About: Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR)     Goto   Sponge   Distinct   Permalink

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Description
  • Distant comets C/2002 A1 and C/2002 A2 make up a peculiar pair that moves about the Sun in virtually identical, somewhat unstable orbits, extending currently between about 4.7 and 29 AU from the Sun. The two objects, observed since late 2001, are unquestionably of common origin. Analysis of their relative motion indicates that their parent body split nontidally most probably between mid-1977 and early 1979 at a heliocentric distance of 22.5 +- 0.1 AU and about 2.5 AU below the ecliptic, with a separation velocity of 2.7 +- 0.2 m s-1. The motion of C/2002 A2, the secondary component that trails behind the primary, is found to be affected by a nongravitational deceleration of (13.4 +- 1.5) × 10-5 units of solar gravitational acceleration relative to C/2002 A1, which is in a range of decelerations that companions of split comets are usually subjected to. C/2002 A2 was somewhat less condensed and, interestingly, brighter than C/2002 A1.
  • Distant comets C/2002 A1 and C/2002 A2 make up a peculiar pair that moves about the Sun in virtually identical, somewhat unstable orbits, extending currently between about 4.7 and 29 AU from the Sun. The two objects, observed since late 2001, are unquestionably of common origin. Analysis of their relative motion indicates that their parent body split nontidally most probably between mid-1977 and early 1979 at a heliocentric distance of 22.5 +- 0.1 AU and about 2.5 AU below the ecliptic, with a separation velocity of 2.7 +- 0.2 m s-1. The motion of C/2002 A2, the secondary component that trails behind the primary, is found to be affected by a nongravitational deceleration of (13.4 +- 1.5) × 10-5 units of solar gravitational acceleration relative to C/2002 A1, which is in a range of decelerations that companions of split comets are usually subjected to. C/2002 A2 was somewhat less condensed and, interestingly, brighter than C/2002 A1. (en)
  • Distant comets C/2002 A1 and C/2002 A2 make up a peculiar pair that moves about the Sun in virtually identical, somewhat unstable orbits, extending currently between about 4.7 and 29 AU from the Sun. The two objects, observed since late 2001, are unquestionably of common origin. Analysis of their relative motion indicates that their parent body split nontidally most probably between mid-1977 and early 1979 at a heliocentric distance of 22.5 +- 0.1 AU and about 2.5 AU below the ecliptic, with a separation velocity of 2.7 +- 0.2 m s-1. The motion of C/2002 A2, the secondary component that trails behind the primary, is found to be affected by a nongravitational deceleration of (13.4 +- 1.5) × 10-5 units of solar gravitational acceleration relative to C/2002 A1, which is in a range of decelerations that companions of split comets are usually subjected to. C/2002 A2 was somewhat less condensed and, interestingly, brighter than C/2002 A1. (cs)
Title
  • Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR)
  • Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR) (en)
  • Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR) (cs)
skos:prefLabel
  • Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR)
  • Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR) (en)
  • Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR) (cs)
skos:notation
  • RIV/00070327:_____/03:00014363!RIV/2005/GA0/JC1005/N
http://linked.open.../vavai/riv/strany
  • L67-L70
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/98/0266), P(GP205/02/P114)
http://linked.open...iv/cisloPeriodika
  • 1
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 620515
http://linked.open...ai/riv/idVysledku
  • RIV/00070327:_____/03:00014363
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • comets;data analysis;astrometry (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [9C1F26121E60]
http://linked.open...i/riv/nazevZdroje
  • Astrophysical journal letters
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 591
http://linked.open...iv/tvurceVysledku
  • Tichá, Jana
  • Tichý, Miloš
  • Chodas, Paul W.
  • Kočer, Michal
  • Sekanina, Zdenek
issn
  • 0004-637X
number of pages
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