Английская Википедия:4789 Sprattia

Материал из Онлайн справочника
Перейти к навигацииПерейти к поиску

Шаблон:Short description Шаблон:Use dmy dates Шаблон:Infobox planet

4789 Sprattia, provisional designation Шаблон:Mp, is a stony background asteroid from the inner regions of the asteroid belt, approximately Шаблон:Convert in diameter. It was discovered on 20 October 1987, by Canadian astronomer David Balam at the Climenhaga Observatory Шаблон:Obscode in Victoria, Canada. The S-type asteroid has a rotation period of 3.1 hours and was named after Canadian amateur astronomer Christopher E. Spratt.[1][2]

Orbit and classification

Sprattia is a non-family asteroid from the main belt's background population.[3] It orbits the Sun in the inner asteroid belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,223 days; semi-major axis of 2.24 AU). Its orbit has an eccentricity of 0.12 and an inclination of 1° with respect to the ecliptic.[4] The body's observation arc begins with its first observation as Шаблон:Mp at the Félix Aguilar Observatory in April 1976, more than 11 years prior to its official discovery observation at Victoria.[1]

Physical characteristics

Sprattia has been characterized as a common, stony S-type asteroid by Pan-STARRS and the Sloan Digital Sky Survey.[2][5][6]

Rotation period

In December 2011, a rotational lightcurve of Sprattia was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 3.136 hours with a brightness amplitude of 0.17 magnitude (Шаблон:Small).[7]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Sprattia measures between 3.54 and 4.172 kilometers in diameter and its surface has an albedo between 0.28 and 0.44.[8][9][10]

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20, and calculates a diameter of 4.22 kilometers based on an absolute magnitude of 14.24.[2]

Naming

This minor planet was named after Canadian amateur astronomer Christopher E. Spratt (born 1942),[11] a long-time member of the Royal Astronomical Society of Canada, whose interests involve comets, minor planets, meteors and variable stars. The official naming citation was published by the Minor Planet Center on 27 June 1991 (Шаблон:Small).[1][12]

References

Шаблон:Reflist

External links

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

  1. 1,0 1,1 1,2 Ошибка цитирования Неверный тег <ref>; для сносок MPC-object не указан текст
  2. 2,0 2,1 2,2 Ошибка цитирования Неверный тег <ref>; для сносок lcdb не указан текст
  3. Ошибка цитирования Неверный тег <ref>; для сносок AstDys-object не указан текст
  4. Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  5. Ошибка цитирования Неверный тег <ref>; для сносок Veres-2015 не указан текст
  6. Ошибка цитирования Неверный тег <ref>; для сносок SDSS-Taxonomy не указан текст
  7. Ошибка цитирования Неверный тег <ref>; для сносок Waszczak-2015 не указан текст
  8. Ошибка цитирования Неверный тег <ref>; для сносок Nugent-2015 не указан текст
  9. Ошибка цитирования Неверный тег <ref>; для сносок Masiero-2011 не указан текст
  10. Ошибка цитирования Неверный тег <ref>; для сносок WISE не указан текст
  11. Ошибка цитирования Неверный тег <ref>; для сносок RASC не указан текст
  12. Ошибка цитирования Неверный тег <ref>; для сносок MPC-Circulars-Archive не указан текст