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2145 Blaauw

From Wikipedia, the free encyclopedia
Main-belt asteroid

2145 Blaauw
Discovery[1]
Discovered byR. M. West
Discovery siteLa Silla Obs.
Discovery date24 October 1976
Designations
(2145) Blaauw
Named after
Adriaan Blaauw[2]
(Dutch astronomer)
1976 UF · 1929 XS
1963 RK · 1980 TW
main-belt · (outer)[1][3]
Ursula[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc41.02 yr (14,983 days)
Aphelion3.5269AU
Perihelion2.9059 AU
3.2164 AU
Eccentricity0.0965
5.77yr (2,107 days)
314.16°
0° 10m 15.24s / day
Inclination15.013°
264.34°
279.04°
Physical characteristics
Dimensions34.06 km(derived)[3]
37.11±0.53 km[5]
38.00±10.68 km[6]
40.549±0.848 km[7]
40.55±0.85 km[7]
12.141±0.003h[8]
0.051±0.011[7]
0.06±0.04[6]
0.0665(derived)[3]
0.076±0.002[5]
C(assumed)[3]
10.60[5] · 10.80[6][7] · 10.83±0.34[9] · 10.9[1][3]

2145 Blaauw, provisional designation1976 UF, is a dark Ursulaasteroid from the outer regions of theasteroid belt, approximately 38 kilometers in diameter. It was discovered on 24 October 1976, by astronomerRichard Martin West at theLa Silla Observatory in northern Chile.[10] The asteroid was named after Dutch astronomerAdriaan Blaauw.[2]

Orbit and classification

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Blaauw is a member of theUrsula family (631),[4] a largefamily ofC- andX-type asteroids, named after its parent body,375 Ursula.[11] It orbits the Sun in theouter asteroid belt at a distance of 2.9–3.5 AU once every 5 years and 9 months (2,107 days;semi-major axis of 3.22 AU). Its orbit has aneccentricity of 0.10 and aninclination of 15° with respect to theecliptic.[1]

The asteroid was first identified as1929 XS atLowell Observatory in December 1929. The body'sobservation arc begins with its identification as1963 RK at theKarl Schwarzschild Observatory in September 1963, or 13 years prior to its official discovery observation at La Silla.[10]

Physical characteristics

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Blaauw is an assumed, carbonaceousC-type asteroid.[3]

Rotation period

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Photometric measurements made from theOakley Southern Sky Observatory during 2012 gave alightcurve with a period of 12.141 ± 0.003 hours and a variation in brightness of 0.18 ± 0.03 inmagnitude (U=2+).[8]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Blaauw measures between 37.11 and 40.55 kilometers in diameter and its surface has analbedo between 0.051 and 0.076.[5][6][7]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0665 and a diameter of 34.06 kilometers based on anabsolute magnitude of 10.9.[3]

Naming

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Thisminor planet was named after Dutch astronomerAdriaan Blaauw (1914–2010), who was director of theEuropean Southern Observatory (1970–74), president of theInternational Astronomical Union (1976–79) and professor at theLeiden Observatory (1975–1981). His study included the structure of theMilky Way andstellar kinematics and associations.[2] The officialnaming citation was published by theMinor Planet Center on 1 July 1979 (M.P.C. 4788).[12]

References

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  1. ^abcde"JPL Small-Body Database Browser: 2145 Blaauw (1976 UF)" (2017-11-01 last obs.).Jet Propulsion Laboratory. Retrieved6 December 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2145) Blaauw".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 174.doi:10.1007/978-3-540-29925-7_2146.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2145) Blaauw". Asteroid Lightcurve Database (LCDB). Retrieved6 December 2017.
  4. ^ab"Asteroid 2145 Blaauw – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  6. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved6 December 2017.
  7. ^abcdeMasiero, 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. Retrieved6 December 2017.
  8. ^abMoravec, Patricia; Cochren, Joseph; Gerhardt, Michael; Harris, Andrew; Karnemaat, Ryan; Melton, Elizabeth; et al. (October 2012)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2012 January-April".The Minor Planet Bulletin.39 (4):213–216.Bibcode:2012MPBu...39..213M.ISSN 1052-8091. Retrieved6 December 2017.
  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. Retrieved6 December 2017.
  10. ^ab"2145 Blaauw (1976 UF)".Minor Planet Center. Retrieved6 December 2017.
  11. ^Nesvorný, 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 9780816532131.
  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.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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