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Comets 25 October 2018
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Introduction The history of comet watching dates back to 1000 BC from the Chinese records and Chaldea, a place in present Iraq. Comets have been regarded as omens, even as recently as 1986. Battle of Hastings – 1066 – Bayeau Tapestry Today Astronomers study Comets from scientific perspectives, and our understanding of these fascinating objects have grown tremendously.
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Dirty Snowballs Comets are dusty chunk of ice
During each orbit around the sun they partially vaporize Have elliptical orbits Courtesy: Calvin J. Hamilton
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Orbits of Comets Elliptical in Shape Randomly oriented
Aphelion distance Comet Sun Earth Perihelion distance
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Comet Hunters Comet are named by International Astronomical Union (IAU) after the person who first discovers them. Many comets are discovered by amateur astronomers. Charles Messier, E. E. Bernard, Shoemaker and Levy, Hale and Bopp, Ikeya, Seki and Hayakutake are popular comet hunters.
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Origins of Comets Comets are thought to be the left over debris from during the time of formation of the solar system. The elliptical orbits of comets suggest that they underwent gravitational pull from the giant planets. This all lead us to infer two possible locations where comets could start their journey towards the sun: Oort Cloud for long period comets; Kuiper Belt for short period.
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Comets Tails Ludwig Biermann propose the idea of solar wind to explain comet tails. Mariner 2 spacecraft captured the one such event in 1962.
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Comet Collisions Courtesy: NASA/JPL
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Kohoutek
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Comet West
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Shoemaker-Levy 9
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Shoemaker-Levy hits Jupiter
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Hale-Bopp Ion tail & Dust tail
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Halley from Giotto
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Hyakutake
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Deep Impact Tempel 1
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Comet ISON 4 October 2013
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Comet ISON 10 April 2013
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Comet ISON 8 October 2013
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ISON’s path through the sky
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ISON approaches the Sun
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ISON is only debris cloud after passing Sun
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Comet Hartley jets
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Comet McNaught 2007
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Siding Spring at Mars October 2014
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MER PanCam
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MAVEN IUVS Siding Spring
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Latest Rosetta Images:
Landing, 12 Nov 2014 Perihelion: 13 August 2015 Orbiter crashed: 30 Sep 2016
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Rosetta with Philae lander, before separation
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Rosetta Target: 67P Churyumov-Gerasimenko
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Boulder ‘Cheops’
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Approaching Perihelion
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Outburst in Action
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View through Camera 4
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P67 Rotation and Regions
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Active Pits
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Comet 67P seen from 10 km
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Reconstructed last image from Rosetta
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Key Concepts Kuiper Belt, exterior to Neptune is the primary source of short period (P<200yr) comets Oort Cloud, 10,000 AU from Sun, reservoir of long period comets, stored there billions of years Small objects are much more abundant Cometary activity is triggered by sunlight Comet tails: dust, shaped by solar radiation; ion or plasma tail shaped by solar wind Comet grains: CHON + refractory matter Comet nucleus: dirty snowball
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