Discovery | |
---|---|
Discovery date | 27 February 1556 |
Designations | |
Great Comet of 1556 | |
Orbital characteristics [1] | |
Epoch | 22 April 1556 (JD 2289499.185) |
Observation arc | 52 days |
Number of observations | 36 |
Perihelion | 0.4908 AU |
Eccentricity | ~1.000 |
Inclination | 32.37° |
181.44° | |
Argument of periapsis | 100.87° |
Last perihelion | 22 April 1556 |
The Great Comet of 1556 (designated C/1556 D1 in modern nomenclature) was a comet that first appeared in February 1556, and which was observed throughout much of Europe. The comet appears to have been seen in some places before the end of February, but it was not generally observed until the middle of the first week in March. Its apparent diameter was equal to half that of the Moon, and the tail was said [ by whom? ] to resemble "the flame of a torch agitated by the wind." Cornelius Gemma (the son of Gemma Frisius) said that the head of the comet, when it first appeared, was as large as Jupiter, and that its color resembled that of Mars. [2]
The course of the comet of 1556 was observed by Paul Fabricius, a mathematician and physician at the court of Charles V, Holy Roman Emperor. [2]
According to NASA, the comet was first reported on 27 February 1556. It was in perigee on 13 March and in perihelion on 22 April. [3]
The Great Comet of 1556 is called the comet of Charles V. When the Emperor first caught sight of it he stood aghast, and exclaimed: "By this dread sign my fates do summon me". Charles had long meditated about retiring from the world after his conquests. Regarding the comet as a sign of Heaven's command to do so, he hastened towards the peaceful monastery of St. Juste, Placentia. [4]
An anonymous English treatise on "Blazing Stares" (1618) spoke of the comet as follows :
In the time of Charles the Emperor, surnamed the Great, a blazing star appeared, in the contemplation whereof the Emperor, having his eyes earnestly bent upon the star and considering profoundly thereupon, at length was wrapped into a great astonishment touching the significance of the same; and sending for a philosopher named Eginard, reasoned with him to and fro about the star, saying in conclusion that the appearing thereof did threaten unto him some dire calamity. [4]
The Portuguese Dominican friar Gaspar da Cruz, who visited Guangzhou in 1556, associated the comet with the devastating 1556 Shaanxi earthquake. In his 1569 book he wondered if the comet was a sign of calamities not just for China, but for the entire world – and could be even the sign of the birth of Antichrist. [5]
Grounding his calculations upon elements deduced from Conrad Wolfhardt's chart along with some other crude data gathered from old records, and comparing the result he obtained with the account given by Friar Giles of Cambridge of a grand comet which appeared in 1264, John Russell Hind was led to conclude, as Richard Dunthorne had been in the previous century, that the comet of Charles V was that of 1264 returned. At any rate, he found a high degree of probability in favor of the conclusion at which he had arrived, and argued that the bodies of these years were identical. Hence he concluded that a return to perihelion might be looked for about the middle of the 19th century, 1848 to 1850. This prediction failed, and as of 2009 no observed comet has matched the orbital elements of either comet. David A. Sargent writes that available evidence points to there being no connection between the comets of 1264 and 1556. [6]
Biela's Comet or Comet Biela was a periodic Jupiter-family comet first recorded in 1772 by Montaigne and Messier and finally identified as periodic in 1826 by Wilhelm von Biela. It was subsequently observed to split in two and has not been seen since 1852. As a result, it is currently considered to have been destroyed, although remnants have survived for some time as a meteor shower, the Andromedids which may show increased activity in 2023.
In astronomy, precovery is the process of finding the image of an object in images or photographic plates predating its discovery, typically for the purpose of calculating a more accurate orbit. This happens most often with minor planets, but sometimes a comet, a dwarf planet, a natural satellite, or a star is found in old archived images; even exoplanet precovery observations have been obtained. "Precovery" refers to a pre-discovery image; "recovery" refers to imaging of a body which was lost to our view, but is now visible again (also see lost minor planet and lost comet).
The 1556 Shaanxi earthquake, known in Chinese colloquially by its regnal year as the Jiajing Great Earthquake "嘉靖大地震" or officially by its epicenter as the Hua County Earthquake "华县地震", occurred in the early morning of 2 February 1556 in Huaxian, Shaanxi during the Ming dynasty.
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