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2010 BK118 est un objet transneptunien pouvant être classé comme centaure (au sens large du terme), ayant une orbite rétrograde et très elliptique qui pourrait peut-être montrer l'existence de la planète X.
, 2010 BK118, também escrito como 2010 BK118, é um corpo celeste que é classificado como um centauro, numa classificação estendida de centauros. Ele possui uma magnitude absoluta de 10,2 e tem um diâmetro estimado de cerca de 46 km.
, 2010 BK118 (also written 2010 BK118) is a … 2010 BK118 (also written 2010 BK118) is a centaur roughly 20–60 km in diameter. It is on a retrograde cometary orbit. It has a barycentric semi-major axis (average distance from the Sun) of ~400 AU. 2010 BK118 came to perihelion in April 2012 at a distance of 6.1 AU from the Sun (outside the orbit of Jupiter). It has a Jupiter-MOID of 1.1 AU. As of 2016, it is 11 AU from the Sun. It will not be 50 AU from the Sun until 2043. After leaving the planetary region of the Solar System, 2010 BK118 will have a barycentric aphelion of 791 AU with an orbital period of 8000 years.1 AU with an orbital period of 8000 years.
, Το 2010 BK118 είναι Κένταυρος με αφήλιο στ … Το 2010 BK118 είναι Κένταυρος με αφήλιο στις 16,6 αστρονομικές μονάδες. Τον Απρίλιο του 2012 είχε έρθει στις 6.1 αστρονομικές μονάδες με τον Ήλιο, ενώ τώρα βρίσκεται στις 11 . Ανακαλύφθηκε τον Ιανουάριο του 2010. Είναι ένας από τους εκατοντάδες χιλιάδες Αστεροειδής που είναι σε τροχιά γύρο από τον Ήλιο μας.που είναι σε τροχιά γύρο από τον Ήλιο μας.
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2010 BK118 est un objet transneptunien pouvant être classé comme centaure (au sens large du terme), ayant une orbite rétrograde et très elliptique qui pourrait peut-être montrer l'existence de la planète X.
, 2010 BK118 (also written 2010 BK118) is a … 2010 BK118 (also written 2010 BK118) is a centaur roughly 20–60 km in diameter. It is on a retrograde cometary orbit. It has a barycentric semi-major axis (average distance from the Sun) of ~400 AU. 2010 BK118 came to perihelion in April 2012 at a distance of 6.1 AU from the Sun (outside the orbit of Jupiter). It has a Jupiter-MOID of 1.1 AU. As of 2016, it is 11 AU from the Sun. It will not be 50 AU from the Sun until 2043. After leaving the planetary region of the Solar System, 2010 BK118 will have a barycentric aphelion of 791 AU with an orbital period of 8000 years.1 AU with an orbital period of 8000 years.
, 2010 BK118, também escrito como 2010 BK118, é um corpo celeste que é classificado como um centauro, numa classificação estendida de centauros. Ele possui uma magnitude absoluta de 10,2 e tem um diâmetro estimado de cerca de 46 km.
, Το 2010 BK118 είναι Κένταυρος με αφήλιο στ … Το 2010 BK118 είναι Κένταυρος με αφήλιο στις 16,6 αστρονομικές μονάδες. Τον Απρίλιο του 2012 είχε έρθει στις 6.1 αστρονομικές μονάδες με τον Ήλιο, ενώ τώρα βρίσκεται στις 11 . Ανακαλύφθηκε τον Ιανουάριο του 2010. Είναι ένας από τους εκατοντάδες χιλιάδες Αστεροειδής που είναι σε τροχιά γύρο από τον Ήλιο μας.που είναι σε τροχιά γύρο από τον Ήλιο μας.
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2010 BK118
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