Английская Википедия:3430 Bradfield

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3430 Bradfield (prov. designation: Шаблон:Mp) is a stony Agnia asteroid from the central regions of the asteroid belt, approximately Шаблон:Convert in diameter. It was discovered on 9 October 1980, by American astronomer Carolyn Shoemaker at the Palomar Observatory in California. The Sq-type asteroid was named after comet hunter William A. Bradfield.[1]

Orbit and classification

When applying the hierarchical clustering method to its proper orbital elements according to Nesvorný, Bradfield is a member of the Agnia family (Шаблон:Small),[2] a very large family of stony asteroids with more than 2000 known members.[3] They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation.[4] The family's parent body and namesake is the asteroid 847 Agnia.[3] In the 1995-HCM analysis by Zappalà, however, it is a member of the Liberatrix family (also described as Nemesis family by Nesvorný).[2][5]

It orbits the Sun in the central main-belt at a distance of 2.5–3.0 AU once every 4 years and 7 months (1,674 days; semi-major axis of 2.76 AU). Its orbit has an eccentricity of 0.10 and an inclination of 4° with respect to the ecliptic.[6] The body's observation arc begins with its observations as Шаблон:Mp at Cerro El Roble Observatory in April 1974, more than 6 years prior to its official discovery observation at Palomar.[1]

Naming

This minor planet was named after New Zealand-born Australian amateur astronomer and rocket engineer William A. Bradfield (1927–2014). A discoverer of several comets himself, he significantly increased the rate of discovery of bright comets from the southern hemisphere during the 1970s and 1980s.[1] The official naming citation was published by the Minor Planet Center on 14 April 1987 (Шаблон:Small).[7]

Physical characteristics

In the SMASS classification, Bradfield is an Sq-subtype, that transitions between the common, stony S-type and Q-type asteroids.[6]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Bradfield measures 8.492 kilometers in diameter and its surface has an albedo of 0.269.[8]

Rotation period

As of 2018, no rotational lightcurve of Bradfield has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[6]

References

Шаблон:Reflist

External links

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

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  3. 3,0 3,1 Ошибка цитирования Неверный тег <ref>; для сносок Nesvorny-2014 не указан текст
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  8. Ошибка цитирования Неверный тег <ref>; для сносок Masiero-2011 не указан текст