Chandra X-ray Observatory - HomeAbout The ChandraEducational MaterialsField GuidePhoto AlbumPress RoomResources
Chandra X-ray Observatory - HomeChandra Education Material - You are here
ObservatoryClassroom-Ready ActivitiesBackgroundGalactic NavigationChandra 101Tracking ChandraAsk an ExpertInteractive GamesPrintable MaterialsEducation Links
Web Site ToolsVisit the Chandra ChroniclesEmail NewsletterSite MapNew & NoteworthyImage Use PolicyQuestions & AnswersGlossaryDownload Guide

Cassiopeia A Composite Image Gallery

This page can be used in conjunction with any of the investigations, tasks, or activities in this section which ask students to compare and contrast images of an object in different wavelengths. These include the CAS Timeline investigation, and the perfomance tasks "Signals from the Cosmos", "Point of View", "The universe Rated R!", and "Portrait Gallery of the X-Ray Universe".

Cassiopeia A, or Cas A is the remnant of a massive star that exploded around three hundred years ago. These images show Cas A as viewed by four different types of telescopes.

You can view composited images by selecting the combinations you would like to see from the pull down menu on the right and then clicking the "Get Composite" button.

Cas A Image


Cas A X-Ray
Cas A in the X-ray range of the spectrum.The X-ray image shows an expanding shell of hot gas produced by the explosion. This gaseous shell is about 10 light years in diameter, and has a temperature of about 50 million degrees.

Cas A Optical
Cas A in the optical range of the spectrum. The optical image of Cas A shows matter with a temperature of about ten thousand degrees. Some of these wisps contain high concentrations of heavy elements and are thought to be dense clumps of ejected stellar material.

Cas A Infrared
Cas A in the infrared range of the spectrum. The infrared image of Cas A shows dust grains that have been swept up and heated to several hundred degrees by the expanding hot gas. It is not known whether the dust grains were ejected by the star millions of years before it exploded or during the explosion.

Cas A Radio
Cas A in the radio range of the spectrum. Cas A gets its name from radio astronomers, who 'rediscovered' it in 1948 as the strongest radio source in the constellation of Cassiopeia. About 5 years later optical astronomers found the faint wisps, and it was determined that Cas A is the remnant of an explosion that occurred about 300 years ago. The radio emission comes from high-energy electrons moving in large spirals around magnetic field

Cas A Overlays | Cas A Timeline Activity | Cas A Photo Album


separator line
CXC Home | Search | Help | Site Map | Image Use Policy | Privacy & Accessibility | Downloads & Plugins
Latest Images | New & Noteworthy | Multimedia | Flash Ecards | Glossary | Q&A | Guestbook


RSS Feed RSS Feed | Podcast Podcast | Blog Blog

[News by email: Chandra Digest]
[Contact us: cxcpub@cfa.harvard.edu]
NASA's Home Page Smithsonian's Home Page CXC Home Page Image Map for NASA's, Smithsonian and Chandra's Home Pages
Harvard-Smithsonian Center for Astrophysics
60 Garden Street, Cambridge, MA 02138 USA
Phone: 617.496.7941 Fax: 617.495.7356


Text Size:
normal font large font larger font
Chandra X-ray Center, Operated for NASA by the Smithsonian Astrophysical Observatory
This site was developed with funding from NASA under Contract NAS8-03060.
Revised: August 29, 2006