Supernovae are powerful explosions of massive stars that have reached a terminal stage in their evolution. A huge amount of energy is released during the explosion in a wide range of wavelengths. The supernova explosion causes a sudden rise in the dead star’s luminosity which may outshine momentarily the entire galaxy in which it resides. The explosion is produced by a catastrophic collapse of the iron core of a massive star or the collapse of a white dwarf after accreting enough mass from its companion to reach the Chandrasekhar limit. The first record of a supernova occurrence goes back to 185 CE. Subsequently, humans have witnessed across the centuries a series of such violent events that appear suddenly in the sky and illuminate the darkness of the night for several weeks or months. In the first part of this paper, we briefly describe the processes that lead to a supernova explosion. In the second part, we discuss historical supernovae as appearing in the records of human civilizations. In the third part, we highlight ancient records relating the sudden appearance of a supernova or a comet to the spread of epidemics in certain regions of the world.
References
[1]
Woosley, S. and Janka, T.H. (2005) The Physics of Core-Collapse Supernovae. https://doi.org/10.1038/nphys172
[2]
Khokhlov, A.M., et al. (1999) Jet-Induced Explosions of Core Collapse Supernovae. The Astrophysical Journal, 524, L107. https://doi.org/10.1086/312305
[3]
Zhao, F.Y., Strom, R.G. and Jiang, S.Y. (2006) The Guest Star of AD185 Must Have Been a Supernova. Chinese Journal of Astronomy and Astrophysics, 6, 635-640. https://doi.org/10.1088/1009-9271/6/5/17
[4]
Stothers, R. (1977) Is the Supernova of A.D. 185 Recorded in Ancient Roman Literature? Isis, 68, 443-447. https://doi.org/10.1086/351822
[5]
NASA, JPL (2011) NASA Telescopes Help Solve Ancient Supernova Mystery. https://www.nasa.gov/mission_pages/spitzer/news/spitzer20111024.html
[6]
Williams, B.J., et al. (2011) RCW 86: A Type Ia Supernova in a Wind-Blown Bubble. The Astrophysical Journal, 741, 96. https://doi.org/10.1088/0004-637X/741/2/96
[7]
Clark, D.H. and Stephenson, F.R. (1976) Which Historical New Stars Were Supernovae? The Quarterly Journal of the Royal Astronomical Society, 17, 290.
[8]
Mizuno, D.R., et al. (2010) A Catalog of MIPSGAL Disk and Ring Sources. The Astronomical Journal, 139, 1542-1552. https://doi.org/10.1088/0004-6256/139/4/1542
[9]
Borkowski, K.J., Reynolds, S.P. and Roberts, M.S.E. (2016) G11.2-0.3: The Young Remnant of a Stripped-Envelope Supernova. The Astrophysical Journal, 819, 160. https://doi.org/10.3847/0004-637X/819/2/160
[10]
Kaspi, V.M., et al. (2001) Chandra X-Ray Observations of G11.2-0.3: Implications for Pulsar Ages. The Astrophysical Journal, 560, 372. https://doi.org/10.1086/322515
[11]
Tam, C. and Roberts, M.S.E. (2003) The Expansion of G11.2-0.3, a Radio Composite Supernova Remnant. The Astrophysical Journal Letters, 598, L27-L30. https://doi.org/10.1086/380557
[12]
Clark, D.H. and Stephenson, F.R. (1975) The Remnants of the Supernovae of AD 185 and AD 393. The Observatory, 95, 190-195.
[13]
Clark, D.H. and Stephenson, F.R. (1978) Application of Early Astronomical Records. Institute of Physics Publishing, London.
