Trans-Neptunian Objects Codexery

(26308) 1998 SM165

A twotino binary with a low-density, icy composition.

(26308) 1998 SM165

(26308) 1998 SM165 is a resonant trans-Neptunian object and binary system from the Kuiper belt, discovered on 16 September 1998 by American astronomer Nichole Danzl at the Kitt Peak National Observatory in Arizona. It is notable as a twotino, meaning it stays in a 1:2 orbital resonance with Neptune, and as a binary system with a minor-planet moon discovered in 2001.

Quick Facts

Minorplanet
yes
Background
#C2E0FF
Discoverer
N. Danzl
Discovery Site
Kitt Peak Obs.
Discovered
16 September 1998
Mpc Name
(26308) 1998 SM · 165
Mp Category
TNOtwotino / Kozaidistant
Epoch
4 September 2017 (JD 2458000.5)
Uncertainty
2
Observation Arc
32.26 yr (11,784 days)
Earliest Precovery Date
12 October 1982
Aphelion
64.968 AU

Facts from the source article.

Lore & Background

1998 SM165 is classified as a twotino by the Deep Ecliptic Survey, meaning it orbits the Sun in a 1:2 resonance with Neptune: for every one orbit of the object, Neptune completes two. Its semi-major axis lies near the edge of the classical Kuiper belt. Observations with the infrared Spitzer Space Telescope and orbits from the Hubble Space Telescope allowed an estimate of its density at 0.51+0.29−0.14 g/cm³, similar to the binary plutino 47171 Lempo and Saturn's moon Hyperion. This low density suggests a highly porous composition dominated by ice. The object is fairly red, with a color comparable to 79360 Sila–Nunam. On 22 December 2001, a minor-planet moon was discovered by American astronomers Michael Brown and Chad Trujillo using the Hubble Space Telescope, announced in January 2002. The satellite measures approximately 96 ± 12 km in diameter and orbits its primary at a distance of 11,310 ± 110 km, completing one orbit in 130.1 ± 1 days, assuming a circular orbit. The minor planet was numbered by the Minor Planet Center on 5 July 2001; as of 2025, it has not been named.

Reader's Guide

The significance of (26308) 1998 SM165 lies in its classification as a twotino, a resonant trans-Neptunian object locked in a 1:2 orbital resonance with Neptune, which helps constrain models of solar system evolution and migration. Its binary nature, with a moon discovered in 2001, provides a rare opportunity to measure physical properties such as density. The estimated density of 0.51+0.29−0.14 g/cm³, derived from Spitzer and Hubble data, is exceptionally low, indicating a highly porous, ice-dominated interior. This density is comparable to other icy bodies like Saturn's moon Hyperion and the binary plutino 47171 Lempo, suggesting a common origin or composition among such objects. The object's red color, similar to 79360 Sila–Nunam, adds to the understanding of surface compositions in the Kuiper belt. As of 2025, it remains unnamed, highlighting the ongoing process of cataloging and characterizing distant solar system bodies.

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