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A Brief History of High-Energy Astronomy: 1000 - 1499
Era
In Reverse Chronological Order
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| 1460 - 1550 |
Radiocarbon (14C) analysis of tree rings and 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
luminosity was also reduced during this interval. |
| 1408 |
Chinese and Japanese astronomers observe and record a
`guest star' which is suspected to be the supernova explosion which
produced the supernova remnant CTB 80 = SNR 069.0+02.7 (Wang et al.
1986, Highlights of Astronomy, 7, 583). |
| 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 maximum brightness brighter
than that of Venus), which produced the supernova remnant SNR
327.6+14.6. |
Acknowledgements
We would like to thank the following individuals for their
contributions to this page:
Jesse S. Allen, and
Ian M. George
along with
JPL's Space Calendar and the
Working Group for the History of Astronomy's
Astronomiae Historia (History of Astronomy) information pages.
Web page author: Stephen A. Drake (based on an original by Jesse S. Allen)
Web page maintainer: Stephen A. Drake
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Last modified: Thursday, 25-Oct-2012 10:19:58 EDT
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