Three-dimensional model of 53 Kalypso created based on light-curve. | |
Discovery | |
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Discovered by | Karl Theodor Robert Luther |
Discovery date | 4 April 1858 |
Designations | |
MPC designation | (53) Kalypso |
Pronunciation | /kəˈlɪpsoʊ/ |
Named after | Calypso |
Minor planet category | Main belt |
Adjectives | Kalypsonian /kælɪpˈsoʊniən/ Kalypsoian /kælɪpˈsoʊ.iən/ |
Orbital characteristics | |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 471.807 Gm (3.154 AU) |
Perihelion | 311.998 Gm (2.086 AU) |
Semi-major axis | 391.903 Gm (2.620 AU) |
Eccentricity | 0.204 |
Orbital period (sidereal) | 1548.736 d (4.24 a) |
Mean anomaly | 98.113° |
Inclination | 5.153° |
Longitude of ascending node | 143.813° |
Argument of perihelion | 312.330° |
Physical characteristics | |
Dimensions | 115.4 km |
Mass | (1.294 ± 0.520/0.412)×10 kg |
Mean density | 1.625 ± 0.653/0.517 g/cm |
Synodic rotation period | 9.036 h |
Geometric albedo | 0.040 |
Absolute magnitude (H) | 8.81 |
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.
Notes
- Assuming a diameter of 115 ± 10.324 km.
References
- ^ "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
- Noah Webster (1884) A Practical Dictionary of the English Language
- "calypsonian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ Yeomans, Donald K., "53 Kalypso", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 April 2013.
- ^ Fienga, A.; Avdellidou, C.; Hanuš, J. (February 2020). "Asteroid masses obtained with INPOP planetary ephemerides". Monthly Notices of the Royal Astronomical Society. 492 (1). doi:10.1093/mnras/stz3407.
- ^ Pilcher, Frederick (April 2010), "Rotation Period Determination for 53 Kalypso", The Minor Planet Bulletin, 37 (2): 75–76, Bibcode:2010MPBu...37...75P.
- Asteroid Data Sets Archived 2009-12-17 at the Wayback Machine
- Šidlichovský, M. (1999), Svoren, J.; Pittich, E. M.; Rickman, H. (eds.), "Resonances and chaos in the asteroid belt", Evolution and source regions of asteroids and comets : proceedings of the 173rd colloquium of the International Astronomical Union, held in Tatranska Lomnica, Slovak Republic, August 24–28, 1998, pp. 297–308, Bibcode:1999esra.conf..297S.
- Pray, Donald P.; et al. (December 2006), "Lightcurve analysis of asteroids 53, 698, 1016, 1523, 1950, 4608, 5080 6170, 7760, 8213, 11271, 14257, 15350 and 17509", The Minor Planet Bulletin, 33 (4): 92–95, Bibcode:2006MPBu...33...92P.
- "Radar-Detected Asteroids and Comets". NASA/JPL Asteroid Radar Research. Retrieved 30 October 2011.
External links
- 53 Kalypso at AstDyS-2, Asteroids—Dynamic Site
- 53 Kalypso at the JPL Small-Body Database
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