JPL
Careers
Education
Science & Technology
JPL Logo
JPL Logo
Stars and Galaxies
.3 min read

NASA Images Help Explain Eating Habits of Massive Black Hole

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ May 9, 2024

Data from NASA’s retired Spitzer Space Telescope has given scientists new insights into why some supermassive black holes shine differently than others.

These images of the Andromeda galaxy use data from NASA’s retired Spitzer Space Telescope. Multiple wavelengths are shown in the image on the left, revealing stars, dust, and areas of star formation. The image on the right shows dust only, making it easier to see the galaxy’s underlying structure. Credit: NASA/JPL-Caltech

In images from NASA’s retired Spitzer Space Telescope, streams of dust thousands of light-years long flow toward the supermassive black hole at the heart of the Andromeda galaxy. It turns out these streams can help explain how black holes billions of times the mass of our Sun satiate their big appetites but remain “quiet” eaters.

As supermassive black holes gobble up gas and dust, the material gets heated up just before it falls in, creating incredible light shows — sometimes brighter than an entire galaxy full of stars. When the material is consumed in clumps of different sizes, the brightness of the black hole fluctuates.

But the black holes at the center of the Milky Way (Earth’s home galaxy) and Andromeda (one of our nearest galactic neighbors) are among the quietest eaters in the universe. What little light they emit does not vary significantly in brightness, suggesting they are consuming a small but steady flow of food, rather than large clumps. The streams approach the black hole little by little, and in a spiral, similar to the way the water swirls down a drain.

Hunting for Andromeda’s Food Source

A study published earlier this year took the hypothesis that a quiet supermassive black hole feeds on a steady stream of gas and applied it to the Andromeda galaxy. Using computer models, the authors simulated how gas and dust in proximity to Andromeda’s supermassive black hole might behave over time. The simulation demonstrated that a small disk of hot gas could form close to the supermassive black hole and feed it continuously. The disk could be replenished and maintained by numerous streams of gas and dust.

But the researchers also found that those streams have to stay within a particular size and flow rate; otherwise, the matter would fall into the black hole in irregular clumps, causing more light fluctuation.

This close-up view of the center of the Andromeda galaxy, taken by NASA’s retired Spitzer Space Telescope, is annotated with blue dotted lines to highlight the path of two dust streams flowing toward the supermassive black hole at the galaxy’s center

This close-up view of the center of the Andromeda galaxy, taken by NASA’s retired Spitzer Space Telescope, is annotated with blue dotted lines to highlight the path of two dust streams flowing toward the supermassive black hole at the galaxy’s center (indicated by a purple dot).

Credit: NASA/JPL-Caltech

When the authors compared their findings to data from Spitzer and NASA’s Hubble Space Telescope, they found spirals of dust previously identified by Spitzer that fit within these constraints. From this, the authors concluded that the spirals are feeding Andromeda’s supermassive black hole.

“This is a great example of scientists reexamining archival data to reveal more about galaxy dynamics by comparing it to the latest computer simulations,” said Almudena Prieto, an astrophysicist at the Institute of Astrophysics of the Canary Islands and the University Observatory Munich, and a co-author on the study published this year. “We have 20-year-old data telling us things we didn’t recognize in it when we first collected it.”

A Deeper Look at Andromeda

Launched in 2003 and managed by NASA’s Jet Propulsion Laboratory, Spitzer studied the universe in infrared light, which is invisible to human eyes. Different wavelengths reveal different features of Andromeda, including hotter sources of light, like stars, and cooler sources, like dust.

By separating these wavelengths and looking at the dust alone, astronomers can see the galaxy’s “skeleton” — places where gas has coalesced and cooled, sometimes forming dust, creating conditions for stars to form. This view of Andromeda revealed a few surprises. For instance, although it is a spiral galaxy like the Milky Way, Andromeda is dominated by a large dust ring rather than distinct arms circling its center. The images also revealed a secondary hole in one portion of the ring where a dwarf galaxy passed through.

Andromeda’s proximity to the Milky Way means it looks larger than other galaxies from Earth: Seen with the naked eye, Andromeda would be about six times the width of the Moon (about 3 degrees). Even with a field of view wider than Hubble’s, Spitzer had to take 11,000 snapshots to create this comprehensive picture of Andromeda.

More About the Mission

JPL managed the Spitzer Space Telescope mission for NASA’s Science Mission Directorate in Washington until the mission was retired in January 2020. Science operations were conducted at the Spitzer Science Center at Caltech. Spacecraft operations were based at Lockheed Martin Space in Littleton, Colorado. Data are archived at the Infrared Science Archive operated by IPAC at Caltech. Caltech manages JPL for NASA.

For more information about Spitzer, visit:

https://www.nasa.gov/spitzer

Media Contacts

Calla Cofield

Jet Propulsion Laboratory, Pasadena, Calif.

626-808-2469

calla.e.cofield@jpl.nasa.gov

2024-063

Related News

Stars and Galaxies.

‘Interstellar Glaciers’: NASA’s SPHEREx Maps Vast Galactic Ice Regions

Stars and Galaxies.

Archival Data From NASA’s NEOWISE Tracks Star Turning Into Black Hole

Stars and Galaxies.

NASA Reveals New Details About Dark Matter’s Influence on Universe

Stars and Galaxies.

NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other

Technology.

NASA Completes Nancy Grace Roman Space Telescope Construction

Stars and Galaxies.

NASA’s Webb Explores Largest Star-Forming Cloud in Milky Way

Stars and Galaxies.

NASA Scientist Finds Predicted Companion Star to Betelgeuse

Stars and Galaxies.

How NASA’s SPHEREx Mission Will Share Its All-Sky Map With the World

Stars and Galaxies.

NASA’s SPHEREx Space Telescope Begins Capturing Entire Sky

Stars and Galaxies.

NASA’s Newest Space Telescope Recognized at New York Stock Exchange

About JPL
Who We Are
Directors
Careers
Internships
The JPL Story
JPL Achievements
Documentary Series
JPL Annual Report
Executive Council
Missions
Current
Past
Future
All
News
All
Earth
Solar System
Stars and Galaxies
Eyes on the News
Subscribe to JPL News
Galleries
Images
Videos
Audio
Podcasts
Apps
Visions of the Future
Slice of History
Robotics at JPL
Events
Lecture Series
Speakers Bureau
Calendar
Visit
Public Tours
Virtual Tour
Directions and Maps
Topics
JPL Life
Solar System
Mars
Earth
Climate Change
Exoplanets
Stars and Galaxies
Robotics
More
Asteroid Watch
NASA's Eyes Visualizations
Universe - Internal Newsletter
Social Media
Accessibility at NASA
Contact Us
Get the Latest from JPL
Follow Us

JPL is a federally funded research and development center managed for NASA by Caltech.

More from JPL
Careers
Education
Science & Technology
Acquisition
JPL Store
Careers
Education
Science & Technology
Acquisition
JPL Store
Related NASA Sites
Basics of Spaceflight
NASA Kids Science - Earth
Earth / Global Climate Change
Exoplanet Exploration
Mars Exploration
Solar System Exploration
Space Place
NASA's Eyes Visualization Project
Voyager Interstellar Mission
NASA
Caltech
Privacy
Image Policy
FAQ
Feedback
Version: v3.1.3 - 5e83a9a
Site Managers:Emilee Richardson, Alicia Cermak
Site Editors:Steve Carney
CL#:21-0018