874 Rotraut

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874 Rotraut
Modelled shape of Rotraut from its lightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date25 May 1917
Designations
(874) Rotraut
Named after
Schön Rotraut
(poem by Eduard Mörike)[2]
A917 KK · 1976 WJ
1917 CC
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc102.67 yr (37,499 d)
Aphelion3.4039 AU
Perihelion2.8992 AU
3.1515 AU
Eccentricity0.0801
5.59 yr (2,044 d)
171.80°
0° 10m 34.32s / day
Inclination11.141°
190.63°
9.4547°
Physical characteristics
Dimensions51.1 km × 37.7 km[5]
  • 56.47±5.5 km[6]
  • 58.287±0.198 km[7]
  • 59.38±0.73 km[8]
14.297 h[9][10]
  • (201.0°, −41.0°) (λ11)[5]
  • (2.0°, −36.0°) (λ22)[5]
  • 0.051±0.002[8]
  • 0.054±0.004[7]
  • 0.0554±0.013[6]
10.1[1][3]

874 Rotraut (prov. designation: A917 KK or 1917 CC) is a dark and elongated background asteroid, approximately 58 kilometers (36 miles) in diameter, located in the outer region of the asteroid belt. It was discovered on 25 May 1917, by astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory is southwest Germany.[1] The hydrated carbonaceous C-type asteroid (Ch) has a rotation period of 14.3 hours. It was likely named after the ballad Schön Rotraut by German lyric poet Eduard Mörike (1804–1875).[2]

Rotraut is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.4 AU once every 5 years and 7 months (2,044 days; semi-major axis of 3.15 AU). Its orbit has an eccentricity of 0.08 and an inclination of 11° with respect to the ecliptic.[3] The body's observation arc begins at Heidelberg Observatory with its official discovery observation on 25 May 1917.[1]

Naming

"Rotraut" is a feminine German first name. This minor planet was likely named after the ballad Schön Rotraut (Pretty Rohtraut) by the German lyric poet Eduard Mörike (1804–1875). Lutz Schmadel, the author of the Dictionary of Minor Planet Names learned about Wolf's source of inspiration from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.[2]

Physical characteristics

References

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