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1097 Vicia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1097 Vicia
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date11 August 1928
Designations
(1097) Vicia
Pronunciation/ˈvɪsiə,-ʃiə/[2]
Named after
Vicia(flowering plant)[3]
1928 PC · 1941 SO2
1958 PF · 1978 BG
A907 VF
main-belt · (middle)[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.40 yr (39,958 days)
Aphelion3.4186AU
Perihelion1.8697 AU
2.6441 AU
Eccentricity0.2929
4.30yr (1,570 days)
274.05°
0° 13m 45.12s / day
Inclination1.5332°
133.86°
176.51°
Physical characteristics
Dimensions19.63±6.08 km[5]
21.02 km(derived)[4]
23.110±0.118 km[6]
23.95±1.04 km[7]
24.93±0.54 km[8]
26.55±0.35 km[6]
26.5±0.1h[9]
0.031±0.004[6]
0.04±0.00[7]
0.044±0.007[6]
0.05±0.02[5]
0.060±0.003[8]
0.0695(derived)[4]
S/C[4]
11.70[8] · 11.90[4][5][6] · 12.0[1] · 12.14±0.26[10] · 12.20[7]

1097 Vicia, provisional designation1928 PC, is anasteroid from the central regions of theasteroid belt, approximately 23 kilometers in diameter. Discovered byKarl Reinmuth at theHeidelberg Observatory in 1928, the asteroid was later named after the flowering plantVicia, commonly known as vetches.

Discovery

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Vicia was discovered by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany on 11 August 1928.[11] On 15 and 22 August, the asteroid was independently discovered by Soviet astronomerPelageya Shajn atSimeiz Observatory on the Crimean peninsula, and by English astronomerHarry Edwin Wood at theJohannesburg Observatory in South Africa, respectively.[3] However, theMinor Planet Center only recognizes the first discoverer.[11]

The asteroid was first identified asA907 VF at Heidelberg in May 1907. The body'sobservation arc begins at Heidelberg in August 1928, six nights after its official discovery observation.[11]

Orbit and classification

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Vicia is a non-family asteroid from the main belt'sbackground population. It orbits the Sun in thecentral main belt at a distance of 1.9–3.4 AU once every 4 years and 4 months (1,570 days). Its orbit has aneccentricity of 0.29 and aninclination of 2° with respect to theecliptic.[1]

Physical characteristics

[edit]

Viciaspectral type has not been determined. Asteroids in the central main belt with asemi-major axis between 2.6 and 2.7 AU, are located in a transitional region where bothstony andcarbonaceous asteroids are frequent and generic assumptions are difficult.[4][a]

Rotation period

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In November 2010, a rotationallightcurve ofVicia was obtained from photometric observations by Gordon Gartrelle at the University of North Dakota (730) and at theBadlands Observatory in North Dakota, United States. Analysis of the fragmentary lightcurve gave arotation period of 26.5 hours with a brightness variation of 0.08magnitude, indicative for a spherical rather than irregular and elongated shape (U=1).[9] As of 2017, however, no other lightcurve has been obtained andVicia's rotation period has not yet been secured.[4]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Vicia measures between 19.63 and 26.55 kilometers in diameter and its surface has analbedo between 0.031 and 0.060.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0695 and a diameter of 21.02 kilometers based on anabsolute magnitude of 11.9.[4]

Naming

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Thisminor planet was named after the flowering plantVicia, member of theFabaceae (legume family). It is commonly known as vetches. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 103).[3]

Reinmuth's flowers

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Due to his many discoveries,Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between(1009) and(1200). This list also contained a sequence of 28 asteroids, starting with1054 Forsytia, that were all named after plants, in particularflowering plants(also see list of minor planets named after animals and plants).[12]

Notes

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  1. ^For central-belt asteroids with 2.6 < a < 2.7, the LCDB assumes an "S/C" class with an albedo of 0.10, a compromise between the stony (p=0.20) and carbonaceous (p=0.057) asteroids

References

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  1. ^abcd"JPL Small-Body Database Browser: 1097 Vicia (1928 PC)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 19 August 2020. Retrieved19 September 2017.
  2. ^"Vicia".Merriam-Webster.com Dictionary. Merriam-Webster.
  3. ^abcSchmadel, Lutz D. (2007). "(1097) Vicia".Dictionary of Minor Planet Names – (1097) Vicia.Springer Berlin Heidelberg. p. 93.doi:10.1007/978-3-540-29925-7_1098.ISBN 978-3-540-00238-3.
  4. ^abcdefgh"LCDB Data for (1097) Vicia". Asteroid Lightcurve Database (LCDB). Retrieved19 September 2017.
  5. ^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. Retrieved19 September 2017.
  6. ^abcdefMasiero, 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. Retrieved19 September 2017.
  7. ^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.
  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. ^abGartrelle, Gordon M. (April 2012)."Lightcurve Results for Eleven Asteroids".The Minor Planet Bulletin.39 (2): 40%–46.Bibcode:2012MPBu...39...40G.ISSN 1052-8091. Retrieved19 September 2017.
  10. ^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. Retrieved19 September 2017.
  11. ^abc"1097 Vicia (1928 PC)".Minor Planet Center. Retrieved19 September 2017.
  12. ^Schmadel, Lutz D. (2007). "(1054) Forsytia".Dictionary of Minor Planet Names – (1054) Forsytia. Springer Berlin Heidelberg. p. 90.doi:10.1007/978-3-540-29925-7_1055.ISBN 978-3-540-00238-3.

External links

[edit]
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