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53 Kalypso
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| bgcolour | #D6D6D6 |
| name | 53 Kalypso |
| image | 53Kalypso (Lightcurve Inversion).png |
| caption | Three-dimensional model of 53 Kalypso created based on light-curve. |
| discovery_ref | |
| discoverer | Karl Theodor Robert Luther |
| discovered | 4 April 1858 |
| mpc_name | (53) Kalypso |
| pronounced | |
| adjective | Kalypsonian |
| Kalypsoian | |
| named_after | Calypso |
| mp_category | Main belt |
| orbit_ref | |
| epoch | December 31, 2006 (JD 2454100.5) |
| semimajor | 391.903 million km (2.620 AU) |
| perihelion | 311.998 million km (2.086 AU) |
| aphelion | 471.807 million km (3.154 AU) |
| eccentricity | 0.204 |
| period | 1548.736 d (4.24 a) |
| inclination | 5.153° |
| asc_node | 143.813° |
| arg_peri | 312.330° |
| mean_anomaly | 98.113° |
| dimensions | 115.4 km |
| mass | (1.294 ± 0.520/0.412) kg |
| density | 1.625 ± 0.653/0.517 g/cm3 |
| rotation | 9.036 h |
| abs_magnitude | 8.81 |
| albedo | 0.040 |
Kalypsoian
53 Kalypso is a large and very dark main belt asteroid that was discovered by German astronomer Robert Luther on April 4, 1858, at Düsseldorf. It is named after Calypso, a sea nymph in Greek mythology, a name it shares with Calypso, a moon of Saturn.
The orbit of 53 Kalypso places it in a mean motion resonance with the planets Jupiter and Saturn. The computed Lyapunov time for this asteroid is 19,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because of gravitational perturbations of the planets.
Photometric observations of this asteroid during 2005–06 gave a light curve with a period of 18.075 ± 0.005 hours and a brightness variation of 0.14 in magnitude. In 2009, a photometric study from a different viewing angle was performed at the Organ Mesa Observatory in Las Cruces, New Mexico, yielding a rotation period of 9.036 ± 0.001 with a brightness variation of 0.14 ± 0.02 magnitude. This is exactly half of the 2005–06 result. The author of the earlier study used additional data observation that favored the 9.036 hour period. The discrepancy was deemed a consequence of viewing the asteroid from different longitudes.
Kalypso has been studied by radar.{{cite web |access-date=2011-10-30}}
Notes
References
References
- Noah Webster (1884) ''A Practical Dictionary of the English Language''
- {{OED. calypsonian
- [http://www.psi.edu/pds/resource/albedo.html Asteroid Data Sets] {{webarchive. link. (2009-12-17)
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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