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Great Comet of 1680

C/1680 V1, also called the Great Comet of 1680, Kirch's Comet, and Newton's Comet, was the first comet discovered by telescope. It was discovered by Gottfried Kirch and was one of the brightest comets of the seventeenth century. It passed about 235000 km from the surface of the Sun.

Overview
The comet was discovered by Gottfried Kirch, a German astronomer, on 14 November 1680 (New Style), in Coburg, and it became one of the brightest comets of the seventeenth century – reputedly visible even in daytime – and was noted for its spectacularly long tail. Passing 0.42 au from Earth on 30 November 1680, It was last observed on 19 March 1681. While the Kirch Comet of 1680–1681 was discovered by – and subsequently named for – Gottfried Kirch, credit must also be given to Eusebio Kino, the Spanish Jesuit priest who charted the comet's course. During his delayed departure for Mexico, Kino began his observations of the comet in Cádiz in late 1680. Upon his arrival in Mexico City, he published his Exposición astronómica de el cometa (Astronomical Account of the Comet; Mexico City, 1681) in which he presented his findings. Kino's Exposición astronómica is among the earliest scientific treatises published by a European in the New World. Basil Ringrose was serving under buccaneer Captain Bartholomew Sharpe and made the following observation shortly before raiding the Spanish port city of Coquimbo, Chile: Friday, November 19th, 1680. This morning about an hour before the day we observed a comet to appear a degree N. from the bright in Libra. The body thereof seemed dull, and its tail extended itself 18 or 20 degrees in length, being of a pale colour and pointing directly N.N.W. Our prisoners hereupon reported to us that the Spaniards had seen very strange sights, both at Lima, the capital city of Peru, Guayaquil, and other places, much about the time of our coming into the South Seas. Although it was undeniably a sungrazing comet, it was probably not part of the Kreutz family. Isaac Newton used the comet to test and verify Kepler's laws. John Flamsteed was the first to propose that the two bright comets of 1680–1681 were the same comet, one traveling inbound to the Sun and the other outbound, and Newton originally disputed this. Newton later changed his mind, and then, with Edmond Halley's help, purloined some of Flamsteed's data to verify this was the case without giving Flamsteed credit. ==Gallery==
Gallery
File:Staartster boven Beverwijk, 1680, RP-T-00-3653.jpg|The comet as it appeared above Beverwijk on 22 December 1680. File:C 1680V1 Nürnberg.jpg|The Great Comet of 1680 over Nuremberg File:Silver medal with comet illustration, Hamburg, 1681.jpg|Commemorative medal depicting the comet, Hamburg, 1681 File:Houghton PFr 275.1.9 - Cometa apparsa in Roma l'Anno 1680.jpg|"Cometa apparsa in Roma l'Anno 1680". From an issue of Mercure Galant, published in Paris File:De komeet van 1680-1681 Comet welcher Anno 1680 und 1681 beobachtet worden (titel op object), RP-P-OB-82.513.jpg|The comet on the background of the signs of the Zodiac in the winter of 1680–1681 File:Newton Comet1680.jpg|The orbit of the comet of 1680, fit to a parabola, as shown in Isaac Newton's Principia File:Richard-Cumberland-John-Maxwell-A-treatise-of-the-laws-of-nature MG 0936.tif|A 1727 chart of the Solar System up to the orbit of the planet Saturn, with the track of the 1680 comet, and two others File:Exposition astronomica de el cometa.jpg|Front page of Exposisión astrónomica de el cometa by Eusebio Francisco Kino, 1681 ==See also==
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