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Шаблон:Use dmy dates Шаблон:Infobox planet

Шаблон:Mp, provisional designation: Шаблон:Mp, is a Jupiter trojan from the Trojan camp, approximately Шаблон:Convert in diameter. It was discovered on 19 June 1998, by astronomers with the Lincoln Near-Earth Asteroid Research at the Lincoln Lab's ETS near Socorro, New Mexico, in the United States.[1] The suspected tumbler is also a slow rotator with a period of 250 hours.[2] It has not been named since its numbering in July 2000.[3]

Orbit and classification

Шаблон:Mp is a Jupiter trojan in a 1:1 orbital resonance with Jupiter. It is located in the trailering Trojan camp at the Gas Giant's Шаблон:L5 Lagrangian point, 60° behind its orbit Шаблон:Cross reference.[4]

It orbits the Sun at a distance of 4.9–5.4 AU once every 11 years and 10 months (4,309 days; semi-major axis of 5.18 AU). Its orbit has an eccentricity of 0.05 and an inclination of 17° with respect to the ecliptic.[5] The body's observation arc begins with a precovery published by the Digitized Sky Survey and taken at Palomar Observatory in December 1953, more than 44 years prior to its official discovery observation at Socorro.[1]

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 26 July 2000 (Шаблон:Small).[3] Шаблон:As of, it has not been named.[1]

Physical characteristics

Шаблон:Mp is an assumed C-type asteroid.[2] It has a typical V–I color index of 0.906 (see table below).[6]

Rotation period

In August 2013, Robert Stephens at the Center for Solar System Studies observed Шаблон:Mp over three nights. However no meaningful rotational lightcurve could be determined, as the lightcurve's amplitude never varied more than 0.02 magnitude. A period of 11.17 hours was only derived for demonstration purpose (Шаблон:Small).[7] In December 2015, Stephens obtained an improved lightcurve with a rotation period of Шаблон:Val hours and a brightness variation of 0.30 magnitude (Шаблон:Small). This time the asteroid was observed on 16 nights over a period of one month. The photometric observations also revealed that this object possibly has a non-principal axis rotation, which is commonly known as tumbling.[8][2]Шаблон:Efn

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and the Japanese Akari satellite, Шаблон:Mp measures 43.53 and 51.53 kilometers in diameter and its surface has an albedo of 0.071 and 0.046, respectively.[9][10] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 46.30 kilometers based on an absolute magnitude of 10.4.[2]

Шаблон:Largest Jupiter trojans

Notes

Шаблон:Notelist

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies

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