Английская Википедия:(24835) 1995 SM55

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Шаблон:Infobox planet

Шаблон:Mp, provisional designation Шаблон:Mp, is a trans-Neptunian object and member of the Haumea family that resides in the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 19 September 1995, by American astronomer Nichole Danzl of the Spacewatch program at Kitt Peak National Observatory near Tucson, Arizona, in the United States.[1] It measures approximately 200 kilometers in diameter and was the second-brightest known object in the Kuiper belt, after Pluto, until Шаблон:Mpl- was discovered.

Origin

Шаблон:Main

Шаблон:Mp is a member of the Haumea family.[2] It has the highest collisional velocity, a δv of 123.3 m/s, of all confirmed members.[3] Based on their common pattern of IR water-ice absorptions, neutral visible spectrum[4] and the clustering of their orbital elements, the other KBOs Шаблон:Mpl-, Шаблон:Mpl-, Шаблон:Mpl- and Шаблон:Mpl- all appear to be collisional fragments broken off of the dwarf planet Шаблон:Dp.

Naming

As of 2018, this minor planet has not been named by the Minor Planet Center.[1]

Orbital diagram

Файл:Haumea family orbits.png
Шаблон:Mp among other members of the Haumea family

References

Шаблон:Reflist

External links

Шаблон:Use dmy dates Шаблон:Haumea Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:Trans-Neptunian objects

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