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220 Stephania

From Wikipedia, the free encyclopedia
Dark background asteroid from the inner regions of the asteroid belt

220 Stephania
Lightcurve-based 3D-model ofStephania
Discovery[1]
Discovered byJ. Palisa
Discovery siteVienna Obs.
Discovery date19 May 1881
Designations
(220) Stephania
Pronunciation/stɪˈfniə/[2]
Named after
Princess Stéphanie[3]
(Belgian royalty)
A881 KA · 1925 VE
1931 FP · 1932 UA
1943 WB · 1946 MA
1950 TT4 · 1961 WB
main-belt · (inner)[4]
background[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.28 yr (31,514 days)
Aphelion2.9543AU
Perihelion1.7443 AU
2.3493 AU
Eccentricity0.2575
3.60yr (1,315 days)
239.16°
0° 16m 25.32s / day
Inclination7.5895°
257.92°
78.480°
Physical characteristics
Dimensions31.04 km(derived)[4]
31.12±1.5 km[6]
31.738±0.219 km[7]
31.96±9.77 km[8]
32.29±0.33 km[9]
33±2 km[10]
35.097±0.260 km[11]
38.46±5.77 km[12]
18.19 h[a]
18.198h[13]
18.2±0.2 h[10]
18.21 h[b]
0.03±0.01[12]
0.05±0.03[8]
0.0571±0.0068[11]
0.0607(derived)[4]
0.069±0.002[9]
0.069±0.016[7]
0.0726±0.007[6]
0.075±0.015[10]
Tholen =XC[1][4]
C[14] · P[11]
11.00[6][9][11] · 11.10[8] · 11.2[1][4] · 11.35[12]

220 Stephania is a dark backgroundasteroid from the inner regions of theasteroid belt, approximately 32 km (20 mi) in diameter. It was discovered on 19 May 1881, by Austrian astronomerJohann Palisa at theVienna Observatory.[15] TheC-type asteroid has arotation period of 18.2 hours.[4] It was named afterPrincess Stéphanie of Belgium.[3]

Classification and orbit

[edit]

Stephania is a non-family asteroid of the main belt'sbackground population, when applying theHierarchical Clustering Method to itsproper orbital elements.[5] It orbits the Sun in theinner asteroid belt at a distance of 1.7–3.0 AU once every 3 years and 7 months (1,315 days). Its orbit has aneccentricity of 0.26 and aninclination of 8° with respect to theecliptic.[1]

Discovery and naming

[edit]

Stephania was discovered byJohann Palisa on May 19, 1881, inVienna.[15] It was the first discovery he made after transferring to the observatory from Pola.[3]

The name honoursCrown Princess Stéphanie (1864–1945), wife of theheir-apparentCrown Prince Rudolf of Austria. The couple was married the year the asteroid was discovered. It was the first time that a naming commemorated a wedding and was given as a wedding gift.[3] The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 27).[3]

Physical characteristics

[edit]

Spectral type

[edit]

In theTholen classification, this asteroid's spectrum is ambiguous, close to anX-type and somewhat similar to that of a carbonaceousC-type asteroid (CX).[4] A French spectroscopic survey that observed two dozens of these X-types classified by Tholen, determined thatStephania is in fact a carbonaceousC-type asteroid (rather than an X-type).[14] TheWide-field Infrared Survey Explorer (WISE) has also characterized it as a primitiveP-type asteroid.[4][11]

Lightcurves

[edit]

Lightcurve data has also been recorded by observers at the Antelope Hill Observatory (H09), which has been designated as an official observatory by theMinor Planet Center.[b]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Stephania measures between 31.12 and 38.46 kilometers in diameter and its surface has a lowalbedo between 0.03 and 0.075.[6][7][8][9][10][11][12] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0607 and a diameter of 31.04 kilometers based on anabsolute magnitude of 11.2.[4]

Notes

[edit]
  1. ^Anonymous lightcurve –CALL-2011 (web): rotation period18.19 hours with a brightness amplitude of0.25 mag. Quality code of 2. Summary figures for (220) Stephania at theLCDB
  2. ^abLightcurve plot of (220) Stephania by Robert A. Koff (a.k.a. William Koff) Antelope Hills Observatory, Colorado (H09); Rotation period18.21 hours with a brightness amplitude of0.21 mag. Quality code of 2. Summary figures at theLCDB

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 220 Stephania" (2017-07-01 last obs.).Jet Propulsion Laboratory. Retrieved28 October 2017.
  2. ^"Stephanian".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcdeSchmadel, Lutz D. (2007). "(220) Stephania".Dictionary of Minor Planet Names – (220) Stephania.Springer Berlin Heidelberg. p. 35.doi:10.1007/978-3-540-29925-7_221.ISBN 978-3-540-00238-3.
  4. ^abcdefghi"LCDB Data for (220) Stephania". Asteroid Lightcurve Database (LCDB). Retrieved28 October 2017.
  5. ^ab"Asteroid 220 Stephania".Small Bodies Data Ferret. Retrieved24 October 2019.
  6. ^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.
  7. ^abcMasiero, 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. Retrieved28 October 2017.
  8. ^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. Retrieved28 October 2017.
  9. ^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.
  10. ^abcdDurech, J.; Delbo', M.; Carry, B.; Hanus, J.; Alí-Lagoa, V. (July 2017)."Asteroid shapes and thermal properties from combined optical and mid-infrared photometry inversion".Astronomy and Astrophysics.604: 8.arXiv:1706.01232.Bibcode:2017A&A...604A..27D.doi:10.1051/0004-6361/201730868.S2CID 54934721. Retrieved28 October 2017.
  11. ^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.
  12. ^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.
  13. ^Mohamed, R. A.; Chiorny, V. G.; Dovgopol, A. N.; Shevchenko, V. G. (November 1994)."Photometry of five asteroids: 189 Phthia, 220 Stephania, 289 Nenetta, 312 Pierretta and 626 Notburga".Astronomy and Astrophysics Supplement.108:69–72.Bibcode:1994A&AS..108...69M. Retrieved28 October 2017.
  14. ^abFornasier, S.; Clark, B. E.; Dotto, E. (July 2011). "Spectroscopic survey of X-type asteroids".Icarus.214 (1):131–146.arXiv:1105.3380.Bibcode:2011Icar..214..131F.doi:10.1016/j.icarus.2011.04.022.S2CID 118549118.
  15. ^ab"220 Stephania".Minor Planet Center. Retrieved28 October 2017.

External links

[edit]
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