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4045 Lowengrub

From Wikipedia, the free encyclopedia
Aluda asteroid

4045 Lowengrub
Discovery [1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date9 September 1953
Designations
(4045) Lowengrub
Named after
Morton Lowengrub [2]
(American mathematician)
1953 RG · 1948 VE
1953 RM · 1959 TT
1961 AJ
main-belt · (outer)[3]
Alauda[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc68.89 yr (25,163 days)
Aphelion3.5607AU
Perihelion2.9011 AU
3.2309 AU
Eccentricity0.1021
5.81yr (2,121 days)
284.41°
0° 10m 10.92s / day
Inclination21.328°
224.29°
245.47°
Physical characteristics
Dimensions29.61±0.64 km[5]
31.322±0.337 km[6]
32.369±0.319 km[7]
32.78 km(derived)[3]
37.07±1.16 km[8]
9.764h[9]
0.051±0.007[8]
0.057(assumed)[3]
0.0614±0.0103[6]
0.062±0.003[5]
C(assumed)[3]
11.00[8] · 11.17[3][6][9] · 11.2[1] · 11.30[5]

4045 Lowengrub, provisional designation1953 RG, is a dark Alaudaasteroid from the outer region of theasteroid belt, approximately 32 kilometers in diameter. It was discovered on 9 September 1953, by astronomers during theIndiana Asteroid Program atGoethe Link Observatory in Brooklyn, Indiana, United States.[10] The asteroid was named after American mathematicianMorton Lowengrub, dean atIndiana University and one of the fathers of theWIYN Observatory.[2]

Orbit and classification

[edit]

Lowengrub is a member of theAlauda family (902),[4] a largefamily of carbonaceous asteroids and named after itsparent body,702 Alauda.[11]: 23 

It orbits the Sun in theoutermost main-belt at a distance of 2.9–3.6 AU once every 5 years and 10 months (2,121 days;semi-major axis of 3.23 AU). Its orbit has aneccentricity of 0.10 and aninclination of 21° with respect to theecliptic.[1]

The body'sobservation arc begins with its first identification as1948 VE atUccle Observatory in November 1948, almost five years prior to its official discovery observation at Goethe.[10]

Physical characteristics

[edit]

Lowengrub is an assumedC-type asteroid.[3]

Rotation period

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A rotationallightcurve ofLowengrub was reported in 1996 and obtained fromphotometric observations by group of French astronomers in the early 1990s. Lightcurve analysis gave a well-definedrotation period of 9.764 hours with a brightness amplitude of 0.40magnitude (U=3).[9]

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,Lowengrub measures between 29.61 and 37.07 kilometers in diameter and its surface has analbedo between 0.051 and 0.062.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and derives a diameter of 32.78 kilometers based on anabsolute magnitude of 11.17.[3]

Naming

[edit]

Thisminor planet was named after American mathematician Morton Lowengrub, dean, professor and administrator atIndiana University. The naming took place on the occasion of the completion of theWIYN Observatory with its 3.5-meter telescope atKitt Peak National Observatory in Arizona. Lowengrub was instrumental for the planning and construction of the WIYN and was a charter member of the WIYN Board of Governors[2]

Lowengrub has authored several books on mathematics including "Crack problems in the classical theory of elasticity" (1969) together with Scottish mathematicianIan Sneddon. The official naming citation was published by theMinor Planet Center on 14 May 1995 (M.P.C. 25229).[12]

References

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  1. ^abcd"JPL Small-Body Database Browser: 4045 Lowengrub (1953 RG)" (2017-10-01 last obs.).Jet Propulsion Laboratory. Retrieved7 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4045) Lowengrub".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 345.doi:10.1007/978-3-540-29925-7_4025.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (4045) Lowengrub". Asteroid Lightcurve Database (LCDB). Retrieved7 November 2017.
  4. ^ab"Asteroid 4045 Lowengrub – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 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. ^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.
  7. ^abMasiero, 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.S2CID 118745497. Retrieved7 November 2017.
  8. ^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.S2CID 46350317. Retrieved7 November 2017.
  9. ^abcAngeli, C. A.; Barucci, M. A. (March 1996)."CCD observations: rotational properties of 13 small asteroids".Planetary and Space Science.44 (3):181–186.Bibcode:1996P&SS...44..181A.doi:10.1016/0032-0633(95)00124-7. Retrieved7 November 2017.
  10. ^ab"4045 Lowengrub (1953 RG)".Minor Planet Center. Retrieved7 November 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 978-0-8165-3213-1.S2CID 119280014.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 November 2017.

External links

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