GRB 101225A
Event typeGamma-ray burst Edit this on Wikidata
ConstellationAndromeda Edit this on Wikidata
Right ascension00h 00m 47.51s
Declination+44° 36′ 01.1″
Distance5,500,000,000 ly (1.7×109 pc)
Other designationsGRB 101225A

GRB 101225A, also known as the "Christmas burst", was a cosmic explosion first detected by NASA's Swift observatory on Christmas Day 2010. The gamma-ray emission lasted at least 28 minutes, which is unusually long. Follow-up observations of the burst's afterglow by the Hubble Space Telescope and ground-based observatories were unable to determine the object's distance using spectroscopic methods.

In papers published in the journal Nature, two different groups of astronomers proposed different theories about the event's origin. Sergio Campana's group proposes that the event was caused by a comet crashing onto a neutron star within our own galaxy. Christina Thöne's group prefers a more conventional supernova mechanism, involving a merger between a helium star and a neutron star at a distance of about 5.5 billion light years from Earth.

Observations

The gamma ray burst, in the constellation Andromeda, was first detected by the NASA Swift Gamma-Ray Burst Mission at 18:38 UT on December 25, 2010. The gamma-ray emission had a duration of at least 28 minutes, which is unusually long. After news of the gamma-ray burst was sent to other observatories, the longer-wavelength "afterglow" of the burst was monitored by on-ground observatories and the Hubble Space Telescope.[1] After the unusually long duration of gamma emissions, x-ray emissions in the afterglow continued for just two days, an unusually short duration for this phase.[2] Optical emissions observed over the first 10 days were characterized as those of "an expanding, cooling blackbody with a large initial radius".[3] A faint light source appeared about 10 days after the burst and reached its maximum brightness 30 days after its appearance; observers described this light source as looking like a supernova.[4]

On January 6, 2011, the 10m Keck-I telescope equipped with the Low Resolution Imaging Spectrometer (LRIS) conducted spectroscopic measurements of the host galaxy of GRB 101225A. A 900s spectrum was obtained; it consisted of blue and red channels, covering the wavelength ranges ~320–550 nm and ~500–820 nm, respectively.[5] Isotropic energy was estimated at (7.8 ± 1.6)×1050 erg from the Burst Alert Telescope (BAT) data.[6]

The unusual characteristics of the afterglow led astronomers to generate novel hypotheses to explain the event.[2] Observers were unable to ascertain the burst's distance from Earth, and the two alternative hypotheses of its origin place the event at radically different distances.[1]

Hypotheses

Christina Thöne, of the Institute of Astrophysics of Andalusia in Spain, was lead author of a paper that proposed that the burst occurred in a binary system where a neutron star orbited a normal helium star that had just entered its red giant phase, which had enormously expanded its outer atmosphere.[7] During the expansion, the red giant star engulfed the neutron star, resulting in both the ejection of the giant's atmosphere and rapid tightening of the neutron star's orbit. Once the two stars became wrapped in a common envelope of gas, the neutron star may have merged with the giant's core after just five orbits, or about 18 months. The end result of the merger was the birth of a black hole or a magnetar and the production of oppositely directed jets of particles moving at nearly the speed of light, followed by a weak supernova, a common envelope jets supernova. The particle jets produced gamma rays. Jet interactions with gas ejected before the merger explain much of the burst's different nature. Based on this interpretation, the event took place about 5.5 billion light-years away (redshift 0.33), and the team has detected what may be a faint galaxy at the right location.[1][8]

An alternative hypothesis, offered by a team led by Sergio Campana of the Brera Astronomical Observatory (INAF), proposes that GRB 101225A was produced by a comet-like object that fell into a neutron star located in our own galaxy, only some 10,000 light-years from Earth.[1] In this model, the comet-like object falls onto the neutron star and is disrupted by tidal forces. Hard X-ray emission (the burst) results from the first matter falling onto the neutron star. X-ray emission and initial variations detected by Swift are attributed to clumps of material striking the star as the disc formed around it. Then the disk cools down and emits only at UV and optical wavelengths.[9]

More recently, at the 2013 Huntsville Gamma-ray Burst Symposium, several scientists proposed that GRB 101225A, along with GRB 111209A and 121027A are part of a new class of gamma ray bursts, termed ultra-long bursts and caused by the collapse of low metallicity blue supergiant stars.

Andrew Levan and his colleagues used the Gemini North Telescope to determine that GRB 101225A was 7 billion light years distant [10][11][12] much further than original estimates. This greater distance gives it a much higher energy level, which combined with longer duration and an absence of a supernova signature have led scientists, such as Bruce Gendre to suggest that these ultra-long bursts are the result of collapsing blue supergiant stars.[13][14]

Significance

Astrophysicist Sergio Campana told Space.com that he thinks this was "the discovery of a completely new astrophysical phenomenon that [had] not been envisaged before." He also said, "If tidal disruption of minor bodies around neutron stars is really happening", this event would not be "unique".[15] Christina Thöne has said, "What the Christmas burst seems to be telling us is that the family of gamma-ray bursts is more diverse than we fully appreciate."[1]

