4754 Panthoos
Discovery | |
---|---|
Discovered by | Cornelis Johannes van Houten, Ingrid van Houten-Groeneveld and Tom Gehrels |
Discovery site | Palomar Observatory |
Discovery date | 16 October 1977 |
Designations | |
MPC designation | 4754 |
Named after | Panthous |
5010 T-3 | |
Orbital characteristics[1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 0 | |
Observation arc | 14031 days (38.41 yr) |
Aphelion | 5.2919 AU (791.66 Gm) |
Perihelion | 5.1831 AU (775.38 Gm) |
5.2375 AU (783.52 Gm) | |
Eccentricity | 0.010394 |
11.99 yr (4378.10 d) | |
118.811° | |
0° 4m 56.017s / day | |
Inclination | 12.327° |
155.060° | |
202.920° | |
Earth MOID | 4.17546 AU (624.640 Gm) |
Jupiter MOID | 0.118533 AU (17.7323 Gm) |
Jupiter Tisserand parameter | 2.954 |
Physical characteristics | |
Dimensions | 59 km[2] |
Mean radius | 26.575 ± 2.1 km |
27.68 h (1.153 d) | |
0.0571 ± 0.010 | |
10.0 | |
|
4754 Panthoos (5010 T-3) is a Jupiter Trojan discovered on October 16, 1977 by Cornelis Johannes van Houten, Ingrid van Houten-Groeneveld and Tom Gehrels at Palomar Observatory.
Photometric observations of this asteroid during 1994 were used to build a light curve showing a rotation period of 27.68 ± 0.05 hours with a brightness variation of 0.09 ± 0.01 magnitude.[2]
References
- ↑ "4754 Panthoos (5010 T-3)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 14 April 2016.
- 1 2 Mottola, Stefano; Di Martino, Mario; Erikson, Anders; Gonano-Beurer, Maria; Carbognani, Albino; Carsenty, Uri; Hahn, Gerhard; Schober, Hans-Josef; Lahulla, Felix; Delbò, Marco; Lagerkvist, Claes-Ingvar (May 2011). "Rotational Properties of Jupiter Trojans. I. Light Curves of 80 Objects". The Astronomical Journal 141 (5): 170. Bibcode:2011AJ....141..170M. doi:10.1088/0004-6256/141/5/170.
External links
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