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2029 Binomi

From Wikipedia, the free encyclopedia
Asteroid

2029 Binomi
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date11 September 1969
Designations
(2029) Binomi
Named after
Alessandro Binomi
(fictitious mathematician)[2]
1969 RB · 1971 BX2
1976 QV1
main-belt · Vesta[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc47.52 yr (17,355 days)
Aphelion2.6515AU
Perihelion2.0477 AU
2.3496 AU
Eccentricity0.1285
3.60yr (1,316 days)
120.75°
0° 16m 25.32s / day
Inclination5.5869°
278.03°
67.217°
Physical characteristics
Dimensions5.39 km(calculated)[3]
6.893±0.164 km[4]
7.050±0.058 km[5]
3.7555±0.010h[6]
3.756±0.0015 h[7]
0.24(assumed)[3]
0.2468±0.0358[5]
0.257±0.048[4]
SMASS =S[1][3]
12.9[5] · 13.0[1] · 13.030±0.210(R)[6] · 13.058±0.001(R)[7] · 13.24±0.26[8] · 13.51[3]

2029 Binomi, provisional designation1969 RB, is a Vestianasteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter.

The asteroid was discovered on 11 September 1969, byPaul Wild atZimmerwald Observatory near Bern, Switzerland.[9] It was named for the fictitious mathematician "Alessandro Binomi" who invented thebinomial formula.[2]

Classification and orbit

[edit]

Binomi is a member of theVesta family, one of the largest collisional populations of the inner asteroid belt. It orbits the Sun at a distance of 2.0–2.7 AU once every 3 years and 7 months (1,316 days). Its orbit has aneccentricity of 0.13 and aninclination of 6° with respect to theecliptic.[1]

The body'sobservation arc begins atCrimea–Nauchnij on 10 September 1969, the night before its official discovery observation at Zimmerwald.[9]

Physical characteristics

[edit]

In theSMASS classification,Binomi is a stonyS-type asteroid.[1]

Lightcurves

[edit]

In January 2014, two rotationallightcurves ofBinomi were obtained from photometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 3.7555 and 3.756 hours with a brightness variation of 0.51 and 0.52magnitude, respectively (U=2/2).[6][7]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Binomi measures 6.893 and 7.050 kilometers in diameter and its surface has analbedo of 0.2468 and 0.257, respectively.[4][5]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of its family – and calculates a diameter of 5.39 kilometers based on anabsolute magnitude of 13.51.[3]

Naming

[edit]

Thisminor planet was named for the fictitious mathematician "Alessandro Binomi", inventor of thebinomial formula. This act ofparody science was common among students at German-speaking universities (de:Binomi). The real inventors of the binomial formula are the Bernoullis, after whom the asteroid2034 Bernoulli was named.[2] The approved naming citation was published by theMinor Planet Center on 1 August 1981 (M.P.C. 6208).[10]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 2029 Binomi (1969 RB)" (2017-03-17 last obs.).Jet Propulsion Laboratory. Retrieved28 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2029) Binomi".Dictionary of Minor Planet Names – (2029) Binomi.Springer Berlin Heidelberg. p. 164.doi:10.1007/978-3-540-29925-7_2030.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2029) Binomi". Asteroid Lightcurve Database (LCDB). Retrieved28 June 2017.
  4. ^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. Retrieved28 June 2017.
  5. ^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.
  6. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved28 June 2017.
  7. ^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. Retrieved28 June 2017.
  8. ^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. Retrieved28 June 2017.
  9. ^ab"2029 Binomi (1969 RB)".Minor Planet Center. Retrieved28 June 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved28 June 2017.


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