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54 Alexandra
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| background | #D6D6D6 |
| name | 54 Alexandra |
| image | 54 Alexandra.png |
| caption | A three-dimensional model of 54 Alexandra based on its light curve (top) and images of the asteroid (bottom) |
| discovery_ref | |
| discoverer | H. Goldschmidt |
| discovered | 10 September 1858 |
| mpc_name | (54) Alexandra |
| pronounced | |
| adjective | Alexandrian |
| named_after | Alexander von Humboldt |
| (German explorer) | |
| mp_category | Main belt |
| epoch | December 31, 2006 (JD 2454100.5) |
| semimajor | 405.763 million km (2.712 AU) |
| perihelion | 326.043 million km (2.179 AU) |
| aphelion | 485.483 million km (3.245 AU) |
| eccentricity | 0.196 |
| period | 1631.620 day |
| inclination | 11.804° |
| asc_node | 313.446° |
| arg_peri | 345.594° |
| pole_ecliptic_lat | |
| pole_ecliptic_lon | |
| mean_anomaly | 103.809° |
| dimensions | 160 × 135 km (± 1 km) |
| mean_diameter | 154.137 km |
| mass | |
| density | |
| rotation | 18.14 h |
| spectral_type | Tholen C |
| SMASS C | |
| abs_magnitude | 7.66 |
| albedo | 0.056 |
(German explorer) SMASS C
54 Alexandra is a carbonaceous asteroid from the intermediate asteroid belt, approximately 155 kilometers in diameter. It was discovered by German-French astronomer Hermann Goldschmidt on 10 September 1858, and named after the German explorer Alexander von Humboldt; it was the first asteroid to be named after a male.
Description
On May 17, 2005, this asteroid occulted a faint star (magnitude 8.5) and the event was observed and timed in a number of locations within the U.S. and Mexico. As a result, a silhouette profile was produced, yielding a roughly oval cross-section with dimensions of 160 × 135 km (± 1 km). The mass of the asteroid can be estimated based upon the mutually perturbing effects of other bodies, yielding an estimate of .
Photometric observations of this asteroid during 1990–92 gave a light curve with a period of 18.14 ± 0.04 hours and a brightness variation of 0.10 in magnitude. Alexandra has been studied by radar. It was the namesake and largest member of the former Alexandra asteroid family; a dynamic group of C-type asteroids that share similar orbital elements. Other members included 70 Panopaea and 145 Adeona. 145 Adeona was subsequently assigned to the Adeona family, with Alexandra and Panopaea being dropped.
In popular culture
In the Swedish film Aniara, it is mentioned that 54 Alexandra is the closest celestial body which the off-course and out-of-control spacecraft will approach before it leaves the Solar System.
References
References
- "Alexandra". [[Oxford University Press]]}}
{{dict.com. - "Asteroid Data Sets".
- D.W. Dunham, "Upcoming Asteroid Occultations", ''Sky & Telescope'', June, 2006, p. 63.
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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