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
Tycho's Supernova Remnant: NASA'S Chandra Finds New Evidence on Origin of Supernovas
tycho2
Tycho's Supernova Remnant
Tycho's Supernova Remnant
Tycho's Supernova Remnant

  • An arc of emission just found in the Tycho supernova remnant provides evidence for what triggered the original explosion.

  • Astronomers think that a shock wave created the arc when a white dwarf exploded and blew material off the surface of a nearby companion star.

  • Tycho belongs to a category of supernovas that are used to measure the expansion of the Universe.

This new image of Tycho's supernova remnant, dubbed Tycho for short, contains striking new evidence for what triggered the original supernova explosion, as seen from Earth in 1572. Tycho was formed by a Type Ia supernova, a category of stellar explosion used in measuring astronomical distances because of their reliable brightness.

Low and medium energy X-rays in red and green show expanding debris from the supernova explosion. High energy X-rays in blue reveal the blast wave, a shell of extremely energetic electrons. Also shown in the lower left region of Tycho is a blue arc of X-ray emission. Several lines of evidence support the conclusion that this arc is due to a shock wave created when a white dwarf exploded and blew material off the surface of a nearby companion star (see accompanying illustration below). Previously, studies with optical telescopes have revealed a star within the remnant that is moving much more quickly than its neighbors, hinting that it could be the companion to the supernova that was given a kick by the explosion.

Tycho

Other details of the arc support the idea that it was blasted away from the companion star. For example, the X-ray emission of the remnant shows an apparent "shadow" next to the arc, consistent with the blocking of debris from the explosion by the expanding cone of material stripped from the companion. This shadow is most obvious in very high energy X-rays showing iron debris.

These pieces of evidence support a popular scenario for triggering a Type Ia supernova, where a white dwarf pulls material from a "normal," or Sun-like, companion star until a thermonuclear explosion occurs. In the other main competing theory, a merger of two white dwarfs occurs, and in this case, no companion star or evidence for material blasted off a companion, should exist. Both scenarios may actually occur under different conditions, but the latest Chandra result from Tycho supports the former one.

The shape of the arc is different from any other feature seen in the remnant. Other features in the interior of the remnant include recently announced stripes, which have a different shape and are thought to be features in the outer blast wave caused by cosmic ray acceleration.

Fast Facts for Tycho's Supernova Remnant:
Credit  NASA/CXC/Chinese Academy of Sciences/F. Lu et al
Release Date  April 26, 2011
Scale  Image is 10 arcmin across (about 38 light years)
Category  Supernovas & Supernova Remnants
Coordinates (J2000)  RA 00h 25m 17s | Dec +64° 08' 37"
Constellation  Cassiopeia
Observation Date  2 pointings between April 29, 2003 and May 3, 2009
Observation Time  283 hours
Obs. ID  3837, 7639, 8551, 10093-10097; 10902-10904; 10906
Instrument  ACIS
Also Known As G120.1+01.4, SN 1572
References Lu, F.J. et al, 2011, ApJ, 732:11
Color Code  Energy: Red 1.6-2.0 keV, Green 2.2-2.6 keV, Blue 4-6 keV
X-ray
Distance Estimate  About 13,000 light years
distance arrow
Visitor Comments (15)

Keep following this type of supernovas it's so interesting and they are one of the most powerful phenomenons in the universe and at the end thanks a lot Chandra

Posted by NASAFan on Friday, 10.3.14 @ 11:26am


I had no clue that stars could explode!! o.o

Posted by Sarita on Friday, 05.17.13 @ 09:57am


Brilliant article & imagery. Makes me wish I was an astrophysicist. Thank you for posting and explaining this fascinating discovery for all to see.
Space is indeed the final frontier!

Posted by Bryan on Thursday, 11.3.11 @ 13:51pm


Amazing!! How wonderful is the Universe.

Posted by Pax on Tuesday, 07.19.11 @ 05:15am


Extremely concise, precise, well-written and explanatory text, with meaningful links.
Congratulations

Posted by Pierre Maes on Tuesday, 05.24.11 @ 20:50pm


Does it not have angular momentum? The clouds are not layered. Photo pond splash ripples, some of the interior ripples undergo entropy, the rest undergoes expansion contraction. For some objects.

Posted by J. J. Madson on Friday, 05.13.11 @ 22:04pm


What is the size of this object in kilometers?

Posted by DNA on Saturday, 04.30.11 @ 21:30pm


We live in the wondrous time of space exploration. We get to see some of the most astonishing sights of this amazing universe we are a part of, a very small part.
Thanks for the great visuals

Posted by G T White on Saturday, 04.30.11 @ 14:32pm


Thanks for the beautiful work and explanation clear enough for a humanities teacher to understand. By the way, I saw this through APOD.

Posted by G. Woodruff on Saturday, 04.30.11 @ 08:22am


What is the pin-point object in the upper left part of the image. Surely a SN-Ia doesn't leave a neutron star, and the image is made from detections in X-ray so it would have to be an x-ray bright object.

Posted by Excalibur on Saturday, 04.30.11 @ 08:10am


Fascinating.

Posted by Spock on Saturday, 04.30.11 @ 07:58am


The most amazing thing I've seen in weeks. I learned a huge amount from your informative well written and well illustrated page.
Thank you

Posted by Peter Beck on Saturday, 04.30.11 @ 03:18am


Wow

Posted by sao on Friday, 04.29.11 @ 13:13pm


My first thought when I looked at the remnant of the supernova was my neighbors 3 year old son Charlie
fifty years ago. The little boy had curly hair and this really floored me. I have Chandra reports that are very interesting and I have many discussions based on your info and pictures sent to me. Friends who never showed interest in anything in space other than the NASA flights have become weekend panelist on Chandra submissions.
Thank U

Posted by Len Gyson on Friday, 04.29.11 @ 10:53am


Most interesting discovery. Ever since the space telescopes were put into orbit, so much has been discovered about this most marvelous universe we live in.
The new discoveries never cease to blow my mind. Eagerly awaiting the next mind blowing discovery.

Marvin L. S.

Posted by Marvin L. S. on Tuesday, 04.26.11 @ 20:34pm


Rate This Image

Rating: 3.8/5
(880 votes cast)
Download & Share

More Information
More Images
Low X-ray Image of
Tycho's Supernova Remnant
Jpg, Tif
X-ray

More Images
Animation & Video
Tour of Tycho's Supernova Remnant
animation

More Animations
More Releases
Related Images
Cassiopeia A
Cassiopeia A
(23 Feb 11)

SN 1006
SN 1006
(01 Jul 08)


Related Information
Related Podcast
Top Rated Images
Data Sonification

30 Doradus B

Brightest Cluster Galaxies




FaceBookTwitterYouTubeFlickr