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1748 Mauderli

From Wikipedia, the free encyclopedia
Hildian asteroid

1748 Mauderli
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date7 September 1966
Designations
(1748) Mauderli
Named after
Sigmund Mauderli
(Swiss astronomer)[2]
1966 RA · 1927 SF
1934 ND1 · 1938 DL2
1943 TP · 1951 UH
1951 XD · A922 BC
main-belt · Hilda[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc95.36 yr (34,830 days)
Aphelion4.8163AU
Perihelion3.0642 AU
3.9403 AU
Eccentricity0.2223
7.82yr (2,857 days)
223.85°
0° 7m 33.6s / day
Inclination3.2937°
125.95°
199.95°
Jupiter MOID0.5342 AU
Physical characteristics
Dimensions40.32 km(derived)[4]
44.908±0.345 km[5]
51.91±1.28 km[6]
6.00 h[7]
6.001±0.001 h[a]
0.037±0.002[6]
0.048±0.013[5]
0.05±0.01[5]
0.057(assumed)[4]
Tholen =D[1] · D[4][5][8]
B–V = 0.710[1]
U–B = 0.264[1]
10.58±0.26[8] · 10.65[1][6] · 10.70[4][7]

1748 Mauderli, provisional designation1966 RA, is a dark and very reddish Hildianasteroid from the outermost region of theasteroid belt, approximately 45 kilometers in diameter.

It was discovered on 7 September 1966, by astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland, and was later named after Swiss astronomerSigmund Mauderli.[2][3]

Orbit and classification

[edit]

Mauderli is a member of theHilda family of asteroids which stay in a 3:2resonance with the gas giantJupiter. Among the Hilda family, it is one of its members with the highest amplitude oflibration relative to the stable periodic orbit.[9]

The asteroid orbits the Sun in theoutermost main-belt at a distance of 3.1–4.8 AU once every 7 years and 10 months (2,857 days). Its orbit has aneccentricity of 0.22 and aninclination of 3° with respect to theecliptic.[1]Mauderli was first identified asA922 BC atHeidelberg Observatory in 1922, extending the body'sobservation arc by 44 years prior to its official discovery observation.[3]

Physical characteristics

[edit]

Mauderli a darkD-type asteroid in theTholen classification.[1] It is also the reddest among the known asteroids of thisspectral type.[10]

Three rotationallightcurves gave a concurringrotation period of 6.00 hours with a brightness variation between 0.10 and 0.12magnitude (U=n.a/3/2-).[7][11][a]

Diameter and albedo

[edit]

Based on the space-based surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE missions,Mauderli measures 44.908 and 51.91 kilometers in diameter and has analbedo of 0.037 and 0.048, respectively.[5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 40.32 kilometers with on anabsolute magnitude of 10.7.[4]

Naming

[edit]

Thisminor planet was named by the discoverer in honor of Sigmund Mauderli (1876–1962), Swiss astronomer and director of the Astronomical Institute at theUniversity of Bern from 1921–1946. He devoted much of his time to orbit determination and perturbation computing of minor planets for theAstronomisches Rechen-Institut in Germany.[2] The officialnaming citation was published by theMinor Planet Center on 1 October 1969 (M.P.C. 2971).[12]

Notes

[edit]
  1. ^abSlyusarev (2012) web: rotation period6.001±0.001 hours with a brightness amplitude of0.1 magnitude. Summary figures for (1748) Mauderli atCollaborative Asteroid Lightcurve Link (CALL).

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 1748 Mauderli (1966 RA)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1748) Mauderli".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 139.doi:10.1007/978-3-540-29925-7_1749.ISBN 978-3-540-00238-3.
  3. ^abc"1748 Mauderli (1966 RA)".Minor Planet Center. Retrieved20 December 2016.
  4. ^abcdef"LCDB Data for (1748) Mauderli". Asteroid Lightcurve Database (LCDB). Retrieved20 December 2016.
  5. ^abcdeGrav, T.; Mainzer, A. K.; Bauer, J.; Masiero, J.; Spahr, T.; McMillan, R. S.; et al. (January 2012)."WISE/NEOWISE Observations of the Hilda Population: Preliminary Results".The Astrophysical Journal.744 (2): 15.arXiv:1110.0283.Bibcode:2012ApJ...744..197G.doi:10.1088/0004-637X/744/2/197.S2CID 44000310. Retrieved11 December 2016.
  6. ^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)
  7. ^abcDahlgren, M.; Lahulla, J. F.; Lagerkvist, C.-I.; Lagerros, J.; Mottola, S.; Erikson, A.; et al. (June 1998)."A Study of Hilda Asteroids. V. Lightcurves of 47 Hilda Asteroids".Icarus.133 (2):247–285.Bibcode:1998Icar..133..247D.doi:10.1006/icar.1998.5919. Retrieved20 December 2016.
  8. ^abVeres, 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. Retrieved20 December 2016.
  9. ^Ferraz-Mello, S. (November 1990)."Regular Motions of Resonant Asteroids".Revista Mexicana de Astronomía y Astrofísica.21: 572.Bibcode:1990RMxAA..21..569F. Retrieved18 November 2015.
  10. ^Weintraub, David A.; Tegler, Stephen C.; Romanishin, W. (August 1997)."Visible and Near-Infrared Photometry of the Centaur Objects 1995 GO and 5145 Pholus".Icarus.128 (2):456–463.Bibcode:1997Icar..128..456W.doi:10.1006/icar.1997.5739. Retrieved18 November 2015.
  11. ^Gonano, M.; Mottola, S.; Neukum, G.; di Martino, M. (December 1990)."Physical study of outer belt asteroids".Space Dust and Debris; Proceedings of the Topical Meeting of the Interdisciplinary Scientific Commission B /Meetings B2.11 (12):197–200.Bibcode:1991AdSpR..11l.197G.doi:10.1016/0273-1177(91)90563-Y.ISSN 0273-1177. Retrieved20 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.

External links

[edit]
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