2002 RN109
2002 RN109 is a minor planet with the third highest orbital eccentricity of any known minor planet, after 2015 ER61 and 2005 VX3. It also has the sixth-largest heliocentric semi-major axis and aphelion of all known minor planets, while its extreme eccentricity brings it well within the orbit of Jupiter when at perihelion. 2002 RN109 has an observation arc 80 days and has not been observed since November 2002 about 2 months before it came to perihelion 2.7 AU from the Sun. During perihelion passage the object was 2.9 AU from Earth.
primaryTopic
2002 RN109
2002 RN109 is a minor planet with the third highest orbital eccentricity of any known minor planet, after 2015 ER61 and 2005 VX3. It also has the sixth-largest heliocentric semi-major axis and aphelion of all known minor planets, while its extreme eccentricity brings it well within the orbit of Jupiter when at perihelion. 2002 RN109 has an observation arc 80 days and has not been observed since November 2002 about 2 months before it came to perihelion 2.7 AU from the Sun. During perihelion passage the object was 2.9 AU from Earth.
apoapsis (km)
1.9326548915733E11
orbital period (μ)
6015553.0
periapsis (km)
4.0533543066165E8
absolute magnitude
has abstract
2002 RN109 is a minor planet w ...... d most near-surface volatiles.
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2002 RN109, também escrito com ...... um diâmetro com cerca de 4 km.
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apoapsis (μ)
1.9326548915733e+14
discovery date
2002-08-16
discoverer
epoch
13 January 2016 (JD2457400.5)
orbital period (s)
5.197437792e+11
periapsis (μ)
4.0533543066165e+11
Wikipage page ID
42,141,194
Wikipage revision ID
731,693,636
arg peri
asc node
background
dimensions
eccentricity
inclination
mean anomaly
minorplanet
mp category
uncertainty
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2002 RN109 is a minor planet w ...... object was 2.9 AU from Earth.
@en
2002 RN109, também escrito com ...... um diâmetro com cerca de 4 km.
@pt
label
2002 RN109
@en
2002 RN109
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2002 RN109
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