X-ray Astronomy
History
Major Milestones
X-ray Universe
X-rays & Light
VS. Medical X-ray
X-ray Absorption
X-ray Images 101
Galactic Navigation
Dark Matter
Dark Energy
Chemistry & Cosmos
X-ray Sources
Solar System
Stars
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Galaxies
Quasars & AGN
Galaxy Clusters
X-ray Background
Brown Dwarfs
Gamma Ray Bursts
Web Shortcuts
Chandra Blog
RSS Feed
Chandra Mobile
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
More Information

Stellar Evolution

Note on Cosmic Distances

Discovering the X-Ray universe

Colossal Clouds of Hot Gas

The "X-ray universe" refers to the universe as observed with telescopes designed to detect X-rays. X-rays are produced in the cosmos when matter is heated to millions of degrees. Such temperatures occur where high magnetic fields, or extreme gravity, or explosive forces, hold sway.

Hydra A Cluster Hydra A Cluster

Comparison of optical image from La Palma & B.McNamara (left) and X-ray imagefrom Chandra (right) of the Hydra A cluster of galaxies. This cluster is so large that it takes light millions of years to cross it.

Above is an example of one of the largest cosmic X-ray sources. This vast cloud of hot gas in a cluster of galaxies is several million light years across and contains enough matter to make hundreds of trillions of stars. The gas cloud is thought to have been heated by gravitational collapse when the universe was half its present size.

X-ray telescopes can also trace the hot gas from an exploding star or detect X-rays from matter swirling as close as 90 kilometers from the event horizon of a stellar black hole.

The Chandra X-ray Observatory, which was launched by Space Shuttle Columbia in 1999, can better define the hot, turbulent regions of space. This increased clarity can help scientists answer fundamental questions about the origin, evolution, and destiny of the universe.