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Belinda (moon) facts for kids

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Belinda
Image of Belinda acquired by Voyager 2
Belinda viewed by Voyager 2 in 1986
Discovery
Discovered by Stephen P. Synnott / Voyager 2
Discovery date January 13, 1986
Designations
MPC designation Uranus XIV
Adjectives Belindian
Orbital characteristics
Mean orbit radius
75,255.613 ± 0.057 km
Eccentricity 0.00007 ± 000073
0.623527470 ± 0.000000017 d
Inclination 0.03063 ± 0.028° (to Uranus' equator)
Satellite of Uranus
Physical characteristics
Dimensions 128 × 64 × 64 km
Mean radius
40.3 ± 8 km
~25,000 km2
Volume ~380,000 km3
Mass ~3.6×1017 kg
Mean density
~1.3 g/cm3 (assumed)
~0.014 m/s2
~0.034 km/s
synchronous
zero
Albedo 0.08 ± 0.01
Temperature ~64 K

Belinda is a small, inner moon of the planet Uranus. It was first seen in pictures taken by the Voyager 2 spacecraft on January 13, 1986. At first, it was given the temporary name S/1986 U 5.

Belinda's Family of Moons

Belinda is part of a group of moons called the Portia group. This family also includes moons like Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Rosalind, and Perdita. These moons all travel in similar paths around Uranus and reflect light in similar ways. We don't know much about Belinda, except for its orbit, its size (about 45 kilometers wide), and how much light it reflects.

What Belinda Looks Like

The pictures from Voyager 2 show that Belinda is shaped like a stretched-out egg. Its longest side always points towards Uranus. The moon is very long and thin, with its short side being about half the length of its long side. Its surface appears to be grey in color.

Belinda's Future

The moons orbiting close to Uranus are not expected to stay in their current paths forever. Over many millions of years, their orbits can become unstable. Scientists believe that Belinda and another smaller moon called Cupid might be the first pair to crash into each other. This collision could happen in about 100,000 to 10 million years. This is because of how their gravity pulls on each other.

See also

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