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Statements

Subject Item
n2:RIV%2F00070327%3A_____%2F03%3A00014363%21RIV%2F2005%2FGA0%2FJC1005%2FN
rdf:type
n8:Vysledek skos:Concept
dcterms: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. 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.
dcterms: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) Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR)
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) Peculiar Pair of Distant Periodic Comets C/2002 A1 and C/2002 A2 (LINEAR)
skos:notation
RIV/00070327:_____/03:00014363!RIV/2005/GA0/JC1005/N
n4:strany
L67-L70
n4:aktivita
n17:P
n4:aktivity
P(GA205/98/0266), P(GP205/02/P114)
n4:cisloPeriodika
1
n4:dodaniDat
n14:2005
n4:domaciTvurceVysledku
n5:1759531 n5:7127243 n5:4260643
n4:druhVysledku
n15:J
n4:duvernostUdaju
n13:S
n4:entitaPredkladatele
n16:predkladatel
n4:idSjednocenehoVysledku
620515
n4:idVysledku
RIV/00070327:_____/03:00014363
n4:jazykVysledku
n9:eng
n4:klicovaSlova
comets;data analysis;astrometry
n4:klicoveSlovo
n6:astrometry n6:data%20analysis n6:comets
n4:kodStatuVydavatele
US - Spojené státy americké
n4:kontrolniKodProRIV
[9C1F26121E60]
n4:nazevZdroje
Astrophysical journal letters
n4:obor
n10:BN
n4:pocetDomacichTvurcuVysledku
3
n4:pocetTvurcuVysledku
5
n4:projekt
n12:GP205%2F02%2FP114 n12:GA205%2F98%2F0266
n4:rokUplatneniVysledku
n14:2003
n4:svazekPeriodika
591
n4:tvurceVysledku
Chodas, Paul W. Kočer, Michal Tichý, Miloš Sekanina, Zdenek Tichá, Jana
s:issn
0004-637X
s:numberOfPages
4