Astronomy:674 Rachele

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674 Rachele
Discovery
Discovered byWilhelm Lorenz
Discovery siteHeidelberg
Discovery date28 October 1908
Designations
(674) Rachele
PronunciationItalian: [raˈkɛːle][1]
1908 EP
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc114.81 yr (41936 d)
|{{{apsis}}}|helion}}3.4928 astronomical unit|AU (522.52 Gm)
|{{{apsis}}}|helion}}2.3488 AU (351.38 Gm)
2.9208 AU (436.95 Gm)
Eccentricity0.19584
Orbital period4.99 yr (1823.3 d)
Mean anomaly147.48°
Mean motion0° 11m 50.82s / day
Inclination13.511°
Longitude of ascending node58.146°
42.025°
Physical characteristics
Mean radius48.675±2.15 km
Rotation period30.982 h (1.2909 d)
Geometric albedo0.2007±0.019
Absolute magnitude (H)7.42


674 Rachele is a minor planet orbiting the Sun. It was discovered by Wilhelm Lorenz on 28 October 1908 in Heidelberg, and was named by orbit computer Emilio Bianchi after his wife.[3] This is classified as an S-type asteroid,[4] indicating a stony composition.

Measurements made using the adaptive optics system at the W. M. Keck Observatory give a size estimate of 89 km. It has a size ratio of 1.08 between the major and minor axes. By comparison, measurements reported in 1998 from the IRAS observatory give a similar size of 97 km and a ratio of 1.15.[5]

References

  1. "(DOP)". http://www.dizionario.rai.it/ricerca.aspx. 
  2. "674 Rachele (1908 EP)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=674;cad=1. 
  3. Schmadel, Lutz D. (2012), Dictionary of Minor Planet Names (6th ed.), Springer, p. 65, ISBN 978-3642297182, https://books.google.com/books?id=aeAg1X7afOoC&pg=PA65. 
  4. Piironen, J. et al. (March 1998), "Physical studies of asteroids. XXXII. Rotation periods and UBVRI-colours for selected asteroids", Astronomy and Astrophysics Supplement 128 (3): 525–540, doi:10.1051/aas:1998393, Bibcode1998A&AS..128..525P. 
  5. Marchis, F. et al. (November 2006), "Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey", Icarus 185 (1): 39–63, doi:10.1016/j.icarus.2006.06.001, PMID 19081813, Bibcode2006Icar..185...39M. 

External links