed when pyroclastic flows left deposits of tuff strewn across the landscape.

NASA Earth Observatory images by Michala Garrison, using Landsat data from the U.S. Geological Survey. Story by Adam Voiland.

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Hubble Glimpses Galactic Gas Making a Getaway

Hubble Glimpses Galactic Gas Making a Getaway

A nearly edge-on spiral galaxy. Its disk holds pink light from star-forming nebulae and blue light from clusters of hot stars. Thick dark clouds of dust block the strong white light from galaxy’s center. A faint, glowing halo of gas surrounds the disk, fading into the black background of space. A bluish plume of gas also extends from the galaxy’s core extending toward the lower-right corner of the image.
This NASA/ESA Hubble Space Telescope image features the galaxy NGC 4388, a member of the Virgo galaxy cluster.
ESA/Hubble & NASA, S. Veilleux, J. Wang, J. Greene

A sideways spiral galaxy shines in this NASA/ESA Hubble Space Telescope image. Located about 60 million light-years away in the constellation Virgo (the Maiden), NGC 4388 is a resident of the Virgo galaxy cluster. This enormous cluster of galaxies contains more than a thousand members and is the nearest large galaxy cluster to the Milky Way.

NGC 4388 appears to tilt at an extreme angle relative to our point of view, giving us a nearly edge-on prospect of the galaxy. This perspective reveals a curious feature that wasn’t visible in a previous Hubble image of this galaxy released in 2016: a plume of gas from the galaxy’s nucleus, here seen billowing out from the galaxy’s disk toward the lower-right corner of the image. But where did this outflow come from, and why does it glow?

The answer likely lies in the vast stretches of space that separate the galaxies of the Virgo cluster. Though the space between galaxies appears empty, this space is occupied by hot wisps of gas called the intracluster medium. As NGC 4388 moves within the Virgo cluster, it plunges through the intracluster medium. Pressure from hot intracluster gas whisks away gas from within NGC 4388’s disk, causing it to trail behind as NGC 4388 moves.

The source of the ionizing energy that causes this gas cloud to glow is more uncertain. Researchers suspect that some of the energy comes from the center of the galaxy, where a supermassive black hole spins gas around it into a superheated disk. The blazing radiation from this disk might ionize the gas closest to the galaxy, while shock waves might be responsible for ionizing filaments of gas farther out.

This image incorporates new data, including several additional wavelengths of light, that bring the ionized gas cloud into view. The image holds data from several observing programs that aim to illuminate galaxies with active black holes at their centers.

Image credit: ESA/Hubble & NASA, S. Veilleux, J. Wang, J. Greene

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Monika Luabeya