Английская Википедия:730 Athanasia

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Шаблон:Use dmy dates Шаблон:Infobox planet

730 Athanasia (prov. designation: Шаблон:Mp or Шаблон:Mp) is a background asteroid from the inner regions of the asteroid belt, approximately Шаблон:Convert in diameter. It was discovered by Austrian astronomer Johann Palisa at the Vienna Observatory on 10 April 1912.[1] The presumed stony S-type asteroid has a rotation period of 5.7 hours and is likely very elongated in shape. It was named Athanasia, the Greek word for "immortality".[2]

Orbit and classification

Located in the region of the Flora family (Шаблон:Small),[3] a giant asteroid family and the largest family of stony asteroids in the main-belt, Athanasia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5][6] It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,228 days; semi-major axis of 2.24 AU). Its orbit has an eccentricity of 0.18 and an inclination of 4° with respect to the ecliptic.[7] The body's observation arc begins at Vienna Observatory on 15 April 1912, or five nights after its official discovery observation.[1]

Naming

This minor planet was named by friends of the discoverer after the Greek word for immortality, "athanasia". Any reference to a person or occurrence is unknown. The Шаблон:MoMP was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (Шаблон:Small).[2]

Physical characteristics

Athanasia is an assumed, stony S-type asteroid.[3]

Rotation period

In February 2016, a rotational lightcurve of Athanasia was obtained from photometric observations by Frederick Pilcher at the Organ Mesa Observatory Шаблон:Obscode in New Mexico, United States. Analysis gave a classically shaped, well-defined bimodal lightcurve with a rotation period of Шаблон:Val hours and a very high brightness variation of Шаблон:Val magnitude, indicative of a highly elongated shape (Шаблон:Small).[8]Шаблон:Efn In May 2013, Pilcher already observed the object and reported a ambiguous period of Шаблон:Val or Шаблон:Val hours with an amplitude of Шаблон:Val magnitude (Шаблон:Small).[9]Шаблон:Efn

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Athanasia measures (Шаблон:Val) kilometers in diameter and its surface has a high albedo of (Шаблон:Val).[10] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a Florian asteroid of 0.24 and calculates a diameter of 4.94 kilometers based on an absolute magnitude of 13.7.[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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