.jpg) A multichord occultation by Tanete | |
| Discovery | |
|---|---|
| Discovered by | A. Massinger |
| Discovery site | Heidelberg Obs. |
| Discovery date | 19 December 1913 |
| Designations | |
| (772) Tanete | |
Named after | Tanete, a place in Sulawesi[1] |
| 1913 TR | |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 101.93 yr (37230 d) |
| Aphelion | 3.2768 AU (490.20 Gm) |
| Perihelion | 2.7244 AU (407.56 Gm) |
| 3.0006 AU (448.88 Gm) | |
| Eccentricity | 0.092055 |
| 5.20 yr (1898.5 d) | |
| 163.71° | |
| 0° 11m 22.668s / day | |
| Inclination | 28.854° |
| 63.832° | |
| 146.061° | |
| Earth MOID | 1.73811 AU (260.018 Gm) |
| Jupiter MOID | 1.78259 AU (266.672 Gm) |
| TJupiter | 3.059 |
| Physical characteristics | |
| 58.83±2 km | |
| 17.258 h (0.7191 d) | |
| 0.0594±0.004 | |
| 8.33 | |
772 Tanete is an asteroid from the asteroid belt. Since 2004 it has been observed in stellar occultation four times.[3] Its size is best described by an ellipsoid measuring 124.1±1.2 km x 116.1±1.2 km. Analysis of a light curve captured during 2014 shows a synodic rotation period of 17.258±0.001 h with an amplitude of 0.15 magnitude.[4]
In 1984, a fly-by of 772 Tanete was considered for a Mariner Mark II rendezvous mission with the short period comet 22P/Kopff.[5]
- ^ (in Indonesian) http://langitselatan.com/2011/01/12/nama-nama-indonesia-pun-tertera-di-angkasa/
- ^ "772 Tanete (1913 TR)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
- ^ "Asteroid Data Sets". sbn.psi.edu. Retrieved 26 May 2018.
- ^ Cite error: The named reference
Martinez_Ferrero_2014was invoked but never defined (see the help page). - ^ Cite error: The named reference
Stetson_et_al_2016was invoked but never defined (see the help page).