comets
DESCRIPTION
Comets. Small dusty/icy chunk of material few kms size (often characterized as “dirty snowball”) Originally condensed out of Solar nebula and still orbit Sun - primitive material Orbits often elliptical, large aphelion Partially vaporized when close to Sun - material - PowerPoint PPT PresentationTRANSCRIPT
CometsCometsCometsComets Small dusty/icy chunk of material few kms Small dusty/icy chunk of material few kms size (often characterized as “dirty size (often characterized as “dirty snowball”)snowball”)
Originally condensed out of Solar nebula Originally condensed out of Solar nebula and still orbit Sun - primitive materialand still orbit Sun - primitive material
Orbits often elliptical, large aphelionOrbits often elliptical, large aphelion Partially vaporized when close to Sun - Partially vaporized when close to Sun - materialmaterial
(gases) then pushed by sunlight makes long (gases) then pushed by sunlight makes long tailtail
Gas tail always points away from SunGas tail always points away from Sun Also dust tail along orbitAlso dust tail along orbit
COMET IKEYA-SEKICOMET IKEYA-SEKICOMET IKEYA-SEKICOMET IKEYA-SEKI
COMET WESTCOMET WESTCOMET WESTCOMET WEST
COMET HALE-BOPPCOMET HALE-BOPPCOMET HALE-BOPPCOMET HALE-BOPP
PARTS of a COMETPARTS of a COMETPARTS of a COMETPARTS of a COMET
Pushed by SunPushed by Sun
Dust along Dust along comet’s orbitcomet’s orbit
COMET TAIL ORIENTATIONCOMET TAIL ORIENTATIONCOMET TAIL ORIENTATIONCOMET TAIL ORIENTATION
Ion trail
Dust trail
Comet Hale-bopComet Hale-bop
Dust trail
Ion trail
RECIPE for a COMETRECIPE for a COMETRECIPE for a COMETRECIPE for a COMET
IngredientsIngredientsFrozen methaneFrozen methaneFrozen waterFrozen waterFrozen ammoniaFrozen ammoniaDust grains (dirt)Dust grains (dirt)Traces of organic compounds and other Traces of organic compounds and other
chemicalschemicals DirectionsDirections
Mix into a ball about 10 km across containing Mix into a ball about 10 km across containing 100,000,000,000,000, (10100,000,000,000,000, (101414) kg of this mixture) kg of this mixture
About the About the mass of Mt. mass of Mt. BakerBaker
COMET HALLEYCOMET HALLEYCOMET HALLEYCOMET HALLEY
COMET HALLEY’S ORBITCOMET HALLEY’S ORBITCOMET HALLEY’S ORBITCOMET HALLEY’S ORBIT
COMET HALLEY’S PATH COMET HALLEY’S PATH 1910 and 19861910 and 1986
COMET HALLEY’S PATH COMET HALLEY’S PATH 1910 and 19861910 and 1986
1910 1986
Returns to Perihelion of Halley’s Comet
239 BC March 30 989 September 9
163 BC October 5 1066 March 23
86 BC August 2 1145 April 22
11 BC October 5 1222 October 1
AD 66 January 26 1301 October 23
141 March 20 1378 November 9
218 May 11 1456 June 9
295 April 20 1531 August 25
274 February 16 1607 October 27
451 June 24 1682 September 15
530 September 25 1759 March 13
760 May 22 1835 November 16
837 February 27 1910 April 20
912 July 9 1986 February
BAYEUX TAPESTRYBAYEUX TAPESTRYBAYEUX TAPESTRYBAYEUX TAPESTRY
Giotto-Adoration of the MagiGiotto-Adoration of the MagiGiotto-Adoration of the MagiGiotto-Adoration of the Magi
ORIGIN of LONG PERIOD ORIGIN of LONG PERIOD COMETSCOMETS
ORIGIN of LONG PERIOD ORIGIN of LONG PERIOD COMETSCOMETS
Originate in Oort CloudOriginate in Oort Cloud-a huge reservoir a huge reservoir ancient Solar Systemancient Solar Systemmaterial far from Sunmaterial far from Sun-likely produced by likely produced by planetesimals ejectedplanetesimals ejectedby Jupiter and Saturnby Jupiter and SaturnEarly on from inner Early on from inner Solar System.Solar System.
Passing star perturbesPassing star perturbesCloud sends lumpsCloud sends lumpsinward - see as cometsinward - see as cometswhen near Sun.when near Sun.
KUIPER BELTPlanetesimals ejected from inner Solar System by strong
gravitational fields of Giant Planets - some interact Jupiter and Saturn flung far out to Oort Cloud, interactions Uranus and
Neptune pushed them out to Kuiper Belt
KUIPER BELTPlanetesimals ejected from inner Solar System by strong
gravitational fields of Giant Planets - some interact Jupiter and Saturn flung far out to Oort Cloud, interactions Uranus and
Neptune pushed them out to Kuiper Belt
Kuiper Belt
KUIPER BELT OBJECTKUIPER BELT OBJECTKUIPER BELT OBJECTKUIPER BELT OBJECT
KUIPER BELT OBJECTSKUIPER BELT OBJECTSKUIPER BELT OBJECTSKUIPER BELT OBJECTSSedna e =0.86Perihelion 76 AUAphelion 975 AU!P =12,000 years
Pluto + 3 Moons
METEORS AND METEORS AND METEORITESMETEORITES
METEORS AND METEORS AND METEORITESMETEORITES
Meteors are parts of Meteors are parts of comets that pass through comets that pass through Earth’s orbit - burn up Earth’s orbit - burn up in Earth’s atmospherein Earth’s atmosphere
Meteorites are ground up Meteorites are ground up pieces of asteroids - off pieces of asteroids - off
orbit - enter Earth’s orbit - enter Earth’s atmosphere and survive atmosphere and survive
passagepassage
Meteor ShowerMeteor ShowerMeteor ShowerMeteor Shower
Comet breakupComet breakupnear perihelionnear perihelion
Material spread outMaterial spread outalong orbitalong orbit
If Earth passesIf Earth passesthrough comet debristhrough comet debris- shower- shower
A METEOR STORMA METEOR STORMA METEOR STORMA METEOR STORM
1833 Wood Cut
Leonid Shower
LEONID METEOR SHOWERLEONID METEOR SHOWERLong ExposureLong Exposure
LEONID METEOR SHOWERLEONID METEOR SHOWERLong ExposureLong Exposure
Dates Some Meteor ShowersDates Some Meteor ShowersDates Some Meteor ShowersDates Some Meteor Showers
ANTARCTIC METEORITEANTARCTIC METEORITEANTARCTIC METEORITEANTARCTIC METEORITE
Easiest to find meteoritesagainst snow.
Most found in Arctic orAntarctic
Primitive material - planetesimals - useful fordating Solar System
Many varieties - stony,metallic, often containorganic material