Comets |
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Comets Their name comes from latin “Stella cometa”, star with hair. Unlike the other small bodies in the solar system, comets have been known since antiquity. There are Chinese records of Comet Halley going back to at least 240 BC. The famous Bayeux Tapestry, which commemorates the Norman Conquest of England in 1066, depicts an apparition of Comet Halley. As of 1995, 878 comets have been cataloged and their orbits at least roughly calculated. Of these 184 are periodic comets (orbital periods less than 200 years); some of the remainder are no doubt periodic as well, but their orbits have not been determined with sufficient accuracy to tell for sure. Comets are sometimes called dirty snowballs or "icy mudballs". They are a mixture of ices (both water and frozen gases) and dust that for some reason didn't get incorporated into planets when the solar system was formed. This makes them very interesting as samples of the early history of the solar system. When they are near the Sun and active, comets have several distinct parts: Comets periods After 500 or so passes near the Sun off most of a comet's ice and gas is lost leaving a rocky object very much like an asteroid in appearance. (Perhaps half of the near-Earth asteroids may be "dead" comets.) A comet whose orbit takes it near the Sun is also likely to either impact one of the planets or the Sun or to be ejected out of the solar system by a close encounter (esp. with Jupiter). Comets are classified according to their orbital periods. Short period comets have orbits of less than 200 years, while Long period comets have longer orbits but remain gravitationally bound to the Sun, and main-belt comets orbit within the asteroid belt. Single-apparition comets have parabolic or hyperbolic orbits which will cause them to permanently exit the solar system after one pass by the Sun. By far the most famous comet is Comet Halley but SL 9 was a "big hit" for a week in the summer of 1994.
Comet Halley (1P/Halley) Comet Halley, officially designated 1P/Halley, more generally known as Halley's Comet after Edmond Halley, is a comet that can be seen every 75-76 years. It is the most famous of all periodic comets, even though in every century many comets appear brighter and more spectacular. Halley's comet last appeared in the inner Solar System in 1986, and will next appear in the summer of 2061. Halley's Comet was the first to be recognized as periodic. Having perceived that the observed characteristics of the comet of 1682 were nearly the same as those of two comets which had appeared in 1531 (observed by Petrus Apianus) and 1607 (observed by Johannes Kepler in Prague), Halley concluded that all three comets were in fact the same object returning every 76 years (a period that has since been amended to every 75–76 years). After a rough estimate of the perturbations the comet would sustain from the attraction of the planets, he predicted its return for 1757. Halley's prediction of the comet's return proved to be correct, although it was not seen until 25 December 1758 by Johann Georg Palitzsch, a German farmer and amateur astronomer, and did not pass through its perihelion until March 1759; the attraction of Jupiter and Saturn having caused a retardation of 618 days, as was computed by a team of three French mathematicians, Alexis Clairault, Joseph Lalande, and Nicole-Reine Lepaute, previous to its return. Halley did not live to see the comet's return, having died in 1742. The most recent appearance of Halley was in 1986 and although it was not as spectacular as the two previous occasions (1834 and 1910), it was very important for the astronomy because a spaceship could be brought near to study it for the first time. On March 13, 1986, the spacecraft Giotto approached at a 596 kilometer distance from Halley's nucleus. The next Halley approach will be in the summer of 2061.
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Diagram of the spacecraft Giotto encounter with Halley on March 13 of 1986.
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Comet Hyakutake images from Hubble Space Telescope, taken on March 27, 1996, during their pass by to Earth at 14.96 millions of kilometers.
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Comet Linear
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Information came from Wikipedia, Bill Arnett’s Nin...Eight Planets, ESA-Giotto's WEB page and cometography.com.
