Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

166 Rhodope

From Wikipedia, the free encyclopedia
Main-belt asteroid

166 Rhodope
Lightcurve-based 3-D model ofRhodope
Discovery[1]
Discovered byC. H. F. Peters
Discovery siteLitchfield Obs.
Discovery date15 August 1876
Designations
(166) Rhodope
Pronunciation/ˈrɒdəp/[2]
Named after
Queen Rhodope[3]
(Greek mythology)
A876 PB
main-belt · (middle)
background[4] · Eunomia[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc132.05 yr (48,233 days)
Aphelion3.2539AU
Perihelion2.1165 AU
2.6852 AU
Eccentricity0.2118
4.40yr (1,607 days)
324.65°
0° 13m 26.4s / day
Inclination12.028°
128.92°
264.50°
Physical characteristics
Dimensions39.04±9.79 km[6]
52.393±0.196 km[7]
53.26±0.62 km[8]
54.551±1.535 km[9]
54.56 km(taken)[5]
54.564 km[10]
62.34±21.46 km[11]
65.29±0.80 km[12]
4.714793h[13]
4.712 h[a]
4.715 h[5]
4.7152±0.0002 h[14]
7.87±0.03 h(poor)[15]
0.046±0.004[12]
0.05±0.03[11]
0.0657±0.0145[9]
0.0747[10]
0.076±0.002[8]
0.10±0.05[6]
Tholen = GC:[1]
SMASS = Xe[1]
C[16] · P[9] · X[5]
B–V = 0.725[1]
U–B = 0.425[1]
9.75[5] · 9.75±0.05[10][15] · 9.89[1][6][8][9][12] · 9.95[11] · 10.22±0.25[16]

166 Rhodope is a dark backgroundasteroid from the central region of theasteroid belt, approximately 55 kilometers in diameter. It was discovered on 15 August 1876, by German–American astronomerChristian Peters at theLitchfield Observatory in Clinton, New York, United States.[17] The asteroid was named afterQueen Rhodope from Greek mythology.[3]

Orbit and classification

[edit]

Rhodope is a non-family asteroid of the main belt'sbackground population, when applying theHierarchical Clustering Method to itsproper orbital elements.[4] Alternatively, it has been dynamically assigned to the stonyEunomia family (502),[5] which have a different spectral class and albedo than that ofRhodope though.[18]: 23  The asteroid has also been considered a member of theAdeona family.[citation needed]

Rhodope orbits the Sun in thecentral asteroid belt at a distance of 2.1–3.3 AU once every 4 years and 5 months (1,607 days). Its orbit has aneccentricity of 0.21 and aninclination of 12° with respect to theecliptic.[1] The body'sobservation arc begins with the first recorded observation by theMPC atVienna Observatory on 10 September 1885, or more than 9 years after its official discovery observation at Clinton.[17]

On 19 October 2005, it was observedocculting the prominent starRegulus fromVibo Valentia, Italy.[19]

Physical characteristics

[edit]

Spectral type

[edit]

Rhodope'sspectral type is ambiguous. In theTholen classification, the noisy spectrum is closest to aG-type and somewhat similar to a commonC-type (GC:).[1] In theSMASS classification, it is an Xe-subtype, that transitions from theX-type to the very brightE-type.[1] In addition,Rhodope has also been characterized as a primitiveP-type and carbonaceous C-type by theWide-field Infrared Survey Explorer (WISE) and byPan-STARRS photometric survey, respectively.[9][16]

Rotation period

[edit]

Two well-defined rotationallightcurves ofRhodope were obtained from photometric observations by French astronomer Matthieu Conjat and by an anonymous observer of theCollaborative Asteroid Lightcurve Link (CALL). Lightcurve analysis gave a consolidatedrotation period of 4.715 hours with a brightness variation of 0.35 to 0.36magnitude (U=3/3).[5][14][a] The result supersedes a period of 7.87 hours measured by Alan Harris in the early 1980s (U=1).[15]

Poles

[edit]

In 2013, the asteroid's lightcurve was also modeled from combined dense and sparsephotometry. It gave a concurring sidereal period of 4.714793 hours. The modelling also determined two spin axis of (345.0°, −22.0°) and (173.0°, −3.0°) inecliptic coordinates (λ, β).[13]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Rhodope measures between 39.04 and 65.29 kilometers in diameter and its surface has analbedo between 0.046 and 0.10.[6][7][8][9][10][11][12]

CALL adoptsPetr Pravec's revised WISE-data, that is, an albedo of 0.0747 and a diameter of 54.56 kilometers based on anabsolute magnitude of 9.75.[5][10]

Naming

[edit]

Thisminor planet was named fromGreek mythology afterQueen Rhodope ofThrace, wife of KingHaemus and attendant ofArtemis,also see(105). In vanity, Rhodope and Haemus compared themselves to the godsZeus andHera,see(5731) and(103), who punished the couple by changing them into theRhodope Mountains andBalkan Mountains, respectively.[3]

Notes

[edit]
  1. ^abAnonymous lightcurve –CALL-2011 (web) web: rotation period4.712 hours with a brightness amplitude of0.35 mag. Quality code of 3. Summary figures for (166) Rhodope atLCDB

References

[edit]
  1. ^abcdefghij"JPL Small-Body Database Browser: 166 Rhodope" (2017-10-01 last obs.).Jet Propulsion Laboratory. Retrieved28 October 2017.
  2. ^Noah Webster (1884)A Practical Dictionary of the English Language
  3. ^abcSchmadel, Lutz D. (2007). "(166) Rhodope".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 30.doi:10.1007/978-3-540-29925-7_167.ISBN 978-3-540-00238-3.
  4. ^ab"Asteroid 166 Rhodope".Small Bodies Data Ferret. Retrieved24 October 2019.
  5. ^abcdefgh"LCDB Data for (166) Rhodope". Asteroid Lightcurve Database (LCDB). Retrieved28 October 2017.
  6. ^abcdNugent, 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.
  7. ^abMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.S2CID 119293330.
  8. ^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)
  9. ^abcdefMainzer, 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 35447010.
  10. ^abcdePravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026.
  11. ^abcdNugent, 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.
  12. ^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.
  13. ^abHanus, J.; Durech, J.; Broz, M.; Marciniak, A.; Warner, B. D.; Pilcher, F.; et al. (March 2013). "Asteroids' physical models from combined dense and sparse photometry and scaling of the YORP effect by the observed obliquity distribution".Astronomy and Astrophysics.551: 16.arXiv:1301.6943.Bibcode:2013A&A...551A..67H.doi:10.1051/0004-6361/201220701.S2CID 118627434.
  14. ^abBehrend, Raoul."Asteroids and comets rotation curves – (166) Rhodope".Geneva Observatory. Retrieved28 October 2017.
  15. ^abcHarris, A. W.; Young, J. W.; Bowell, E.; Tholen, D. J. (November 1999). "Asteroid Lightcurve Observations from 1981 to 1983".Icarus.142 (1):173–201.Bibcode:1999Icar..142..173H.doi:10.1006/icar.1999.6181.
  16. ^abcVeres, 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.
  17. ^ab"166 Rhodope".Minor Planet Center. Retrieved28 October 2017.
  18. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.S2CID 119280014.
  19. ^Sigismondi, Costantino; Troise, Davide (September 2008). "Asteroidal Occultation of Regulus: Differential Effect of Light Bending".The Eleventh Marcel Grossmann Meeting. pp. 2594–2596".Bibcode:2008mgm..conf.2594S.doi:10.1142/9789812834300_0469.ISBN 978-981-283-426-3.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=166_Rhodope&oldid=1263481732"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp