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1301 Yvonne

From Wikipedia, the free encyclopedia

1301 Yvonne
Modelled shape ofYvonne from itslightcurve
Discovery[1]
Discovered byL. Boyer
Discovery siteAlgiers Obs.
Discovery date7 March 1934
Designations
(1301) Yvonne
Named after
Yvonne Boyer[2]
(discoverer's sister)
1934 EA
main-belt · (outer)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc83.32 yr (30,433 days)
Aphelion3.5134AU
Perihelion2.0225 AU
2.7680 AU
Eccentricity0.2693
4.61yr (1,682 days)
96.456°
0° 12m 50.4s / day
Inclination34.030°
161.56°
302.27°
Physical characteristics
18.693±4.943 km[5]
20.44±5.24 km[6]
21.438±0.088 km[7]
21.54±0.25 km[8]
21.681±0.204 km[9]
21.95±0.41 km[10]
22.77±2.4 km[11]
7.2536±0.0002 h[12]
7.3196±0.0001 h[12]
7.3200±0.0001 h[13]
7.320±0.005 h[14]
(39.0°, 41.0°) (λ11)[15]
0.10±0.12[6]
0.111±0.020[10]
0.1167±0.0700[5]
0.1632±0.040[11]
0.1806±0.0479[9]
0.201±0.006[8]
SMASS =C[1][3] · C[16]
10.80[8][9][11] · 11.30[1][3][5][10] · 11.32[6] · 11.40±0.22[16]

1301 Yvonne (prov. designation:1934 EA) is a carbonaceousbackground asteroid from thebackground population of the intermediateasteroid belt, approximately 21 kilometers (13 miles) in diameter. It was discovered on 7 March 1934, by French astronomerLouis Boyer at theAlgiers Observatory in North Africa.[17] The asteroid was named for the discoverer's sister, Yvonne Boyer

Orbit and classification

[edit]

Yvonne is a non-family of the main belt'sbackground population.[4] It orbits the Sun in thecentral asteroid belt at a distance of 2.0–3.5 AU once every 4 years and 7 months (1,682 days;semi-major axis of 2.77 AU). Its orbit has aneccentricity of 0.27 and aninclination of 34° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Algiers in March 1934.[17]

Naming

[edit]

Thisminor planet was named after Yvonne Boyer, sister of discoverer. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 101).[2]

Physical characteristics

[edit]

In theSMASS classification,Yvonne is a carbonaceousC-type asteroid.[1]PanSTARRS photometric survey also characterized the asteroid as a C-type.[16]

Rotation period and pole

[edit]
Lightcurve-based 3D-model ofYvonne

Between 2003 and 2017, four rotationallightcurves ofYvonne have been obtained from photometric observations.[12][13][14] Analysis gave a consolidatedrotation period of 7.320 hours with a brightness amplitude between 0.52 and 0.90magnitude (U=3/3/3/3).[3] In 2011, a modeled lightcurve using data from the Uppsala Asteroid Photometric Catalogue (UAPC) and other sources gave a concurring period7.31968±0.00005 hours, as well as aspin axis of (39.0°, 41.0°) inecliptic coordinates (λ, β).[15]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Yvonne measures between 18.693 and 22.77 kilometers in diameter and its surface has analbedo between 0.10 and 0.201.[5][6][7][8][9][10][11]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1054 (which is untypically high for a carbonaceous body) and a diameter of 22.50 kilometers based on anabsolute magnitude of 11.3.[3]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1301 Yvonne (1934 EA)" (2017-07-02 last obs.).Jet Propulsion Laboratory. Retrieved11 December 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1301) Yvonne".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 107.doi:10.1007/978-3-540-29925-7_1302.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1301) Yvonne". Asteroid Lightcurve Database (LCDB). Retrieved11 December 2017.
  4. ^ab"Asteroid 1301 Yvonne – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^abcdMasiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017)."NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos".The Astronomical Journal.154 (4): 10.arXiv:1708.09504.Bibcode:2017AJ....154..168M.doi:10.3847/1538-3881/aa89ec.
  6. ^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.
  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. ^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 35447010.
  10. ^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. Retrieved11 December 2017.
  11. ^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.
  12. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1301) Yvonne". Geneva Observatory. Retrieved11 December 2017.
  13. ^abOey, Julian; Vilagi, J.; Gajdos, S.; Kornos, L.; Galad, A. (September 2007)."Light curve Analysis of 8 Asteroids from Leura and Other Collaborating Observatories"(PDF).Minor Planet Bulletin.34 (3):81–83.Bibcode:2007MPBu...34...81O.ISSN 1052-8091. Retrieved16 March 2020.
  14. ^abPray, Donald P. (March 2004)."Lightcurve analysis of asteroids 1225, 1301, 2134, 2741, and 3974"(PDF).Minor Planet Bulletin.31 (1):6–8.Bibcode:2004MPBu...31....6P.ISSN 1052-8091. Retrieved16 March 2020.
  15. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved11 December 2017.
  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. Retrieved11 December 2017.
  17. ^ab"1301 Yvonne (1934 EA)".Minor Planet Center. Retrieved11 December 2017.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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