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1168 Brandia

From Wikipedia, the free encyclopedia
Asteroid

1168 Brandia
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date25 August 1930
Designations
(1168) Brandia
Named after
Eugène Brand[2]
(Belgian mathematician)
1930 QA
main-belt · (middle)
Eunomia[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc82.70 yr (30,208 days)
Aphelion3.1088AU
Perihelion1.9931 AU
2.5510 AU
Eccentricity0.2187
4.07yr (1,488 days)
120.52°
0° 14m 30.84s / day
Inclination12.735°
218.65°
122.91°
Physical characteristics
Dimensions10.110±0.057 km[5][6]
10.58 km(derived)[3]
10.61±0.7 km[7]
11.444h[8]
11.444 h[9]
0.1375(derived)[3]
0.150±0.038[5]
0.1505±0.0383[6]
0.1526±0.021[7]
S[3]
B–V = 0.860[1]
U–B = 0.470[1]
12.30±0.23[10] · 12.53[1][7] · 12.65[3][6][9]

1168 Brandia, provisional designation1930 QA, is a stony Eunomianasteroid from the central regions of theasteroid belt, approximately 10 kilometers in diameter. Discovered by astronomerEugène Delporte atUccle Observatory in 1930, the asteroid was later named after mathematicianEugène Brand.[2]

Discovery

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Brandia was discovered on 25 August 1930, by astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle. Six nights later, the asteroid was independently discovered by Soviet astronomerGrigory Neujmin atSimeiz Observatory on 31 August 1930. TheMinor Planet Center, however, only recognizes the first discoverer.[2][11] The body'sobservation arc begins at Uccle, two nights after its official discovery observation.[11]

Orbit and classification

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This asteroid is a member of theEunomia family (502), a prominentfamily of stony asteroids and the largest one in the intermediate main belt with more than 5,000 members.[3][4][12]: 23 

Brandia orbits the Sun in thecentral main-belt at a distance of 2.0–3.1 AU once every 4 years and 1 month (1,488 days). Its orbit has aneccentricity of 0.22 and aninclination of 13° with respect to theecliptic.[1]

Physical characteristics

[edit]

Brandia is an assumedS-type asteroid,[3] which corresponds to the overallspectral type of the Eunomia family.[12]: 23 

Rotation period

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In September 1989, a rotationallightcurve ofBrandia was obtained from photometric observations by American astronomerRichard Binzel atCTIO andMcDonald Observatory. Lightcurve analysis gave a well-definedrotation period of hours with a relatively high brightness variation of 0.62magnitude (U=3).[9]

An identical period of 11.444 hours with an amplitude of 0.50 magnitude was measured with a Celestron 14-inch telescope byFrederick Pilcher and published in 1985 (U=2).[8]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Brandia measures 10.110 and 10.61 kilometers in diameter, and its surface has analbedo of 0.150 and 0.1526, respectively.[5][6][7]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1375 and a diameter of 10.58 kilometers based on anabsolute magnitude of 12.65.[3]

Naming

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Thisminor planet was named after Belgian mathematicianEugène Brand, professor at theUniversity of Brussels in Belgium. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 109).[2]

References

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  1. ^abcdef"JPL Small-Body Database Browser: 1168 Brandia (1930 QA)" (2017-03-24 last obs.).Jet Propulsion Laboratory. Retrieved6 September 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1168) Brandia".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 98.doi:10.1007/978-3-540-29925-7_1169.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1168) Brandia". Asteroid Lightcurve Database (LCDB). Retrieved6 September 2017.
  4. ^ab"Asteroid 1168 Brandia – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved6 September 2017.
  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.
  7. ^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.
  8. ^abPilcher, Frederick; Binzel, R. P.; Tholen, D. J. (March 1985)."Rotations of 1168 Brandia and 1219 Britta".The Minor Planet Bulletin.12: 10.Bibcode:1985MPBu...12...10P. Retrieved6 September 2017.
  9. ^abcBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved6 September 2017.
  10. ^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. Retrieved6 September 2017.
  11. ^ab"1168 Brandia (1930 QA)".Minor Planet Center. Retrieved6 September 2017.
  12. ^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 978-0-8165-3213-1.

External links

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