Astronomy:713 Luscinia
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Discovery | |
---|---|
Discovered by | J. Helffrich |
Discovery site | Heidelberg Obs. |
Discovery date | 18 April 1911 |
Designations | |
(713) Luscinia | |
Pronunciation | /luːˈsɪniə/[1] |
1911 LS | |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 105.00 yr (38350 d) |
|{{{apsis}}}|helion}} | 3.9473 astronomical unit|AU (590.51 Gm) |
|{{{apsis}}}|helion}} | 2.8350 AU (424.11 Gm) |
3.3912 AU (507.32 Gm) | |
Eccentricity | 0.16400 |
Orbital period | 6.24 yr (2281.0 d) |
Mean anomaly | 133.98° |
Mean motion | 0° 9m 28.188s / day |
Inclination | 10.359° |
Longitude of ascending node | 217.687° |
137.252° | |
Physical characteristics | |
Mean radius | 52.76±1.55 km |
Rotation period | 9.9143 h (0.41310 d) |
Geometric albedo | 0.0410±0.003 |
Absolute magnitude (H) | 8.97 |
713 Luscinia is a large, main belt asteroid orbiting the Sun. It is a member of the Cybele asteroid group.[3]
References
- ↑ "Luscinia". Merriam-Webster Dictionary. https://www.merriam-webster.com/dictionary/Luscinia.
- ↑ "713 Luscinia (1911 LS)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=713;cad=1.
- ↑ Lagerkvist, Claes-Ingvar et al. (January 2001), "A Study of Cybele Asteroids. I. Spin Properties of Ten Asteroids", Icarus 149 (1): 190–197, doi:10.1006/icar.2000.6507, Bibcode: 2001Icar..149..190L.
External links
- Lightcurve plot of (713) Luscinia, Antelope Hills Observatory
- 713 Luscinia at AstDyS-2, Asteroids—Dynamic Site
- 713 Luscinia at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/713 Luscinia.
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