Precise Timings of Galilean Satellite Eclipses and Assessment of the E5 Ephemeris

Details Precise Timings of Galilean Satellite Eclipses and Assessment of the E5 Ephemeris Precise Timings of Galilean Satellite Eclipses and Assessment of the E5 Ephemeris

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000icar..147..348m&link_type=abstract

Icarus, Volume 147, Issue 2, pp. 348-352 (2000).

Astronomy and Astrophysics

Astrophysics

12

Scientific paper

Galilean satellite astrometry has been derived from CCD photometry of nearly 200 eclipses in the shadow of Jupiter between the years 1990 and 2000. The root-mean-square differences as compared to predictions from J. H. Lieske's E5 ephemeris (1998, Astron. Astrophys. Suppl. 129, 205-217), expressed as along-track distances, are Io, 62 km&semi Europa, 267 km; Ganymede, 142 km; and Callisto, 146 km.

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