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674 Rachele

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674 Rachele
Discovery
Discovered byWilhelm Lorenz
Discovery siteHeidelberg
Discovery date28 October 1908
Designations
MPC designation(674) Rachele
PronunciationItalian: [raˈkɛːle]
Alternative designations1908 EP
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc114.81 yr (41936 d)
Aphelion3.4928 AU (522.52 Gm)
Perihelion2.3488 AU (351.38 Gm)
Semi-major axis2.9208 AU (436.95 Gm)
Eccentricity0.19584
Orbital period (sidereal)4.99 yr (1823.3 d)
Mean anomaly147.48°
Mean motion0° 11 50.82 / day
Inclination13.511°
Longitude of ascending node58.146°
Argument of perihelion42.025°
Physical characteristics
Mean diameter96.171±2.708 km
Mass(1.452 ± 0.709/0.29)×10 kg
Mean density3.117 ± 1.522/0.623 g/cm
Synodic 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. This is classified as an S-type asteroid, 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.

References

  1. "(DOP)". Archived from the original on 21 June 2013. Retrieved 18 March 2020.
  2. ^ "674 Rachele (1908 EP)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 7 May 2016.
  3. ^ Fienga, A.; Avdellidou, C.; Hanuš, J. (February 2020). "Asteroid masses obtained with INPOP planetary ephemerides". Monthly Notices of the Royal Astronomical Society. 492 (1): 589–602. doi:10.1093/mnras/stz3407.
  4. Schmadel, Lutz D. (2012), Dictionary of Minor Planet Names (6th ed.), Springer, p. 65, ISBN 978-3642297182.
  5. 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, Bibcode:1998A&AS..128..525P, doi:10.1051/aas:1998393.
  6. Marchis, F.; et al. (November 2006), "Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey", Icarus, 185 (1): 39–63, Bibcode:2006Icar..185...39M, doi:10.1016/j.icarus.2006.06.001, PMC 2600456, PMID 19081813.

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