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Collisional properties of ice spheres at low impact velocitiesThe results of experimental studies on the impact properties of water ice are discussed. Stable temperatures of 85 K and pressures as low as 10 to the -5th Torr were achieved using a new apparatus consisting of a compound disk pendulum and a stainless steel, temperature-controlled cryostat. The coefficient of restitution as a function of velocity was obtained for ice spheres with four different radii of curvature and with a variety of surface conditions. These data can be well fitted by an exponetial law epsilon of given form for most measurements. Surface conditions can drastically alter the resulting value of epsilon, however. In particular, the presence of frost or a roughened contact surface can lower epsilon at a given velocity by 10-30 percent from that of a smooth sphere. It is shown how the presence of frost can change the velocity behavior of epsilon from an exponential to a power-law form. The applications of the results to the dynamics of Saturn's rings are discussed.
Document ID
19880047765
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hatzes, Artie P.
(Lick Observatory Santa Cruz, CA, United States)
Lin, D. N. C.
(Lick Observatory Santa Cruz, CA, United States)
Bridges, Frank G.
(California, University Santa Cruz, United States)
Date Acquired
August 13, 2013
Publication Date
April 15, 1988
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 231
ISSN: 0035-8711
Subject Category
Lunar And Planetary Exploration
Accession Number
88A34992
Funding Number(s)
CONTRACT_GRANT: NAGW-590
Distribution Limits
Public
Copyright
Other

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