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The Charon-Pluto mass ratio from MKO astrometryUsing 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 10(exp 24) 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.
Document ID
19950030751
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Young, L. A.
(Massachusetts Institute of Technology, Cambridge, MA United States)
Olkin, C. B.
(Massachusetts Institute of Technology, Cambridge, MA United States)
Elliot, J. L.
(Massachusetts Institute of Technology, Cambridge, MA United States)
Tholen, D. J.
(University of Hawaii, Honolulu, HI United States)
Buie, M. W.
(Lowell Observatory, Flagstaff, AZ United States)
Date Acquired
August 16, 2013
Publication Date
April 1, 1994
Publication Information
Publication: ICARUS
Volume: 108
Issue: 2 pt
ISSN: 0019-1035
Subject Category
Astronomy
Accession Number
95A62350
Funding Number(s)
CONTRACT_GRANT: NAGW-3296
CONTRACT_GRANT: NAGW-1991
CONTRACT_GRANT: NSF AST-89-06011
CONTRACT_GRANT: NAGW-1494
Distribution Limits
Public
Copyright
Other

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