133 Cyrene

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Short description: Main-belt asteroid
133 Cyrene
Орбита астероида 133.png
Orbital diagram
Discovery
Discovered byJames Craig Watson
Discovery date16 August 1873
Designations
(133) Cyrene
Pronunciation/sˈrn/[1]
Named afterCyrene (nymph)
A873 QA; 1910 NB;
1936 HO; 1948 QC;
1959 UR
Minor planet categoryMain belt
AdjectivesCyrenean /srɪˈnən/, Cyrenian /sˈrniən/[2]
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc142.65 yr (52104 d)
|{{{apsis}}}|helion}}3.48274 astronomical unit|AU (521.010 Gm)
|{{{apsis}}}|helion}}2.64706 AU (395.995 Gm)
3.06490 AU (458.503 Gm)
Eccentricity0.13633
Orbital period5.37 yr (1959.9 d)
Average Orbital speed17.03 km/s
Mean anomaly316.166°
Mean motion0° 11m 1.273s / day
Inclination7.21561°
Longitude of ascending node319.066°
289.646°
Earth MOID1.64415 AU (245.961 Gm)
Jupiter MOID1.65199 AU (247.134 Gm)
TJupiter3.206
Physical characteristics
Dimensions66.57±6.0 km
Mass3.1 × 1017 kg
Mean density2.0? g/cm3
Equatorial surface gravity
0.0186 m/s²
Equatorial escape velocity
0.0352 km/s
Rotation period12.708 h (0.5295 d)[3]
12.707 h (0.5295 d)[4]
Geometric albedo0.2563±0.053[3]
0.2563[5]
Physics~133 K
S[5]
Absolute magnitude (H)7.98,[3] 7.990[6]


Cyrene, minor planet designation 133 Cyrene, is a fairly large and very bright main-belt asteroid that was discovered by J. C. Watson on 16 August 1873 in Ann Arbor, Michigan, and named after Cyrene, a nymph, daughter of king Hypseus and beloved of Apollo in Greek mythology.[7] It is classified as an S-type asteroid based upon its spectrum. It is listed as a member of the Hecuba group of asteroids that orbit near the 2:1 mean-motion resonance with Jupiter.[8]

In the Tholen classification system, it is categorized as a stony SR-type asteroid.[9] Photometric observations of this asteroid at the Altimira Observatory in 1985 gave a light curve with a period of 12.707 ± 0.015 hours and a brightness variation of 0.22 in magnitude. This result matches previous measurements reported in 1984 and 2005.[4]

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. Cyrenean (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Cyrenean  (Subscription or UK public library membership required.)
  3. 3.0 3.1 3.2 3.3 Yeomans, Donald K., "133 Cyrene", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=133, retrieved 12 May 2016. 
  4. 4.0 4.1 Buchheim, Robert K. (June 2006), "Photometry of asteroids 133 Cyrene, 454 Mathesis, 477 Italia, and 2264 Sabrina", Astronomy and Astrophysics Supplement Series 33 (2): pp. 29–30, Bibcode2006MPBu...33...29B. 
  5. 5.0 5.1 Richmond, Michael (1 March 2001), "Asteroid Lightcurve Data File", Astronomy and Astrophysics Supplement Series, http://spiff.rit.edu/richmond/parallax/phot/LCSUMPUB.TXT, retrieved 2013-03-29. 
  6. Pravec, P. et al. (May 2012), "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations", Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16–20, 2012 in Niigata, Japan (1667), Bibcode2012LPICo1667.6089P. 
  7. Schmadel, Lutz D.; International Astronomical Union (2003), Dictionary of minor planet names, Berlin; New York: Springer-Verlag, p. 27, ISBN 978-3-540-00238-3, https://books.google.com/books?id=VoJ5nUyIzCsC&pg=PA27. 
  8. McDonald, Sophia Levy (June 1948), "General perturbations and mean elements, with representations of 35 minor planets of the Hecuba group", Astronomical Journal 53: p. 199, doi:10.1086/106097, Bibcode1948AJ.....53..199M, http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1948AJ.....53..199M&link_type=ARTICLE&db_key=AST&high=. 
  9. DeMeo, Francesca E. et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared", Icarus 202 (1): pp. 160–180, doi:10.1016/j.icarus.2009.02.005, Bibcode2009Icar..202..160D, archived from the original on 2014-03-17, https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf, retrieved 2013-04-08.  See appendix A.

External links





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