687 Tinette
| Discovery | |
|---|---|
| Discovered by | J. Palisa |
| Discovery site | Vienna |
| Discovery date | 16 August 1909 |
| Designations | |
| 1909 HG | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 97.38 yr (35569 d) |
| Aphelion | 3.4628 AU (518.03 Gm) |
| Perihelion | 1.9794 AU (296.11 Gm) |
| 2.7211 AU (407.07 Gm) | |
| Eccentricity | 0.27256 |
| 4.49 yr (1639.5 d) | |
| 260.701° | |
| 0° 13m 10.488s / day | |
| Inclination | 14.878° |
| 334.346° | |
| 52.932° | |
| Earth MOID | 1.01691 AU (152.128 Gm) |
| Jupiter MOID | 2.18126 AU (326.312 Gm) |
| Jupiter Tisserand parameter | 3.257 |
| Physical characteristics | |
| 7.40 h (0.308 d)[2][1] | |
| 11.71 | |
|
| |
687 Tinette is a minor planet orbiting the Sun. It was discovered by Austrian astronomer Johann Palisa on August 16, 1909 from Vienna and was given the preliminary designation 1909 HG.
Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado in 1999 were used to build a light curve for this object. The asteroid displayed a rotation period of 7.40 ± 0.02 hours and a brightness variation of 0.25 ± 0.01 in magnitude.[2]
References
- 1 2 "687 Tinette (1909 HG)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
- 1 2 Warner, Brian D. (January 2011), "Upon Further Review: IV. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory", The Minor Planet Bulletin, 38 (1), pp. 52–54, Bibcode:2011MPBu...38...52W.
External links
This article is issued from Wikipedia - version of the 9/10/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.