2004 Lexell
Florian asteroid
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2004 Lexell, provisional designation 1973 SV2, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7.5 kilometers in diameter. The asteroid was discovered on 22 September 1973, by Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula, and later named for Swedish-Russian astronomer and mathematician Anders Johan Lexell.[2][10]
| Discovery[1] | |
|---|---|
| Discovered by | N. Chernykh |
| Discovery site | Crimean Astrophysical Obs. |
| Discovery date | 22 September 1973 |
| Designations | |
| (2004) Lexell | |
Named after | Anders Johan Lexell (Swedish-Russian astronomer)[2] |
| 1973 SV2 · 1938 WL 1941 SN1 · 1959 GC 1972 HK | |
| main-belt · Flora[3] | |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 78.55 yr (28,689 days) |
| Aphelion | 2.3451 AU |
| Perihelion | 1.9986 AU |
| 2.1718 AU | |
| Eccentricity | 0.0798 |
| 3.20 yr (1,169 days) | |
| 215.94° | |
| 0° 18m 28.44s / day | |
| Inclination | 2.4967° |
| 4.5440° | |
| 58.504° | |
| Physical characteristics | |
| Dimensions | 7.255±0.216 km[4] 7.456±0.084 km[5] 7.82 km (calculated)[3] 14.7 km[6] |
| 5.44±0.02 h[7] 5.441±0.002 h[8] 5.4429±0.0003 h[6] | |
| 0.056[6] 0.24 (assumed)[3] 0.2908±0.0522[5] 0.306±0.041[4] | |
| LS[9] · S[3] | |
| 12.6[5] · 12.7[1][3] · 12.908±0.064[6] · 13.04±0.00[9] | |
Classification and orbit
Lexell is a member of the Flora family, one of the largest collisional populations of stony asteroids. It orbits the Sun at a distance of 2.0–2.3 AU once every 3 years and 2 months (1,169 days). Its orbit has an eccentricity of 0.08 and an inclination of 2° with respect to the ecliptic.[1]
The asteroid was first identified as 1938 WL at the Finnish Turku Observatory in November 1938, extending the body's observation arc by 35 years prior to its official discovery observation at Nauchnij.[10]
Physical characteristics
Pan-STARRS' photometric survey characterized Lexell as a LS-type asteroid, which transitions between the common S-type and rare L-type asteroid.[9]
Rotation period
In March 2013, two rotational lightcurves of Lexell were obtained from photometric observations by Gary Haagen at Stonegate Observatory, Massachusetts, and by a group of astronomers at the Oakley Southern Sky Observatory (E09), Australia. Lightcurve analysis gave a well-defined rotation period of 5.441 and 5.4429 hours with a brightness variation of 0.45 and 0.42 magnitude, respectively (U=3/3).[6][8]
In February 2013, observations made by French amateur astronomer Pierre Antonini gave a concurring period of 5.44 hours with an amplitude of 0.51 magnitude (U=3-).[7]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lexell measures 7.255 and 7.456 kilometers in diameter and its surface has an albedo of 0.306 and 0.2908, respectively.[4][5] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 7.82 kilometers based on an absolute magnitude of 12.7.[3]
Naming
This minor planet was named after Anders Johan Lexell (1740–1784), a Swedish-Russian astronomer and mathematician. The official naming citation was published by the Minor Planet Center on 15 October 1977 (M.P.C. 4238).[11] The lunar crater Lexell was also named in his honor, as is Lexell's Comet, of which he computed its orbit.[2]