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20 periodic comets | ||||||||||
Comet | 1P/Halley | 2P/Encke | 3D/Biela | 4P/Faye | 5D/Brorsen | 6P/d'Arrest | 7P/Pons-Winnecke | 8P/Tuttle | 9P/Tempel (Tempel 1) | 10P/Tempel (Tempel 2) |
Discoverer | Prehistoric; Named after Edmond Halley | Pierre Méchain | Wilhelm von Biela | Hervé Faye | Theodor Brorsen | Heinrich Louis d'Arrest | Jean Louis Pons & Friedrich Winnecke | Horace Parnell Tuttle | Ernst Wilhelm Leberecht Tempel | Ernst Wilhelm Leberecht Tempel |
Discovery date | 1758 (first predicted perihelion) | 1786 | February 27, 1826 | November 25, 1843 | 26 February 1846 | June 28, 1851 | June 12, 1819 & March 9, 1858 | January 5, 1858 | April 3, 1867 | July 4, 1873 |
Eccentricity (e) | 0.967 | 0.85 | 0.7559 | 0.5666 | 0.8098 | 0.613 | 0.634 | 0.8198 | 0.5175 | 0.5355 |
Semi-major axis (a) | 17.8 AU | 2.22 AU | 3.5253 AU | 3.847 AU | 3.100 AU | 3.496 AU | 3.434 AU | 5.693 AU | 3.122 AU | 3.071 AU |
Perihelion (q) | 0.586 AU | 0.33 AU | 0.8606 AU | 1.667 AU | 0.5898 AU | 1.353 AU | 1.257 AU | 1.026 AU | 1.506 AU | 1.427 AU |
Aphelion (Q) | 35.1 AU | 4.11 AU | 6.190 AU | 6.026 AU | 5.610 AU | 5.639 AU | 5.611 AU | 10.36 AU | 4.737 AU | 4.716 AU |
Orbital period (P) | 75.3 a | 3.3 a | 6.619 a | 7.545 a | 5.461 a | 6.51 a | 6.37 a | 13.58 a | 5.515 a | 5.382 a |
Inclination (i) | 162.3° | 12.8° | 12.550° | 9.0317° | 29.382° | 19.5° | 22.28° | 54.9902° | 10.5301° | 12.0184° |
Last perihelion date | February 9, 1986 | December 29, 2003 | September 24, 1852 | May 6, 1999 | March 31, 1879 | February 3, 2002 | May 15, 2002 | June 25, 1994 | July 5, 2005 | February 15, 2005 |
Next est. perihelion date | Summer of 2061 | 19 April 2007 | Broke up | 2006 | Lost | 2008 | 2008 | 2008 | 2011 | 2010 |
Comet | 11P/Tempel-Swift-LINEAR | 12P/Pons-Brooks | 13P/Olbers | 14P/Wolf | 15P/Finlay | 16P/Brooks (Brooks 2) | 17P/Holmes | 18D/Perrine-Mrkos | 19P/Borrelly | 20D/Westphal |
Discoverer | Ernst Tempel, Lewis Swift & LINEAR | Jean-Louis Pons & William Robert Brooks | Heinrich Olbers | Max Wolf | William Henry Finlay | William Robert Brooks | Edwin Holmes | Charles Dillon Perrine & Antonín Mrkos | Alphonse Louis Nicolas Borrelly | J. G. Westphal |
Discovery date | November 27, 1869 | July 12, 1812 | March 6, 1815 | September 17, 1884 | September 26, 1886 | 7 July 1889 | November 6, 1892 | December 9, 1896 | December 28, 1904 | July 24, 1852 |
Eccentricity (e) | 0.54 | 0.955 | ? | 0.407 | 0.71 | 0.5666 | 0.412 | 0.64 | 0.624 | ? |
Semi-major axis (a) | 3.437 AU | 17.13 AU | ? | 4.07 AU | 3.57 AU | 3.611 AU | 3.68 AU | 3.57 AU | 3.59 AU | ? |
Perihelion (q) | 1.584 AU | 0.77 AU | ? | 2.72 AU | 1.034 AU | 1.86 AU | 2.165 AU | ? | 1.35 AU | ? |
Aphelion (Q) | ? | 33.8 AU | ? | ? | ? | 5.66 AU | ? | ? | 5.83 AU | ? |
Orbital period (P) | 6.372 a | 70.9 a | 72 to 77 a | 8.74 a | 6.75 a | 6.86 a | 7.068 a | 6.75 a | 6.8 a | 61.20 a |
Inclination (i) | 13.46° | 74.2° | ? | 27.52° | 3.674° | 5.5481° | 19.19° | 17.86° | 30.3° | ? |
Last perihelion date | December 30, 2001 | May 22, 1954 | June 15, 1956 | November 21, 2000 | February 7, 2002 | 19 July 2001 | May 4, 2007 | September 10, 2002 (unobserved) | 2001 | January 3, 1976 (unobserved) |
Next est. perihelion date | 2007 | 2024 | June 30, 2024 | 2009 | 2008 | 2008 | 2014 | Lost? | 2008 | ? |
Non-periodic comets seen after 1910 | ||
Year | Comet (other names) | Discoverer(s) or Namesake, Date of discovery |
