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1611 Beyer

From Wikipedia, the free encyclopedia
Asteroid

1611 Beyer
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date17 February 1950
Designations
(1611) Beyer
Named after
Max Beyer(astronomer)[2]
1950 DJ · 1958 RE
main-belt · (outer)[3]
Hygiea[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc67.10 yr (24,510 days)
Aphelion3.6837AU
Perihelion2.6637 AU
3.1737 AU
Eccentricity0.1607
5.65yr (2,065 days)
150.69°
0° 10m 27.48s / day
Inclination4.2818°
237.54°
75.717°
Physical characteristics
15.46±4.34 km[5]
23.25±1.77 km[6]
24.30 km(calculated)[3]
24.444±0.192 km[7]
13.2608±0.0113h[8]
13.29 h[9]
0.057(assumed)[3]
0.062±0.014[7]
0.10±0.08[5]
0.101±0.017[6]
C(assumed)[3]
11.30[6] · 11.538±0.001(R)[8] · 11.70[7] · 11.8[1][3] · 11.93±0.21[10] · 12.08[5]

1611 Beyer, provisional designation1950 DJ, is a carbonaceous Hygieanasteroid from the outer region of theasteroid belt, approximately 20 kilometers in diameter. It was discovered on 17 February 1950, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany.[11] It was named after astronomer Max Beyer.[2]

Classification and orbit

[edit]

Beyer is a member of theHygiea family (601),[4] a very largefamily of carbonaceous outer-belt asteroids, named after thefourth-largest asteroid,10 Hygiea.[12] It orbits the Sun in theouter main-belt at a distance of 2.7–3.7 AU once every 5 years and 8 months (2,065 days). Its orbit has aneccentricity of 0.16 and aninclination of 4° with respect to theecliptic.[1] Itsobservation arc begins with its official discovery observation, as noprecoveries were taken, and no prior identifications were made.[11]

Physical characteristics

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Beyer is a carbonaceousC-type asteroid.[3]

Rotation period

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AstronomersPierre Antonini andSilvano Casulli obtained a rotationallight-curve ofBeyer from photometric observations taken in July 2009. It gave arotation period of 13.29 hours with a brightness variation of 0.35magnitude (U=2+).[9] In October 2010, observations in the R-band at thePalomar Transient Factory gave a similar period of 13.2608 hours and an amplitude of 0.12 magnitude (U=2).[8]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Beyer measures between 15.46 and 24.44 kilometers in diameter, and its surface has analbedo between 0.062 and 0.101.[5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 24.30 kilometers with anabsolute magnitude of 11.8.[3]

Naming

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Thisminor planet was named by the discoverer for Max Beyer (1894–1982), German astronomer at theBergedorf Observatory in Hamburg.[2] Beyer was also on the post-war editorial board of theAstronomische Gesellschaft. The officialnaming citation was published by theMinor Planet Center in December 1959 (M.P.C. 1948).[13]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1611 Beyer (1950 DJ)" (2017-03-27 last obs.).Jet Propulsion Laboratory. Retrieved5 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1611) Beyer".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 128.doi:10.1007/978-3-540-29925-7_1612.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1611) Beyer". Asteroid Lightcurve Database (LCDB). Retrieved28 December 2016.
  4. ^ab"Asteroid 1611 Beyer – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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.
  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. ^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. Retrieved28 December 2016.
  8. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved28 December 2016.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1611) Beyer".Geneva Observatory. Retrieved28 December 2016.
  10. ^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. Retrieved28 December 2016.
  11. ^ab"1611 Beyer (1950 DJ)".Minor Planet Center. Retrieved28 December 2016.
  12. ^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.
  13. ^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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