References

  1. 1 2 3 4 5 "NASA's Swift Finds a Gamma-Ray Burst With a Dual Personality". NASA. November 30, 2011. Retrieved December 1, 2011.
  2. 1 2 "Mysterious Christmas Day "Starburst" Explained?". Victoria Jaggard. National Geographic. November 30, 2011. Archived from the original on December 1, 2011. Retrieved December 11, 2011.
  3. ↑ C. Thöne; A. de Ugarte Postigo; C. Fryer; K. Page; J. Gorosabel; M. A. Aloy; D. Perley; C. Kouveliotou; H. T. Janka; the Christmas burst collaboration (November 2011). "GRB 101225A – an unusual stellar death on Christmas Day" (abstract of presentation). La Palma, Canary Islands, Spain: Fourth "Science with the GTC" Meeting. Retrieved December 10, 2011. {{cite journal}}: Cite journal requires |journal= (help)
  4. ↑ "Cosmic Explosion Explained Just in Time for Christmas; Texas-Korea Astronomical Partnership Contributes". McDonald Observatory. Retrieved December 10, 2011.
  5. ↑ Dong Xu, Weizmann Institute (January 6, 2011). "GCN CIRCULAR Number 11522". Retrieved December 11, 2011.
  6. ↑ Palmer; et al. (December 26, 2010). "GCN CIRCULAR Number 11500". Retrieved December 11, 2011.
  7. ↑ Thöne, C. C.; A. de Ugarte Postigo, C. L. Fryer, K. L. Page, J. Gorosabel, M. A. Aloy, D. A. Perley, C. Kouveliotou, H. T. Janka, P. Mimica, J. L. Racusin, H. Krimm, J. Cummings, S. R. Oates, S. T. Holland, M. H. Siegel, M. De Pasquale, E. Sonbas, M. Im, W.-K. Park, D. A. Kann, S. Guziy, L. Hernández García, A. Llorente, K. Bundy; et al. (November 30, 2011). "The unusual γ-ray burst GRB 101225A from a helium star/neutron star merger at redshift 0.33". Nature. 480 (7375): 72–74. arXiv:1105.3015. Bibcode:2011Natur.480...72T. doi:10.1038/nature10611. PMID 22129726. S2CID 4423462.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  8. ↑ Charles Q. Choi (November 30, 2011). "Competing Explanations Proposed for Strange Christmas Space Explosion". SPACE.com. Retrieved December 1, 2011.
  9. ↑ Campana, S.; Lodato, G.; d’Avanzo, P.; Panagia, N.; Rossi, E. M.; Valle, M. Della; Tagliaferri, G.; Antonelli, L. A.; Covino, S.; et al. (2011). "The unusual gamma-ray burst GRB 101225A explained as a minor body falling onto a neutron star". Nature. 480 (7375): 69–71. arXiv:1112.0018. Bibcode:2011Natur.480...69C. doi:10.1038/nature10592. PMID 22129725. S2CID 205226843.
  10. ↑ Levan, A. J.; Tanvir, N. R.; Starling, R. L. C.; Wiersema, K.; Page, K. L.; Perley, D. A.; Schulze, S.; Wynn, G. A.; Chornock, R.; Hjorth, J.; Cenko, S. B.; Fruchter, A. S.; O'Brien, P. T.; Brown, G. C.; Tunnicliffe, R. L.; Malesani, D.; Jakobsson, P.; Watson, D.; Berger, E.; Bersier, D.; Cobb, B. E.; Covino, S.; Cucchiara, A.; De Ugarte Postigo, A.; Fox, D. B.; Gal-Yam, A.; Goldoni, P.; Gorosabel, J.; Kaper, L.; et al. (2014). "A New Population of Ultra-Long Duration Gamma-Ray Bursts". The Astrophysical Journal. 781 (1): 13. arXiv:1302.2352. Bibcode:2014ApJ...781...13L. doi:10.1088/0004-637X/781/1/13. S2CID 24657235.
  11. ↑ Dying Supergiant Stars Implicated in Hours-long Gamma-Ray Bursts http://www.nasa.gov/mission_pages/swift/bursts/supergiant-stars.html April 16, 2013. Retrieved April 18, 2013.
  12. ↑ Strange new bursts of gamma-rays point to a new way to destroy a star, http://www2.warwick.ac.uk/newsandevents/grb, April 16, 2013. Retrieved April 18, 2013.
  13. ↑ Dying Supergiant Stars Implicated in Hours-long Gamma-Ray Bursts http://www.nasa.gov/mission_pages/swift/bursts/supergiant-stars.html April 16, 2013. Retrieved April 18, 2013.
  14. ↑ Gendre, B.; Stratta, G.; Atteia, J. L.; Basa, S.; Boër, M.; Coward, D. M.; Cutini, S.; d'Elia, V.; Howell, E. J.; Klotz, A.; Piro, L. (2013). "The Ultra-Long Gamma-Ray Burst 111209A: The Collapse of a Blue Supergiant?". The Astrophysical Journal. 766 (1): 30. arXiv:1212.2392. Bibcode:2013ApJ...766...30G. doi:10.1088/0004-637X/766/1/30. S2CID 118618287.
  15. ↑ Charles Q. Choi (November 30, 2011). "What caused explosion that lit up Christmas sky". NBC News. Retrieved December 10, 2011.
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