1911 | Comet Beljawsky (C/1911 S3, 1911 IV, 1911g) | Beljawsky, September 29, 1911 |
1911 | Comet Brooks (C/1911 O1, 1911 V, 1911c) | Brooks, July 21, 1911 |
1927 | Comet Skjellerup-Maristany (C/1927 X1, 1927 IX, 1927k) | Skjellerup, November 28, 1927, and Maristany, December 6, 1927 |
1941 | Comet de Kock-Paraskevopoulos (C/1941 B2, 1941 IV, 1941c) | de Kock, January 15, 1941 and Paraskevopoulos, January 23, 1941 |
1947 | Great Southern Comet (C/1947 X1, 1947 XII, 1947n) | December 7, 1947 |
1948 | Eclipse Comet (C/1948 V1, 1948 XI, 1948l) | First spotted during the Nairobi total solar eclipse of November 1, 1948 (magnitude about ?2) |
1956 | Comet Arend-Roland (C/1956 R1, 1957 III, 1956h) | Arend and Roland, November 8, 1956 |
1957 | Comet Mrkos (C/1957 P1, 1957 V, 1957d) | Mrkos, July 29, 1957 |
1961 | Comet Humason (C/1961 R1, 1962 VIII, 1961e) | Humason, September 1, 1961 |
1961 | Comet Wilson-Hubbard (C/1961 O1, 1961 V, 1961d, Drakesen, Portlock-Weinberg) | Wilson and Hubbard, July 23, 1961 |
1962 | Comet Seki-Lines (C/1962 C1, 1962 III, 1962c, Reitberg-Blakesen, Khokhlov) | Seki and Lines, February 4, 1962 |
1965 | Comet Ikeya-Seki (C/1965 S1, 1965 VIII, 1965f) | Ikeya, Seki, September 18, 1965 |
1969 | Comet Bennett (C/1969 Y1, 1970 II, 1969i) | Bennett, December 28, 1969 |
1970 | Comet White-Ortiz-Bolelli (C/1970 K1, 1970 VI, 1970f) | White, May 18, 1970, Ortiz, May 21, 1970, and Bolelli, May 22, 1970 |
1973 | Comet Kohoutek (C/1973 E1, 1973 XII, 1973f) | Kohoutek, March 7, 1973 |
1975 | Comet West (C/1975 V1, 1976 VI, 1975n) | West, August 10, 1975 |
1989 | Comet Skorichenko-George (C/1989 Y1, 1990 VI, 1989e1) | Skorichenko and George, December 17, 1989 |
1993 | Comet Shoemaker-Levy 9 (D/1993 F2, 1994 X, 1993e) | E. Shoemaker, C. Shoemaker, Levy, March 24, 1993 |
1995 | Comet Hale-Bopp (C/1995 O1) | Hale and Bopp, July 23, 1995 one of only four comets known to have had a negative absolute magnitude (?2.7) |
1996 | Comet Hyakutake (C/1996 B2) | Hyakutake, January 30, 1996 |
1997 | Comet Zhu-Balam (C/1997 L1) | Zhu (June 3, 1997) and Balam (June 8, 1997 [1]) |
2004 | Comet Machholz (C/2004 Q2) | Machholz, August 27, 2004 |
2006 | Comet Pojmański (C/2006 A1) | Pojmański, January 2, 2006 |
2006 | SWAN (C/2006 M4) | Robert D. Matson and Michael Mattiazzo, June 20, 2006 |
2006 | McNaught (C/2006 P1) | Robert McNaught, August 7, 2006 (max. brightness −5m) |
2007 | LONEOS (C/2007 F1) | Lowell Observatory Near-Earth-Object Search, March 19, 2007 |
2007 | Siding Spring (C/2007 Q3) | Donna Burton at Siding Spring Observatory, August 25, 2007 |
2007 | Lulin (C/2007 N3) | Ye Quanzhi and Lin Chi-Sheng, Lulin Observatory, July 11, 2007 |
2007 | Boattini (C/2007 W1) | Andrea Boattini, November 20, 2007 |
2008 | Matičič (C/2008 Q1) | Stanislav Matičič, Črni Vrh Observatory (the first comet discovered in Slovenia) |
2009 | Yi–SWAN (C/2009 F6) | Yi Dae am and Robert D. Matson of SOHO, March 26, 2009 (maximum apparent magnitude +8.5m) |
2009 | McNaught (C/2009 R1) | Robert McNaught, September 9, 2009 |
2010 | Elenin (C/2010 X1) | Leonid Elenin, December 10, 2010 |
2011 | PANSTARRS (C/2011 L4) | PanSTARRS, June 6, 2011 |
2011 | Beljawsky (C/1911 S3, 1911 IV, 1911g) | Sergei Ivanovich Beljawsky, September 29, 1911 |
2011 | Lovejoy (C/2011 W3) | Terry Lovejoy, November 27, 2011 |
2012 | SWAN (C/2012 E2) | Vladimir Bezugly, March 8, 2012 |
2012 | Lemmon (C/2012 F6) | A. R. Gibbs, March 23, 2012 |