Precise timings of Galilean satellite eclipses and assessment of the E-3 ephemeris

Details Precise timings of Galilean satellite eclipses and assessment of the E-3 ephemeris Precise timings of Galilean satellite eclipses and assessment of the E-3 ephemeris

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994icar..107..212m&link_type=abstract

Icarus, vol. 107, p. 212

Astronomy and Astrophysics

Astronomy

5

Galilean Satellites, Eclipses, Astronomical Coordinates, Planet Ephemerides, Position Errors, Charge Coupled Devices, Root-Mean-Square Errors, Galileo Spacecraft

Scientific paper

Astrometric positions for the Galilean satellites are derived from high-precision timings of their Jovian eclipses observed with CCD cameras in 1990-1993. The results are compared with the E-3 ephemeris obtained by Lieske (1991). Much smaller observational scatter values are obtained than the rms residuals of the observations of the E-3 ephemeris.

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