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1574 Meyer

From Wikipedia, the free encyclopedia

1574 Meyer
Discovery[1]
Discovered byL. Boyer
Discovery siteAlgiers Obs.
Discovery date22 March 1949
Designations
(1574) Meyer
Named after
Georges Meyer
(astronomer, director)[2]
1949 FD · 1930 KE
1935 CW
main-belt · (outer)[1]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.03 yr (31,786 days)
Aphelion3.6602AU
Perihelion3.4133 AU
3.5368 AU
Eccentricity0.0349
6.65yr (2,429 days)
137.01°
0° 8m 53.52s / day
Inclination14.479°
245.64°
262.24°
Physical characteristics
Dimensions57.785±0.435 km[3]
58.88 km(derived)[4]
60.82±1.30 km[5]
69.966±3.256 km[6]
12.64±0.05h[7]
0.0274±0.0105[6]
0.036±0.002[5]
0.042±0.011[3]
0.0559(derived)[4]
C[4]
9.87±0.16[8] · 9.9[1][4] · 10.3[5][6]

1574 Meyer, provisional designation1949 FD, is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 59 kilometers in diameter. It was discovered on 22 March 1949, by French astronomerLouis Boyer atAlgiers Observatory in Algeria, northern Africa.[9] It was named after French astronomerM. Georges Meyer.[2]

Orbit and classification

[edit]

TheC-type asteroid orbits the Sun in theouter main-belt at a distance of 3.4–3.7 AU once every 6 years and 8 months (2,429 days). It is a member of theCybele group,[10] with anorbital eccentricity of 0.04 and aninclination of 14° with respect to theecliptic.[1] First identified as1930 KE atJohannesburg Observatory,Meyer'sobservation arc was extended by 19 years prior to its official discovery observation at Algiers.[9] On 10 September 1998,Meyerocculted PPM 172432.[11]

Lightcurve

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In March 2009, a rotationallightcurve ofMeyer was obtained from photometric observations by Landry Carbo at the Oakley Southern Sky Observatory in Australia. The lightcurve analysis gave arotation period of 12.64 hours with a brightness variation of 0.12magnitude (U=2).[7]

Diameter and albedo

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According to the space-based surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Meyer measures between 57.78 and 69.97 kilometers in diameter, and its surface has analbedo between 0.027 and 0.042.[3][5][6] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0559 and calculates a diameter of 58.88 kilometers with anabsolute magnitude of 9.9.[4]

Naming

[edit]

Thisminor planet was named for French astronomer M. Georges Meyer (born 1894), director of the discovering Algiers Observatory.[2] The officialnaming citation was published by theMinor Planet Center in November 1952 (M.P.C. 837).[12]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1574 Meyer (1949 FD)" (2017-06-03 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1574) Meyer".Dictionary of Minor Planet Names – (1574) Meyer.Springer Berlin Heidelberg. p. 125.doi:10.1007/978-3-540-29925-7_1575.ISBN 978-3-540-00238-3.
  3. ^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.
  4. ^abcde"LCDB Data for (1574) Meyer". Asteroid Lightcurve Database (LCDB). Retrieved29 December 2016.
  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.
  7. ^abCarbo, Landry; Green, Dawson; Kragh, Katherine; Krotz, Jonathan; Meiers, Andrew; Patino, Bernadette; et al. (October 2009)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2008 October thru 2009 March".The Minor Planet Bulletin.36 (4):152–157.Bibcode:2009MPBu...36..152C.ISSN 1052-8091. Retrieved29 December 2016.
  8. ^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. Retrieved29 December 2016.
  9. ^ab"1574 Meyer (1949 FD)".Minor Planet Center. Retrieved29 December 2016.
  10. ^De Prá, M. N.; et al. (September 2018), "PRIMASS visits Hilda and Cybele groups",Icarus,311:35–51,arXiv:1711.02071,Bibcode:2018Icar..311...35D,doi:10.1016/j.icarus.2017.11.012.
  11. ^Miles, R. (November 1998)."1998 September 10 occultation of PPM 172432 by asteroid 1574 Meyer".Occultation Newsl.7 (3): 24.Bibcode:1998OccN....7...24M. Retrieved29 December 2016.
  12. ^Schmadel, Lutz D. "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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