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1543 Bourgeois

From Wikipedia, the free encyclopedia
Main-belt asteroid

1543 Bourgeois
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Observatory
Discovery date21 September 1941
Designations
(1543) Bourgeois
Named after
Paul Bourgeois[2]
(Belgian astronomer)
1941 SJ · A911 MF
main-belt · (middle)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc75.81 yr (27,689 days)
Aphelion3.4854AU
Perihelion1.7812 AU
2.6333 AU
Eccentricity0.3236
4.27yr (1,561 days)
307.06°
0° 13m 50.52s / day
Inclination11.021°
287.95°
25.799°
Physical characteristics
Dimensions11.985±0.673 km[5]
16.73 km(calculated)[3]
2.48±0.01h[6]
0.1(assumed)[3]
0.214±0.033[5]
S/C(assumed)[3]
11.90[5] · 12.0[1][3] · 12.06±0.18[7]

1543 Bourgeois (provisional designation1941 SJ) is a stonyasteroid from the centralasteroid belt'sbackground population, approximately 12 kilometers in diameter. It was discovered on 21 September 1941, by astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle.[8] The asteroid was named after Belgian astronomerPaul Bourgeois.[2]

Orbit and classification

[edit]

Bourgeois is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in thecentral asteroid belt at a distance of 1.8–3.5 AU once every 4 years and 3 months (1,561 days). Its orbit has aneccentricity of 0.32 and aninclination of 11° with respect to theecliptic.[1]

The asteroid was first identified asA911 MF atJohannesburg Observatory in June 1911. The body'sobservation arc begins at Istanbul Observatory (080), eight days prior to its official discovery observation at Uccle.[8]

Physical characteristics

[edit]

Nospectral type has been determined. The Lightcurve Data Base considers Bourgeois equally likely to be of astony orcarbonaceous, while albedo measurements byWide-field Infrared Survey Explorer suggest that it is a stonyS-type asteroid(see below).[3]

Rotation period

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In August 2005, a rotationallightcurve of Bourgeois was obtained from photometric observations by French amateur astronomerLaurent Bernasconi. Analysis of the fragmentary lightcurve gave arotation period of 2.48 hours with a brightness amplitude of 0.03magnitude (U=1).[6] As of 2017, no secure period has been obtained.[3]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA's WISE telescope, Bourgeois measures 11.985 kilometers in diameter and its surface has analbedo of 0.214.[5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.1 – a compromise albedo between the stony (0.20) and carbonaceous (0.057) types, used as a default for asteroids with a semi-major axis between 2.6 and 2.7 AU – and calculates a diameter of 16.73 kilometers based on anabsolute magnitude of 12.0.[3]

Naming

[edit]

Thisminor planet was named in memory ofPaul Bourgeois (1898–1974), director of thediscovering observatory at Uccle, professor at theFree University of Brussels, crediteddiscoverer of asteroid1547 Nele, author of various publications inastrometry, astrophysics,meridian astronomy and stellar statistics.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3930).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1543 Bourgeois (1941 SJ)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Retrieved7 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1543) Bourgeois".Dictionary of Minor Planet Names – (1543) Bourgeois.Springer Berlin Heidelberg. p. 122.doi:10.1007/978-3-540-29925-7_1544.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1543) Bourgeois". Asteroid Lightcurve Database (LCDB). Retrieved7 October 2017.
  4. ^ab"Asteroid 1543 Bourgeois – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^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. Retrieved7 October 2017.
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1543) Bourgeois".Geneva Observatory. Retrieved7 October 2017.
  7. ^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. Retrieved7 October 2017.
  8. ^ab"1543 Bourgeois (1941 SJ)".Minor Planet Center. Retrieved7 October 2017.
  9. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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