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Comets, Centaurs, & TNOs AS3141 Benda Kecil dalam Tata Surya Prodi Astronomi 2006/2007 B. Dermawan AS3141 Benda Kecil dalam Tata Surya Prodi Astronomi 2006/2007 B. Dermawan
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Benda Kecil Tata Surya Asteroids (MBAs, NEAs) Comets (periode pendek, panjang; ekliptik, isotropik) Meteoroids ( meteors, meteorites) (Edgeworth)-Kuiper Belt Objects or Trans- Neptunian Objects Centaurs (Jupiter-Neptune), Damocloids Hipotesis: vulcanoids, ‘awan’ Oort Asteroids (MBAs, NEAs) Comets (periode pendek, panjang; ekliptik, isotropik) Meteoroids ( meteors, meteorites) (Edgeworth)-Kuiper Belt Objects or Trans- Neptunian Objects Centaurs (Jupiter-Neptune), Damocloids Hipotesis: vulcanoids, ‘awan’ Oort
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Comets, Centaurs, Damocloids, & TNOs
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Comets (1)
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Comets (2) Periode Pendek (SPC, < 200 th) - Halley Type Comets (HTC, 200-20 th) - Jupiter Family Comets (JFC, < 20 th) Periode Panjang (LPC, > 200 th) Periode Pendek (SPC, < 200 th) - Halley Type Comets (HTC, 200-20 th) - Jupiter Family Comets (JFC, < 20 th) Periode Panjang (LPC, > 200 th) Ekliptik: T > 2 JFC Isotropik: T < 2 LPC, HTC, Damocloids Ekliptik: T > 2 JFC Isotropik: T < 2 LPC, HTC, Damocloids Parameter Tisserand:
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Comets (3) Active comet: detectable coma volatile & dust Inactive comet: no detectable coma Dormant comet: lost the ability to generate a detectable coma in any part of its present orbit might be reactivated Extinct comet: incapable of generating a coma (lost its ices, or its ices buried under a nonvolatile crust) Active comet: detectable coma volatile & dust Inactive comet: no detectable coma Dormant comet: lost the ability to generate a detectable coma in any part of its present orbit might be reactivated Extinct comet: incapable of generating a coma (lost its ices, or its ices buried under a nonvolatile crust)
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Dormant & Extinct Comets Weissman et al. 2003
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Comet-like Asteroids & Extinct Comets Weissman et al. 2003
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Sun-grazing Comets
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Insitu Explorations Giotto → Halley Deep Space 1 – Borrelly Stardust – Wild2 Deep Impact → Temple 1 Giotto → Halley Deep Space 1 – Borrelly Stardust – Wild2 Deep Impact → Temple 1
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Isotopic Abundances Hutsemékers 2005
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Centaurs: Asteroid-like objects with semimajor axes between those of Jupiter and Neptune Centaurs unusual Johnston 2005
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Centaurs Albedo Colors Dotto & Barucci 2004
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Damocloids (1) Jewitt (2004) Comet-like asteroids whose T 2 Inactive nuclei of HTC & LPC Have subsequently developed comae About 25% possess retrograde orbits Jewitt (2004) Comet-like asteroids whose T 2 Inactive nuclei of HTC & LPC Have subsequently developed comae About 25% possess retrograde orbits
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Damocloids (2) The distribution of inclinations is indistinguishable from that of the HFC Lack ultrared matter The distribution of inclinations is indistinguishable from that of the HFC Lack ultrared matter : ~4000Å - ~8000Å Jewitt 2004
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(Edgeworth)-Kuiper Belt Objects [(E)KBO] Trans-Neptunian Objects (TNOs)
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TNOs: Non-cometary objects with semimajor axes beyond Neptune's orbit Plutinos: Near the 2:3 resonance with Neptune. Pluto is the largest object near this resonance. Resonance objects: Other than Plutinos but near resonances (4:5, 3:4, 3:5, 4:7, 1:2, 2:5) with Neptune. Cubewanos: Eccentricities below 0.15 with semimajor axes between 41.8 AU and 48 AU. Scattered disk objects (SDOs): Aphelion distances near Neptune's orbit and semimajor axes greater than 50 AU. Other TNOs not fitting in the above groups. Plutinos: Near the 2:3 resonance with Neptune. Pluto is the largest object near this resonance. Resonance objects: Other than Plutinos but near resonances (4:5, 3:4, 3:5, 4:7, 1:2, 2:5) with Neptune. Cubewanos: Eccentricities below 0.15 with semimajor axes between 41.8 AU and 48 AU. Scattered disk objects (SDOs): Aphelion distances near Neptune's orbit and semimajor axes greater than 50 AU. Other TNOs not fitting in the above groups.
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TNOs: Orbital Dist. (1) Johnston 2005
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TNOs: Orbital Dist. (2) Lykawka & Mukai 2005
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TNOs: Orbital Dist. (3) Jewitt 2004
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TNOs: Sizes (1) Thermal Flux: Density: Effective temp.: Standard Thermal Model (STM, Lebofsky et al. 1989) Near-Earth Asteroid Thermal Model (NEATM, Harris 1998) Thermo-Physical Model (TPM, Lagerros 1997) Bond Albedo & Geometric Albedo: Optical Constraints:
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Size & Albedo of Unusual Minor Planet C/2002 CE 10 Sekiguchi et al. 2005
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TNOs: Sizes (2) Johnston 2005
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TNOs: Spectrum Dotto & Barucci 2004
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TNOs: Binary (1) Richardson & Walsh 2005 NEAsMBAs Trojan Pluto- Charon TNOs
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TNOs: Binary (2) Richardson & Walsh 2005 NEAsMBAs Trojan Pluto- Charon TNOs
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Albedo & Spectral Gradient Jewitt 2004 Dotto & Barucci 2004
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Albedo vs Diameter Lykawka & Mukai 2005
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Colors (1) Jewitt 2004 Peixinho 2003
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Colors (2) Doressoundiram & Peixinho 2005
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Atmospheres? Lykawka & Mukai 2005
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Stellar Encounter (1) Kenyon & Bromley 2004
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Stellar Encounter (2) Kenyon & Bromley 2004
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Stellar Encounter (3) Kenyon & Bromley 2004
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