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(91205) 1998 US43

Plutino


Plutino

FieldValue
minorplanetyes
name(91205)
background#C2E0FF
discovery_ref
discovererM. W. Buie
discovery_siteKitt Peak National Obs.
discovered22 October 1998
mpc_name(91205)
alt_names
named_after
mp_categoryTNOplutino
distant
orbit_ref
epoch27 April 2019 (JD 2458600.5)
uncertainty4
observation_arc17.29 yr (6,314 d)
aphelion44.196 AU
perihelion33.932 AU
semimajor39.064 AU
eccentricity0.1314
period244.16 yr (89,179 d)
mean_anomaly66.411°
mean_motion/ day
inclination10.628°
asc_node223.94°
arg_peri138.70°
mean_diameter(est.)
(est.)
albedo0.04 (assumed)
0.09 (assumed)
spectral_typeBB–BR
B–R =
B–V =
R–I =
V–R =
abs_magnitude8.0

distant (est.) 0.09 (assumed) B–R = B–V = R–I = V–R =

**** (provisional designation ****) is a resonant trans-Neptunian object of the plutino group, located in the Kuiper belt in the outermost region of the Solar System. The rather bluish body measures approximately 111 km in diameter. It was discovered on 22 October 1998, by American astronomer Marc Buie at the Kitt Peak National Observatory in the United States.

Classification and orbit

belongs to the plutino population, a large population of resonant trans-Neptunian objects named after the group's largest member, Pluto. Thus, is in a 2:3 orbital resonance with Neptune, orbiting the Sun twice for every three times Neptune does.

It orbits the Sun with a semi-major axis of 39.06 AU, a perihelion of 33.9 AU, and an aphelion of 44.2 AU, completing an orbit once every 244 years and 2 months (89,179 days). Its orbit has an eccentricity of 0.13 and an inclination of 11° with respect to the ecliptic. The body's observation arc begins with its official discovery observation. Its orbit still has a fair amount of uncertainty.

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 28 October 2004 (M.P.C. 52912). As of 2025, it has not been named.

Physical characteristics

Based on an absolute magnitude of 8.0 and an assumed albedo of 0.09, Johnston's Archive estimates a diameter of 111 kilometers. The body's spectrum (BB–BR) suggests a somewhat bluish color. As of 2018, no rotational lightcurve of has been obtained from photometric observations. is an unlikely dwarf planet candidate due to its small size, estimated by Michael Brown to measure 154 kilometers with a low albedo of 0.04.

References

Info: Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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