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4834 Thoas
Jupiter trojan from the Greek camp
Jupiter trojan from the Greek camp
| Field | Value |
|---|---|
| minorplanet | yes |
| name | 4834 Thoas |
| background | #C2FFFF |
| discovery_ref | |
| discoverer | C. Shoemaker |
| discovery_site | Palomar Obs. |
| discovered | 11 January 1989 |
| mpc_name | (4834) Thoas |
| alt_names | |
| 1986 XN | |
| adjective | Thoantian |
| pronounced | |
| named_after | Thoas (Greek mythology) |
| mp_category | Jupiter trojan |
| Greekbackground | |
| orbit_ref | |
| epoch | 23 March 2018 (JD 2458200.5) |
| uncertainty | 0 |
| observation_arc | 30.59 yr (11,172 d) |
| aphelion | 5.9248 AU |
| perihelion | 4.5156 AU |
| semimajor | 5.2202 AU |
| eccentricity | 0.1350 |
| period | 11.93 yr (4,356 d) |
| mean_anomaly | 210.23° |
| mean_motion | / day |
| inclination | 28.466° |
| asc_node | 76.035° |
| arg_peri | 351.66° |
| jupiter_moid | 0.5567 AU |
| tisserand | 2.7420 |
| mean_diameter | |
| (derived) | |
| rotation | |
| albedo | |
| (derived) | |
| spectral_type | C (assumed) |
| V–I | |
| abs_magnitude | 9.0 |
| 9.1 | |
| 9.20 | |
1986 XN Greekbackground
(derived)
(derived)
V–I
9.1
9.20
4834 Thoas is a large Jupiter trojan from the Greek camp, approximately 86 km in diameter. It was discovered on 11 January 1989, by astronomer Carolyn Shoemaker at the Palomar Observatory. The C-type asteroid is one of the 50 largest Jupiter trojans and has a rotation period of 18.19 hours. It was named after Thoas from Greek mythology.
Orbit and classification
Thoas is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's Lagrangian point, 60° ahead of its orbit in a 1:1 resonance (see Trojans in astronomy). It is a non-family asteroid in the Jovian background population. It orbits the Sun at a distance of 4.5–5.9 AU once every 11 years and 11 months (4,356 days; semi-major axis of 5.22 AU). Its orbit has an eccentricity of 0.14 and an inclination of 28° with respect to the ecliptic.
The asteroid was first observed as ** Crimea–Nauchnij in December 1975. The body's observation arc begins in December 1986, with its observation as at Anderson Mesa Station, more than 2 years prior to its official discovery observation at Palomar.
Physical characteristics
Thoas is an assumed C-type asteroid.
Rotation period
In September 1996, observations by Stefano Mottola using the now decommissioned Bochum 0.61-metre Telescope at ESO's La Silla Observatory in Chile gave a rotation period of 18.22 hours with a brightness amplitude of 0.14 magnitude (). Between 2010 and 2015, refined photometric observations by Robert Stephens, Daniel Coley, Brian Warner and collaborators at the Center for Solar System Studies in Landers, California, gave three concurring periods of 18.14–18.216 hours and a brightness variation of 0.22–0.39 magnitude, with the best rated result of 18.192 hours and an amplitude of 0.22 magnitude ().
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Thoas measures between 72.33 and 96.21 kilometers in diameter and its surface has an albedo between 0.040 and 0.085.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0536 and a diameter of 86.90 kilometers based on an absolute magnitude of 9.1.
Naming
This minor planet was named by the discoverer after the Greek hero Thoas from the Trojan War. Thoas was the commander of the Aetolians. He was impersonated by Poseidon, who, in Thoas's voice, rallied the Greeks and fought by their side in the shape of Thoas, when the Trojans were close to the Greek ships. The official naming citation was published by the Minor Planet Center on 25 August 1991 (M.P.C. 18647).
Notes
References
References
- Noah Webster (1884) ''A Practical Dictionary of the English Language''
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
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