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1906 Naef

From Wikipedia, the free encyclopedia
Asteroid

1906 Naef
Modelled shape ofNaef from itslightcurve
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date5 September 1972
Designations
(1906) Naef
Named after
Robert A. Naef
(amateur astronomer)[2]
1972 RC · 1943 VF
1952 DG1 · 1965 WF
main-belt · Vestoid[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc51.33 yr (18,749 days)
Aphelion2.6944AU
Perihelion2.0517 AU
2.3731 AU
Eccentricity0.1354
3.66yr (1,335 days)
94.839°
0° 16m 10.56s / day
Inclination6.4757°
354.84°
14.485°
Physical characteristics
Dimensions6.64 km(calculated)[3]
7.923±0.090[4]
8.057±0.083 km[5]
11.00818±0.00001h[6]
11.009±0.0012 h[a]
11.0090±0.0002 h[7]
11.03±0.02 h[8]
0.2282±0.0466[5]
0.234±0.052[4]
0.4(assumed)[3]
SQ[9] · V[3]
12.5[1][3] · 12.7[5] · 13.36±0.31[9]

1906 Naef (prov. designation:1972 RC) is a stony vestoidasteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter. It was discovered on 5 September 1972, by Swiss astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland.[10] It was later named after Swiss banker and amateur astronomerRobert A. Naef.[2]

Orbit and classification

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Naef orbits the Sun in theinner main-belt at a distance of 2.1–2.7 AU once every 3 years and 8 months (1,335 days). Its orbit has aneccentricity of 0.14 and aninclination of 6° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Zimmerwald, as previous observation atTurku Observatory (1943 VF) andMcDonald Observatory (1952 DG1) in 1943 and 1952, respectively, remain unused.[10]

Physical characteristics

[edit]

According to observations by theWide-field Infrared Survey Explorer'sNEOWISE mission,Naef measures 7.9 and 8.1 kilometers in diameter, and its surface has analbedo of 0.23,[4][5] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.40 and calculates a diameter of 6.6 kilometer with anabsolute magnitude of 12.5.[3]

Naef is avestoid or V-type asteroid, with itsspectral type comparable to that of the group's namesake,4 Vesta. V-type asteroids are less common than the abundantS-type asteroids, but they are similar in their stony composition, except for their higher concentration ofpyroxenes, an aluminium-rich silicate mineral.PanSTARRS' photometric survey has characterized it as a SQ-type that transitions to theQ-type asteroids.[9]

Four rotationallightcurves, obtained during 2005–2009, gave a well-definedrotation period between 11.01 and 11.03 hours, and a brightness variation of 0.92–0.95magnitude (U=n.a./3/n.a./2+).[6][7][8][a]

Naming

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Thisminor planet was named after Swiss banker Robert A. Naef (1907–1975) fromZürich, an ardentamateur astronomer, who produced the yearly observers almanac,Der Sternenhimmel, since 1940.[2] The officialnaming citation was published by theMinor Planet Center on 18 April 1977 (M.P.C. 4157).[11]

Notes

[edit]
  1. ^abPravec (2005) web: rotation period11.009±0.0012 hours with a brightness amplitude of0.92 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1906) Naef

References

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  1. ^abcd"JPL Small-Body Database Browser: 1906 Naef (1972 RC)" (2017-03-21 last obs.).Jet Propulsion Laboratory. Retrieved9 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1906) Naef".Dictionary of Minor Planet Names – (1906) Naef.Springer Berlin Heidelberg. p. 153.doi:10.1007/978-3-540-29925-7_1907.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1906) Naef". Asteroid Lightcurve Database (LCDB). Retrieved11 December 2016.
  4. ^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. Retrieved11 December 2016.
  5. ^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.
  6. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved11 December 2016.
  7. ^abDurkee, Russell I.; Pravec, Petr (June 2007)."The Lightcurve of Asteroid 1906 NAEF".The Minor Planet Bulletin.34 (2): 49.Bibcode:2007MPBu...34...49D.ISSN 1052-8091. Retrieved11 December 2016.
  8. ^abPolishook, David (April 2010)."Lightcurves and Spin Periods from the Wise Observatory - 2009".The Minor Planet Bulletin.37 (2):65–69.Bibcode:2010MPBu...37...65P.ISSN 1052-8091. Retrieved11 December 2016.
  9. ^abcVeres, 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. Retrieved11 December 2016.
  10. ^ab"1906 Naef (1972 RC)".Minor Planet Center. Retrieved11 December 2016.
  11. ^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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