Английская Википедия:717 Wisibada

Материал из Онлайн справочника
Перейти к навигацииПерейти к поиску

Шаблон:Use dmy dates Шаблон:Infobox planet

717 Wisibada (prov. designation: Шаблон:Mp or Шаблон:Mp) is a dark background asteroid from the outer regions of the asteroid belt. It was discovered on 26 August 1911, by German astronomer Franz Kaiser at the Heidelberg-Königstuhl State Observatory in southwest Germany.[1] The D-type asteroid measures approximately Шаблон:Convert in diameter with no rotation period yet determined. It was named after the discoverer's birthplace, the city of Wiesbaden in Hesse, Germany.[2]

Orbit and classification

Wisibada is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[3][4][5] It orbits the Sun in the outer asteroid belt at a distance of 2.3–4.0 AU once every 5 years and 7 months (2,031 days; semi-major axis of 3.14 AU). Its orbit has an eccentricity of 0.26 and an inclination of 2° with respect to the ecliptic.[6] The body's observation arc begins at Vienna Observatory on 22 August 1922, or one year after its official discovery observation at the Heidelberg Observatory.[1]

Naming

This minor planet was named by the discoverer Franz Kaiser after his birthplace, the city of Wiesbaden in Hesse, Germany. Kaiser also named asteroid 765 Mattiaca after Wiesbaden using the city's Latin name, Aquae Mattiacorum, which means "Waters of the Mattiaci". The Шаблон:MoMP was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (Шаблон:Small).[2]

Physical characteristics

In the Tholen classification, WisibadaШаблон:'s spectral type is closest to a dark D-type asteroid, and somewhat similar to an X-type asteroid, though with a noisy spectrum (DX:).[6]

Rotation period

As of 2020, no rotational lightcurve of Wisibada has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[6][4][7][8]

Diameter and albedo

According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), the Infrared Astronomical Satellite IRAS, and the Japanese Akari satellite, Wisibada measures (Шаблон:Val), (Шаблон:Val) and (Шаблон:Val) kilometers in diameter and its surface has an albedo of (Шаблон:Val), (Шаблон:Val) and (Шаблон:Val), respectively.[9][10][11] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0796 and a diameter of 31.12 kilometers based on an absolute magnitude of 10.9.[7] Alternative mean-diameters published by the WISE team include (Шаблон:Val) and (Шаблон:Val) with a corresponding albedo of (Шаблон:Val) and (Шаблон:Val).[4][7]

References

Шаблон:Reflist

External links

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

  1. 1,0 1,1 Ошибка цитирования Неверный тег <ref>; для сносок MPC-object не указан текст
  2. 2,0 2,1 Ошибка цитирования Неверный тег <ref>; для сносок springer не указан текст
  3. Ошибка цитирования Неверный тег <ref>; для сносок AstDys-object не указан текст
  4. 4,0 4,1 4,2 Ошибка цитирования Неверный тег <ref>; для сносок Ferret не указан текст
  5. Ошибка цитирования Неверный тег <ref>; для сносок Zappala-family не указан текст
  6. 6,0 6,1 6,2 Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  7. 7,0 7,1 7,2 Ошибка цитирования Неверный тег <ref>; для сносок lcdb не указан текст
  8. Ошибка цитирования Неверный тег <ref>; для сносок geneva-obs не указан текст
  9. Ошибка цитирования Неверный тег <ref>; для сносок Mainzer-2016 не указан текст
  10. Ошибка цитирования Неверный тег <ref>; для сносок SIMPS не указан текст
  11. Ошибка цитирования Неверный тег <ref>; для сносок AKARI не указан текст