Orbital elements of the eight major satellites of Saturn determined from a fit of their theories of motion to observations from 1886 to 1985

Details Orbital elements of the eight major satellites of Saturn determined from a fit of their theories of motion to observations from 1886 to 1985 Orbital elements of the eight major satellites of Saturn determined from a fit of their theories of motion to observations from 1886 to 1985

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...267..292d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 267, no. 1, p. 292-299.

Astronomy and Astrophysics

Astrophysics

24

Orbital Elements, Planetary Orbits, Saturn Satellites, Celestial Mechanics, Planet Ephemerides, Saturn, Orbital Elements, Satellites, Motion, Celestial Mechanics, Ephemeris, Astrometry, Hyperion, Iapetus, Theoretical Studies, Mimas, Coordinates, Earth-Based Observations, Enceladus, Tethys, Dione, Rhea, Titan, Procedure, Analysis, Parameters, Comparisons

Scientific paper

A century of positional observations of the eight major Saturnian
satellites are collected. Every observed coordinate is presented under a
unique homogeneous form. This ephemeris is an improvement over the
previous one from Rapaport (1977), particularly for Hyperion and
Iapetus, and for the recent period.

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