The Bayeux tapestry representation of Comet Halley in their appearance in 1066.

 

Comet Holmes

The outstanding comet 17P Holmes, became the bigger object in Solar System.
The Nov. 1 photo at left, by an amateur astronomer, shows Comet Holmes' coma consists of concentric shells of dust and a faint tail. The Hubble image at right, made Nov. 4 and enhanced to reveal details, reveals the bow-tie appearance created by twice as much dust existing along the horizontal direction.
The coma's diameter on Nov. 9 was 869,900 miles (1.4 million kilometers), based on measurements by Rachel Stevenson, Jan Kleyna and Pedro Lacerda of the University of Hawaii Institute for Astronomy. They used observations from the Canada-France-Hawaii Telescope. The sun's diameter, stated differently by various sources and usually rounded to the nearest 100, is about 864,900 miles (1.392 million kilometers).
Text taken from: http://www.space.com/
Image credit: NASA, ESA, and H. Weaver (The Johns Hopkins University Applied Physics Laboratory); Alan Dyer

 

The Comet Haley in a picture taken by Giotto spacecraft in 1986 - ESA

 

This spectacular image of comet Tempel 1 was taken 67 seconds after it obliterated Deep Impact's impactor spacecraft. - 5/07/2005 NASA/JPL-Caltech/UMD

 

This picture show the fragmented Shoemaker-Levy 9 comet before their crash with Jupiter in 1994 - NASA

 

The inactive comet Borrelly nucleus as seen by the spacecraft Deep Space 1 in September 2001 - NASA/JPL

 

 
 

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:
Nucleus: relatively solid and stable, mostly ice and gas with a small amount of dust and other solids
Coma: dense cloud of water, carbon dioxide and other neutral gases sublimed from the nucleus; (planet size: 40,000 km in diameter)
Hydrogen cloud: huge (millions of km in diameter) but very sparse envelope of neutral hydrogen;
Dust tail: up to 10 million km long composed of smoke-sized dust particles driven off the nucleus by escaping gases; this is the most prominent part of a comet to the unaided eye;
Ion tail: as much as several hundred million km long composed of plasma and laced with rays and streamers caused by interactions with the solar wind.

Comets periods
Comets are invisible except when they are near the Sun. Most comets have highly eccentric orbits which take them far beyond the orbit of Pluto; these are seen once and then disappear for millennia. Only the short- and intermediate-period comets (like Comet Halley), stay within the orbit of Pluto for a significant fraction of their orbits.

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.
Meteor shower sometimes occur when the Earth passes thru the orbit of a comet. Some occur with great regularity: the Perseid meteor shower occurs every year between August 9 and 13 when the Earth passes thru the orbit of Comet Swift-Tuttle. Comet Halley is the source of the Orionid shower in October.

 

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.
Images showed Halley's nucleus to be a dark peanut-shaped body, 15 km long, 7 to 10 km wide. Only 10% of the surface was active, with at least three outgassing jets seen on the sunlit side.
Of the volume of material ejected by Halley: 80% was water, 10% carbon monoxide, and 2.5% a mix of methane and ammonia. Other hydrocarbons, iron, and sodium were detected in trace amounts.
Halley's nucleus was blacker than soot, which suggests there is proportionally more dust than ice.
The nucleus's surface was rough and of a porous quality, with the density of whole nucleus only 0.3 kg/m3.
The quantity of material ejected was found to be 3 tons per second for seven jets, and these caused the comet to wobble over long time periods.
The dust ejected was mostly only the size of cigarette smoke particles, the largest being 40 milligram. Although the one that sent Giotto spinning was not measured, from its effects its mass has been estimated to lie between 0.1 and 1 gram.
Analysis showed the comet formed 4.5 billion years ago from volatiles (mainly ice) that had condensed onto interstellar dust particles. It had remained practically unaltered since its formation.

The next Halley approach will be in the summer of 2061.

 

Giotto

Diagram of the spacecraft Giotto encounter with Halley on March 13 of 1986.
Blue: Giotto orbit. Green: Earth orbit. Yellow: Halley orbit. (a): Launching point on July 2, 1985. (b): Rendezvous point on 03/13/1986. (c): Earth’s position at rendezvous date. - ESA diagram.

 

Comet Hyakutake

Comet Hyakutake images from Hubble Space Telescope, taken on March 27, 1996, during their pass by to Earth at 14.96 millions of kilometers.

 

Comet Linear

Comet Linear
Comet that was observed to break apart as it approached the Sun. C/1999 S4 was discovered by the LINEAR program in September 1999. On Jul. 21-22, 2000, a couple of days before perihelion on Jul. 24 (0.75 AU). The disintegration of C/1999 S4 after perihelion had more to do with solar heating than with the Sun’s gravitational force. The comet receives their name after the short for “Lincoln Near Earth Asteroid Research”.

 

   

Information came from Wikipedia, Bill Arnett’s Nin...Eight Planets, ESA-Giotto's WEB page and cometography.com.

 

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

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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