Английская Википедия:(202421) 2005 UQ513
Шаблон:Mp, also written as 2005 UQ513, is a cubewano with an absolute magnitude of 3.97.[1] Its spectrum has a weak signature of absorption by water ice.[2][3] Like Quaoar, it has a very red spectrum,[4][5] which indicates that its surface probably contains many complex, processed organic molecules.[4] Its light curve shows variations of Δm=0.3 mag, but no period has been determined.[5]
Classification
Шаблон:Mp has a perihelion of 37.3 AU.[1] The Minor Planet Center (MPC) classifies it as a cubewano[6] while the Deep Ecliptic Survey (DES) classifies it as ScatExt (scattered-extended).[7] Although dynamically it would have been a good candidate to be a member of the Haumea collisional family, given its red spectrum, it is not.[4][5]
Distance
As of December 2018, it is currently 48.0 AU from the Sun.[8] It will come to perihelion in 2123.[9]
It has been observed 194 times over 14 oppositions with precovery images back to 1990.[1]
See also
References
External links
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 сносокjpldataне указан текст - ↑ Шаблон:Cite journal
- ↑ Trujillo, C. A., Sheppard, S. S., & Schaller E. L. (2011). A Photometric System for Detection of Water and Methane Ices on Kuiper Belt Objects Шаблон:ArXiv
- ↑ 4,0 4,1 4,2 Pinilla-Alonso, N., Licandro, J., & Lorenzi, V. (2008). Visible spectroscopy in the neighborhood of Шаблон:Mp (Haumea) Шаблон:ArXiv
- ↑ 5,0 5,1 5,2 Snodgrass, C., Carry, B., Dumas, C., & Hainaut, O. (2009). Characterisation of candidate members of (136108) Haumea’s family Шаблон:ArXiv
- ↑ Ошибка цитирования Неверный тег
<ref>; для сносокMPEC2010-S44не указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокBuieне указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокAstDySEphне указан текст - ↑ Ошибка цитирования Неверный тег
<ref>; для сносокperihelionне указан текст
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