Jupiter LXIV: Difference between revisions
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| avg_speed = <!--(Average orbital speed)--> |
| avg_speed = <!--(Average orbital speed)--> |
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| eccentricity = 0.148<ref name="ScottSS">{{cite web |last1=Sheppard |first1=Scott S. |title=Jupiter's Moons |url=https://sites.google.com/carnegiescience.edu/sheppard/moons/jupitermoons |website=carnegiescience.edu |publisher=sites.google.com |accessdate=18 July 2018}}</ref> |
| eccentricity = 0.148<ref name="ScottSS">{{cite web |last1=Sheppard |first1=Scott S. |title=Jupiter's Moons |url=https://sites.google.com/carnegiescience.edu/sheppard/moons/jupitermoons |website=carnegiescience.edu |publisher=sites.google.com |accessdate=18 July 2018}}</ref> |
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| period = |
| period = 605.76 days<ref name="mpec"/><!--(Orbital period)--> |
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| inclination = 147.9°<ref name="ScottSS" /> |
| inclination = 147.9°<ref name="ScottSS" /> |
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| angular_dist = |
| angular_dist = |
Revision as of 08:30, 1 August 2018
Discovery | |
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Discovered by | Scott S. Sheppard et al. |
Discovery date | 2017 |
Orbital characteristics | |
Mean orbit radius | 20,694,000 km[1] |
Eccentricity | 0.148[1] |
605.76 days[2] | |
Inclination | 147.9°[1] |
S/2017 J 3 is an outer natural satellite of Jupiter. It was discovered by Scott S. Sheppard and his team in 2017, but not announced until July 17, 2018 via a Minor Planet Electronic Circular from the Minor Planet Center.[2] It is about 2 kilometers in diameter and orbits at a semi-major axis of about 20,694,000 km with an inclination of about 147.9°. It belongs to the Ananke group.[1]
References
- ^ a b c d Sheppard, Scott S. "Jupiter's Moons". carnegiescience.edu. sites.google.com. Retrieved 18 July 2018.
- ^ a b "MPEC 2018-O11 : S/2017 J 3". Minor Planet Center. International Astronomical Union. Retrieved 17 July 2018.