Images by Date
Images by Category
Solar System
Stars
Exoplanets
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
Photo Blog
Top Rated Images
Image Handouts
Desktops
Fits Files
Visual descriptions
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
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
G350.1-0.3 Animations
Click for low-resolution animation
Tour of G350.1-0.3
Quicktime MPEG
G350.1+0.3 is a young and exceptionally bright supernova remnant located nearly 15,000 light years from Earth toward the center of the Milky Way. While many supernova remnants are nearly circular, G350.1+0.3 has a strikingly unusual appearance. X-rays from Chandra and infrared data from Spitzer outline this bizarre shape, which astronomers think comes from the stellar debris field expanding into a nearby cloud of cold gas. With an age of between 600 and 1,200 years old, G350.1+0.3 is in the same time frame as other famous supernovas that formed the Crab and SN 1006 supernova remnants. However, it is unlikely that anyone on Earth would have seen the explosion because too much gas and dust lies along our line of sight to the remnant, blocking the view.
[Runtime: 00:59]

(Credit: NASA/CXC/A. Hobart)



Return to G350.1-0.3 (February 1, 2012)