3850 Peltier, provisional designation 1986 TK2, is a Florian asteroid and suspected interloper from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 7 October 1986, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station, near Flagstaff, Arizona.[6] The asteroid was named after American amateur astronomer Leslie Peltier.[2]
Discovery [1] | |
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Discovered by | E. Bowell |
Discovery site | Anderson Mesa Stn. |
Discovery date | 7 October 1986 |
Designations | |
MPC designation | (3850) Peltier |
Named after | Leslie Peltier (American amateur astronomer)[2] |
Alternative designations | 1986 TK2 · 1949 PC 1969 OC1 · 1979 OX13 1982 OW |
Minor planet category | main-belt · Flora [3] |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 47.47 yr (17,339 days) |
Aphelion | 2.5967 AU |
Perihelion | 1.8718 AU |
Semi-major axis | 2.2342 AU |
Eccentricity | 0.1622 |
Orbital period (sidereal) | 3.34 yr (1,220 days) |
Mean anomaly | 126.84° |
Mean motion | 0° 17m 42.36s / day |
Inclination | 5.2687° |
Longitude of ascending node | 124.13° |
Argument of perihelion | 207.30° |
Physical characteristics | |
Dimensions | 4.00 km (calculated)[3] |
Synodic rotation period | 2.4287±0.0002 h[lower-alpha 1] 2.4289±0.0001 h[4] |
Geometric albedo | 0.4 (assumed)[3] |
Spectral type | SMASS = V [1] · V [3] |
Absolute magnitude (H) | 13.6[1][3] · 13.62±0.37[5] |
In the SMASS taxonomy, Peltier is a V-type asteroid but possesses the orbital characteristics of a member of the Flora family, which is one of the largest groups of stony S-type asteroids in the main-belt. It is therefore thought to be an unrelated interloper that does not origin from the Flora family's parent body. Peltier orbits the Sun in the inner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,220 days). Its orbit has an eccentricity of 0.16 and an inclination of 5° with respect to the ecliptic.[1] In 1949, it was first identified as 1949 PC at Johannesburg. The body's observation arc begins at Crimea-Nauchnij in 1979, when it was identified as 1979 OX13, 10 years prior to its official discovery observation at Anderson Mesa.[6]
A rotational lightcurve of Peltier was obtained by Czech astronomer Petr Pravec at Ondřejov Observatory in October 2006.[lower-alpha 2] Lightcurve analysis gave a rotation period of 2.4287 hours with a brightness variation of 0.09 magnitude (U=2).[lower-alpha 1] In December 2013, photometric observations by Australian amateur astronomer Julian Oey gave a concurring period of 2.4289 hours and an amplitude of 0.10 magnitude (U=3).[4]
Peltier has not been observed by any space-based surveys such as the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, or NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for V-type asteroids of 0.40 and calculates a diameter of 4.00 kilometers using an absolute magnitude of 13.6.[3]
This minor planet was named in memory of American amateur astronomer Leslie Peltier (1900–1980), who has discovered 12 comets and several novae including Nova Herculis 1963.[2] Naming citation was provided by David H. Levy and published by the MPC on 20 May 1989 (M.P.C. 14633).[7]
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