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1341 Edmée

From Wikipedia, the free encyclopedia
Main-belt asteroid

1341 Edmée
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date27 January 1935
Designations
(1341) Edmée
Named after
Édmée Chandon
(French astronomer)[2]
1935 BA · 1929 WB1
1932 NK · 1957 YK
1963 KJ · A917 DA
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc100.28 yr (36,626 days)
Aphelion2.9612AU
Perihelion2.5227 AU
2.7420 AU
Eccentricity0.0799
4.54yr (1,658 days)
298.49°
0° 13m 1.56s / day
Inclination13.084°
107.54°
141.11°
Physical characteristics
Dimensions23.859±0.556 km[4]
26.79±8.56 km[5]
27.14±0.73 km[6]
27.49±1.1 km(IRAS:17)[7]
5.9476±0.0011 h[8]
11.89±0.01h[9]
23.745±0.005 h[10]
23.75±0.01 h[11]
0.1371±0.011(IRAS:17)[7]
0.144±0.009[6]
0.16±0.06[5]
0.182±0.028[4]
Tholen = XB[1] · XB[3]
B–V = 0.700[1]
U–B = 0.262[1]
10.14±0.41[12] · 10.320±0.001(R)[8] · 10.58[1][3][4][5][6][7]

1341 Edmée, provisional designation1935 BA, is a rare-type metallicasteroid from the central region of theasteroid belt, approximately 27 kilometers in diameter.

It was discovered on 27 January 1935, by Belgian astronomerEugène Joseph Delporte atUccle Observatory in Belgium, and later named after French astronomerÉdmée Chandon.[2][13]

Orbit and classification

[edit]

Edmée orbits the Sun in themiddle main-belt at a distance of 2.5–3.0 AU once every 4 years and 6 months (1,658 days). Its orbit has aneccentricity of 0.08 and aninclination of 13° with respect to theecliptic.[1] In 1917 it was first identified asA917 DA atHeidelberg Observatory. The body'sobservation arc begins at Uccle, on the night following its official discovery observation in 1935.[13]

Physical characteristics

[edit]

Edmée is classified as a rare XB-type in theTholen taxonomy, an intermediary between theX andB type asteroids.[1][3]

Rotation period

[edit]

American astronomerRobert Stephens obtained several rotationallightcurves ofEdmée between 2004 and 2014. Best rated results include an observation taken at the Goat Mountain Research Observatory (G79) during the body's 2009-opposition, which gave arotation period of 23.745 hours with a brightness variation of 0.05magnitude (U=2+),[10] superseding an alternative period solution of 11.89 (U=2).[9]

BecauseEdmée's rotation is similar to that of Earth, photometric observations are challenging.[11][a] In 2013, a much shorter period was derived from a fragmentary lightcurve at thePalomar Transient Factory in California (U=1).[8]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Edmée measures between 23.86 and 27.49 kilometers in diameter, and its surface has analbedo between 0.137 and 0.182.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link adopt the results from IRAS, that is, an albedo of 0.1371 and a diameter of 27.49 kilometers with anabsolute magnitude of 10.58.[3]

Naming

[edit]

Thisminor planet was named in honour of French astronomer Édmée Chandon.[2] Naming citation was first mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 122).[2]

Notes

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  1. ^Lightcurve plot of (1341) Edmée from its2014-observation (Robert Stephens), published by the Center for Solar System Studies(CS3) in Landers, California.

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 1341 Edmee (1935 BA)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1341) Edmée".Dictionary of Minor Planet Names – (1341) Edmée.Springer Berlin Heidelberg. p. 109.doi:10.1007/978-3-540-29925-7_1342.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1341) Edmée". Asteroid Lightcurve Database (LCDB). Retrieved13 January 2017.
  4. ^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. Retrieved13 January 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. Retrieved13 January 2017.
  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. ^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.
  8. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved13 January 2017.
  9. ^abStephens, Robert D. (December 2004)."Photometry of 1196 Sheba, 1341 Edmee, 1656 Suomi, 2577 Litva, and 2612 Kathryn".The Minor Planet Bulletin.31 (4):95–97.Bibcode:2004MPBu...31...95S.ISSN 1052-8091. Retrieved13 January 2017.
  10. ^abStephens, Robert D. (January 2010)."Asteroids Observed from GMARS and Santana Observatories: 2009 June - September".The Minor Planet Bulletin.37 (1):28–29.Bibcode:2010MPBu...37...28S.ISSN 1052-8091. Retrieved13 January 2017.
  11. ^abStephens, Robert D. (January 2015)."Asteroids Observed from CS3: 2014 July - September".The Minor Planet Bulletin.42 (1):70–74.Bibcode:2015MPBu...42...70S.ISSN 1052-8091. Retrieved13 January 2017.
  12. ^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. Retrieved13 January 2017.
  13. ^ab"1341 Edmee (1935 BA)".Minor Planet Center. Retrieved13 January 2017.

External links

[edit]
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