[14]
Wang, Z.-R. (2005) The Impact of Historical Chinese Astronomical Records. Astrophysics and Space Science, 305, 207-210. https://doi.org/10.1007/s10509-006-9187-8
[15]
Wang, Z.-R., Qu, Q.Y. and Chen, Y. (1998) The AD 393 Guest Star: The SNR RX 51713.7-3946. The Hot Universe. In: Koyama, K., Kitamoto, S. and Itoh, M., Eds., Proceedings of IAU Symposium #188, Kluwer Academic, Dordrecht, 262. https://doi.org/10.1007/978-94-011-4970-9_75
[16]
Berezhko, E.G. and Völk, H.J. (2010) Nonthermal and Thermal Emission from the Supernova Remnant RX J1713.7-3946. Astronomy and Astrophysics, 511, A34. https://doi.org/10.1051/0004-6361/200913312
[17]
National Optical Astronomy Observatory (2003) Astronomers Peg Brightness of History’s Brightest Star. Press Release. https://noirlab.edu/public/news/noao0305
[18]
Murdin, P. and Murdin, L. (1985) Supernovae. Cambridge University Press, Cambridge, 14-16.
[19]
Burnham, R. (1978) Celestial Handbook. Dover, New York, 1117-1122.
[20]
Rada, W. and Heuhaeuser, R. (2015) Supernova SN 1006 in Two Historic Yemeni Reports. Astronomische Nachrichten, 336, 249-257. https://doi.org/10.1002/asna.201412152
[21]
Than, K. (2006) Ancient Rock Art Depicts Exploding Star. Space.com. https://www.space.com/2458-ancient-rock-art-depicts-exploding-star.html
[22]
Goldstein, B.R. (1965) Evidence for a Supernova of A.D. 1006. The Astronomical Journal, 70,105-114. https://doi.org/10.1086/109679
[23]
Winkler, P.F., et al. (2002) The SN 1006 Remnant: Optical Proper Motions, Deep Imaging, Distance, and Brightness at Maximum. https://doi.org/10.1086/345985
[24]
Gardner, F.F. and Milne, D.K. (1965) The Supernova of A.D. 1006. The Astronomical Journal, 70, 754. https://doi.org/10.1086/109813
[25]
Green, D.A. (2014) A Catalogue of 294 Galactic Supernova Remnants. Bulletin of the Astronomical Society of India, 42, 47-58.
[26]
Acero, F., et al. (2010). First Detection of VHE γ-Rays from SN 1006 by HESS. Astronomy and Astrophysics, 516, A62. https://doi.org/10.1051/0004-6361/200913916
[27]
Wheeler, J.C. (2000) Cosmic Catastrophes: Supernovae, Gamma-Ray Bursts, and Adventures in Hyperspace. Cambridge University Press, Cambridge.
[28]
González Hernández, J.I., et al. (2012) No Surviving Evolved Companions of the Progenitor of SN1006. Nature, 489, 533-536. https://doi.org/10.1038/nature11447
[29]
Lampland, C.O. (1921) Observed Changes in the Structure of the “Crab” Nebula. Publications of the Astronomical Society of the Pacific, 33, 79-84. https://doi.org/10.1086/123039
[30]
Baade, W. and Zwicky, F. (1934) On Supernovae. Proceedings of the National Academy of Sciences, 20, 254-259. https://doi.org/10.1073/pnas.20.5.254
[31]
Zwicky, F. (1938) On Collapsed Neutron Stars. The Astrophysical Journal, 88, 522-525. https://doi.org/10.1086/144003
[32]
Mayall, N.U. (1939) The Crab Nebula, a Probable Supernova. Astronomical Society of the Pacific Leaflets, 3, 145-154.
[33]
Brill (n.d.) A Literary History of Medicine. Oxford Center for Islamic Studies, Oxford. https://www.oxcis.ac.uk/news/literary-history-of-medicine-the-uyun-al-anba-fi-tabaqat-al-atibba-of-ibn-abi-usaybiah
[34]
Collins, G.W., Claspy, W.P. and Martin, J.C. (1999) A Reinterpretation of Historical References to the Supernova of A.D. 1054. Publications of the Astronomical Society of the Pacific, 111, 871-880. https://doi.org/10.1086/316401
[35]
Dall’Olmo, U. (1980) Latin Terminology Relating to Aurorae, Comets, Meteors and Novae. Journal for the History of Astronomy, 11, 10-27. https://doi.org/10.1177/002182868001100103
[36]
Williams, L.P. (1981) The Supernova of 1054: A Medieval Mystery. In: Woolf, H., Ed., The Analytic Spirit: Essays in the History of Science in Honor of Henry Guerlac, Cornell University Press, Ithaca, 329-349.
