Open Access
Cratering Time Scales for the Galilean Satellites
E. M. Shoemaker,R. F. Wolfe +1 more
- 01 Jan 1982
pp 277
143
TL;DR: In this paper, an attempt is made to estimate the present cratering rate for each Galilean satellite within the correct order of magnitude and to extend the cratering rates back into the geologic past on the basis of evidence from the earth-moon system.
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Abstract: An attempt is made to estimate the present cratering rate for each Galilean satellite within the correct order of magnitude and to extend the cratering rates back into the geologic past on the basis of evidence from the earth-moon system For collisions with long and short period comets, the magnitudes and size distributions of the comet nuclei, the distribution of their perihelion distances, and the completeness of discovery are addressed The diameters and masses of cometary nuclei are assessed, as are crater diameters and cratering rates The dynamical relations between long period and short period comets are discussed, and the population of Jupiter-crossing asteroids is assessed Estimated present cratering rates on the Galilean satellites are compared and variations of cratering rate with time are considered Finally, the consistency of derived cratering time scales with the cratering record of the icy Galilean satellites is discussed
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Citations
Cratering Records in the Inner Solar System in Relation to the Lunar Reference System
TL;DR: In this paper, the size-frequency distribution (SFD) for lunar craters is used to estimate the SFD for projectiles which formed craters on terrestrial planets and on asteroids, and the result shows the relative stability of these distributions during the past 4 Gyr.
733
Does Europa have a subsurface ocean? Evaluation of the geological evidence
Robert T. Pappalardo,M. J. S. Belton,H. Herbert Breneman,Michael H. Carr,Clark R. Chapman,Geoffrey C. Collins,Tilmann Denk,Sarah A. Fagents,Paul Geissler,Bernd Giese,Ronald Greeley,Richard Greenberg,James W. Head,Paul Helfenstein,Gregory V. Hoppa,S. D. Kadel,Kenneth P. Klaasen,James E. Klemaszewski,K. Magee,K. Magee,Alfred S. McEwen,Jeffrey M. Moore,William B. Moore,Gerhard Neukum,Cynthia B. Phillips,Louise M. Prockter,Gerald Schubert,David A. Senske,David A. Senske,R. J. Sullivan,B. R. Tufts,Elizabeth P. Turtle,Robert Wagner,K. K. Williams +33 more
TL;DR: In this article, the authors summarize the geological evidence regarding an extant subsurface ocean, concentrating on Galileo imaging data and assess nine pertinent lines of geological evidence: impact morphologies, lenticulae, cryovolcanic features, pull-apart bands, chaos, ridges, surface frosts, topography, and global tectonics.
459
Energetic Ion and Electron Irradiation of the Icy Galilean Satellites
TL;DR: Galileo Orbiter measurements of energetic ions (20 keV to 100 MeV) and electrons (20-700 keV) in Jupiter's magnetosphere are used, in conjunction with the JPL electron model (less than 40 MeV), to compute irradiation effects in the surface layers of Europa, Ganymede, and Callisto as mentioned in this paper.
445
Nonuniform cratering of the Moon and a revised crater chronology of the inner Solar System
TL;DR: In this article, a semi-analytical model of the Moon and terrestrial planets from the present knowledge of the orbital and size distribution of asteroids and comets in the inner Solar System was used to refine the crater chronology method.
361
The tides of Io
TL;DR: In this paper, a theory for the origin and evaluation of the orbital resonances between the Galilean satellites Io, Europa and Ganymede as a result of the effects of dissipative tides in Jupiter and its satellites is developed.
302
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