Large impact features on Europa: Results of the Galileo Nominal Mission
The Galileo Orbiter examined several impact features on Europa at considerably better resolution than was possible from Voyager. The new data allow us to describe the morphology and infer the geology of the largest impact features on Europa, which are probes into the crust. We observe two basic types of large impact features: (1) “classic” impact craters that grossly resemble well-preserved lunar craters of similar size but are more topographically subdued (e.g., Pwyll) and (2) very flat circular features that lack the basic topographic structures of impact craters such as raised rims, a central depression, or central peaks, and which largely owe their identification as impact features to the field of secondary craters radially sprayed about them (e.g., Callanish). Our interpretation is that the classic craters (all
Citation Information
| Publication Year | 1998 |
|---|---|
| Title | Large impact features on Europa: Results of the Galileo Nominal Mission |
| DOI | 10.1006/icar.1998.5973 |
| Authors | Jeffrey M. Moore, Erik Asphaug, Robert J. Sullivan, James E. Klemaszewski, Kelly C. Bender, Ronald Greeley, Paul E. Geissler, Alfred S. McEwen, Elizabeth P. Turtle, Cynthia B. Phillips, B. Randy Tufts, James W. Head, Robert T. Pappalardo, Kevin B. Jones, Clark R. Chapman, Michael J.S. Belton, Randolph L. Kirk, David Morrison |
| Publication Type | Article |
| Publication Subtype | Journal Article |
| Series Title | Icarus |
| Index ID | 70020067 |
| Record Source | USGS Publications Warehouse |
| USGS Organization | Astrogeology Science Center |