Astronomy:26 Proserpina
 Three-dimensional model of 26 Proserpina created based on light-curve inversions. | |
| Discovery | |
|---|---|
| Discovered by | R. Luther |
| Discovery date | May 5, 1853 |
| Designations | |
| (26) Proserpina | |
| Pronunciation | /proʊˈsɜːrpɪnə/[1] |
| Named after | Proserpina |
| 1935 KK; 1954 WD1 | |
| Minor planet category | Main belt |
| Adjectives | Proserpinian /ˌprɒsərˈpɪniən/[2] |
| Orbital characteristics | |
| Epoch June 14, 2006 (JD 2453900.5) | |
| |{{{apsis}}}|helion}} | 431.898 Gm (2.887 AU) |
| |{{{apsis}}}|helion}} | 362.816 Gm (2.425 AU) |
| 397.357 Gm (2.656 AU) | |
| Eccentricity | 0.087 |
| Orbital period | 1581.184 d (4.33 a) |
| Mean anomaly | 115.619° |
| Inclination | 3.562° |
| Longitude of ascending node | 45.884° |
| 193.120° | |
| Physical characteristics | |
| Dimensions | 94.8 ± 1.7 km (IRAS)[3] 89.63 ± 3.55 km[4] |
| Mass | (7.48 ± 8.95) × 1017 kg[4] |
| Mean density | 1.98 ± 2.38 g/cm3[4] |
| Rotation period | 13.11 h[3][5] |
| Geometric albedo | 0.1966[3][6] |
| S[3] | |
| Absolute magnitude (H) | 7.5[3] |
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Proserpina (minor planet designation: 26 Proserpina) is a main-belt asteroid discovered by German astronomer R. Luther on May 5, 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 in the pipeline for Unicode 17.0 as U+1CECD (.svg){kind=small}
).[7][8]
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.[9] This was refined by a 2008 study, giving a period of 13.110 ± 0.001 hours.[10]
References
- ↑ Noah Webster (1884) A Practical Dictionary of the English Language
- ↑ E.g. Andrew & Reid (2003) Two Hundred Years of Pushkin
- ↑ 3.0 3.1 3.2 3.3 3.4 "JPL Small-Body Database Browser: 26 Proserpina". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=26. Retrieved 2012-01-28.
- ↑ 4.0 4.1 4.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73 (1): 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode: 2012P&SS...73...98C. See Table 1.
- ↑ "Asteroid lightcurve derived data". http://www.psi.edu/pds/asteroid/EAR_A_5_DDR_DERIVED_LIGHTCURVE_V8_0/data/lc.tab.
- ↑ "Asteroid Albedos". http://www.psi.edu/pds/asteroid/EAR_A_5_DDR_ALBEDOS_V1_1/data/albedos.tab.
- ↑ Bala, Gavin Jared; Miller, Kirk (18 September 2023). "Unicode request for historical asteroid symbols". Unicode. https://www.unicode.org/L2/L2023/23207-historical-asteroids.pdf.
- ↑ Unicode. "Proposed New Characters: The Pipeline". The Unicode Consortium. https://unicode.org/alloc/Pipeline.html.
- ↑ Ditteon, Richard; Hawkins, Scot (September 2007), "Asteroid Lightcurve Analysis at the Oakley Observatory - October-November 2006", The Minor Planet Bulletin 34 (3): 59–64, Bibcode: 2007MPBu...34...59D.
- ↑ Pilcher, Frederick (September 2008), "Period Determinations for 26 Proserpina, 34 Circe 74 Galatea, 143 Adria, 272 Antonia, 419 Aurelia, and 557 Violetta", The Minor Planet Bulletin 35 (3): 135–138, Bibcode: 2008MPBu...35..135P.
External links
- 26 Proserpina at AstDyS-2, Asteroids—Dynamic Site
- 26 Proserpina at the JPL Small-Body Database
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