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26 Proserpina
Main-belt asteroid
Main-belt asteroid
| Field | Value | |
|---|---|---|
| image | A713.M1189.shape.png | |
| caption | Three-dimensional model of 26 Proserpina created based on light-curve inversions. | |
| minorplanet | yes | |
| background | #D6D6D6 | |
| name | 26 Proserpina | |
| symbol | [[Image:Proserpina symbol (bold).svg | 24px]] (historical) |
| discoverer | R. Luther | |
| discovered | 5 May 1853 | |
| pronounced | ||
| adjective | Proserpinian | |
| mpc_name | (26) Proserpina | |
| alt_names | 1935 KK; | |
| named_after | Proserpina | |
| mp_category | Main belt | |
| orbit_ref | ||
| epoch | 21 November 2025 (JD 2461000.5) | |
| semimajor | 2.655 AU | |
| perihelion | 2.420 AU | |
| aphelion | 2.890 AU | |
| eccentricity | 0.089 | |
| period | 4.327 yr (1580.27 d) | |
| inclination | 3.555° | |
| asc_node | 45.685° | |
| arg_peri | 196.057° | |
| mean_anomaly | 289.591° | |
| jupiter_moid | 2.106 AU | |
| tisserand | 3.380 | |
| dimensions | 94.8 ± 1.7 km (IRAS) | |
| 89.63 ± 3.55 km | ||
| mass | (7.48 ± 8.95) × 1017 kg | |
| density | 1.98 ± 2.38 g/cm3 | |
| rotation | 13.11 h | |
| spectral_type | S | |
| abs_magnitude | 7.5 | |
| albedo | 0.1966 |
89.63 ± 3.55 km
26 Proserpina is a main-belt asteroid discovered by German astronomer R. Luther on 5 May 1853. It is named after the Roman goddess Proserpina, the daughter of Ceres and the Queen of the Underworld. Another main-belt asteroid, 399 Persephone, discovered in 1895, is named after her Greek counterpart. Its historical symbol was a star inside a pomegranate; it is encoded in Unicode as ([[File:Proserpina symbol (fixed width).svg|12px]]).{{cite web | access-date = September 9, 2025 | url-status = live
This object is orbiting the Sun with a period of 4.33 years. It has a cross-section size of around 90 km and a stony (S-type) composition. Photometric observations of this asteroid have produced discrepant estimates of the rotation period. A period of 12.13 hours was reported in 1979, followed by 10.6 hours in 1981 and 6.67 hours in 2001. Observations made in 2007 at the Oakley Observatory in Terre Haute, Indiana produced a light curve with a period of 13.06 ± 0.03 hours and a brightness variation of 0.21 ± 0.01 in magnitude. This was refined by a 2008 study, giving a period of 13.110 ± 0.001 hours.
References
References
- Noah Webster (1884) ''A Practical Dictionary of the English Language''
- E.g. Andrew & Reid (2003) ''Two Hundred Years of Pushkin''
- "Asteroid lightcurve derived data".
- (18 September 2023). "Unicode request for historical asteroid symbols". Unicode.
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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