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
Space Scoop 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
M82 SN2014J: NASA's Chandra Observatory Searches for Trigger of Nearby Supernova

  • Chandra data is being used to help determine what caused SN 2014J to explode.

  • Astronomers first spotted SN 2014J in the M82 galaxy on January 21, 2014, making it one of the closest supernovas discovered in decades.

  • SN 2014J is a Type Ia supernova, an important class of objects used to measure the expansion of the Universe.

  • The non-detection of X-rays from Chandra gives information about the environment around the star before SN 2014J exploded.

New data from NASA's Chandra X-ray Observatory has provided stringent constraints on the environment around one of the closest supernovas discovered in decades. The Chandra results provide insight into possible cause of the explosion, as described in our press release.

On January 21, 2014, astronomers witnessed a supernova soon after it exploded in the Messier 82, or M82, galaxy. Telescopes across the globe and in space turned their attention to study this newly exploded star, including Chandra. Astronomers determined that this supernova, dubbed SN 2014J, belongs to a class of explosions called "Type Ia" supernovas. These supernovas are used as cosmic distance-markers and played a key role in the discovery of the Universe's accelerated expansion, which has been attributed to the effects of dark energy. Scientists think that all Type Ia supernovas involve the detonation of a white dwarf. One important question is whether the fuse on the explosion is lit when the white dwarf pulls too much material from a companion star like the Sun, or when two white dwarf stars merge. This image contains Chandra data, where low, medium, and high-energy X- rays are red, green, and blue respectively. The boxes in the bottom of the image show close-up views of the region around the supernova in data taken prior to the explosion (left), as well as data gathered on February 3, 2014, after the supernova went off (right). The lack of X-rays detected by Chandra is an important clue for astronomers looking for the exact mechanism of how this star exploded.

The non-detection of X-rays reveals that the region around the site of the supernova explosion is relatively devoid of material. Astronomers expect that if a white dwarf exploded because it had been steadily collecting matter from a companion star prior to exploding, the mass transfer process would not be 100% efficient, and the white dwarf would be immersed in a cloud of gas. If a significant amount of material were surrounding the doomed star, the blast wave generated by the supernova would have struck it by the time of the Chandra observation, producing a bright X-ray source. Since they do not detect any X-rays, the researchers determined that the region around SN 2014J is exceptionally clean.

A viable candidate for the cause of SN 2014J must explain the relatively gas-free environment around the star prior to the explosion. One possibility is the merger of two white dwarf stars, in which case there might have been little mass transfer and pollution of the environment before the explosion. Another is that several smaller eruptions on the surface of the white dwarf cleared the region prior to the supernova. Further observations a few hundred days after the explosion could shed light on the amount of gas in a larger volume, and help decide between these and other scenarios.

A paper describing these results was published in the July 20 issue of The Astrophysical Journal and is available online. The first author is Raffaella Margutti from the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, MA, and the co-authors are Jerod Parrent (CfA), Atish Kamble (CfA), Alicia Soderberg (CfA), Ryan Foley (University of Illinois at Urbana-Champaign), Dan Milisavljevic (CfA), Maria Drout (CfA), and Robert Kirshner (CfA).

Fast Facts for M82 SN2014J:
Credit  NASA/CXC/SAO/R.Margutti et al
Release Date  August 14, 2014
Scale  Image is 12.75 arcmin across (42,000 light years)
Category  Normal Galaxies & Starburst Galaxies, Supernovas & Supernova Remnants
Coordinates (J2000)  RA 09h 55m 50.70s | Dec +69 40' 37.00"
Constellation  Ursa Major
Observation Date  22 pointings from 20 Sep 1999 to 03 Feb 2014
Observation Time  228 hours 26 min (9 days, 12 hours, 26 min).
Obs. ID  361, 378-380, 1302, 2933, 5644, 6097, 6361, 8190, 10025-10027, 10542-10545, 10925, 11104, 11800, 13796, 15616
Instrument  ACIS
References Margutti, R. et al, 2014, ApJ, 790, 52; arXiv:1405.1488
Color Code  Red (0.5-1.2 keV); Green (1.2-2.0 keV); Blue (2.0-7.0 kev)
X-ray
Distance Estimate  About 11.4 million light years
Visitor Comments (6)

This article was amazing but how eruptions on the surface of a white dwarf can clean the environment? In addition, what are the closest stars or black holes to SN2014J? Can't they have a role to clean the space around this new supernova?

Posted by NASAFan on Wednesday, 09.10.14 @ 13:02pm


This article about SN 2014J was the most interesting article so far. I really enjoy these new findings about our wonderful Universe. Keep up the good work.
Mark T. Milhous

Posted by Mark Milhous on Monday, 08.25.14 @ 22:01pm


It is nice to see this image from a supernova so closer and to know more about this kind of star. Thank you for your information.

Posted by corleone graciela on Sunday, 08.17.14 @ 11:56am


It appears the small box on the right middle side may be the entry point of whatever caused the explosion. Blue is right across from this point.
What is the red spot in lower left?

Posted by Susan on Friday, 08.15.14 @ 19:23pm


Outstanding.

Posted by james garland on Friday, 08.15.14 @ 16:50pm


Hi folks, we are not there yet, but we are getting there. Keep up the great work.
Alan Soden.

Posted by alan soden on Friday, 08.15.14 @ 15:07pm


Leave Your Comment

Name:

Email:

Comments:


 
 

Rules

Rate This Image

Rating: 2.9/5
(203 votes cast)
Download & Share

Desktops

1024x768 - 358.9 kb
1280x1024 - 537.7 kb
1680x1050 - 643 kb
More Information
Press Room: M82 SN2014J
Blog: M82 SN2014J
More Images
X-ray Image of M82 SN2014J
Jpg, Tif
X-ray

More Images
Animation & Video
Tour of M82 SN2014J
animation

More Animations
Related Images
SN2014J
SN 2014J
(27 Jan 14)

M82
M82
(13 Jan 11)

SN 1970G
SN 1970G
(29 Nov 05)


Related Information
Related Podcast
Top Rated Images
WASP-18

Eta Carinae

Puppis A




FaceBookTwitterYouTubeFlickr