Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994icar..108..186y&link_type=abstract
Icarus, vol. 108, no. 2, pt. 1, p. 186-199
Astronomy and Astrophysics
Astronomy
19
Astrometry, Center Of Gravity, Charon, Mass Ratios, Planetary Mass, Pluto (Planet), Astronomical Photography, Charge Coupled Devices, Telescopes
Scientific paper
Using the University of Hawaii (UH) 2.2-m telescope, we obtained charge coupled device (CCD) images of Pluto as it passed through a single field of 10 stars during 6 nights of Charon's 6.4-day orbital period. From these data, Charon's orbital semimajor axis is found to be 19,460 +/- 58 km, which is consistent with the recent measurement by Null et al. (1993), of 19,405 +/- 86 km. Our semimajor axis implies a system mass of (14.32 +/- 0.13) x 1024 g. From the motions of Pluto and Charon around their barycenter, we find that the ratio of Charon's mass to Pluto's is 0.1566 +/- 0.0035, indicating that the bodies both have densities near 2 g/cc. Our ratio is nearly twice that of Null et al., who find a ratio of 0.0837 +/- 0.0147. Possible reasons for the large discrepancy are discussed.
Buie Marc William
Elliot James L.
Olkin Catherine B.
Tholen David J.
Young Larry A.
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