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1615 Bardwell

From Wikipedia, the free encyclopedia
Rare-type main-belt asteroid

1615 Bardwell
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date28 January 1950
Designations
(1615) Bardwell
Named after
Conrad Bardwell(astronomer)[2]
1950 BW · 1926 TO
1937 TJ · 1948 RB1
1948 RH1 · 1948 TG
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc90.49 yr (33,053 days)
Aphelion3.6887AU
Perihelion2.5664 AU
3.1275 AU
Eccentricity0.1794
5.53yr (2,020 days)
169.71°
0° 10m 41.52s / day
Inclination1.6901°
152.55°
252.97°
Physical characteristics
Dimensions21.92±5.97 km[4]
25.01±1.49 km[5]
27.78±1.6 km(IRAS:5)[6]
28.8±2.9 km[7]
29.139±0.148 km[8]
31±3 km[9]
31.579±0.250 km[10]
18h[a]
0.0497±0.0192[10]
0.05±0.01[9]
0.060±0.010[8][7]
0.0642±0.008(IRAS:5)[6]
0.079±0.015[5]
0.09±0.06[4]
Tholen =B[1] · B[3]
B–V = 0.692[1]
U–B = 0.329[1]
11.38[1][3][5][6][7][9][10] · 11.46[4]

1615 Bardwell, provisional designation1950 BW, is a rare-type Themistianasteroid from the outer region of theasteroid belt, approximately 27 kilometers in diameter. It was discovered on 28 January 1950, byIU'sIndiana Asteroid Program atGoethe Link Observatory near Brooklyn, Indiana, United States.[11] It is named for American astronomerConrad Bardwell.[2]

Orbit and classification

[edit]

Bardwell is a member of theThemis family, a dynamical family ofouter-belt asteroids with nearly coplanarecliptical orbits. It orbits the Sun at a distance of 2.6–3.7 AU once every 5 years and 6 months (2,020 days). Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to theecliptic.[1]

Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to the ecliptic.[1] It was first identified as1926 TO atSimeiz Observatory in 1926, extending the body'sobservation arc by 24 years prior to its official discovery observation.[11]

Naming

[edit]

Thisminor planet was named forConrad M. Bardwell (1926–2010), who was a research associate at theCincinnati Observatory and later associate director of theMinor Planet Center in Cambridge, Massachusetts, United States. Bardwell successfully established numerous identifications from observations in widely separated oppositions and provided observers with reliable data oforbital elements.[2] The officialnaming citation was published by theMinor Planet Center on 15 June 1974 (M.P.C. 3643).[12]

Physical characteristics

[edit]

In theTholen taxonomy,Bardwell is a blueishB-type asteroid, a rare subtype of the abundant carbonaceousC-types found in the outer belt. The spectra of B-type bodies show a broadabsorption feature at onemicron wavelength that is associated with the presence ofmagnetite and is what gives the asteroid its blue tint.[13] There are only a few dozens asteroids of this type known to exist.[14]

Rotation period

[edit]

In the late 1970s, a rotationallightcurve ofBardwell was obtained by American astronomer Edward Tedesco. It gave a provisionalrotation period of 18 hours with a change in brightness of 0.2magnitude (U=1).[a] As of 2017, no other photometric analysis ofBardwell has been made.

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bardwell measures between 21.92 and 31.58 kilometers in diameter, and its surface has analbedo between 0.049 and 0.09.[4][6][7][8][10] TheCollaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS, that is, an albedo of 0.0642 and a diameter of 27.78 kilometers based on anabsolute magnitude of 11.38.[3]

Notes

[edit]
  1. ^abTedesco, E.F. (1979) PhD Dissertation, New. Mex. State Univ. 280pp.; Rotation period of 18 hours with a brightness amplitude of0.2. Summary figures atAsteroid Lightcurve Database for (1615) Bardwell

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 1615 Bardwell (1950 BW)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved4 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1615) Bardwell".Dictionary of Minor Planet Names – (1615) Bardwell.Springer Berlin Heidelberg. p. 128.doi:10.1007/978-3-540-29925-7_1616.ISBN 978-3-540-00238-3.
  3. ^abcd"LCDB Data for (1615) Bardwell". Asteroid Lightcurve Database (LCDB). Retrieved28 December 2016.
  4. ^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.
  5. ^abcMasiero, 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.S2CID 46350317. Retrieved28 December 2016.
  6. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  7. ^abcdAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614.
  8. ^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. Retrieved28 December 2016.
  9. ^abcAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680.S2CID 119214002. Retrieved28 December 2016.
  10. ^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.
  11. ^ab"1615 Bardwell (1950 BW)".Minor Planet Center. Retrieved28 December 2016.
  12. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.
  13. ^Yang, Bin; Jewitt, David (September 2010)."Identification of Magnetite in B-type Asteroids".The Astronomical Journal.140 (3):692–698.arXiv:1006.5110.Bibcode:2010AJ....140..692Y.doi:10.1088/0004-6256/140/3/692.S2CID 724871. Retrieved28 December 2016.
  14. ^"JPL db query spectral type = B (SMASSII and/or Tholen)".JPL Small-Body Database. Jet Propulsion Laboratory. Retrieved15 November 2015.

External links

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