Images by Date
Images by Category
Solar System
White Dwarfs
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Galaxy Clusters
Cosmology/Deep Field
Images by Interest
Space Scoop for Kids
Sky Map
Photo Blog
Top Rated Images
Image Handouts
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
More Information
Supernovas & Supernova Remnants
Neutron Stars/X-ray Binaries
X-ray Astronomy Field Guide: Neutron Stars/X-ray Binaries
Questions and Answers: Neutron Stars/X-ray Binaries
Chandra Images: Neutron Stars/X-ray Binaries
Related Podcasts
Tour: NASA's Chandra Releases Doubleheader of Blockbuster Hits
Download Image

More Information
Handout: html | pdf

More Images
RCW 103 with Scale Bar

Animation & Video

More Releases
RCW 103
RCW 103
(08 Sep 16)

Related Images
RCW 86
(18 Sep 06)
(02 Jun 04)
(29 Nov 06)
RCW 103:
A Star with a Mystery Partner?

Credit: NASA/CXC/Penn State/G.Garmire et al

When stars are more massive than about 8 times the Sun, they end their lives in a spectacular explosion called a supernova. The outer layers of the star are hurtled out into space at millions of miles per hour, leaving a debris field of gas and dust. Where the star once was located, a small, incredibly dense object called a neutron star is often found. While only 10 miles or so across, the tightly packed neutrons in such a star contain more mass than the entire Sun.

A new X-ray image shows the 2,000 year-old-remnant of such a cosmic explosion, known as RCW 103, which occurred about 10,000 light years from Earth. In Chandra's image, the colors of red, green, and blue are mapped to low, medium, and high-energy X-rays. At the center, the bright blue dot is likely the neutron star that astronomers believe formed when the star exploded. For several years astronomers have struggled to understand the behavior of the this object, which exhibits unusually large variations in its X-ray emission over a period of years. New evidence from Chandra implies that the neutron star near the center is rotating once every 6.7 hours, confirming recent work from XMM-Newton. This is much slower than a neutron star of its age should be spinning. One possible solution to this mystery is that the massive progenitor star to RCW 103 may not have exploded in isolation. Rather, a low-mass star that is too dim to see directly may be orbiting around the neutron star. Gas flowing from this unseen neighbor onto the neutron star might be powering its X-ray emission, and the interaction of the magnetic field of the two stars could have caused the neutron star to slow its rotation.

Fast Facts for RCW 103:
Credit  NASA/CXC/Penn State/G.Garmire et al
Scale  Image is 11.9 arcmin across
Category  Supernovas & Supernova Remnants , Neutron Stars/X-ray Binaries
Coordinates (J2000)  RA 16h 17m 36.30s | Dec -51° 02´ 24.40"
Constellation  Norma
Observation Dates  02/08/2000 and 03/03/2002
Observation Time  18 hours and 53 minutes
Obs. IDs  970, 2759
Color Code  Red (0.3 - 0.7 keV); Green (0.7 - 1.69 keV); Blue (1.69 - 3 keV)
Instrument  ACIS
References G. Garmire et al. 2006, 36th COSPAR Scientific Assembly. p.3451
Distance Estimate  About 10,700 light years
Release Date  July 10, 2007