Jupiter LV: Perbedaan antara revisi

Yupiter LV memiliki diameter sekitar 2 kilometer, dan mengorbit Yupiter dari jarak rata-rata 20,220&nbsp;Gm selama 587,38 hari, di [[inklinasi]] sebesar 146° terhadap [[ekliptika]] (148° terhadap khatulistiwa Yupiter), dalam arah ''[[gerak retrograde dan prograde|retrograde]]'' dan dengan [[eksentrisitas orbit|eksentrisitas]] sebesar 0,1048.<ref>[http://www.minorplanetcenter.net/mpec/K17/K17L09.html MPEC 2017-L09: S/2003 J 18] 2 Juni 2017 (pememuan kembali dan efemeris)</ref>

 

 

Satelit ini hilang setelah penemuannya pada tahun 2003.<ref>{{cite web |url=http://www.skyandtelescope.com/astronomy-news/outer-planet-moons-found-and-lost/ |title=Outer-Planet Moons Found — and Lost |last=Beatty |first=Kelly |date=4 April 2012 |website=www.skyandtelescope.com |publisher=[[Sky & Telescope]] |access-date=27 June 2017}}</ref><ref name=Jacobson>{{cite journal |last1=Brozović |first1=Marina |last2=Jacobson |first2=Robert A. |date=9 Maret 2017 |title=The Orbits of Jupiter's Irregular Satellites |journal=The Astronomical Journal |volume=153 |issue=4 |pages=147 |doi=10.3847/1538-3881/aa5e4d|bibcode = 2017AJ....153..147B }}</ref><ref>{{cite journal |last1=Jacobson |first1=B. |last2=Brozović |first2=M. |first3=B. |last3=Gladman |first4=M. |last4=Alexandersen |first5=P. D. |last5=Nicholson |first6=C. |last6=Veillet |date=28 September 2012 |title=Irregular Satellites of the Outer Planets: Orbital Uncertainties and Astrometric Recoveries in 2009–2011 |journal=The Astronomical Journal |volume=144 |issue=5 |pages=132 |doi=10.1088/0004-6256/144/5/132 |bibcode = 2012AJ....144..132J }}</ref><ref>{{cite web |url=http://home.dtm.ciw.edu/users/sheppard/satellites/jup2017.html |title=New Moons of Jupiter Announced in 2017 |last=Sheppard |first=Scott S. |date=2017 |website=home.dtm.ciw.edu |access-date=27 June 2017 |quote=We likely have all of the lost moons in our new observations from 2017, but to link them back to the remaining lost 2003 objects requires more observations a year later to confirm the linkages, which will not happen until early 2018. ... There are likely a few more new moons as well in our 2017 observations, but we need to reobserve them in 2018 to determine which of the discoveries are new and which are lost 2003 moons.}}</ref> Satelit ini ditemukan kembali pada tahun 2017 dan diberikan sebutan permanen pada tahun yang sama.<ref>{{cite web |url=http://home.dtm.ciw.edu/users/sheppard/satellites/jupsatdata.html |title=Jupiter's Known Satellites |last=Sheppard |first=Scott S. |date=2017 |website=home.dtm.ciw.edu |access-date=10 Agustus 2017}}</ref>