Discovery [1] [2] | |
---|---|
Discovered by | Scott S. Sheppard |
Discovery site | Cerro Tololo Obs. |
Discovery date | 11 May 2018 |
Designations | |
S/2018 J 4 | |
Orbital characteristics [3] | |
Epoch 1 January 2000 ( JD 2451545.0) | |
Observation arc | 4.55 yr (1,663 d) |
Satellite of | Jupiter |
Group | Carpo |
Proper orbital elements | |
Proper
semi-major axis | 16,328,500 km (0.109149 AU) AU |
Proper
eccentricity | 0.177 |
Proper
inclination | 50.2° (to ecliptic) |
Proper
mean motion | 307.484673 deg / yr |
Proper
orbital period | 1.17079
yr (427.631 d) |
Precession of
perihelion | N/A arcsec / yr |
Precession of the
ascending node | 6638.868 arcsec / yr |
Physical characteristics | |
Mean diameter | ≈2 km [4] |
Albedo | 0.04 (assumed) [4] |
23.5 [4] | |
16.7 [1] | |
S/2018 J 4 is a small outer natural satellite of Jupiter discovered by Scott S. Sheppard on 11 May 2018, using the 4.0-meter Víctor M. Blanco Telescope at Cerro Tololo Observatory, Chile. It was announced by the Minor Planet Center on 20 January 2023, after observations were collected over a long enough time span to confirm the satellite's orbit. [1] The satellite has a diameter of about 2 km (1.2 mi) for an absolute magnitude of 16.7. [4]
S/2018 J 4 is an irregular moon of Jupiter on an highly inclined prograde orbit at an angle of 53° with respect to the ecliptic plane. It belongs to the same group as the similarly-inclined moon Carpo, which was long thought to be an outlier until the discovery of S/2018 J 4. [4] Like all irregular moons of Jupiter, S/2018 J 4's orbit is highly variable over time due to gravitational perturbations by the Sun and other planets. [5] On average, S/2018 J 4's orbit has a semi-major axis of 16.3 million km (10.1 million mi), an eccentricity of 0.18, and a very high inclination of 50° with respect to the ecliptic. [3]
Like Carpo, S/2018 J 4's very high inclination subjects it to the Lidov–Kozai resonance, where there is a periodic exchange between its orbital eccentricity and inclination while its argument of pericenter oscillates about a constant value without apsidally precessing. [6] For example, the Lidov–Kozai resonance causes Carpo's eccentricity and inclination to fluctuate between 0.19–0.69 and 44–59°, respectively. [5] S/2018 J 4's argument of pericenter oscillates about 270° with respect to the ecliptic, which keeps its perijove always above Jupiter and apojove below Jupiter. [3]