Abstract
Tidal torques on Europa due to Jupiter would tend to drive Europa's rotation to a rate slightly faster than synchronous, unless synchroneity is maintained by a permanent asymmetry in Europa's mass distribution. Moreover, global fracture patterns on Europa's surface, as well as the complex fine-scale tectonics revealed by Galileo high-resolution imagery, may be evidence of stress due to nonsynchronous rotation. A direct measurement of Europa's rotation rate is made from the positions of surface features relative to the terminator in a Galileo image and comparing the results with similar measurements of the positions of the same features relative to the terminator in a Voyager 2 image taken 17 years earlier. Any nonsynchronous rotation must be slower than a few tenths of a degree in 17 years (a complete rotation in >104years) relative to the direction of Jupiter.
Original language | English (US) |
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Pages (from-to) | 341-347 |
Number of pages | 7 |
Journal | Icarus |
Volume | 137 |
Issue number | 2 |
DOIs | |
State | Published - Feb 1 1999 |
Keywords
- Europa
- Rotation
- Satellites of Jupiter
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science