We present two Arabic texts of historic observations of supernova SN 1006 from Yemen as reported by al-Yamani and Ibn al-Dayba (14th to 16th century AD). An English translation of the report by the latter was given before (Stephenson & Green 2002), but the original Arabic text was not yet published. In addition, we present for the first time the earlier report, also from Yemen, namely by al-Yamani in its original Arabic and with our English translation. It is quite obvious that the report by Ibn al-Dayba is based on the report by al-Yamani (or a common source), but the earlier report by al-Yamani is more detailed and in better (Arabic) language. We discuss in detail the dating of these observations. The most striking difference to other reports about SN 1006 is the apparent early discovery in Yemen in the evening of 15th of Rajab of the year 396h (i.e. AD 1006 Apr 17 \pm 2 on the Julian calendar), as reported by both al-Yamani and Ibn al-Dayba. i.e. about 1.5 weeks earlier than the otherwise earliest known reports. We also briefly discuss other information from the Yemeni reports on brightness, light curve, duration of visibility, location, stationarity, and color.Comment: 9 pages with 3 figure
Of the many astronomical observations which are recorded in ancient and medieval history, perhaps the most interesting and useful relate to solar eclipses. Obscurations of the Sun are often noticed by the casual observer and may indeed leave a profound impression on him if the degree of obscuration of the Sun is very large. In particular, total solar eclipses are responsible for the onset of sudden and intense darkness, during which the brighter planets and stars may become visible. Hence ancient and medieval accounts of solar eclipses (and to a lesser extent lunar obscurations) are not confined to treatises on astronomy. They also tend to be reported fairly frequently in chronicles and other writings of a historical nature. The only other celestial phenomena regularly to attract widespread attention in ancient and medieval times were comets. However, in chronological studies, eclipses have a distinct advantage over comets. Both solar and lunar obscurations last for only a few hours and their exact date of occurrence can be computed, as well as the time of day (or night) when the event took place. Comets, on the other hand, often remain visible for several weeks and only for Halley's Comet can useful computations of visibility be made.
We present Arabic texts about supernovae SN 1572 and SN 1604. The short observational reports were found in the Yemeni history book entitled Rawḥ al-Rūḥ written by cĪsā b. Luṭf Allāh b. al-Muṭahhar. The text about SN 1604 specifies the location of a new star at the beginning of the zodiacal sign of Sagittarius, consistent with SN 1604 in the constellation of Ophiuchus. It was observed in fall a.d. 1604 for some 40 days (probably limited by its heliacal setting after around a.d. 1604 22 November). The object is called a najm (star) of the nayāzik (transient celestial objects), from which we can conclude that it was a tailless and/or stationary new star (rather than, e.g., a comet). It was specified to be as (large/bright as) Jupiter, consistent with the supernova in a.d. 1604 October and November The text confirms other reports about SN 1604. Furthermore, a short text reports a new star ( najm) in the north-east, larger than Venus, observed in the year a.h. 980 (a.d. 1572 May to 1573 May), connected to the death of a leader on a.d. 1572 9 ± 2 November; this could well be SN 1572, otherwise observed to be as bright as Venus since a.d. 1572 6 November. These new findings may indicate that more Yemeni reports about Galactic supernovae can be uncovered. The description of the new star of a.d. 1604 as najm (star) of the nayāzik (transient celestial objects) and of the comet of a.d. 1577 as “a star [ najm] … of the nayāzik, with a tail … with a visible movement” shows that the author distinguished between cometary and star-like transient celestial objects.
The recently published Yemeni observation report about SN 1006 from al‐Yamānī clearly gives AD 1006 April 17 ± 2 (mid‐Rajab 396h) as the first observation date. Since this is ∼1.5 weeks earlier than the otherwise earliest reports (April 28 or 30) as discussed so far, we were motivated to investigate an early sighting in more depth. We searched for additional evidences from other areas like East Asia and Europe. We found that the date given by al‐Yamānī is fully consistent with other evidence, including the following: (a) SN 1006 rose several times half an hour after sunset (al‐Yamānī), which is correct for the location of Ṣancā' in Yemen for the time around April 17, but it would not be correct for late April or early May. (b) The date (third year, third lunar month, 28th day wuzi, Ichidai Yoki) for an observation of a guest star in Japan is inconsistent (there is no day wuzi in that lunar month), but may be dated to April 16 by reading a wuwu date rather than a wuzi date. (c) There is observational evidence that SN 1006 was observed in East Asia in early or mid‐April; for the second half of April, a bad weather (early monsoon) period is not unlikely— there is a lack of night reports. (d) The observer in St. Gallen reported to have seen SN 1006 for 3 months, which must have ended at the very latest on AD 1006 July 10, given his northern location, so that his observations probably started in April. We conclude that the correctly reported details give quite high confidence in the fully self‐consistent report of al‐Yamānī, so that the early discovery date should be considered seriously.
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.
hi@scite.ai
10624 S. Eastern Ave., Ste. A-614
Henderson, NV 89052, USA
Copyright © 2024 scite LLC. All rights reserved.
Made with 💙 for researchers
Part of the Research Solutions Family.