26 Proserpina

Main-belt asteroid From Wikipedia, the free encyclopedia

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 Roman 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 U+1CECD 𜻍 ASTRONOMICAL SYMBOL FOR ASTEROID PROSERPINA ().[7][8]

Discoverydate5 May 1853
(26) Proserpina
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26 Proserpina
Three-dimensional model of 26 Proserpina created based on light-curve inversions.
Discovery
Discovered byR. Luther
Discovery date5 May 1853
Designations
(26) Proserpina
Pronunciation/proʊˈsɜːrpɪnə/[1]
Named after
Proserpina
1935 KK; 1954 WD1
Main belt
AdjectivesProserpinian /ˌprɒsərˈpɪniən/[2]
Symbol (historical)
Orbital characteristics[3]
Epoch 21 November 2025 (JD 2461000.5)
Aphelion2.890 AU
Perihelion2.420 AU
2.655 AU
Eccentricity0.089
4.327 yr (1580.27 d)
289.591°
Inclination3.555°
45.685°
196.057°
Jupiter MOID2.106 AU
TJupiter3.380
Physical characteristics
Dimensions94.8 ± 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]
13.11 h[3][5]
0.1966[3][6]
S[3]
7.5[3]
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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

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