(434620) 2005 VD
(434620) 2005 VD is a centaur and damocloid. It has the second most highly inclined orbit of any known object in the solar system, second to 2013 LA2. It was the most highly inclined known object between 2005 and 2013.
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(434620) 2005 VD
(434620) 2005 VD is a centaur and damocloid. It has the second most highly inclined orbit of any known object in the solar system, second to 2013 LA2. It was the most highly inclined known object between 2005 and 2013.
apoapsis (km)
1.247887094209827E9
orbital period (μ)
periapsis (km)
7.464027184833558E8
absolute magnitude
has abstract
(434620) 2005 VD is a centaur ...... object between 2005 and 2013.
@en
2005 VDは、ダモクレス族（ケンタウルス族とされる場合もある）の小惑星である。レモン山天文台のサーベイで発見された。
@ja
albedo
apoapsis (μ)
1.247887094209827e+12
discovery date
2005-11-01
epoch
13 January 2016 (JD2457400.5)
orbital period (s)
5.43076704e+8
periapsis (μ)
7.464027184833558e+11
thumbnail
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Wikipage page ID
19,685,678
Wikipage revision ID
736,975,938
arg peri
1.784741e+2
asc node
1.732668e+2
background
dimensions
eccentricity
inclination
1.728679e+2
mean anomaly
2.055636e+2
mean motion
minorplanet
mp category
mp name
observation arc
3.596832E8
tisserand
uncertainty
subject
hypernym
comment
(434620) 2005 VD is a centaur ...... object between 2005 and 2013.
@en
2005 VDは、ダモクレス族（ケンタウルス族とされる場合もある）の小惑星である。レモン山天文台のサーベイで発見された。
@ja
label
(434620) 2005 VD
@en
2005 VD
@ja
wasDerivedFrom
depiction
isPrimaryTopicOf
name
(434620) 2005 VD
@en