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
Chandra 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
SXP 1062 Animations
Click for low-resolution animation
Tour of SXP 1062
Quicktime MPEG
The Milky Way galaxy has several small satellite galaxies very close to it. One of them is called the Small Magellanic Cloud. Astronomers using several telescopes - including the Chandra X-ray Observatory - spotted an unusual object in the SMC. The source is known as SXP 1062 and may be the first pulsar found within the remains of a supernova explosion. X-ray data from Chandra and XMM-Newton also show that SXP 1062 is rotating unusually slowly - about once every 18 minutes. In contrast, some pulsars are found to revolve multiple times per second, including most newly born pulsars. Scientists have determined the pulsar was born between ten and forty thousand years ago. While this may sound like a long time, it is a blink of an eye in astronomical terms. Therefore, it is a mystery why SXP 1062 has been able to slow down by so much, so quickly.
[Runtime: 01:12]

(Credit: NASA/CXC/A. Hobart)


Return to SXP 1062 (December 20, 2011)