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885 Ulrike

From Wikipedia, the free encyclopedia
Main-belt asteroid

885 Ulrike
Modelled shape ofUlrike from itslightcurve
Discovery[1]
Discovered byS. Belyavskyj
Discovery siteSimeiz Obs.
Discovery date23 September 1917
Designations
(885) Ulrike
Named after
Ulrike von Levetzow[2]
(friend and love ofGoethe)
1917 CX · 1933 QQ
1934 XL · A906 SE
1917 CX · 1906 SE
main-belt[1][3] · (outer)
background[4] · Themis[5]
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc112.98yr (41,267 d)
Aphelion3.6720AU
Perihelion2.5253 AU
3.0987 AU
Eccentricity0.1850
5.45 yr (1,992 d)
318.39°
0° 10m 50.52s / day
Inclination3.3056°
148.90°
203.78°
Physical characteristics
  • 30.537±0.756 km[6]
  • 33.43±5.3 km[7]
  • 44.69±1.06 km[8]
4.90±0.05 h[9][10]
  • (13.0°, −64.0°) (λ11)[4][11]
  • (207.0°, −60.0°) (λ22)[4][11]
  • 0.047±0.003[8]
  • 0.083±0.034[7]
  • 0.109±0.025[6]
C(assumed)[9]
10.7[1][3][7][8]

885 Ulrike (prov. designation:A917 SVor1917 CX) is an elongatedThemistian asteroid from the outer regions of theasteroid belt. It was discovered on 23 September 1917, by Soviet astronomerSergey Belyavsky at theSimeiz Observatory on the Crimean peninsula.[1] The presumedC-type asteroid has a shortrotation period of 4.9 hours and measures approximately 33 kilometers (21 miles) in diameter. It was likely named afterUlrike von Levetzow, last love ofGoethe.[2]

Orbit and classification

[edit]

When applying the synthetichierarchical clustering method (HCM) byZappalà,Milani andKnežević (AstDys),Ulrike is a core member of theThemis family (602), a largeasteroid family of carbonaceous asteroids named after24 Themis. However, according to another HCM-analysis byNesvorný, it is abackground asteroid.[4][5][12]: 23  It orbits the Sun in theouter main-belt at a distance of 2.5–3.7 AU once every 5 years and 5 months (1,992 days;semi-major axis of 3.1 AU). Its orbit has aneccentricity of 0.19 and aninclination of 3° with respect to theecliptic.[3] The asteroid was first observed atLowell Observatory in August 1906. The body'sobservation arc begins atHeidelberg Observatory on 27 September 1906, more than a decade prior to its official discovery observation at Simeiz.[1]

Naming

[edit]

Thisminor planet was allegedly named afterUlrike von Levetzow (1804–1899), a friend and last love of the German poetJohann Wolfgang von Goethe, who met Ulrike during summertime 1821–1823 in Marienbad, Bohemia.[2] After she declined to marry him, Goethe started writingMarienbad Elegy, one of his finest poems.Lutz Schmadel, the author of theDictionary of Minor Planet Names, considers this interpretation the most likely because the discoverer, who studied at Göttingen University, was an expert in German literature.[2]

Physical characteristics

[edit]

Ulrike'spectral type is unknown. It is an assumed carbonaceousC-type asteroid,[9] which agrees with the overall spectral type assigned to members of theThemis family.[12]: 23 

Rotation period

[edit]

In September 2010, a rotationallightcurve ofUlrike was obtained fromphotometric observations by John Menke at the Menke Observatory. Lightcurve analysis gave arotation period of4.90±0.05 hours with a high brightness variation of0.55±0.05magnitude, indicative of an elongated shape (U=3).[9][10] An alternative period determination of4.9268±0.0002 hours with an even higher amplitude of0.72±0.12 was made byLaurent Bernasconi one month later in October 2010 (U=2).[13] A modeled lightcurve using photometric data from theLowell Photometric Database gave a sidereal period of4.906164±0.000001 and twospin axes at (13.0°, −64.0°) and (207.0°, −60.0°) inecliptic coordinates (λ, β).[11]

Diameter and albedo

[edit]

According to the survey carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE),Ulrike measures (30.537±0.756), (33.43±5.3) and (44.69±1.06) kilometers in diameter and its surface has analbedo of (0.109±0.025), (0.083±0.034) and (0.047±0.003), respectively.[6][7][8] TheCollaborative Asteroid Lightcurve Link adopts the results from IRAS, that is an albedo of 0.083 and a diameter of 33.43 kilometers based on anabsolute magnitude of 10.7.[9] The WISE team also published an alternative mean-diameter of (42.20±14.76 km) with an albedo of (0.08±0.06).[4][9]

References

[edit]
  1. ^abcde"885 Ulrike (1917 CX)".Minor Planet Center. Retrieved5 July 2018.
  2. ^abcdSchmadel, Lutz D. (2007). "(885) Ulrike".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 80.doi:10.1007/978-3-540-29925-7_886.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 885 Ulrike (A917 SV)" (2019-08-18 last obs.).Jet Propulsion Laboratory. Retrieved27 February 2020.
  4. ^abcde"Asteroid 885 Ulrike".Small Bodies Data Ferret. Retrieved27 February 2020.
  5. ^ab"Asteroid 885 Ulrike – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved27 February 2020.
  6. ^abcMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0".NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0.Bibcode:2016PDSS..247.....M. Retrieved5 July 2018.
  7. ^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. Retrieved25 February 2020.
  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. ^abcdef"LCDB Data for (885) Ulrike". Asteroid Lightcurve Database (LCDB). Retrieved27 February 2020.
  10. ^abMenke, John (December 2005)."Asteroid lightcurve results from Menke Observatory"(PDF).Minor Planet Bulletin.32 (4):85–88.Bibcode:2005MPBu...32...85M.ISSN 1052-8091.
  11. ^abcĎurech, J.; Hanuš, J.; Oszkiewicz, D.; Vančo, R. (March 2016). "Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: A48.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.ISSN 0004-6361.
  12. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV:297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.
  13. ^Behrend, Raoul."Asteroids and comets rotation curves – (885) Ulrike".Geneva Observatory. Retrieved27 February 2020.

External links

[edit]
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