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1340 Yvette

From Wikipedia, the free encyclopedia
Main-belt asteroid

1340 Yvette
Discovery[1]
Discovered byL. Boyer
Discovery siteAlgiers Obs.
Discovery date27 December 1934
Designations
(1340) Yvette
Named after
Yvette(discoverer's niece)[2]
1934 YA · 1930 DO
1942 GW
main-belt · (outer)
Themis[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc82.84 yr (30,256 days)
Aphelion3.5930AU
Perihelion2.7754 AU
3.1842 AU
Eccentricity0.1284
5.68yr (2,075 days)
123.54°
0° 10m 24.6s / day
Inclination0.4161°
345.69°
224.26°
Physical characteristics
Dimensions25.87±2.6 km[5]
28.40±1.70 km[6]
28.63±0.55 km[7]
29.451±0.278 km[8]
30.3±3.0 km[9]
32±3 km[10]
33.061±0.632 km[11]
3.525h[12]
0.0587±0.0044[11]
0.06±0.01[10]
0.07±0.01[9]
0.078±0.018[7]
0.082±0.011[6]
0.095±0.015[8]
0.0958±0.023[5]
C[3][13]
11.10[1][3][5][6][7][9][10][11] · 11.12±0.29[13]

1340 Yvette, provisional designation1934 YA, is a carbonaceous Themistianasteroid from the outer regions of theasteroid belt, approximately 29 kilometers in diameter. It was discovered on 27 December 1934, by astronomerLouis Boyer at theAlgiers Observatory, who named it after his niece, Yvette.[2][14]

Orbit and classification

[edit]

Yvette is a Themistian asteroid that belongs to theThemis family (602),[3][4] a very largefamily of nearly 5,000 member asteroids, named after24 Themis.[15]: 23  It orbits the Sun in theouter main belt at a distance of 2.8–3.6 AU once every 5 years and 8 months (2,075 days;semi-major axis of 3.18 AU). Its orbit has aneccentricity of 0.13 and aninclination of 0° with respect to theecliptic.[1]

The asteroid was first identified as1930 DO atHeidelberg Observatory in February 1930. The body'sobservation arc begins with its official discovery observation at Algiers in 1934.[14]

Physical characteristics

[edit]

Yvette has been characterized as a carbonaceousC-type asteroid byPan-STARRS photometric survey,[13] in line with the overallspectral type of the Themis family.[15]: 23 

Rotation period

[edit]

Published in 2004, a first rotationallightcurve ofYvette was obtained from photometric observations by Brazilian and Argentinian astronomers. Lightcurve analysis gave a relatively shortrotation period of 3.525 hours with a brightness amplitude of 0.16magnitude (U=2).[12]

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,Yvette measures between 25.87 and 33.061 kilometers in diameter and its surface has analbedo between 0.0587 and 0.0958.[5][6][7][8][9][10][11]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is an albedo of 0.0958 and a diameter of 25.87 kilometers based on anabsolute magnitude of 11.1.[3][5]

Naming

[edit]

Thisminor planet was named by the discoverer in honor of his niece, Yvette. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 122).[2]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1340 Yvette (1934 YA)" (2017-10-28 last obs.).Jet Propulsion Laboratory. Retrieved28 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1340) Yvette".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 109.doi:10.1007/978-3-540-29925-7_1341.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1340) Yvette". Asteroid Lightcurve Database (LCDB). Retrieved28 November 2017.
  4. ^ab"Asteroid 1340 Yvette – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdeTedesco, 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.
  6. ^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)
  7. ^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. Retrieved28 November 2017.
  8. ^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.
  9. ^abcdAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614.
  10. ^abcdAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680. Retrieved28 November 2017.
  11. ^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.
  12. ^abAlvarez-Candal, Alvaro; Duffard, René; Angeli, Cláudia A.; Lazzaro, Daniela; Fernández, Silvia (December 2004)."Rotational lightcurves of asteroids belonging to families".Icarus.172 (2):388–401.Bibcode:2004Icar..172..388A.doi:10.1016/j.icarus.2004.06.008. Retrieved28 November 2017.
  13. ^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. Retrieved28 November 2017.
  14. ^ab"1340 Yvette (1934 YA)".Minor Planet Center. Retrieved28 November 2017.
  15. ^abNesvorný, 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.

External links

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