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(24835) 1995 SM55 (provisional designation 1995 SM55) is an icy 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. Stellar occultation observations in 2025 show that it has highly reflective surface and a diameter of about 200 km (120 mi). This highly reflective surface is typical for Haumea family Kuiper belt objects, which are believed to be icy fragments of the dwarf planet Haumea.
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