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1047 Geisha

From Wikipedia, the free encyclopedia
Florian asteroid

1047 Geisha
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date17 November 1924
Designations
(1047) Geisha
Named after
The Geisha[2]
(British musical)
1924 TE · 1932 BP
1941 YG · 1947 NC
1950 JF · 1974 HU2
A916 HB
main-belt · (inner)
Flora[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc92.63 yr (33,833d)
Aphelion2.6723AU
Perihelion1.8094 AU
2.2409 AU
Eccentricity0.1925
3.35yr (1,225 days)
256.96°
0° 17m 37.68s / day
Inclination5.6667°
78.223°
300.39°
Physical characteristics
Dimensions9.96±2.15 km[5]
10.555±0.095 km[6]
10.729±0.112 km[7]
11.52 km(calculated)[3]
25.62±0.02h[8]
0.24(assumed)[3]
0.277±0.029[7]
0.2897±0.0802[6]
0.30±0.13[5]
Tholen =S[1] · S[3]
B–V = 0.913[1]
U–B = 0.541[1]
11.86[1][3][6] · 12.20[5]

1047 Geisha, provisional designation1924 TE, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 11 kilometers in diameter. It was discovered on 17 November 1924, by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[9] The asteroid was named after the British musicalThe Geisha.[2]

Orbit and classification

[edit]

Geisha is a member of theFlora family (402),[3][4] a giantasteroid family and the largest family of stony asteroids in the main-belt.[10]: 23  It orbits the Sun in theinner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,225 days;semi-major axis 2.24 AU). Its orbit has aneccentricity of 0.19 and aninclination of 6° with respect to theecliptic.[1]

The asteroid was first observed asA916 HB at Heidelberg in April 1916. The body'sobservation arc begins with its official discovery observation in November 1924.[9]

Physical characteristics

[edit]

In theTholen classification,Geisha is stonyS-type asteroid,[1] which is also the overallspectral type for members of the Flora family.[10]: 23 

Rotation period

[edit]

In February 2006, a rotationallightcurve ofGeisha was obtained from photometric observations by Italian amateur astronomerLaurent Bernasconi. Lightcurve analysis gave a somewhat longer-than-averagerotation period of 25.62 hours with a brightness amplitude of 0.33magnitude (U=3-).[8]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Geisha measures between 9.96 and 10.729 kilometers in diameter and its surface has analbedo between 0.277 and 0.30.[5][6][7]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, namesake andparent body of the Flora family – and calculates a diameter of 11.52 kilometers based on anabsolute magnitude of 11.86.[3]

Naming

[edit]

Thisminor planet was named after the British musicalThe Geisha, a story of a tea house (1896). The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 100).[2]

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 1047 Geisha (1924 TE)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved11 January 2018.
  2. ^abcSchmadel, Lutz D. (2007).Dictionary of Minor Planet Names – (1047) Geisha. Springer Berlin Heidelberg. p. 89.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1047) Geisha". Asteroid Lightcurve Database (LCDB). Retrieved11 January 2018.
  4. ^ab"Asteroid 1047 Geisha – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved24 October 2019.
  5. ^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.S2CID 119289027.
  6. ^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 118700974.
  7. ^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.S2CID 119293330.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1047) Geisha". Geneva Observatory. Retrieved11 January 2018.
  9. ^ab"1047 Geisha (1924 TE)".Minor Planet Center. Retrieved11 January 2018.
  10. ^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.S2CID 119280014.

External links

[edit]
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