Hats Off to NASA’s Webb: Sombrero Galaxy Dazzles in New Image

Hats Off to NASA’s Webb: Sombrero Galaxy Dazzles in New Image

5 Min Read

Hats Off to NASA’s Webb: Sombrero Galaxy Dazzles in New Image

Image of a galaxy on the black background of space. The galaxy is a very oblong, blue disk that extends from left to right at an angle (from about 10 o’clock to 5 o’clock). The galaxy has a small bright core at the center. There is an inner disk that is clearer, with speckles of stars scattered throughout. The outer disk of the galaxy is whiteish-blue, and clumpy, like clouds in the sky. There are different colored dots, distant galaxies, speckled among the black background of space surrounding the galaxy.
NASA’s James Webb Space Telescope recently imaged the Sombrero galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring.
Credits:
NASA, ESA, CSA, STScI

In a new image from NASA’s James Webb Space Telescope, a galaxy named for its resemblance to a broad-brimmed Mexican hat appears more like an archery target.

In Webb’s mid-infrared view of the Sombrero galaxy, also known as Messier 104 (M104), the signature, glowing core seen in visible-light images does not shine, and instead a smooth inner disk is revealed. The sharp resolution of Webb’s MIRI (Mid-Infrared Instrument) also brings into focus details of the galaxy’s outer ring, providing insights into how the dust, an essential building block for astronomical objects in the universe, is distributed. The galaxy’s outer ring, which appeared smooth like a blanket in imaging from NASA’s retired Spitzer Space Telescope, shows intricate clumps in the infrared for the first time.

Image A: Sombrero Galaxy (MIRI Image)

Image of a galaxy on the black background of space. The galaxy is a very oblong, blue disk that extends from left to right at an angle (from about 10 o’clock to 5 o’clock). The galaxy has a small bright core at the center. There is an inner disk that is clearer, with speckles of stars scattered throughout. The outer disk of the galaxy is whiteish-blue, and clumpy, like clouds in the sky. There are different colored dots, distant galaxies, speckled among the black background of space surrounding the galaxy.
NASA’s James Webb Space Telescope recently imaged the Sombrero galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring. This image includes filters representing 7.7-micron light as blue, 11.3-micron light as green, and 12.8-micron light as red.
NASA, ESA, CSA, STScI

Image B: Sombrero Galaxy (Hubble and Webb Image)

Image Before/After

Researchers say the clumpy nature of the dust, where MIRI detects carbon-containing molecules called polycyclic aromatic hydrocarbons, can indicate the presence of young star-forming regions. However, unlike some galaxies studied with Webb, including Messier 82, where 10 times as many stars are born than the Milky Way galaxy, the Sombrero galaxy is not a particular hotbed of star formation. The rings of the Sombrero galaxy produce less than one solar mass of stars per year, in comparison to the Milky Way’s roughly two solar masses a year.

Even the supermassive black hole, also known as an active galactic nucleus, at the center of the Sombrero galaxy is rather docile, even at a hefty 9-billion-solar masses. It’s classified as a low luminosity active galactic nucleus, slowly snacking on infalling material from the galaxy, while sending off a bright, relatively small, jet.

Also within the Sombrero galaxy dwell some 2,000 globular clusters, collections of hundreds of thousands of old stars held together by gravity. This type of system serves as a pseudo laboratory for astronomers to study stars — thousands of stars within one system with the same age, but varying masses and other properties is an intriguing opportunity for comparison studies.

In the MIRI image, galaxies of varying shapes and colors litter the background of space. The different colors of these background galaxies can tell astronomers about their properties, including how far away they are.

The Sombrero galaxy is around 30 million light-years from Earth in the constellation Virgo.

Video: Sombrero Galaxy Fade (Spitzer, Webb, Hubble)

A Bright Future Ahead

Stunning images like this, and an array of discoveries in the study of exoplanets, galaxies through time, star formation, and our own solar system, are still just the beginning. Recently, scientists from all over the world applied for observation time with Webb during its fourth year of science operations, which begins in July 2025.

General Observer time with Webb is more competitive than ever. A record-breaking 2,377 proposals were submitted by the Oct. 15, 2024, deadline, requesting about 78,000 hours of observation time. This is an oversubscription rate, the ratio defining the observation hours requested versus the actual time available in one year of Webb’s operations, of around 9 to 1.

The proposals cover a wide array of science topics, with distant galaxies being among the most requested observation time, followed by exoplanet atmospheres, stars and stellar populations, then exoplanet systems.

The Space Telescope Science Institute manages the proposal and program selection process for NASA. The submissions will now be evaluated by a Telescope Allocation Committee, a group of hundreds of members of the worldwide astronomical community, on a dual-anonymous basis, with selections announced in March 2025.

While time on Webb is limited, data from all of Webb’s programs is publicly archived, immediately after it’s taken, or after a time of exclusive access, in the Mikulski Archive for Space Telescopes (MAST) so it can be used by anyone in the world.

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).

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Media Contacts

Laura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Hannah Braunhbraun@stsci.edu, Christine Pulliamcpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.

Related Information

Article: Types of Galaxies

Video: Celestial Tour: Different types of galaxies

Article: Sombrero Galaxy’s Halo Suggests Turbulent Past

More images: Images of the Sombrero Galaxy in different types of light

Video: Sonification of Sombrero Galaxy images

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Space Deilvery Arrives at Station Aboard Progress Cargo Craft

Space Deilvery Arrives at Station Aboard Progress Cargo Craft

The Progress 90 cargo craft carrying nearly three tons of food, fuel, and supplies approaches the International Space Station for a docking to the Poisk module. Credit: NASA+
The Progress 90 cargo craft carrying nearly three tons of food, fuel, and supplies approaches the International Space Station for a docking to the Poisk module. Credit: NASA+

The unpiloted Progress 90 spacecraft arrived at the space-facing port of the International Space Station’s Poisk module at 9:31 a.m. EST, Saturday, Nov. 23. The spacecraft launched at 7:22 a.m. (5:22 p.m. Baikonur time) Nov. 21, on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan.

