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7066 Nessus facts for kids

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7066 Nessus
Discovery
Discovered by David L. Rabinowitz
Discovery date April 26, 1993
Designations
1993 HA2
Centaur
Orbital characteristics
Epoch December 31, 2006 (JD 2454100.5)
Aphelion 5607.451 Gm (37.483 AU)
Perihelion 1769.167 Gm (11.826 AU)
3688.309 Gm (24.655 AU)
Eccentricity 0.520
44714.802 d (122.42 a)
5.57 km/s
43.762°
Inclination 15.647°
31.216°
170.814°
Physical characteristics
Dimensions 60±16 km
Mass ~1.6×1017 kg
Mean density
2.0? g/cm³
Equatorial surface gravity
~0.0148 m/s²
Equatorial escape velocity
~0.0280 km/s
? d
Pole ecliptic latitude
?
Pole ecliptic longitude
?
0.06
Temperature ~56 K
?
9.6

7066 Nessus is a small, icy space object. It belongs to a group called centaurs. These objects orbit the Sun between Jupiter and Neptune.

Nessus was found by David L. Rabinowitz on April 26, 1993. He was working with the Spacewatch project at Kitt Peak. Nessus was the second centaur he discovered. It was also the third centaur ever found.

What is a Centaur?

Centaurs are like a mix between asteroids and comets. They are icy bodies that orbit the Sun. Their orbits are often unstable because of the gravity from the giant planets.

Nessus's Journey Around the Sun

Nessus takes about 122.4 years to go around the Sun once. Its path is not a perfect circle. It is quite stretched out.

Closest and Farthest Points

When Nessus is closest to the Sun, this point is called perihelion. At perihelion, it gets closer to the Sun than Uranus. When it is farthest from the Sun, this point is called aphelion. At aphelion, Nessus travels even farther out than Neptune.

How its Orbit Changes

The orbits of centaurs like Nessus can change over time. This happens because of the strong gravity of the giant planets in our Solar System. Scientists believe Nessus's orbit will stay stable for a very long time.

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