ENCELADUS GEODETIC FRAMEWORK

Oberst, J.; Hussmann, H.; Giese, B.; Sohl, F.; Shoji, D.; Stark, A.; Wickhusen, K.; Wählisch, M.

The small (approximately 500 km in diameter) satellite Enceladus is moving near the equatorial plane and deep in the gravity field of its parent planet Saturn. Owing to tidal interaction with its parent, Enceladus has adopted a pronounced 3-axial ellipsoidal shape and is tidally locked, with rotational and orbital periods of about 1.37 days. As the equator of Saturn is inclined to the planet’s orbital plane, Enceladus, like most of the other satellites of Saturn, undergoes pronounced seasons. This paper gives a summary of the current status as well as shortcomings of our current knowledge regarding Enceladus’ geodetic and dynamic parameters.

Zitieren

Zitierform:

Oberst, J. / Hussmann, H. / Giese, B. / et al: ENCELADUS GEODETIC FRAMEWORK. 2017. Copernicus Publications.

Zugriffsstatistik

Gesamt:
Volltextzugriffe:
Metadatenansicht:
12 Monate:
Volltextzugriffe:
Metadatenansicht:

Grafik öffnen

Rechte

Rechteinhaber: J. Oberst et al.

Nutzung und Vervielfältigung:

Export