Английская Википедия:(172034) 2001 WR1

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Шаблон:Use dmy dates Шаблон:Infobox planet

Шаблон:Mp, provisional designation: Шаблон:Mp, is a sub-kilometer near-Earth object of the Amor group, approximately Шаблон:Convert in diameter. The S-type asteroid has been identified as a potential flyby target of the Hayabusa2 mission.[1] It was discovered on 17 November 2001, by astronomers with the Lincoln Near-Earth Asteroid Research at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States.[2] The asteroid has a rotation period of 8.0 hours and possibly an elongated shape.[3] It remains unnamed since its numbering in December 2007.[2]

Orbit and classification

Файл:Animation of (172034) 2001 WR1 orbit.gif
Animated orbital diagram for Шаблон:Mp from 1 January 2020 to 31 December 2023
Шаблон:Legend2Шаблон:·Шаблон:Legend2Шаблон:·Шаблон:Legend2 Шаблон:·Шаблон:Legend2

Шаблон:Mp is an Amor asteroid – a subgroup of near-Earth asteroids that approach the orbit of Earth from beyond, but do not cross it. The object orbits the Sun at a distance of 1.02–1.54 AU once every 17 months (527 days; semi-major axis of 1.28 AU). Its orbit has an eccentricity of 0.20 and an inclination of 25° with respect to the ecliptic.[4] The body's observation arc begins with its first observation in February 1953, more than 48 years prior to its official discovery observation at Socorro. The precovery was taken at Palomar Observatory and published by the Digitized Sky Survey.[2]

Close encounters

Шаблон:Mp has an Earth minimum orbital intersection distance of Шаблон:Convert which corresponds to 29.1 lunar distances.[4] In September 1926, it approached Earth to Шаблон:Convert, its closest approach of all close encounters since 1900. Only in September 2199, it will approach Earth at a similar distance of Шаблон:Convert.[4]

Hayabusa2 mission

Шаблон:Mp was proposed as a target of the Hayabusa2 extended mission for a flyby planned to occur on 27 June 2023.[1] When the spacecraft returned to Earth and delivered the sample capsule in December 2020, it was expected to retain 30 kg of xenon propellant, which can be used to extend its service and flyby new targets to explore.[1] However, this asteroid was not selected as a target for Hayabusa2; two other asteroids were selected instead.

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 24 December 2007 (Шаблон:Small).[5] Шаблон:As of, it has not been named.[2]

Physical characteristics

Шаблон:Mp has been characterized as a common, stony S-type asteroid.[6]

Rotation period

In March 2018, a rotational lightcurve of Шаблон:Mp was obtained from photometric observations by Brian Warner at the Palmer Divide Station Шаблон:Obscode in California. Lightcurve analysis gave a rotation period of Шаблон:Val hours with a brightness amplitude of 0.95 magnitude (Шаблон:Small), indicative of a non-spherical shape.[7]Шаблон:Efn

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Шаблон:Mp has an albedo of 0.34 and measures 0.63 and 0.66 kilometers in diameter, respectively.[8][9][10] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 0.818 kilometers based on an absolute magnitude of 17.8.[3]

Notes

Шаблон:Notelist

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:Authority control

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