65 Cybele

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65 Cybele
000065-asteroid shape model (65) Cybele.png
Discovery  [1] [2]
Discovered by E. W. Tempel
Discovery site Marseille Obs.
Discovery date8 March 1861
Designations
(65) Cybele
Pronunciation /ˈsɪbəliː/ [3]
Named after
 Cybele   [4]
(Hellenistic deity)
1949 YQ
main belt  ·(outer) [1]
Cybele [5]
Adjectives Cybelean /ˌsɪbəˈliːən/ , rarely Cybelian /sɪˈbɛliən/
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 155.98 yr (56,971 d)
Aphelion 3.8102 AU
Perihelion 3.0464 AU
3.4283 AU
Eccentricity 0.1114
6.35 yr (2,319 days)
168.06°
0° 9m 19.08s / day
Inclination 3.5627°
155.63°
102.37°
Physical characteristics
Dimensions297 km × 291 km × 213 km [6]
Mean diameter
263±3 km [6]
Mass est. (14.8±1.8)×1018 kg [6]
Mean density
1.55±0.19 g/cm3 [6]
3.98704 h [7]
4.036 h [8]
4.04 h [9]
4.04052 h [10] [11]
6.07 h [12]
6.07 h [13]
6.08±0.05 h [14]
6.081±0.001 h [lower-alpha 1]
6.0814±0.0001 h [15]
6.081434±0.000005 h [16]
6.082±0.001 h [17]
0.044 [18]
0.050±0.005 [19]
0.06±0.03 [20]
0.06±0.04 [21]
0.0706±0.003 [22] [23]
Tholen = P   [1]
SMASS = Xc   [1]  · X   [23]
B–V = 0.690 [1]
U–B = 0.271 [1]
V–R = 0.400±0.007 [24]
10.67 to 13.64
6.58±0.06 [24]  ·6.62 [1] [22] [23] [21] [18]  ·6.88±0.26 [25]  ·6.95 [20]

    Cybele, minor planet designation 65 Cybele, is one of the largest asteroids in the Solar System. It is located in the outer asteroid belt. It is thought to be a remnant primordial body. [6] It gives its name to the Cybele group of asteroids [5] that orbit outward from the Sun from the 2:1 orbital resonance with Jupiter. The X-type asteroid has a relatively short rotation period of 6.0814 hours. It was discovered by Wilhelm Tempel in 1861, and named after Cybele, the earth goddess.

    Contents

    Discovery and naming

    Cybele was discovered on 8 March 1861, by German astronomer Wilhelm Tempel from the Marseilles Observatory in southeastern France. [2] A minor controversy arose from its naming process. Tempel had awarded the honour of naming the asteroid to Carl August von Steinheil in recognition of his achievements in telescope production. Von Steinheil elected to name it "Maximiliana" after the reigning monarch Maximilian II of Bavaria. At the time, asteroids were conventionally given classical names, and a number of astronomers protested this contemporary appellation. The name Cybele was chosen instead, referring to the Phrygian goddess of the earth. [4] (The previously discovered 45 Eugenia, 54 Alexandra, and 64 Angelina had nevertheless also been given non-classical names; 64 Angelina had also been discovered by Tempel, but its name stood despite similar protests.)

    Physical characteristics

    The first Cybelian stellar occultation was observed on 17 October 1979, in the Soviet Union. The asteroid appeared to have an irregular shape, with the longest chord being measured as 245 km, closely matching results determined by the IRAS satellite in 1983 (see below). During the same 1979 occultation, a hint of a possible 11 km wide minor-planet moon at 917 km distance was detected, [26] but has since never been corroborated. As of 2017, neither the Asteroid Lightcurve Data Base nor Johnston's archive consider Cybele to be a binary asteroid. [23] [27]

    Diameter estimates

    Mean-diameter estimates for Cybele range between 218.56 and 300.54 kilometers. According to observations by the Infrared Astronomical Satellite IRAS in 1983, the asteroid has a diameter of 237.26 km. [22] The NEOWISE mission of NASA's Wide-field Infrared Survey Explorer gave a diameter of 218.56 and 276.58 km. [20] [21] The largest estimates of 300.54 km is from the Japanese Akari satellite. [18] In 2004, Müller estimated Cybele using thermophysical modelling (TPM) to have dimensions of 302 × 290 × 232 km, which corresponds to a mean-diameter of 273.0 km. [19]

    Spectrum

    Examination of the asteroid's infrared spectrum shows an absorption feature that is similar to the one present in the spectrum of 24 Themis. This can be explained by the presence of water ice. The asteroid may be covered in a layer of fine silicate dust mixed with small amounts of water-ice and organic solids. [28]

    Recent occultations

    On August 24, 2008, Cybele occulted 2UCAC 24389317, a 12.7-magnitude star in the constellation Ophiuchus which showed a long axis of at least 294 km. [29] On 11 October 2009, Cybele occulted a 13.4-magnitude star in the constellation Aquarius. [30]

    Notes

    1. ↑ Pilcher (2014m). Rotation period for (65) Cybele: 6.081±0.001 hours with a brightness amplitude of 0.03±0.01 mag. Quality Code of 3-. Summary figures at the LCDB; not available as 2014MPBu...41..250F at ADS

