By Length
Full (4-12 min)
Short (1-4 min)
By Date
2024 | 2023 | 2022 | 2021
2020 | 2019 | 2018 | 2017
2016 | 2015 | 2014 | 2013
2012 | 2011 | 2010 | 2009
2008 | 2007 | 2006
By Category
Solar System
Stars
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Groups of Galaxies
Cosmology/Deep Field
Miscellaneous
HTE
STOP
Space Scoop for Kids!
Chandra Sketches
Light
AstrOlympics
Quick Look
Visual Descriptions
Subscribe
How To
RSS Reader
Audio-only format podcast
Web Shortcuts
Chandra Blog
RSS Feed
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader


A Tour of NGC 5813

View/Listen
Narrator (April Hobart, CXC): Galaxy groups are families of galaxies that are bound together by gravity. They are very similar to their larger cousins, galaxy clusters. Instead of containing hundreds or even thousands of galaxies like clusters do, galaxy groups are typically comprised of 50 or fewer galaxies. Like galaxy clusters, groups of galaxies are enveloped by giant amounts of hot gas that emit X-rays. They also often contain a giant black hole at their center that can impact what's happening throughout the group.

Astronomers used NASA's Chandra X-ray Observatory to study this in the galaxy group NGC 5813, which is located about 105 million light years from Earth. They found three pairs of cavities, or bubbles, that have been carved into the hot gas. These cavities were produced by jets of material that blasted out of the central black hole, including multiple eruptions that lasted for some 50 million years. Similar to how air bubbles will rise to the surface of water, these cavities have moved away from the galaxy group's center toward the edge of the hot gas. By studying the details of these cavities, astronomers can get a better understanding of just how supermassive black holes affect their cosmic surroundings.

Return to Podcasts