S/2017 J 10
Discovery images of S/2017 J 10 from the 4.0-m Victor M. Blanco Telescope's Dark Energy Camera (DECam) at Cerro Tololo Observatory in March 2023. | |
| Discovery | |
|---|---|
| Discovered by | Scott S. Sheppard |
| Discovery site | Cerro Tololo Obs. |
| Discovery date | 23 March 2017 |
| Orbital characteristics | |
| Epoch 5 May 2025 (JD 2460800.5) | |
| Earliest precovery date | 27 February 2003 |
| 0.14088302 AU (21,075,800 km) | |
| Eccentricity | 0.2587634 |
| −645.09 d | |
| 62.49100° | |
| 0° 33m 29.014s / day | |
| Inclination | 145.57259° (to ecliptic) |
| 38.65145° | |
| 239.09093° | |
| Satellite of | Jupiter |
| Group | Ananke group |
| Physical characteristics | |
| 1 km | |
| Albedo | 0.28 (assumed) |
| 24.1 | |
| 17.0 | |
S/2017 J 10 is a small outer natural satellite of Jupiter discovered by Scott S. Sheppard on 23 March 2017, using the 4.0-meter Víctor M. Blanco Telescope at Cerro Tololo Observatory, Chile. It was announced by the Minor Planet Center on 30 April 2025, after observations were collected over a long enough time span to confirm the satellite's orbit.[1]
S/2017 J is part of the Ananke group, a cluster of retrograde irregular moons of Jupiter that follow similar orbits to Ananke at semi-major axes between 19–22 million km (12–14 million mi), orbital eccentricities between 0.1 and 0.4, and inclinations between 139 and 155°. It has a diameter of about 1 km (0.62 mi) for an absolute magnitude of 17.0.[2]
See also
References
- ^ "MPEC 2025-H210 : S/2017 J 10". www.minorplanetcenter.net. Retrieved 2025-08-29.
- ^ Sheppard, Scott S. "Scott S. Sheppard - JupiterMoons". sites.google.com. Retrieved 2025-08-29.