SN 2008D

Source: Wikipedia, the free encyclopedia.
SN 2008D
Colour (B-V)
Unknown
Notable featuresFirst supernova detected by the X-rays released very early on in its formation.
Other designationsSN 2008D
  Related media on Commons
]
SWIFT images galaxy NGC 2770 with SN 2007uy before SN 2008D, with X-ray view (left) and visible light (right).

SN 2008D is a

Alicia Soderberg and Edo Berger, and Albert Kong and Tom Maccarone independently using Swift.[1] They alerted eight other orbiting and ground-based observatories to record the event. This was the first time that astronomers have ever observed a supernova as it occurred.[2][3][4]

The supernova was determined to be of Type Ibc. The velocities measured from SN2008D indicated expansion rates of more than 10,000 kilometers per second. The explosion was off-center, with gas on one side of the explosion moving outward faster than on the other. This was the first time the X-ray emission pattern of a supernova (which only lasted about five minutes) was captured at the moment of its birth. Now that it is known what X-ray pattern to look for, the next generation of X-ray satellites is expected to find hundreds of supernovae every year exactly when they explode, which will allow searches for neutrino and gravitational wave bursts that are predicted to accompany the collapse of stellar cores and the birth of neutron stars.

See also

References

  1. ^
    S2CID 453215
  2. ^ "SN 2008D: First Supernova Observed Live". Universe for Facts. Retrieved 21 December 2014.
  3. ^ "Supernova Birth Seen For First Time". ScienceDaily. 21 May 2008.
  4. ^ "Birth cry of a supernova". Discover Magazine. 21 May 2008. Archived from the original on 20 July 2008. Retrieved 12 October 2008.

External links