162 Laurentia
Synodic rotation period | 11.8686 h (0.49453 d)[2][4] | |
| 0.051±0.006[2] | ||
| C | ||
| 9.16[2] | ||
162 Laurentia is a large and dark main-belt asteroid that was discovered by the French brothers Paul Henry and Prosper Henry on 21 April 1876, and named after Joseph Jean Pierre Laurent, an amateur astronomer who discovered asteroid 51 Nemausa.
An occultation by Laurentia was observed from Clive, Alberta on 21 November 1999.[citation needed]
Photometric observations of this asteroid from multiple observatories during 2007 gave a light curve with a period of 11.8686 ± 0.0004 hours and a brightness variation of 0.40 ± 0.05 in magnitude. This is in agreement with previous studies in 1994 and 2007.[4]
References
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
"Laurentian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.) - ^ NASA Jet Propulsion Laboratory, retrieved 12 May 2016.
- ^ .
- ^ Bibcode:2008MPBu...35...47O.
External links
- 162 Laurentia at AstDyS-2, Asteroids—Dynamic Site
- 162 Laurentia at the JPL Small-Body Database
_mathilde.jpg){kind=small} | This article about an S-type asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |