Английская Википедия:471143 Dziewanna
Шаблон:Short description Шаблон:Infobox planet
471143 Dziewanna (provisional designation Шаблон:Mp) is a trans-Neptunian object in the scattered disc, orbiting the Sun in the outermost region of the Solar System.
Dziewanna was discovered on 13 March 2010 by astronomers Andrzej Udalski, Scott Sheppard, Marcin Kubiak and Chad Trujillo at the Las Campanas Observatory in Chile.[1] Based on its absolute magnitude and assumed albedo, it is estimated to have a diameter of approximately 470 kilometers.[2] It was named after Devana (Polish form: Dziewanna), a Slavic goddess of the wilderness, forests and the hunt,[1] in honor of the fact that it was discovered during the Polish OGLE project of Warsaw University, which was led by Udalski.[3]
Distance
Dziewanna orbits the Sun at a distance of 32.6 to 108.3 AU once every 591 years and 4 months (215,992 days). Its orbit has an eccentricity of 0.54 and an inclination of 29° with respect to the ecliptic.[5] It is currently 39.1 AU from the Sun and will reach perihelion in 2038.[5][6] A ten-million-year integration of the orbit shows that this object is in a 2:7 resonance with Neptune.[7]
A precovery image was taken by the Near-Earth Asteroid Tracking at Palomar Observatory in 2002. This extends Dziewanna's observation arc to 8 years prior to discovery. It has since been observed 143 times over 6 oppositions and has an orbit quality of 1.[1]
Physical properties
In 2010, the thermal radiation of Dziewanna was observed by the Herschel Space Telescope, which allowed astronomers to estimate its diameter at about Шаблон:Cvt.[2] A stellar occultation by Dziewanna was observed on 17 May 2019, yielding a single-chord diameter of Шаблон:Cvt.[8]
A rotational lightcurve was obtained from photometric observations at the discovering observatory, with the 2.5-meter Irénée du Pont Telescope, and published in May 2013. The lightcurve shows that the rotation period is Шаблон:Val hours; the variation in brightness is of magnitude 0.12 (Шаблон:Small).[9]
Observations by American astronomer Michael Brown at the Keck telescope in March 2012 failed to find a satellite. There is therefore currently no means to determine Dziewanna's mass.[2]
See also
References
External links
- MPEC 2010 G50 : 2010 EK139, Minor Planet Electronic Circular, issued on 8 April 2010
- OCKS: OGLE Carnegie Kuiper belt Survey (OCKS is a Southern sky survey searching for Kuiper-belt objects and dwarf planets)
- List Of Centaurs and Scattered-Disk Objects, Minor Planet Center
- Шаблон:JPL small body
Шаблон:Trans-Neptunian objects Шаблон:Dwarf planets Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:Authority control
- ↑ 1,0 1,1 1,2 Ошибка цитирования Неверный тег
<ref>; для сносокMPC-objectне указан текст - ↑ 2,0 2,1 2,2 Ошибка цитирования Неверный тег
<ref>; для сносокTNOsCool7не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокKrzysztofне указан текст - ↑ Шаблон:Cite web
- ↑ 5,0 5,1 Ошибка цитирования Неверный тег
<ref>; для сносокjpldataне указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокAstDysне указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокBuieне указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокLuckyStarне указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокBenecchi-2013не указан текст
- Английская Википедия
- Страницы с неработающими файловыми ссылками
- Scattered disc and detached objects
- Trans-Neptunian objects in a 2:7 resonance
- Discoveries by Andrzej Udalski
- Discoveries by Scott S. Sheppard
- Discoveries by Chad Trujillo
- Named minor planets
- Possible dwarf planets
- Objects observed by stellar occultation
- Astronomical objects discovered in 2010
- Страницы, где используется шаблон "Навигационная таблица/Телепорт"
- Страницы с телепортом
- Википедия
- Статья из Википедии
- Статья из Английской Википедии
- Страницы с ошибками в примечаниях
