Discovery[1] | |
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Discovered by | Scott S. Sheppard |
Discovery site | Las Campanas Obs. |
Discovery date | 12 May 2018 |
Orbital characteristics[1][2] | |
Epoch 25 February 2023 (JD 2460000.5) | |
Observation arc | 4.35 yr (1590 d) |
0.1525861 AU (22,826,560 km) | |
Eccentricity | 0.2731285 |
–1.93 yr (–704.56 days) | |
16.59790° | |
0° 30m 39.453s / day | |
Inclination | 164.90043° (toecliptic) |
240.00514° | |
296.52870° | |
Satellite of | Jupiter |
Group | Carme group |
Physical characteristics | |
≈1 km[3] | |
23.9[3] | |
17.3[1] | |
S/2018 J 3 is a small outer natural satelliteofJupiter discovered by Scott S. Sheppard on 12 May 2018, using the 6.5-meter Magellan-Baade TelescopeatLas Campanas Observatory, Chile. It was announced by the Minor Planet Center on 19 January 2023, after observations were collected over a long enough time span to confirm the satellite's orbit.[1]
S/2018 J 3 is part of the Carme group, a tight cluster of retrograde irregular moons of Jupiter that follow similar orbits to Carmeatsemi-major axes between 22–24 million km (14–15 million mi), orbital eccentricities between 0.2–0.3, and inclinations between 163–166°.[3] It has a diameter of about 1 km (0.62 mi) for an absolute magnitude of 17.3, making it one of Jupiter's smallest known moons.[3]
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Listed in increasing approximate distance from Jupiter | |
Inner moons |
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Galilean moons |
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Themisto |
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Himalia group (9) |
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Carpo group (2) |
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Valetudo |
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Ananke group (26) |
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Carme group (30) |
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Pasiphae group (18) |
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See also |
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