National Aeronautics and Space Administration

A Brief History of High-Energy Astronomy: 1000 - 1499 Era

In Reverse Chronological Order

1460 - 1550	Radiocarbon (14C) analysis of tree rings and historical observations of the aurora borealis indicate a 90-year period of lower than average solar activity, now called the Spörer Minimum. This period was, likely not coincidentally, one with cooler than average global temperatures, implying that the solar bolometric luminosity was also reduced during this interval.
11 Mar 1437	Korean astronomers observe and record a `guest star' in the modern constellation of Scorpius which fades out of sight 2 weeks later, consistent with the duration of a classical nova eruption. Almost 6 centuries later, Shara et al. (2017, Nature, 548, 558) identified the dwarf nova-type catalcysmic variable 2MASS J17012815-4306123 as the progenitor of this eruption and the 1.5-arcminute diameter expanding shell of material as the ejecta from this nova eruption, confirming the hypothesis that many old classical novae "become dwarf novae for part of the millennia between successive nova eruptions".
1408	Chinese and Japanese astronomers observe and record a `guest star' which has been suspected by some researchers, e.g., Wang et al. (1986, Highlights of Astronomy, 7, 583), to be a supernova explosion, specifically the SN that produced the supernova remnant CTB 80 = SNR 069.0+02.7, although this has hypothesis not been universally accepted (e.g., Stephenson & Yau 1986, JQRAS, 27, 559).
circa 1320	The supernova that nobody noticed? ROSAT discovered a previously unknown, relatively nearby (200-700 pc) supernova remnant (SNR) during its All-Sky Survey phase, RX J0852.0-4622, which appears to coincide with a Compton Observatory/COMPTEL gamma-ray source GRO J0852.0-4642. The latter appears to have an emission line due to radioactive 44Ti indicative of formation in a recent (680 years old) supernova, according to Iyudin et al. (2005, A&A, 429, 225). This age estimate coincides with a spike in nitrate concentration in an Antarctic ice core: a number of such spikes have been proposed to be results of the effect of nearby historical supernovae on the Earth's atmosphere (Burgess & Zuber 2000, Astroparticle Physics, 14, 1). The big puzzle is why there are no historical records of a supernova (see Ashenbach et al. 1999, A&A, 350, 997 for more discussion): Redman and Meaburn (2005, MNRAS, 356, 969) have noted that if the pulsar PSR J0855-4644 is the stellar remnant of the supernova, its off-center position within the SNR implies a much older age of at least 3000 years (well before the period when detailed astronomical records were made and/or have survived from).
1280 - 1350	Radiocarbon (14C) analysis of tree rings indicate a 70-year period of lower than average solar activity, now called the Wolf Minimum.
1181	Chinese and Japanese astronomers observe and record a `guest star' which is now considered to be the supernova explosion SN 1181 which produced the supernova remnant 3C 58 (SNR 130.7+03.1).
1066	The Norman invasion of England, led by William the Conqueror. The invasion is recorded in the Bayeux tapestry : among other features, the tapestry records the appearance of Halley's Comet (P1/Halley) around the time of the invasion.
4 Jul 1054	Chinese and Japanese astronomers observe and record a `guest star' which is now considered to be the supernova SN 1054 which produced the Crab Nebula (SNR 184.6-05.8).
1010 - 1080	Radiocarbon (14C) analysis of tree rings indicate a 70-year period of lower than average solar activity, now called the Oort Minimum.
1006	Chinese, Japanese, and possibly Korean astronomers observe and record a `guest star' which is now considered to be the supernova explosion SN 1006 , the brightest recorded supernova (with a brightness at maximum brighter than Venus), which produced the supernova remnant SNR 327.6+14.6.

Return to main History of High-Energy Astronomy page

Acknowledgements

Web page author: Stephen A. Drake (based on an original by Jesse S. Allen)

Web page maintainer: Stephen A. Drake