Comets and Life 10 October 2016
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.
Dirty Snowballs Comets are dusty chunk of ice During each orbit around the sun they partially vaporize Have elliptical Orbits Courtesy: Calvin J. Hamilton
Orbits of Comets Elliptical in Shape Randomly oriented Aphelion distance Comet Sun Earth Perihelion distance
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.
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.
Comets Tails Ludwig Biermann propose the idea of solar wind to explain comet tails. Mariner 2 spacecraft captured the one such event in 1962.
Comet Collisions Courtesy: NASA/JPL
Kohoutek
Comet West
Shoemaker-Levy 9
Shoemaker-Levy hits Jupiter
Hale-Bopp Ion tail & Dust tail
Halley from Giotto
Hyakutake
Deep Impact Tempel 1
Comet ISON 4 October 2013
Comet ISON 10 April 2013
Comet ISON 8 October 2013
ISON’s path through the sky
ISON approaches the Sun
ISON is only debris cloud after passing Sun
Comet Hartley jets
Comet McNaught 2007
Siding Spring at Mars October 2014
MER PanCam
MAVEN IUVS Siding Spring
Latest Rosetta Images: Philae Landing, 12 Nov 2014 Perihelion: 13 August 2015 Orbiter Landing: 30 September 2016
Rosetta Instruments
Rosetta Target: 67P C-G
Boulder ‘Cheops’
Philae Found!
Osiris from 16km
30 September 2016: Rosetta’s last image from 51m
Comet Outbursts Are common near perihelion Studied by JB Vincent (MPS) etal Published last week in MNRAS I will show pictures and paper figures from the paper
View through Camera 4
Approaching Perihelion
Outburst in Action
Active Pits
Location of the outburst node
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 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
Comets and Life Comets are full of organics and water They supplied and continue to supply these to planet and moon surfaces Interstellar life could hitch a ride on a comet from another star’s Oort cloud: may have infected Earth with life from space: panspermia They preserve the material from the early solar system in ‘cold storage’