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740 Cantabia

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740 Cantabia
Discovery
Discovered byJoel Hastings Metcalf
Discovery siteWinchester, Massachusetts
Discovery date10 February 1913
Designations
MPC designation(740) Cantabia
Pronunciation/kænˈteɪbiə/
Alternative designations1913 QS
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc103.10 yr (37,659 d)
Aphelion3.3892 AU (507.02 Gm)
Perihelion2.7145 AU (406.08 Gm)
Semi-major axis3.0519 AU (456.56 Gm)
Eccentricity0.11053
Orbital period (sidereal)5.33 yr (1,947.4 d)
Mean anomaly133.938°
Mean motion0° 11 5.532 / day
Inclination10.846°
Longitude of ascending node116.099°
Argument of perihelion47.844°
Physical characteristics
Mean radius45.45±0.85 km
Synodic rotation period64.453 h (2.6855 d)
Geometric albedo0.0552±0.002
Absolute magnitude (H)9.1

740 Cantabia is a minor planet orbiting the Sun. It was discovered on 10 February 1913 at Winchester, Massachusetts by American amateur astronomer J. H. Metcalf. Cantabia is a contraction of Cantabrigia, Latin for Cambridge, named in honor of Cambridge, Massachusetts. It is orbiting at a distance of 3.05 AU with a period of 5.33 years and an eccentricity (ovalness) of 0.11. Between 2014 and 2021, 740 Cantabia has been observed to occult three stars.

This asteroid shows an exceptionally slow rate of spin. Photometry observations from two independent teams during 2009 were combined to generate a light curve showing a rotation period of 64.453 hours (2.69 days) with a brightness variation of 0.16±0.03 in magnitude. The spectrum is classified as type CX in the Tholen taxonomy. It spans a girth estimated at ~91 km.

See also

References

  1. Per 'Cantabria' in Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ "740 Cantabia (1913 QS)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
  3. Stephens, Robert D.; et al. (January 2010), "Lightcurve Analysis of 740 Cantabia", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 37 (1): 17, Bibcode:2010MPBu...37...17S.
  4. Lazzaro, D.; et al. (November 2004), "SOS: the visible spectroscopic survey of 820 asteroids", Icarus, 172 (1): 179–220, Bibcode:2004Icar..172..179L, doi:10.1016/j.icarus.2004.06.006.

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