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
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
Chandra Mobile
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
More Information
Supernovas & Supernova Remnants
Related Podcasts
A Tour of Puppis A
A Tour of Puppis A (2014-09-15)
Download Image

More Information

More Images
Chandra X-ray Image with Scale Bar
(Credit: NASA/CXC/Rutgers/
J.Warren & J.Hughes et al.)

More Releases

Related Images
Cassiopeia A
Cassiopeia A
(13 Jun 05)
Tycho's Supernova Remnant:
Tycho's Remnant Provides Shocking Evidence for Cosmic Rays


Tycho's Supernova Remnant
Credit: NASA/CXC/Rutgers/J.Warren & J.Hughes et al.

In 1572, the Danish astronomer Tycho Brahe observed and studied the explosion of a star that became known as Tycho's supernova. More than four centuries later, Chandra's image of the supernova remnant shows an expanding bubble of multimillion degree debris (green and red) inside a more rapidly moving shell of extremely high energy electrons (filamentary blue).

The supersonic expansion (about six million miles per hour) of the stellar debris has created two X-ray emitting shock waves - one moving outward into the interstellar gas, and another moving back into the debris. These shock waves produce sudden, large changes in pressure and temperature, like an extreme version of sonic booms produced by the supersonic motion of airplanes.

According to the standard theory, the outward-moving shock wave should be about 2 light years ahead of the stellar debris. What Chandra found instead is that the stellar debris has kept pace with the outer shock and is only about half a light year behind.

The most likely explanation for this behavior is that a large fraction of the energy of the outward-moving shock wave is going into the acceleration of atomic nuclei to speeds approaching the speed of light. The Chandra observations provide the strongest evidence yet that nuclei are indeed accelerated and that the energy contained in the high-speed nuclei in Tycho's remnant is about 100 times that observed in high-speed electrons.

This finding is important for understanding the origin of cosmic rays, the high-energy nuclei which pervade the Galaxy and constantly bombard the Earth. Since their discovery in the early years of the 20th century, many sources of cosmic rays have been proposed, including flares on the sun and similar events on other stars, pulsars, black hole accretion disks, and the prime suspect - supernova shock waves. Chandra's observations of Tycho's supernova remnant strengthen the case for this explanation.

Fast Facts for Tycho's Supernova Remnant:
Credit  NASA/CXC/Rutgers/J.Warren & J.Hughes et al.
Scale  Image is 10.5 arcmin across.
Category  Supernovas & Supernova Remnants
Coordinates (J2000)  RA 00h 25m 17s | Dec +64 08' 37
Constellation  Cassiopeia
Observation Dates  29 Apr 2003
Observation Time  41 hours
Obs. IDs  3837
Color Code  Energy: Red 0.95-1.26 keV, Green 1.63-2.26 keV, Blue 4.1-6.1 keV
Instrument  ACIS
Also Known As G120.1+01.4, SN 1572
References tycho
Distance Estimate  About 13,000 light years
Release Date  September 22, 2005