Astronomy:SN 2006gy

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Short description: 2006 hypernova in constellation Perseus
SN 2006gy
Sn2006gy CHANDRA x-ray.jpg
SN 2006gy and the core of its home galaxy, NGC 1260, viewed in x-ray light from the Chandra X-ray Observatory. The NGC 1260 galactic core is on the lower left and SN 2006gy is on the upper right.
Spectral classIIn[1]
Date18 September 2006
ConstellationPerseus
Right ascension 03h 17m 27.10s[2]
Declination+41° 24′ 19.50″[2]
EpochJ2000
Galactic coordinates150.2568 -13.5916
Distance238,000,000 Ly (73 Mpc)[3]
RemnantN/A
HostNGC 1260
ProgenitorHypergiant in NGC 1260 galaxy
Progenitor typeHypergiant star very similar to Eta Carinae
Colour (B-V)−0.50 ~ +1.60
Notable featuresis located 2.0" W and 0.4" N of the center of NGC 1260
Peak apparent magnitude+14.2
[edit on Wikidata]

SN 2006gy was an extremely energetic supernova, also referred to as a hypernova or quark-nova,[4] that was discovered on September 18, 2006. It was first observed by Robert Quimby and P. Mondol,[2][5] and then studied by several teams of astronomers using facilities that included the Chandra, Lick, and Keck Observatories.[6][7] In May 2007 NASA and several of the astronomers announced the first detailed analyses of the supernova, describing it as the "brightest stellar explosion ever recorded".[8] In October 2007 Quimby announced that SN 2005ap had broken SN 2006gy's record as the brightest-ever recorded supernova, and several subsequent discoveries are brighter still.[9][10] Time magazine listed the discovery of SN 2006gy as third in its Top 10 Scientific Discoveries for 2007.[11]

Characteristics

Light curve of SN 2006gy (uppermost intermittent squares) compared with other types of supernovae

SN 2006gy occurred in a distant galaxy (NGC 1260), approximately 238 million[3] light-years (73 megaparsecs) away. The energy radiated by the explosion has been estimated at 1051 ergs (1044 J), making it a hundred times more powerful than the typical supernova explosion which radiates 1049 ergs (1042 J) of energy. Although at its peak the SN 2006gy supernova was intrinsically 400 times as luminous as SN 1987A, which was bright enough to be seen by the naked eye, SN 2006gy was more than 1,400 times as far away as SN 1987A, and too far away to be seen without a telescope.

SN 2006gy is classified as a type II supernova because it showed lines of hydrogen in its spectrum, although the extreme brightness indicates that it is different from the typical type II supernova. Several possible mechanisms have been proposed for such a violent explosion, all requiring a very massive progenitor star.[10] The most likely explanations involve the efficient conversion of explosive kinetic energy to radiation by interaction with circumstellar material, similar to a type IIn supernova but on a larger scale. Such a scenario might occur following mass loss of 10 or more M☉ in a luminous blue variable eruption, or through pulsational pair instability ejections.[12] Denis Leahy and Rachid Ouyed, Canadian scientists from the University of Calgary, have proposed that SN 2006gy was the birth of a quark star.[13]

Similarity to Eta Carinae

Eta Carinae (η Carinae or η Car) is a highly luminous hypergiant star located approximately 7,500 light-years from Earth in the Milky Way galaxy. Since Eta Carinae is 32,000 times closer than SN 2006gy, the light from it will be about a billion-fold brighter. It is estimated to be similar in size to the star which became SN 2006gy. Dave Pooley, one of the discoverers of SN 2006gy, says that if Eta Carinae exploded in a similar fashion, it would be bright enough that one could read by its light on Earth at night, and would even be visible during the daytime. SN 2006gy's apparent magnitude (m) was 15,[2] so a similar event at Eta Carinae will have an m of about −7.5. According to astrophysicist Mario Livio, this could happen at any time, but the risk to life on Earth would be low.[14]

  • This diagram illustrates the pair-instability process that astronomers think triggered the explosion in SN 2006gy. A sufficiently massive star can produce gamma rays of such high energy that some of the photons convert into pairs of electrons and positrons causing a runaway reaction which destroys the star.

