Eukelade (Moon)
Retrograde motion, Irregular moon, Jupiter, Scott S. Sheppard, Orbital inclination, Ecliptic, Retrograde motion
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Eukelade, also known as Jupiter XLVII, is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2003, and received the temporary designation S/2003 J 1. Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484 Mm in 735.200 days, at an inclination of 164° to the ecliptic, in a retrograde direction and with an eccentricity of 0.2829. It wa...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Eukelade, also known as Jupiter XLVII, is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2003, and received the temporary designation S/2003 J 1. Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484 Mm in 735.200 days, at an inclination of 164° to the ecliptic, in a retrograde direction and with an eccentricity of 0.2829. It was named in March 2005 after Eukelade, described by some Greek writers as one of the Muses, and thus a daughter of Zeus.
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