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1739 Meyermann

From Wikipedia, the free encyclopedia
Main-belt asteroid

1739 Meyermann
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date15 August 1939
Designations
(1739) Meyermann
Named after
Bruno Meyermann
(German astronomer)[2]
1939 PF · 1929 TB1
1935 GN · 1952 HN3
1953 XO1 · 1963 TG
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.57 yr (31,984 days)
Aphelion2.5407AU
Perihelion1.9812 AU
2.2610 AU
Eccentricity0.1237
3.40yr (1,242 days)
26.730°
0° 17m 23.64s / day
Inclination3.4093°
203.35°
82.116°
Physical characteristics
Dimensions6.62±0.79 km[4]
7.47 km(calculated)[3]
7.858±0.124[5]
8.688±0.063 km[6]
2.8212±0.0002h[a]
2.8219±0.0002 h[b]
0.1961±0.0376[6]
0.24(assumed)[3]
0.254±0.015[5]
0.336±0.116[4]
S[3]
12.63±0.27[7] · 12.7[4][6] · 12.8[1][3]

1739 Meyermann, provisional designation1939 PF, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 7.5 kilometers in diameter. It was discovered by German astronomerKarl Reinmuth atHeidelberg Observatory on 15 August 1939.[8] It was later named in memory of astronomerBruno Meyermann.[2]

Orbit and classification

[edit]

Meyermann is a member of theFlora family, a large group ofS-type asteroids in the inner main-belt. It orbits the Sun at a distance of 2.0–2.5 AU once every 3 years and 5 months (1,242 days). Its orbit has aneccentricity of 0.12 and aninclination of 3° with respect to theecliptic.[1]Meyermann was first identified as1929 TB1 atLowell Observatory in 1929, extending the body'sobservation arc by 10 years prior to its official discovery observation at Heidelberg.[8]

Rotation period

[edit]

Two rotationallightcurves ofMeyermann were obtained from photometric observations taken by Czech astronomerPetr Pravec at Ondřejov Observatory in 2007 and 2014. They gave arotation period of 2.8212 and 2.8219 hours with a brightness variation of 0.12 and 0.17magnitude, respectively (U=3/3).[a][b]

Diameter and albedo

[edit]

According to the refitted 2014-results from the survey carried out by theWide-field Infrared Survey Explorer with itsNEOWISE missions,Meyermann measures 7.858 kilometers in diameter, and its surface has analbedo of 0.254.[5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of its family – and calculates a diameter of 7.47 kilometers based on anabsolute magnitude of 12.8.[3]

Naming

[edit]

Thisminor planet was named in memory of Bruno Meyermann (1876–1963), a classical astronomer and academic teacher atGöttingen Observatory in Lower Saxony, Germany. His fields of interest includedpolar motion andrelativistic effects.[2] The officialnaming citation was published by theMinor Planet Center on 18 April 1977 (M.P.C. 4155).[9]

Notes

[edit]
  1. ^abPravec (2014) web: rotation period2.8212±0.0002 hours with a brightness amplitude of0.17. Quality Code of 3. Summary figures atAsteroid Lightcurve Database
  2. ^abPravec (2007) web: rotation period2.8219±0.0002 hours with a brightness amplitude of0.22. Quality Code of 3. Summary figures atAsteroid Lightcurve Database

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1739 Meyermann (1939 PF)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved7 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1739) Meyermann".Dictionary of Minor Planet Names – (1739) Meyermann.Springer Berlin Heidelberg. p. 138.doi:10.1007/978-3-540-29925-7_1740.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1739) Meyermann". Asteroid Lightcurve Database (LCDB). Retrieved20 December 2016.
  4. ^abcMasiero, 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. Retrieved20 December 2016.
  5. ^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. Retrieved20 December 2016.
  6. ^abcMainzer, 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. ^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. Retrieved20 December 2016.
  8. ^ab"1739 Meyermann (1939 PF)".Minor Planet Center. Retrieved20 December 2016.
  9. ^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

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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