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2038 Bistro

From Wikipedia, the free encyclopedia
Main-belt asteroid

2038 Bistro
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date24 November 1973
Designations
(2038) Bistro
Pronunciation/ˈbstr/
Named after
Bistro
(Small restaurant; French)[2]
1973 WF · 1941 KD
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc43.53 yr (15,899 days)
Aphelion2.6556AU
Perihelion2.2139 AU
2.4347 AU
Eccentricity0.0907
3.80yr (1,388 days)
5.0403°
0° 15m 33.84s / day
Inclination14.809°
73.475°
183.69°
Physical characteristics
Dimensions10.55±0.76 km[4]
10.959±0.083 km[5]
11.82±2.64 km[6]
12.192±0.028 km[7]
12.58±1.2 km[8]
12.69 km(derived)[3]
13.52±0.37 km[9]
7.88h(dated)[10]
7.89 h(dated)[a]
8 h(dated)[11]
17.051±0.006 h[12]
0.1342±0.030[8]
0.1433±0.0218[7]
0.168±0.032[9]
0.1739(derived)[3]
0.191±0.029[4]
0.25±0.10[6]
SMASS = Sa[1] · S[3]
11.90[6][9] · 12.0[1][3] · 12.3[4][7][8] · 12.39±0.46[13]

2038 Bistro (/ˈbstr/), provisional designation1973 WF, is a stonyasteroid from the inner regions of theasteroid belt, approximately 12 kilometers in diameter. The asteroid was discovered on 24 November 1973, by Swiss astronomerPaul Wild at theZimmerwald Observatory near Bern, Switzerland.[14] It was named for theBistro restaurant.[2]

Orbit and classification

[edit]

Bistro orbits the Sun in theinner main-belt at a distance of 2.2–2.7 AU once every 3 years and 10 months (1,388 days). Its orbit has aneccentricity of 0.09 and aninclination of 15° with respect to theecliptic.[1] The asteroid'sobservation arc begins with its official discovery observation at Zimmerwald.[14]

Physical characteristics

[edit]

In theSMASS classification,Bistro is a Sa-type asteroid, which transitions from the commonS-types to theA-type asteroids.[1]

Lightcurves

[edit]

In April 2013, a rotationallightcurve ofBistro was obtained from photometric observations at theBassano Bresciano Observatory in Italy. Lightcurve analysis gave arotation period of 17.051 hours with a brightness variation of 0.12magnitude (U=2-).[12]

The results supersede three previously published results from fragmentary lightcurves that gave a much shorter period between 7.88 and 8 hours (U=1/1/1).[10][11][a]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bistro measures between 10.55 and 13.52 kilometers in diameter and its surface has analbedo between 0.1342 and 0.25.[4][5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1739 and a diameter of 12.69 kilometers based on anabsolute magnitude of 12.0.[3]

Naming

[edit]

Thisminor planet was namedBistro, the small type of restaurant that originated from Paris. As with the precedingly numbered2037 Tripaxeptalis, the name may also alludes to a numbers game, this time to1019 Strackea, as(2038) = 2 × (1019) Strackea.[2] The approved naming citation was published by theMinor Planet Center on 1 June 1980 (M.P.C. 5359).[15]

Notes

[edit]
  1. ^abDeGraff-2003b: unpublished lightcurve data for (2038) Bistro. Summary figures atCollaborative Asteroid Lightcurve Link (CALL)

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 2038 Bistro (1973 WF)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 13 September 2020. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2038) Bistro".Dictionary of Minor Planet Names – (2038) Bistro.Springer Berlin Heidelberg. p. 165.doi:10.1007/978-3-540-29925-7_2039.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2038) Bistro". Asteroid Lightcurve Database (LCDB). Retrieved3 July 2017.
  4. ^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)
  5. ^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. Retrieved3 July 2017.
  6. ^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. Retrieved3 July 2017.
  7. ^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.
  8. ^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.
  9. ^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. Retrieved3 July 2017.
  10. ^abDegraff, D. R.; Robbins, A. M.; Gutermuth, R. A. (December 1998)."Rotation Curves for 13 Asteroids".American Astronomical Society.30: 1390.Bibcode:1998AAS...193.9608D. Retrieved3 July 2017.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2038) Bistro".Geneva Observatory. Retrieved3 July 2017.
  12. ^abStrabla, Luca; Quadri, Ulisse; Girelli, Roberto (October 2013)."3 Asteroids' Lightcurve Analysis from Bassano Bresciano Observatory".The Minor Planet Bulletin.40 (4):232–233.Bibcode:2013MPBu...40..232S.ISSN 1052-8091. Retrieved3 July 2017.
  13. ^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. Retrieved3 July 2017.
  14. ^ab"2038 Bistro (1973 WF)".Minor Planet Center. Retrieved3 July 2017.
  15. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 July 2017.


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