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    References

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    2. 1 2 "(65) Cybele". Minor Planet Center. Retrieved 21 April 2017.
    3. ↑ Noah Webster (1884) A Practical Dictionary of the English Language
    4. 1 2 Schmadel, Lutz D. (2007). "(65) Cybele". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 21. doi:10.1007/978-3-540-29925-7_66. ISBN   978-3-540-00238-3.
    5. 1 2 Linda T. Elkins-Tanton - Asteroids, Meteorites, and Comets (2010) - Page 96 (Google Books)
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    7. ↑ Drummond, J. D.; Weidenschilling, S. J.; Chapman, C. R.; Davis, D. R. (October 1988). "Photometric geodesy of main-belt asteroids. II - Analysis of lightcurves for poles, periods, and shapes". Icarus. 76 (1): 19–77. Bibcode:1988Icar...76...19D. doi:10.1016/0019-1035(88)90139-X. ISSN   0019-1035 . Retrieved 22 December 2017.
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    10. ↑ De Angelis, G. (May 1995). "Asteroid spin, pole and shape determinations". Planetary and Space Science. 43 (5): 649–682. Bibcode:1995P&SS...43..649D. doi:10.1016/0032-0633(94)00151-G . Retrieved 22 December 2017.
    11. ↑ Drummond, J. D.; Weidenschilling, S. J.; Chapman, C. R.; Davis, D. R. (January 1991). "Photometric geodesy of main-belt asteroids. IV - an updated analysis of lightcurves for poles, periods, and shapes". Icarus. 89 (1): 44–64. Bibcode:1991Icar...89...44D. doi:10.1016/0019-1035(91)90086-9. ISSN   0019-1035 . Retrieved 22 December 2017.
    12. ↑ Weidenschilling, S. J.; Chapman, C. R.; Davis, D. R.; Greenberg, R.; Levy, D. H.; Vail, S. (May 1987). "Photometric geodesy of main-belt asteroids. I - Lightcurves of 26 large, rapid rotators". Icarus. 70 (2): 191–245. Bibcode:1987Icar...70..191W. doi:10.1016/0019-1035(87)90131-X. ISSN   0019-1035 . Retrieved 22 December 2017.
    13. ↑ Schober, H. J.; Scaltriti, F.; Zappala, V.; Harris, A. W. (November 1980). "The remaining large minor planets with unknown rotational properties - 31 Euphrosyne and 65 Cybele". Astronomy and Astrophysics. 91 (1–2): 1–6.ResearchsupportedbytheOesterreichischerFondszurFoerderungderWissenschaftlichenForschung. Bibcode:1980A&A....91....1S . Retrieved 22 December 2017.
    14. ↑ Behrend, Raoul. "Asteroids and comets rotation curves – (65) Cybele". Geneva Observatory. Retrieved 22 December 2017.
    15. ↑ Pilcher, Frederick (April 2012). "Rotation Period Determinations for 31 Euphrosyne, 65 Cybele, 154 Bertha 177 Irma, 200 Dynamene, 724 Hapag, 880 Herba, and 1470 Carla". The Minor Planet Bulletin. 39 (2): 57–60. Bibcode:2012MPBu...39...57P. ISSN   1052-8091 . Retrieved 22 December 2017.
    16. ↑ Franco, Lorenzo; Pilcher, Frederick (July 2015). "Lightcurve Inversion for 65 Cybele". The Minor Planet Bulletin. 42 (3): 204–206. Bibcode:2015MPBu...42..204F. ISSN   1052-8091 . Retrieved 22 December 2017.
    17. ↑ Pilcher, Frederick (January 2010). "Rotation Period Determination for 65 Cybele". The Minor Planet Bulletin. 37 (1): 8. Bibcode:2010MPBu...37....8P. ISSN   1052-8091 . Retrieved 22 December 2017.
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    19. 1 2 Müller, T. G.; Blommaert, J. A. D. L. (April 2004). "65 Cybele in the thermal infrared: Multiple observations and thermophysical analysis". Astronomy and Astrophysics. 418: 347–356. arXiv: astro-ph/0401458 . Bibcode:2004A&A...418..347M. doi:10.1051/0004-6361:20040025. S2CID   18524619 . Retrieved 21 April 2017.
    20. 1 2 3 Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv: 1606.08923 . Bibcode:2016AJ....152...63N. doi: 10.3847/0004-6256/152/3/63 .
    21. 1 2 3 Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv: 1509.02522 . Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID   9341381 . Retrieved 19 October 2017.
    22. 1 2 3 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T . Retrieved 22 October 2019.
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    25. ↑ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv: 1506.00762 . Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. S2CID   53493339 . Retrieved 19 October 2017.
    26. ↑ "IAUC 3439: 1979l; Occn OF AGK3 +19 599 BY (65)". IAU – Central Bureau for Astronomical Telegrams. 4 January 1980. Retrieved 21 April 2017.
    27. ↑ Johnston, Robert (25 March 2017). "Asteroids with Satellites". johnstonsarchive.net. Retrieved 21 April 2017.
    28. ↑ Licandro, J.; Campins, H.; Kelley, M.; Hargrove, K.; Pinilla-Alonso, N.; Cruikshank, D.; et al. (January 2011). "(65) Cybele: detection of small silicate grains, water-ice, and organics". Astronomy and Astrophysics. 525: 7. Bibcode:2011A&A...525A..34L. doi: 10.1051/0004-6361/201015339 .
    29. ↑ IOTA. "(65) Cybele 2008 Aug 24 profile". Archived from the original on 3 March 2012. Retrieved 2 December 2010.
    30. ↑ Steve Preston. "(65) Cybele / 2UCAC 28838190 event on 2009 Oct 11, 01:30 UT" . Retrieved 21 September 2009.[ permanent dead link ]
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