  • SN2006gy (top right) in infrared

  • SN2006gy (top right) in ultraviolet

  • NASA artist's impression of the explosion of SN 2006gy

References

  1. ↑ Gal-Yam, A. (2012). "Luminous Supernovae". Science 337 (6097): 927–32. doi:10.1126/science.1203601. PMID 22923572. Bibcode: 2012Sci...337..927G. 
  2. ↑ 2.0 2.1 2.2 2.3 "List of Supernovae". http://www.cbat.eps.harvard.edu/lists/Supernovae.html. Retrieved 2011-01-08. 
  3. ↑ 3.0 3.1 "Fast Facts for SN2006gy". http://chandra.harvard.edu/photo/2007/sn2006gy/. Retrieved 2014-04-30. 
  4. ↑ Leahy, Denis A. (2008). "Superluminous Supernovae SN2006gy, SN2005gj and SN2005ap: Signs for a New Explosion Mechanism". American Astronomical Society 212: 255. Bibcode: 2008AAS...212.6401L. 
  5. ↑ IAU Circular No. 8754 , accessed May 8, 2007
  6. ↑ Ofek, E. O.; Cameron, P. B.; Kasliwal, M. M.; Gal-Yam, A.; Rau, A.; Kulkarni, S. R.; Frail, D. A.; Chandra, P. et al. (2007). "SN 2006gy: An Extremely Luminous Supernova in the Galaxy NGC 1260". The Astrophysical Journal 659 (1): L13–L16. doi:10.1086/516749. Bibcode: 2007ApJ...659L..13O. 
  7. ↑ Smith, Nathan; Li, Weidong; Foley, Ryan J.; Wheeler, J. Craig; Pooley, David; Chornock, Ryan; Filippenko, Alexei V.; Silverman, Jeffrey M. et al. (2007). "SN 2006gy: Discovery of the Most Luminous Supernova Ever Recorded, Powered by the Death of an Extremely Massive Star like η Carinae". The Astrophysical Journal 666 (2): 1116–1128. doi:10.1086/519949. Bibcode: 2007ApJ...666.1116S. 
  8. ↑ NASA's Chandra Sees Brightest Supernova Ever , NASA Press Release on the Discovery, May 7, 2007
  9. ↑ Stevenson, D. S. (2014). "The Mysterious SN 2005ap and Luminous Blue Flashes". Extreme Explosions. Astronomers' Universe. pp. 239–251. doi:10.1007/978-1-4614-8136-2_10. ISBN 978-1-4614-8135-5. 
  10. ↑ 10.0 10.1 Quimby, R. M. (2012). "Superluminous Supernovae". Proceedings of the International Astronomical Union 7: 22–28. doi:10.1017/S174392131201263X. Bibcode: 2012IAUS..279...22Q. 
  11. ↑ "Top 10 Scientific Discoveries: #3. Brightest Supernova Recorded" , Time (magazine) , 2007
  12. ↑ Smith, N.; Chornock, R.; Silverman, J. M.; Filippenko, A. V.; Foley, R. J. (2010). "Spectral Evolution of the Extraordinary Type IIn Supernova 2006gy". The Astrophysical Journal 709 (2): 856–883. doi:10.1088/0004-637X/709/2/856. Bibcode: 2010ApJ...709..856S. 
  13. ↑ Leahy, Denis; Ouyed, Rachid (2008). "Supernova SN2006gy as a first ever Quark Nova?". Monthly Notices of the Royal Astronomical Society 387 (3): 1193. doi:10.1111/j.1365-2966.2008.13312.x. Bibcode: 2008MNRAS.387.1193L. 
  14. ↑ "Megastar explodes in brightest supernova ever seen". Reuters. 2007. https://www.cnet.com/news/megastar-explodes-in-brightest-supernova-ever-seen/. Retrieved 2007-05-07. 

External links

Coordinates: Sky map 03h 17m 27.10s, +41° 24′ 19.50″



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