742 Edisona
Appearance
Discovery | |
---|---|
Synodic rotation period | 18.52 h (0.772 d) |
0.1286±0.022 | |
9.55 | |
742 Edisona is a
plane of the ecliptic.[1] This is a member of the dynamic Eos family of asteroids that most likely formed as the result of a collisional breakup of a parent body.[3]
rotation period of 18.52±0.01 with a brightness variation of 0.30±0.01 in magnitude.[4] It spans a girth of approximately 45.6 km.[1]
References
- ^ NASA Jet Propulsion Laboratory, retrieved 5 May 2016.
- ISBN 9783662028049.
- .
- Bibcode:2008MPBu...35..179B.
External links
- 742 Edisona at AstDyS-2, Asteroids—Dynamic Site
- 742 Edisona at the JPL Small-Body Database