Title of article
Mass and interior of Enceladus from Cassini data analysis
Author/Authors
Rappaport، نويسنده , , Nicole J. and Iess، نويسنده , , Luciano and Tortora، نويسنده , , Paolo and Anabtawi، نويسنده , , Aseel and Asmar، نويسنده , , Sami W. and Somenzi، نويسنده , , Lucia and Zingoni، نويسنده , , Francesco، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2007
Pages
4
From page
175
To page
178
Abstract
Gravity results are available from radio Doppler data acquired by the Deep Space Network during the encounter of the Cassini spacecraft with Enceladus in February 2005. We report the mass of Enceladus to be ( 1.0798 ± 0.0016 ) × 10 20 kg , which implies a density of 1608.9 ± 4 kg m −3 . For a core made of hydrated silicates with a density of 2500 kg m−3 the core radius is ∼ 190 km and the quadrupole moment C 22 ∼ 1.4 × 10 −3 . If Enceladus is in hydrostatic equilibrium, the larger than previously anticipated density implies that the recently proposed secondary spin–orbit resonance cannot be present. Therefore, the source of endogenic activity of Enceladus remains unexplained.
Keywords
Saturnsatellites , interiors
Journal title
Icarus
Serial Year
2007
Journal title
Icarus
Record number
2375423
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