1999
DOI: 10.1177/002182869903000203
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A Survey of Muslim Material on Comets and Meteors

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Cited by 34 publications
(22 citation statements)
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“…Duration : The duration of visibility given ( qarīban min thalāthat ashhur for close to 3 months ) can mean a little less or a little more than 3 months, and it is consistent with most other Arabic scholars: c Alī ibn Riḍwān (4 months); Ibn al‐Jawzī and Ibn al‐Athīr ( beginning of Sha c bān … until the middle of Dhū al‐Qa c dah , that is, 3.5 months); Moroccan report ( This star stayed for 6 months ); Yaḥyā ibn Sa c īd al‐Anṭākī ( it continued for 4 months , Cook, 1999); al‐Yamānī ( On the night of mid‐Rajab in the year 396h, a star appeared… In the night of mid‐Ramaḍān, its light started to decrease and gradually faded away , i.e., more than 2 months); and similarly Ibn al‐Dayba c ( on the night of mid‐Rajab a star like Venus appeared … It remained unchanged until the night of mid‐Ramaḍān , i.e., not less than 2 months). In particular, if Ibn Sīnā (or his source) observed SN 1006 since about late April or early May 1006, and then for close to 3 months , then he could have observed until heliacal setting for his location.…”
Section: Discussionsupporting
confidence: 84%
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“…Duration : The duration of visibility given ( qarīban min thalāthat ashhur for close to 3 months ) can mean a little less or a little more than 3 months, and it is consistent with most other Arabic scholars: c Alī ibn Riḍwān (4 months); Ibn al‐Jawzī and Ibn al‐Athīr ( beginning of Sha c bān … until the middle of Dhū al‐Qa c dah , that is, 3.5 months); Moroccan report ( This star stayed for 6 months ); Yaḥyā ibn Sa c īd al‐Anṭākī ( it continued for 4 months , Cook, 1999); al‐Yamānī ( On the night of mid‐Rajab in the year 396h, a star appeared… In the night of mid‐Ramaḍān, its light started to decrease and gradually faded away , i.e., more than 2 months); and similarly Ibn al‐Dayba c ( on the night of mid‐Rajab a star like Venus appeared … It remained unchanged until the night of mid‐Ramaḍān , i.e., not less than 2 months). In particular, if Ibn Sīnā (or his source) observed SN 1006 since about late April or early May 1006, and then for close to 3 months , then he could have observed until heliacal setting for his location.…”
Section: Discussionsupporting
confidence: 84%
“…Such historical observations have been used very successfully for SNe 1006 (from Eastern Asia, Arabia, and Europe), 1054 (from Eastern Asia and Arabia), 1181 (only from Eastern Asia), and SNe 1572 and 1604 (from Eastern Asia and Europe), plus a few more SNe from the first millennium AD (see Stephenson & Green, 2002, henceforth SG02, and references therein). While the Arabic report about SN 1054 merely confirms a bright new star in Gemini/Taurus around AD 1054, Arabic reports on SN 1006 present a lot of detailed information (Cook, 1999; Goldstein, 1965; Rada & Neuhäuser, 2015; SG02).…”
Section: Introduction: Supernova 1006mentioning
confidence: 99%
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“…Goldstein () also gives an English translation of a Syriac report on SN 1006 by Bar Hebraeus (born in AD 1226 in Malatya in Turkey, died in 1286 in Maragha, now Iran), where it was specified that the new star was observed in the zodiacal sign of Scorpius. Cook () presented another Arabic report on SN 1006 from Yaḥyā ibn Sa c īd al‐Anṭākī, Patriarch of Antioch (now Antakya, Turkey), who extended the chronicle of Eutychius of Alexandria (Egypt) for the time since circa AD 939 and died in AD 1066, according to which the new star was seen for 4 months since Saturday, second day in Sha c bān of the year 396h (AD 1006 May 3/4). Most recently, Neuhäuser, Ehrig‐Eggert, and Kunitzsch (2017) presented another original report about SN 1006, written by Ibn Sīnā (Avicenna).…”
Section: Introduction: Sn 1006mentioning
confidence: 99%
“…However, there are some previous attempts to cover this issue for European sources, including the early works of Newton 2 and the most recent from Dall"Olmo 3 , whose list was mainly based in the Monumenta Germaniae Historica (MGH) and the Rerum Italicarum Scriptores (RIS). For the Arab sources, see the works of Rada and Stephenson 4 (including the comments of Kidger 5 ) and Cook 6 . Spanish sources are scarcely represented in these surveys 7 .…”
Section: Introductionmentioning
confidence: 99%