Английская Википедия:1444 Pannonia
Шаблон:Use dmy dates Шаблон:Infobox planet
1444 Pannonia (prov. designation: Шаблон:Mp) is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately Шаблон:Convert in diameter. It was discovered on 6 January 1938, by Hungarian astronomer György Kulin at Konkoly Observatory in Budapest, Hungary.[1] It was named after the ancient province of the Roman Empire, Pannonia.[2]
Orbit and classification
Pannonia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun at a distance of 2.7–3.6 AU once every 5 years and 7 months (2,044 days). Its orbit has an eccentricity of 0.14 and an inclination of 18° with respect to the ecliptic.[3] PannoniaШаблон:'s observation arc begins 3 weeks after its official discovery at Konkoly, as no precoveries were taken, and no prior identifications were made.[1]
Naming
This minor planet was named for Pannonia, an ancient province of the Roman Empire, which was partially located over the territory of the present-day western Hungary.[2] The official Шаблон:MoMP was published by the Minor Planet Center on 1 February 1980 (Шаблон:Small).[4]
Physical characteristics
Rotation period
In April 2001, astronomer Colin Bembrick obtained the first rotational lightcurve of Pannonia at Tarana Observatory Шаблон:Obscode in Australia. Lightcurve analysis gave a well-defined rotation period of 10.756 hours with a brightness amplitude of 0.16 magnitude (Шаблон:Small).[5] In 2002 and 2004, photometric observations by French astronomers Laurent Bernasconi and Bernard Christophe Additional periods of 6.2 and 6.205 hours with an amplitude of 0.57 and 0.37, respectively (Шаблон:Small).[6]
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Pannonia measures between 26.36 and 31.49 kilometers in diameter, and its surface has an albedo between 0.04 and 0.47.[7][8][9][10][11][12] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0501 and a diameter of 27.14 kilometers with an absolute magnitude of 11.7.[13]
References
External links
- Lightcurve Database Query (LCDB), at www.minorplanet.info
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- Шаблон:AstDys
- Шаблон:JPL small body
Шаблон:Minor planets navigator Шаблон:Small Solar System bodies
- ↑ 1,0 1,1 Ошибка цитирования Неверный тег
<ref>
; для сносокMPC-Pannonia
не указан текст - ↑ 2,0 2,1 Ошибка цитирования Неверный тег
<ref>
; для сносокspringer
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокjpldata
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокMPC-Circulars-Archive
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокBembrick-2002b
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокgeneva-obs
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокWISE
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокAli-Lagoa-2016
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокSIMPS
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокAKARI
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокNugent-2016
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокNugent-2015
не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>
; для сносокlcdb
не указан текст
- Английская Википедия
- Background asteroids
- Discoveries by György Kulin
- Named minor planets
- Astronomical objects discovered in 1938
- Страницы, где используется шаблон "Навигационная таблица/Телепорт"
- Страницы с телепортом
- Википедия
- Статья из Википедии
- Статья из Английской Википедии
- Страницы с ошибками в примечаниях