(251732) 1998 HG49
(251732) 1998 HG49, also written as (251732) 1998 HG49, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit. It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit. Between 1900 and 2200 its closest approach to Earth is more than 0.14 AU.
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(251732) 1998 HG49
(251732) 1998 HG49, also written as (251732) 1998 HG49, is an asteroid on a low-eccentricity and low-inclination orbit between the orbits of Earth and Mars. This is within a region of stability where bodies may survive for the age of the Solar System, and hence it may have formed near its current orbit. It is classified as an Amor asteroid because its perihelion is less than 1.3 AU and does not cross Earth's orbit. Between 1900 and 2200 its closest approach to Earth is more than 0.14 AU.
apoapsis (km)
1.998169349233833E8
orbital period (μ)
480.48000000000013
periapsis (km)
1.593879443130718E8
absolute magnitude
has abstract
(251732) 1998 HG49, also writt ...... to Earth is more than 0.14 AU.
@en
apoapsis (μ)
1.998169349233833e+11
discovery date
1998-04-27
discoverer
epoch
13 January 2016 (JD2457400.5)
orbital period (s)
4.151347200000001e+7
periapsis (μ)
1.593879443130718e+11
Wikipage page ID
32,986,667
Wikipage revision ID
738,565,762
arg peri
3.2426152e+2
asc node
4.4832211e+1
background
dimensions
eccentricity
1.125514e-1
inclination
4.1953173e+0
mean anomaly
1.1052123e+1
mean motion
minorplanet
mp category
observation arc
tisserand
uncertainty
subject
hypernym
comment
(251732) 1998 HG49, also writt ...... to Earth is more than 0.14 AU.
@en
label
(251732) 1998 HG49
@en