307261 Máni

307261 Máni
Máni imaged by the Hubble Space Telescope on 9 April 2006
Discovery
Discovered byChadwick A. Trujillo
Michael E. Brown
Discovery sitePalomar Obs.
Discovery date18 June 2002
Designations
(307261) Máni
Pronunciation/ˈmɑːn/
Named after
Máni
2002 MS4
TNO · classical (hot)
distant · Scat-Ext
Orbital characteristics (barycentric)
Epoch 25 February 2023 (JD 2460000.5)
Uncertainty parameter 1
Observation arc68.24 yr (24,924 d)
Earliest precovery date8 April 1954
Aphelion47.801 AU
Perihelion35.677 AU
41.739 AU
Eccentricity0.1453
269.48 yr (98,429 d)
226.844°
0° 0m 13.167s / day
Inclination17.693°
216.075°
≈ 10 June 2123
±0.4 days
214.575°
Known satellites0
Physical characteristics
Dimensions(824±20) × (770±34) km (projected)
796±24 km
Flattening≥0.066±0.034
14.251 h
7.33 h or 10.44 h (single-peaked)
0.100±0.025 or 0.098±0.004 (geometric)
0.039±0.005 (Bond)
Temperature65 K
20.5
3.56±0.03
3.63±0.05
3.62

307261 Máni (provisional designation 2002 MS4) is a large trans-Neptunian object in the Kuiper belt, a region of icy planetesimals beyond Neptune. It was discovered on 18 June 2002 by Chad Trujillo and Michael Brown during their search for Pluto-sized Kuiper belt objects at Palomar Observatory. With a diameter of about 800 km (500 mi), Máni is large enough that it might be a dwarf planet, though its irregular shape suggests that (as with 4 Vesta) this may not be the case.

The surface is dark gray and is composed of water and carbon dioxide ices. Máni has been observed making stellar occultations, which revealed massive topographic features along the outline of its shape. These features include a mountain-like peak that is 25 km (16 mi) tall and a crater-like depression that is 320 km (200 mi) wide and 45 km (28 mi) deep. Máni's topographic features are among the tallest and deepest known for bodies of the Solar System.