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1319 Disa

From Wikipedia, the free encyclopedia
Main-belt asteroid

1319 Disa
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date19 March 1934
Designations
(1319) Disa
Pronunciation/ˈdsə/[2]
Named after
Disa(orchidflowering plant)[3]
1934 FO · 1929 GE
1970 FM · A908 EA
main-belt · (outer)[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.20 yr (39,885 days)
Aphelion3.6026AU
Perihelion2.3684 AU
2.9855 AU
Eccentricity0.2067
5.16yr (1,884 days)
41.069°
0° 11m 27.96s / day
Inclination2.8007°
256.10°
316.25°
Physical characteristics
Dimensions16.88±1.12 km[5]
24.00±0.37 km[6]
25.651±0.321 km[7]
25.894±0.180 km[8]
40.33 km(calculated)[4]
7.080±0.003h[9][a]
7.082±0.001 h[10]
7.0820±0.0077 h[11]
0.057(assumed)[4]
0.0959±0.0034[8]
0.097±0.012[7]
0.116±0.004[6]
0.391±0.038[5]
P[8] · C[4]
10.391±0.002(R)[11] · 10.50[5] · 10.7[1][4] · 11.1[6][8]

1319 Disa, provisional designation1934 FO, is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 25 kilometers in diameter. It was discovered on 19 March 1934, by English-born, South African astronomerCyril Jackson atJohannesburg Observatory in South Africa.[12] It is named for the orchidDisa.[3]

Orbit

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Disa orbits the Sun in theouter main-belt at a distance of 2.4–3.6 AU once every 5 years and 2 months (1,884 days). Its orbit has aneccentricity of 0.21 and aninclination of 3° with respect to theecliptic.[1] It was first identified asA908 EA atHeidelberg Observatory in 1908. The body'sobservation arc begins in 1929, when it was identified as1929 GE at the discovering observatory, 6 years prior to its official discovery observation.[12]

Physical characteristics

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Rotation period

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A rotationallightcurve ofDisa was obtained by American astronomerBrian D. Warner at his Palmer Divide Observatory in March 2006, and by French amateur astronomerPierre Antonini in February 2011, respectively. Analysis of both lightcurves gave a well-definedrotation period of 7.08 hours with a brightness variation of 0.26 and 0.27magnitude (U=3/3).[9][10][a]

In September 2013, photometric observations in the R-band at thePalomar Transient Factory gave a concurring lightcurve of 7.082 hours and an amplitude of 0.24 magnitude (U=2).[11]

Diameter, albedo and spectral type

[edit]

According to the surveys carried out by the JapaneseAkari satellite, and the 2014-results by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Disa measures 24.00 and 25.65 kilometers in diameter, and its surface has analbedo of 0.116 and 0.097, respectively.[6]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceousC-type asteroids of 0.057 and calculates a diameter of 40.33 kilometers with anabsolute magnitude of 10.7.[4] Preliminary results by NEOWISE also characterized the body as a dark and reddishP-type asteroid.[8]

Naming

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Thisminor planet was named afterDisa, also known as "African weed-orchid", a large genus of more than a hundred tropicalorchids, common in southern Africa.[3] In 1955, this naming citation was also published byPaul Herget inThe Names of the Minor Planets (H 120).[3]

Notes

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  1. ^abLightcurve plot of 1319 Disa, Palmer Divide Observatory, Brian D. Warner (2006)

References

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  1. ^abcd"JPL Small-Body Database Browser: 1319 Disa (1934 FO)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^"disa".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcdSchmadel, Lutz D. (2007). "(1319) Disa".Dictionary of Minor Planet Names – (1319) Disa.Springer Berlin Heidelberg. p. 108.doi:10.1007/978-3-540-29925-7_1320.ISBN 978-3-540-00238-3.
  4. ^abcdef"LCDB Data for (1319) Disa". Asteroid Lightcurve Database (LCDB). Retrieved16 January 2017.
  5. ^abcMasiero, 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. Retrieved16 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. ^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. Retrieved16 January 2017.
  8. ^abcdeMainzer, 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.
  9. ^abWarner, Brian D. (December 2006)."Asteroid lightcurve analysis at the Palmer Divide Observatory - February - March 2006".The Minor Planet Bulletin.33 (4):82–84.Bibcode:2006MPBu...33...82W.ISSN 1052-8091. Retrieved16 January 2017.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1319) Disa".Geneva Observatory. Retrieved16 January 2017.
  11. ^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. Retrieved16 January 2017.
  12. ^ab"1319 Disa (1934 FO)".Minor Planet Center. Retrieved16 January 2017.

External links

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