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321 Florentina
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| background | #D6D6D6 |
| name | 321 Florentina |
| image | 321Florentina (Lightcurve Inversion).png |
| caption | A three-dimensional model of 321 Florentina based on its light curve |
| discoverer | Johann Palisa |
| discovered | 15 October 1891 |
| mpc_name | (321) Florentina |
| pronounced | |
| mp_category | Main belt (Koronis) |
| epoch | 31 July 2016 (JD 2457600.5) |
| semimajor | 2.88657 AU |
| perihelion | 2.7543 AU |
| aphelion | 3.01879 AU |
| eccentricity | 0.045806 |
| period | 1791.3 days |
| inclination | 2.5876° |
| asc_node | 40.224° |
| arg_peri | 37.310° |
| mean_anomaly | 120.99° |
| dimensions | |
| rotation | 2.871 h |
| abs_magnitude | 10.1 |
| albedo | |
| mean_motion | / day |
| orbit_ref | |
| observation_arc | 118.15 yr (43153 d) |
| uncertainty | 0 |
321 Florentina is an S-type (stony) main belt asteroid with a diameter of . It was discovered by Johann Palisa on 15 October 1891 in Vienna. He named the asteroid for his daughter, Florentine.{{cite book
This asteroid is a dynamic member of the Koronis family. It is orbiting the Sun at a distance of with an eccentricity (ovalness) of 0.046 and an orbital period of 1791.3 days. The orbital plane is inclined at an angle of 2.59° to the plane of the ecliptic. Photometric data collected during the asteroid opposition of 2011 was used to construct a light curve that displayed a rotation period of . This is consistent with previous rotation estimates.{{cite journal
A group of astronomers, including Lucy d'Escoffier Crespo da Silva, contributed data toward the discovery of spin-vector alignments in the Koronis family, which includes (321) Florentina. This was based on observations made between 1998 through 2000. The collaborative work resulted in the creation of 61 new individual rotation lightcurves to augment previous published observations.{{cite journal
References
References
- "321 Florentina". [[NASA]]/[[Jet Propulsion Laboratory]].
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