The Roscosmos spacecraft is delivering about three tons of food, fuel, and supplies for the Expedition 72 crew aboard the International Space Station and will remain docked for approximately six months before departing for a re-entry into Earth’s atmosphere to dispose of trash loaded by the crew.


Learn more about station activities by following the space station blog, @space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark Garcia

Progress Cargo Craft Approaching Station Live on NASA+

Progress Cargo Craft Approaching Station Live on NASA+

The Progress 90 spacecraft is pictured moments before launching on Nov. 21, 2024, from the Baikonur Cosmodrome in Kazakhstan. Credit: NASA
The Progress 90 spacecraft is pictured moments before launching on Nov. 21, 2024, from the Baikonur Cosmodrome in Kazakhstan. Credit: NASA

NASA’s live coverage of rendezvous and docking is underway on NASA+ and the agency’s website. Learn how to watch NASA content through a variety of platforms, including social media.

The unpiloted Roscosmos Progress 90 spacecraft will automatically dock at 9:36 a.m. EST, to the space-facing port of the International Space Station’s Poisk module.

The spacecraft launched at 7:22 a.m. (5:22 p.m. Baikonur time) Nov. 21, on a Soyuz rocket from the Baikonur Cosmodrome in Kazakhstan.


Learn more about station activities by following the space station blog, @space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark Garcia

Sol 4370-4371: All About the Polygons

Sol 4370-4371: All About the Polygons

2 min read

Sol 4370-4371: All About the Polygons

A grayscale photograph of the Martian surface from the Curiosity rover captures medium gray, very uneven terrain in front of the rover, with many angular, lighter-toned, medium-sized rocks protruding from the smooth soil. The bottom of the frame shows part of the rover, running from the middle left to the lower right corner of the image, including part of its robotic arm which carries a nameplate imprinted with “Curiosity” outlined in all capital letters, and to the right of that a line drawing of the rover.
NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on Nov. 20, 2024 — sol 4369, or Martian day 4,369 of the Mars Science Laboratory mission — at 05:47:04 UTC.
NASA/JPL-Caltech

Earth planning date: Wednesday, Nov. 20, 2024

We planned two very full sols today! The sol 4369 drive completed successfully, and the rover was in a stable enough position that we could unstow the arm — something we don’t take for granted in the exceedingly rocky terrain of the sulfate unit! Today the team decided to investigate several rocks in our workspace that are covered in cracks, or fractures, that form polygonal patterns. We are interested to better characterize the geometry of these cracks and to see if they are associated with any compositional differences from the rock. Both pieces of information will give us clues about how they formed. Did they form when stresses pushed on the rock in just the right manner to fracture it into polygonal shapes? Or do the cracks record the rock expanding and contracting, either due to massive changes in temperatures on the Martian surface, or minerals within the rock gaining and losing water? Or perhaps it is something different?

We selected two contact science targets to investigate in our attempt to answer these questions. The target named “Buttermilk” is one of the skinny raised ridges associated with these cracks. We will be placing APXS at three different places over this feature to try to characterize its chemistry.  Our second contact science target,  “Lee Vining,” gives us a nice 3D view into these cracks. Here, we will collect two MAHLI mosaics, one on each side of the rock that’s close to the rover, to characterize the geometry of the fractures. ChemCam will also get in on the action with a LIBS observation on a fracture fill named “Crater Crest,” as well as an observation on a dark-toned, platy rock called “Lost Arrow.” Mastcam will collect observations of several more polygonally fractured rocks further away from Curiosity in “The Dardanelles” series of mosaics. Some environmental science observations will round out the plan before our drive will take us about 25 meters further (about 82 feet) to the southwest.

Written by Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory

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Nov 23, 2024

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Dr. Misty Davies – American Institute of Aeronautics and Astronautics (AIAA) 2024 Fellow

Dr. Misty Davies – American Institute of Aeronautics and Astronautics (AIAA) 2024 Fellow

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Misty Davies holding a framed AIAA Fellowship certificate with a red rose on her lapel, standing against a dark background.
Dr. Misty Davies receives the prestigious AIAA Fellowship in May 2024 for her contributions to aerospace safety and autonomous systems, recognized at a ceremony in Washington, DC.
NASA

In May 2024, Dr. Misty Davies joined the American Institute of Aeronautics and Astronautics (AIAA) Class of 2024 Fellows at a ceremony in Washington, DC.  The AIAA website states that, “AIAA confers Fellow upon individuals in recognition of their notable and valuable contributions to the arts, sciences or technology of aeronautics and astronautics.”  The first AIAA Fellows were elected in 1934; since then only 2064 people have been selected for the honor.  Dr. Davies has focused her career at NASA Ames Research Center on developing tools and techniques that enable the safety assurance of increasingly autonomous systems.  She currently serves as the Associate Chief for Aeronautics Systems in the Intelligent Systems Division at NASA Ames and is the Aerospace Operations and Safety Program (AOSP) Technical Advisor for Assurance and Safety. More information on AIAA Fellows is at https://www.aiaa.org/news/news/2024/02/08/aiaa-announces-class-of-2024-honorary-fellows-and-fellows

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Nov 22, 2024

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Osvaldo R. Sosa Valle