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2033 Basilea

From Wikipedia, the free encyclopedia
Main-belt asteroid

2033 Basilea
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date6 February 1973
Designations
(2033) Basilea
Named after
Basel(Swiss city)[2]
1973 CA · 1953 DA
1953 EY · 1955 WD
1955 XD
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.33 yr (23,133 days)
Aphelion2.4734AU
Perihelion1.9765 AU
2.2250 AU
Eccentricity0.1117
3.32yr (1,212 days)
191.60°
0° 17m 49.2s / day
Inclination8.4634°
321.72°
14 November 2025[4]
134.56°
Physical characteristics
Dimensions5.710±0.088 km[5]
6.25±1.51 km[6]
6.322±0.051 km[7]
7.82 km(calculated)[3]
6.5287±0.0002h[a]
0.20(assumed)[3]
0.29±0.13[6]
0.3688±0.0966[7]
0.419±0.088[5]
S[3]
14.9[8] to 18.4
12.7[7] · 12.9[1][3] · 13.01±0.09[9] · 13.19[6]

2033 Basilea, provisional designation1973 CA, is a stonyasteroid from the inner regions of theasteroid belt, approximately 6 kilometers in diameter. It was discovered on 6 February 1973, by astronomerPaul Wild at theZimmerwald Observatory near Bern, Switzerland.[10] The asteroid was named for the Swiss city ofBasel.[2] It came toperihelion in November 2025 andopposition on 23 January 2026 atapparent magnitude 15 in the constellation ofCancer.[11]

Classification and orbit

[edit]

Basilea orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,212 days). Its orbit has aneccentricity of 0.11 and aninclination of 8° with respect to theecliptic.[1]

The asteroid was first identified as1953 DA atGoethe Link Observatory in February 1953, extending the body'sobservation arc by 20 years prior to its official discovery observation at Zimmerwakd.[10]

Physical characteristics

[edit]

Lightcurves

[edit]

In December 2015, a rotationallightcurve ofBasilea was obtained from photometric observations by astronomersPetr Pravec,Peter Kušnirák andDonald Pray. Lightcurve analysis gave arotation period of 6.5287 hours with a brightness variation of 0.28magnitude (U=3-).[a]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Basilea measures between 5.710 and 6.322 kilometers in diameter and its surface has analbedo between 0.29 and 0.419.[5][6][7]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forstony asteroids of 0.20 and calculates a diameter of 7.82 kilometers based on anabsolute magnitude of 12.9.[3]

Naming

[edit]

Thisminor planet was named for the Swiss city ofBasel, as well as for theAstronomical Institute of the University of Basel on the occasion of its 50th anniversary.[2] The approved naming citation was published by theMinor Planet Center on 1 June 1980 (M.P.C. 5359).[12]

Notes

[edit]
  1. ^abPravec (2015) web:lightcurve plot of (2033) Basilea with a rotation period6.5287±0.0002 hours with a brightness amplitude of0.28 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) andOndrejov Asteroid Photometry Project, also seedata sheet.

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2033 Basilea (1973 CA)" (2016-06-21 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2033) Basilea".Dictionary of Minor Planet Names – (2033) Basilea.Springer Berlin Heidelberg. p. 165.doi:10.1007/978-3-540-29925-7_2034.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2033) Basilea". Asteroid Lightcurve Database (LCDB). Retrieved3 July 2017.
  4. ^Perihelion
  5. ^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.S2CID 119293330. Retrieved3 July 2017.
  6. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  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.S2CID 35447010.
  8. ^Perihelic opposition (2026–2050)
  9. ^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.S2CID 53493339. Retrieved3 July 2017.
  10. ^ab"2033 Basilea (1973 CA)".Minor Planet Center. Retrieved3 July 2017.
  11. ^2026 opposition
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 July 2017.



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