首页 | 本学科首页   官方微博 | 高级检索  
     


Characteristics of Icy Surfaces
Authors:Louise M. Prockter  Rosaly M. C. Lopes  Bernd Giese  Ralf Jaumann  Ralph D. Lorenz  Robert T. Pappalardo  Gerald W. Patterson  Peter C. Thomas  Elizabeth P. Turtle  Roland J. Wagner
Affiliation:1. Applied Physics Laboratory, Johns Hopkins University, MP3-E169, 11100 Johns Hopkins Road, Laurel, MD, 20723, USA
2. Jet Propulsion Laboratory, California Institute of Technology, M/S 183-601, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA
3. German Aerospace Center (DLR), Institute of Planetary Research, Planetary Geodesy, Rutherfordstra?e 2, 12489, Berlin, Germany
4. Cornell University, 422 Space Sciences Building, Ithaca, NY, 14853, USA
Abstract:
The surfaces of the Solar System’s icy satellites show an extraordinary variety of morphological features, which bear witness to exchange processes between the surface and subsurface. In this paper we review the characteristics of surface features on the moons of Jupiter, Saturn, Uranus and Neptune. Using data from spacecraft missions, we discuss the detailed morphology, size, and topography of cryovolcanic, tectonic, aeolian, fluvial, and impact features of both large moons and smaller satellites.
Keywords:
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号