Images by Date
Images by Category
Solar System
Stars
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Galaxy Clusters
Cosmology/Deep Field
Miscellaneous
Images by Interest
Space Scoop for Kids
4K JPG
Multiwavelength
Sky Map
Constellations
3D Wall
Photo Blog
Top Rated Images
Image Handouts
Desktops
High Res Prints
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
Getting Hard Copies
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
3C295

3C295 in Context

Optical of 3C295
Palomar Observatory image made by R. Minkowski in 1960, giving the optical identification of the central galaxy in the cluster 3C295. Angular size of box = 15 arc min.
3C295 is enveloped by a vast cloud of fifty million degree gas. The gas cloud, which is visible only with an X-ray telescope, contains more than a hundred galaxies and enough material to make a thousand more. The galaxies in most cases do not contain enough hot gas to be observed with an X-ray telescope, but they do show up in optical photographs. Because the galaxies were discovered before the hot gas cloud, these objects are called galaxy clusters, or clusters of galaxies.

Galaxy clusters are formed through the merger of smaller groups and clusters over billions of years. The gas in clusters is thought to have been heated to fifty million degrees or more when the cloud collapsed about five to ten billion years ago. Galaxy clusters are the most massive gravitationally bound objects in the universe.

X-ray of 3C295
X-ray image of 3C295
NASA/CXC/SAO
In recent years X-ray observations have shown that galaxy clusters must contain large amounts of dark matter to hold the hot gas cloud together. The total mass of the dark matter needed is typically about five times as great as the mass of the gas and the galaxies. Chandra observations may provide insight into what constitutes dark matter and how it is distributed.

The gas in the central regions of the 3C295 cluster shows signs that it is cooling and settling onto the central galaxy. Astronomers think that the material falling onto 3C295 over the eons has caused it to grow into its present size and shape. It contains several times the mass of our Milky Way galaxy and resembles a giant glowing basketball.

X-ray/Radio Composite of 3C295
X-ray-radio composite of 3C295
NASA/CXC/SAO/NRAO/AUI/NSF/R.Perley & G. Taylor
The explosion that wracked 3C295 about a million years ago and produced the X-ray knots and radio lobes was probably due to the infall of gas onto the galaxy. In much the same way that a torrent of water pouring down a drain can produce a back pressure if the flow is more than the drain can handle, the enormous energy released by too much matter flowing into a supermassive black hole could trigger an explosion. Great quantities of matter and energy would be hurled back into the surrounding gas cloud, in a powerful payback for eons of being dumped on by a cosmic bully.

Return to 3C295 (16 Nov 99)