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666 Desdemona

From Wikipedia, the free encyclopedia
Main-belt asteroid
For the moon of Uranus, seeDesdemona (moon).

666 Desdemona
Discovery[1]
Discovered byA. Kopff
Discovery siteHeidelberg Obs.
Discovery date23 July 1908
Designations
(666) Desdemona
Pronunciation/dɛzdɪˈmnə/[2]
Named after
Desdemona
(character inOthello)[3]
1908 DM
main-belt · (middle)
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc107.90 yr (39,410 days)
Aphelion3.2102AU
Perihelion1.9755 AU
2.5928 AU
Eccentricity0.2381
4.18yr (1,525 days)
309.91°
0° 14m 9.96s / day
Inclination7.5856°
215.41°
174.16°
Physical characteristics
Dimensions27.04±1.0 km(IRAS:17)[4]
27.22 km(derived)[5]
27.37±0.71 km[6]
31.485±0.116 km[7]
32.74±0.37 km[8]
13.52±0.5km
9.6h[9][a]
14.607±0.004 h[10]
15.45±0.01 h[11]
0.095±0.015[8]
0.1026±0.0207[7]
0.105±0.006[6]
0.1055±0.008(IRAS:17)[4]
0.1372(derived)[5]
S[5]
10.6[1][5][7][8] · 10.90[4][6]

666 Desdemona is a stonyasteroid from the middle region of theasteroid belt, approximately 29 kilometers in diameter. It was discovered on 23 July 1908, by German astronomerAugust Kopff atHeidelberg Observatory in southern Germany, and named afterDesdemona, character in Shakespeare'sThe Tragedy of Othello, the Moor of Venice. The name may have been inspired by the asteroid's provisional designation1908 DM.[3][12]

Classification and orbit

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Desdemona is a stonyS-type asteroid that orbits the Sun in themiddle main-belt at a distance of 2.0–3.2 AU once every 4 years and 2 months (1,525 days). Its orbit has aneccentricity of 0.24 and aninclination of 8° with respect to theecliptic.[1] As noprecoveries were taken, the asteroid'sobservation arc begins with its official discovery observation at Heidelberg.[12]

Physical characteristics

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Rotation period

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In 2013, a rotationallightcurve for this asteroid was obtained from photometric observations made by astronomer Anna Marciniak atPoznań Observatory, Poland. It gave arotation period of14.607±0.004 hours with a brightness variation of 0.22 inmagnitude (U=2+),[10] superseding a period from in 2000, obtained at the CalifornianSantana Observatory (646), which gave a slightly longer period of15.45±0.01 hours and an amplitude of 0.11 (U=2).[11]

Between 2004 and 2006, three more lightcurves were constructed from photometric observations, but they were all fragmentary and based on results with less than full coverage (U=2-/1+/2-).[9][a]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer (WISE) with its subsequentNEOWISE mission, the asteroid's surface has analbedo between 0.095 and 0.106. While theCollaborative Asteroid Lightcurve Link agrees with the space-based IRAS and Akari surveys on a diameter of approximately 27 kilometers, the results from WISE and NEOWISE found a larger diameter of 31.5 to 32.7 kilometers, respectively.[4][5][6][7][8]

Naming

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Thisminor planet was named afterDesdemona, the wife ofOthello in the playThe Tragedy of Othello, the Moor of Venice written by William Shakespeare in 1604(also see2985 Shakespeare). It is presumed that the naming of "Desdemona" could have been inspired by the two letters of its provisional designation (1908 DM). One of thesatellites of Uranus (Uranus X), discovered by theVoyager 2 in 1986, is also namedDesdemona (H 68).[3]

Notes

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  1. ^abThree different observations byLaurent Bernasconi, Jean Strajnic et al., andRené Roy between 2004 and 2006 rendered a rotation period9.6 hours with a brightness variation of0.07,0.16 and0.09 in magnitude, respectively. All observations are labelled tentative and CALL assigned aQuality-Code between 1+ and -2. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) and Asteroids and comets rotation curves – (666) DesdemonaGeneva Observatory, Light-curves

References

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  1. ^abcd"JPL Small-Body Database Browser: 666 Desdemona (1908 DM)" (2016-06-16 last obs.).Jet Propulsion Laboratory. Retrieved12 December 2016.
  2. ^"Desdemona".Merriam-Webster.com Dictionary. Merriam-Webster.
  3. ^abcSchmadel, Lutz D. (2007). "(666) Desdemona".Dictionary of Minor Planet Names – (666) Desdemona.Springer Berlin Heidelberg. pp. 65–66.doi:10.1007/978-3-540-29925-7_667.ISBN 978-3-540-00238-3.
  4. ^abcdTedesco, 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. Retrieved22 October 2019.
  5. ^abcde"LCDB Data for (666) Desdemona". Asteroid Lightcurve Database (LCDB). Retrieved4 July 2016.
  6. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  7. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.S2CID 118700974.
  8. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.S2CID 46350317. Retrieved4 July 2016.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (666) Desdemona".Geneva Observatory. Retrieved4 July 2016.
  10. ^abMarciniak, A.; Pilcher, F.; Oszkiewicz, D.; Santana-Ros, T.; Urakawa, S.; Fauvaud, S.; et al. (December 2015)."Against the biases in spins and shapes of asteroids".Planetary and Space Science.118:256–266.arXiv:1711.02429.Bibcode:2015P&SS..118..256M.doi:10.1016/j.pss.2015.06.002.S2CID 118212841. Retrieved4 July 2016.
  11. ^abStephens, R. D. (June 2001)."Rotational Periods and Lightcurves of 1277 Dolores, 666 Desdemona and (7505) 1997 AM2".The Minor Planet Bulletin.28:28–29.Bibcode:2001MPBu...28...28S. Retrieved4 July 2016.
  12. ^ab"666 Desdemona (1908 DM)".Minor Planet Center. Retrieved4 July 2016.

External links

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