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20000 Varuna

File:20000-varuna_hst.jpg · Wikimedia Commons · See Wikimedia Commons

EntityQ15609· pop 55· linked from 89 articles

20000 Varuna

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Also known as Varuna, 2000 WR106, (20000) 2000 WR106

Kuiper belt object

AI overview

20000 Varuna is a large icy body orbiting the Sun in the distant Kuiper Belt region beyond Neptune. It is scientifically important because studying objects like Varuna helps astronomers understand the composition and history of the early solar system.

AI-generated from the Wikipedia summary — may contain errors.

In the Vinony graph

Within Vinony's link graph, 20000 Varuna is referenced by 89 other articles, and connects out to apsis, semi-axis and organic compound.

It sits within the topics Astronomical objects discovered in 2000, Classical Kuiper belt objects and Discoveries by the Spacewatch project.

Its subject is documented across 54 Wikipedia language editions.

Wikidata facts

Diameter
900.0
Orbital period
103632.4453155141
Image
20000-varuna hst.jpg
Show 16 more facts
longitude of ascending node
97.21030234100793
Commons category
20000 Varuna
provisional designation
2000 WR106
time of discovery or invention
2000-11-28
orbital inclination
17.13812404484431
orbital eccentricity
0.05254516459334936
color index
0.88
absolute magnitude
3.79
periapsis
40.90942694015417
apoapsis
45.44704180401708
semi-major axis of an orbit
43.17823437208563
mean anomaly
115.0289798413239
argument of periapsis
273.2206220996139
albedo
0.07
rotation period
6.3436
time of periapsis
2427887.3487135964
Sources (3)

via Wikidata · CC0

~27 min read

Encyclopedic overview

20000 Varuna (provisional designation 2000 WR106) is a large trans-Neptunian object in the Kuiper belt. It was discovered in November 2000 by American astronomer Robert McMillan during a Spacewatch survey at the Kitt Peak National Observatory. It is named after the Hindu deity Varuna, one of the oldest deities mentioned in the Vedic texts.

Varuna's light curve is compatible with the body being a Jacobi ellipsoid, suggesting that it has an elongated shape due to its rapid rotation. Varuna's surface is moderately red in color due to the presence of complex organic compounds on its surface. Water ice is also present on its surface, and is thought to have been exposed by past collisions which may have also caused Varuna's rapid rotation. Although no natural satellites have been found or directly imaged around Varuna, analysis of variations in its light curve in 2019 suggests the presence of a possible satellite orbiting closely around Varuna. Assumptions that the body is in hydrostatic equilibrium (and thus a dwarf planet) result in a calculated density too low for it to be a dwarf planet.

Excerpted from Wikipedia’s “20000 Varuna” article, available under the CC BY-SA 4.0 licence.

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