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2201 Oljato

Asteroid


Asteroid

FieldValue
minorplanetyes
name2201 Oljato
background#FFC2E0
discovery_ref
discovered12 December 1947
discovererH. L. Giclas
discovery_siteLowell Obs.
mpc_name(2201) Oljato
alt_names1947 XC
1979 XA
named_afterOljato–Monument Valley
(Navajo Reservation)
mp_categoryNEOPHAAmor
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc84.90 yr (31,008 days)
earliest_precovery_date3 December 1931
aphelion3.7257 AU
perihelion0.6243 AU
semimajor2.1750 AU
eccentricity0.7130
period3.21 yr (1,172 days)
mean_anomaly255.69°
inclination2.5224°
asc_node74.991°
arg_peri98.264°
moid0.0031 AU1.2 LD
dimensionskm (IRAS:11)
km
rotationh
h
albedo
(IRAS:11)
spectral_typeSMASS = SqCS
abs_magnitude15.0015.2515.5015.55

1979 XA (Navajo Reservation) km h (IRAS:11)

2201 Oljato, provisional designation , is a stony and extremely eccentric active asteroid and sizable near-Earth object of the Apollo group, approximately 2 kilometers in diameter. It has an Earth minimum orbit intersection distance of 0.0031 AU and is associated with the Beta Taurids daytime meteor shower.

Discovery

Oljato was discovered by American astronomer Henry L. Giclas at the U.S Lowell Observatory in Flagstaff, Arizona, on 12 December 1947. After its discovery, this near-Earth Apollo asteroid became a lost asteroid for 32 years and was recovered under the provisional designation , by the American astronomers Passey and Bus at the Californian Palomar Observatory in 1979.

Orbit and classification

Oljato is a member of the Apollo asteroids, a subgroup of near-Earth asteroids which cross the orbit of Earth. It is also a potentially hazardous object due to its size and its Earth minimum orbit intersection distance (MOID) of 0.0031 AU, which is only about 1.2 lunar distances . It orbits the Sun at a distance of 0.6–3.7 AU once every 3 years and 3 months (1,172 days). Its orbit has an eccentricity of 0.71 and an inclination of 3° with respect to the ecliptic.

It was a target of Hubble search for transition comets, a spectroscopic study involving amateur astronomers and the use of the Hubble Space Telescope. The asteroid belongs to the Taurid Complex (also see Taurids), a group of near-Earth asteroids thought to be extinct cometary nuclei, that are associated with four meteor showers on Earth, due to their disintegration. The Taurid Complex includes several other Apollo asteroids such as 4183 Cuno, 4341 Poseidon, 5143 Heracles, and 5731 Zeus.

Close approaches

The next notable close approach to Earth will be on 28 November 2024, passing at a nominal distance of 0.47 AU. Due to the eccentricity of its orbit, Earth is not the only planet it passes. In 2044 it will pass close to Venus (on 24 Apr at 0.08 AU) as well as Earth (on 30 May at 0.129 AU), and in 2046 it will pass Jupiter (on 15 Jan at 1.4 AU). However, although it crosses the orbit of Mars, it will pass Earth, Venus and Jupiter several times before the next notable close approach to Mars, which will not be until 30 July 2127, passing at a nominal distance of 0.0306 AU

Physical characteristics

Oljato has a rotation period of 26 hours. The stony asteroid is classified as a Sq-subtype in the SMASS taxonomic scheme, with a geometric albedo of 0.24. An alternative and exceptionally high albedo of 0.43 was determined by 11 observations from the Infrared Astronomical Satellite, IRAS.

Naming

This minor planet was named after the Oljato–Monument Valley in Utah, on the Navajo Indian Reservation. The official naming citation was published by the Minor Planet Center on 28 March 1983 (M.P.C. 7782).

Notes

References

References

  1. (2015). "Asteroids IV". [[University of Arizona]].
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