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90482 Orcus facts for kids

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90482 Orcus
Orcus nasa.jpg
Discovery
Discovered by M. Brown,
C. Trujillo,
D. Rabinowitz
Discovery date February 17, 2004
Designations
2004 DW
Plutino
Orbital characteristics
Epoch November 30, 2008 (JD 2 454 800)
Aphelion 7 188.17 Gm (48.05 AU)
Perihelion 4 535.80 Gm (30.32 AU)
5 862.44 Gm (39.188 AU)
Eccentricity 0.226 18
89 606 d (245.33 yr)
4.68 km/s
164.68°
Inclination 20.593°
268.722°
72.474°
Known satellites 1 (92-432 km)
Physical characteristics
Dimensions 946.3 +74.1−72.3 km (diameter)
Mass ~7.5×1020 kg
Mean density
~1.5 g/cm³ (assumed)
~0.2 m/s²
~0.44 km/s
13.19h
Albedo 19.75 +3.40−2.76 %
Temperature ~45 K
Spectral type
B-V=0.68; V-R=0.37
19.1 (opposition)
2.3

90482 Orcus is a dwarf planet that lives in the Kuiper belt. The Kuiper belt is a huge ring of icy objects beyond Neptune. Orcus was first called 2004 DW when it was found.

Three scientists named Michael Brown, Chad Trujillo, and David Rabinowitz discovered Orcus. They found it on February 17, 2004. Interestingly, it had been seen in older pictures from November 8, 1951, but wasn't recognized as a dwarf planet then.

Orcus is special because it moves around the Sun in a way similar to Pluto. It has an orbital resonance with Neptune. This means that for every two times Neptune goes around the Sun, Orcus goes around three times. But here's the cool part: Orcus always stays on the opposite side of the Sun from Pluto!

Orcus's Moon

Orcus has its own moon! This moon was discovered on February 22, 2007.

Scientists found the moon very close to Orcus. They used special tools to measure its brightness. Based on how bright it is, they think the moon is about 220 kilometers (about 137 miles) wide. They believe this moon might be a smaller object from the Kuiper belt that Orcus's gravity pulled in.


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See also

Kids robot.svg In Spanish: (90482) Orcus para niños

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