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● H e l p ● L e a r n t o e d i t ● C o m m u n i t y p o r t a l ● R e c e n t c h a n g e s ● U p l o a d f i l e
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( T o p )
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F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
(508869) 2002 VT130 2002 VT130 , is a trans-Neptunian object and binary system from the classical Kuiper belt , located in the outermost region of the Solar System . It was discovered by American astronomer Marc Buie at Kitt Peak Observatory on 7 November 2002.[1] [2] [7]
Physical properties
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The object belongs to the cold classical population and is a binary . The companion was discovered by Keith Noll, Will Grundy, Susan Benecchi, and Hal Levison using Hubble Space Telescope on 21 September 2008. The discovery was announced on 24 September 2009. The moon's apparent separation from the primary was ± 90 km orbital period of ± 0.0064 d [8] 2002 VT130 is about 324 km.[7] mean diameter of 251 km for the primary, and 205 km for the satellite based on a secondary-to-primary diameter ratio of 0.817.[4]
2002 VT130 shows significant photometric variability with the lightcurve amplitude of 0.21. This may indicate that 2002 VT130 binary is a result of a collision.[9]
References
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^ a b c "JPL Small-Body Database Browser: 508869 (2002 VT130)" (2017-03-29 last obs.). Jet Propulsion Laboratory . Retrieved 13 January 2020 .
^ a b c d e Johnston, Wm. Robert (27 May 2019). "Asteroids with Satellites Database – (508869) 2002 VT130" . Johnston's Archive . Retrieved 13 January 2020 .
^ Marc W. Buie . "Orbit Fit and Astrometric record for 508869" . SwRI (Space Science Department). Retrieved 18 February 2018 .
^ Brown, Mike. "How many dwarf planets are there in the Solar System" . Retrieved 18 February 2018 .
^ a b c d Vilenius, E.; Kiss, C.; Mommert, M.; et al. (2014). "Astronomy & Astrophysics . 564 : A35. arXiv :1403.6309 Bibcode :2014A&A...564A..35V . doi :10.1051/0004-6361/201322416 . S2CID 118513049 .
^ a b Grundy, W.M.; Noll, K.S.; Roe, H.G.; Buie, M.W.; Porter, S.B.; Parker, A.H.; Nesvorný, D.; Levison, H.F.; Benecchi, S.D.; Stephens, D.C.; Trujillo, C.A. (December 2019). "Mutual orbit orientations of transneptunian binaries". Icarus . 334 : 62–78. doi :10.1016/j.icarus.2019.03.035 .
^ A. Thirouin; K.S. Noll; J.L. Ortiz; N. Morales (2014). "Rotational properties of the binary and non-binary populations in the trans-Neptunian belt". Astronomy & Astrophysics . 569 : A3. arXiv :1407.1214 Bibcode :2014DPS....4642109T . doi :10.1051/0004-6361/201423567 . S2CID 119244456 .
External links
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R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=(508869)_2002_VT130&oldid=1229659987 " C a t e g o r i e s : ● M i n o r p l a n e t o b j e c t a r t i c l e s ( n u m b e r e d ) ● C o l d c l a s s i c a l K u i p e r b e l t o b j e c t s ● D i s c o v e r i e s b y M a r c B u i e ● B i n a r y t r a n s - N e p t u n i a n o b j e c t s ● A s t r o n o m i c a l o b j e c t s d i s c o v e r e d i n 2 0 0 2 H i d d e n c a t e g o r i e s : ● U s e d m y d a t e s f r o m D e c e m b e r 2 0 1 8 ● J P L S m a l l - B o d y D a t a b a s e I D d i f f e r e n t f r o m W i k i d a t a ● A r t i c l e s w i t h J P L S B D B i d e n t i f i e r s
● T h i s p a g e w a s l a s t e d i t e d o n 1 8 J u n e 2 0 2 4 , a t 0 1 : 1 3 ( U T C ) . ● T e x t i s a v a i l a b l e u n d e r t h e C r e a t i v e C o m m o n s A t t r i b u t i o n - S h a r e A l i k e L i c e n s e 4 . 0 ;
a d d i t i o n a l t e r m s m a y a p p l y . B y u s i n g t h i s s i t e , y o u a g r e e t o t h e T e r m s o f U s e a n d P r i v a c y P o l i c y . W i k i p e d i a ® i s a r e g i s t e r e d t r a d e m a r k o f t h e W i k i m e d i a F o u n d a t i o n , I n c . , a n o n - p r o f i t o r g a n i z a t i o n . ● P r i v a c y p o l i c y ● A b o u t W i k i p e d i a ● D i s c l a i m e r s ● C o n t a c t W i k i p e d i a ● C o d e o f C o n d u c t ● D e v e l o p e r s ● S t a t i s t i c s ● C o o k i e s t a t e m e n t ● M o b i l e v i e w