[37]
Guidoboni, E., Marmo, C. and Polcaro, V.F. (1994) Do We Need to Redate the Birth of the Crab Nebula? Memorie della Società Astronomia Italiana, 65, 623-637.
[38]
McCarthy, D. and Breen, A. (1997) An Evaluation of Astronomical Observations in the Irish Annals. Vistas in Astronomy, 41, 117-138. https://doi.org/10.1016/S0083-6656(96)00052-9
[39]
Stephenson, F.R. and Green, D.A. (2003) Was the Supernova of AD 1054 Reported in European History? Journal of Astronomical History and Heritage, 6, 46-52.
[40]
Breen, A. and McCarthy, D. (1995) A Re-Evaluation of the Eastern and Western Records of the Supernova of 1054. Vistas in Astronomy, 39, 363-379. https://doi.org/10.1016/0083-6656(95)96619-S
[41]
Stephenson, F.R. and Green, D.A. (2003) The Historical Supernovae.
[42]
Miller, W.C. (1955) Two Prehistoric Drawings of Possible Astronomical Significance. Astronomical Society of the Pacific Leaflets, 7, 105-112.
[43]
Panagia, N. and Weiler, K.W. (1980) The Absolute Magnitude and the Type Classification of SN 1181 Equals 3C58. Astronomy and Astrophysics, 82, 389-391.
[44]
Galas, C.M.F., Tuohy, I.R. and Garmire, G.P. (1980) Soft X-Ray Observations of the Supernova Remnants HB 3 and 3C58. The Astrophysical Journal Letters, 236, L13-L16. https://doi.org/10.1086/183188
[45]
Science Daily (2008) Blast from the Past: Astronomers Resurrect 16th-Century Supernova. https://www.sciencedaily.com/releases/2008/12/081203133809.htm
[46]
Dick, O.L. (1949) Aubrey’s Brief Lives. Edited from the Original Manuscript “Thomas Allen”. 5.
[47]
Huang, R. (1981) 1587, a Year of No Significance. Yale University Press, London.
[48]
Krause, O., et al. (2008) Tycho Brahe’s 1572 Supernova as a Standard Type Ia as Revealed by Its Light-Echo Spectrum. Nature, 456, 617-619. https://doi.org/10.1038/nature07608
[49]
Sharaf-Eldine, I. (n.d.) Rawh El-Rooh. Arabic Manuscript (Not Published).
[50]
Hayato, A., et al. (2010) Expansion Velocity of Ejecta in Tycho’s Supernova Remnant Measured by Doppler Broadened X-Ray Line Emission. The Astrophysical Journal, 725, 894-903. https://doi.org/10.1088/0004-637X/725/1/894
[51]
Kerzendorf, W.E., et al. (2013) A High-Resolution Spectroscopic Search for the Remaining Donor for Tycho’s Supernova. The Astrophysical Journal, 774, 99. https://doi.org/10.1088/0004-637X/774/2/99
[52]
Fesen, R.A., et al. (2006) The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant. The Astrophysical Journal, 645, 283-292. https://doi.org/10.1086/504254
[53]
NASA, Chandra (2008) G1.9+0.3: Discovery of Most Recent Supernova in Our Galaxy. https://chandra.harvard.edu/photo/2008/g19
[54]
Krause, O., et al. (2008) The Cassiopeia A Supernova Was of Type IIb. Science, 320, 1195-1197. https://doi.org/10.1126/science.1155788
[55]
Clark, D.H. and Stephenson, F.R. (1981) The Historical Supernovae. In: Supernovae: A Survey of Current Research, D. Reidel Publishing Co., Dordrecht, 355-370. https://doi.org/10.1007/978-94-009-7876-8_22
[56]
Hoyle, F. and Wickramasinghe, C. (1984) Evolution from Space. Simon & Schuster, New York.
