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4607 Seilandfarm

From Wikipedia, the free encyclopedia
Main belt asteroid

4607 Seilandfarm
Discovery [1]
Discovered byK. Endate
K. Watanabe
Discovery siteKitami Obs.
Discovery date25 November 1987
Designations
(4607) Seilandfarm
Named after
Seilandfarm
(Japanesefarm)[2]
1987 WR · 1951 CK1
1975 EO4
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc42.23 yr (15,424 days)
Aphelion2.3083AU
Perihelion2.2194 AU
2.2638 AU
Eccentricity0.0196
3.41yr (1,244 days)
225.75°
0° 17m 21.84s / day
Inclination2.2522°
250.50°
219.80°
Knownsatellites1 [a][4]
Physical characteristics
Dimensions6.33±0.27 km[5]
7.13 km(calculated)[3]
7.389±0.115 km[6]
7.482±0.136[7]
3.9681±0.0002h[b]
3.9683±0.0001 h[b][4]
0.178±0.032[7]
0.20(assumed)[3]
0.2239±0.0142[6]
0.279±0.035[5]
SMASS =L[1] · L[3]
12.89±0.34[8] · 12.9[6] · 13.00[5] · 13.1[1] · 13.2[3]

4607 Seilandfarm, provisional designation1987 WR, is a rare-typebinary[a]asteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter.

It was discovered on 25 November 1987, by Japanese amateur astronomersKin Endate andKazuro Watanabe atKitami Observatory on the Japanese island of Hokkaidō.[9] It was named for a dairy and cattle farm with the same name, located near the Japanese city of Kitami.[2]

Classification and orbit

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Seilandfarm orbits the Sun in theinner main-belt at a distance of 2.2–2.3 AU once every 3 years and 5 months (1,244 days). Its orbit has aneccentricity of 0.02 and aninclination of 2° with respect to theecliptic.[1]

In February 1951, the asteroid was first identified as1951 CK1 at Abastuman Observatory (119) in Georgia. The body'sobservation arc begins with its official discovery observation at Kitami.[9]

Binary system

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Primary

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On theSMASS taxonomic scheme,Seilandfarm is classified as a rare and reddishL-type asteroid.[1]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with itsNEOWISE mission,Seilandfarm measures between 6.3 and 7.5 and kilometers in diameter, and its surface has a correspondingalbedo between 0.178 and 0.279,[5][6][7] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 7.1 kilometers, in agreement with the results obtained by the space-based observations.[3]

In February 2009 and September 2014, three rotationallightcurves were obtained from photometric observations by astronomersDonald P. Pray andPetr Pravec at the U.S. Carbuncle and the Czech Ondřejov Observatory, respectively. The lightcurves rendered a well-definedrotation period of3.9681 and3.9683 hours with a corresponding brightness variation of 0.15 and 0.17magnitude, indicating that the asteroid's shape is nearly spheroidal (U=3/3/3).[b][4]

Moon

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During the photometric observations in February 2009, it was discovered thatSeilandfarm is in fact abinary system. Itsminor-planet moon has an orbital period of 31.6 hours. Based on mutual eclipse/occultation events, the satellite is thought to be at least 29% the size ofSeilandfarm,[a] which translates into a diameter of approximately 2 kilometers or more.

Naming

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Thisminor planet was named forSeilandfarm, a 50-hectare dairy and cattle farm, located in a hilly terrain, near the Japanese city of Kitami and not far from the observatory where this minor planet was discovered(also see3785 Kitami). The farm was established by Akio Seino in 1942, and is now operated by four members of the Seino family.[2] The approved naming citation was published by theMinor Planet Center on 14 July 1992 (M.P.C. 20521).[10]

Notes

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  1. ^abcCBET No. 1716, 2009 March 11 – Central Bureau for Astronomical Telegrams for (4607) Seilandfarm:
    Photometric observations obtained between 17 January and 25 February 2009, show that4607 Seilandfarm is a binary system with an orbital period of31.63±0.02 hours. The primary has a period of3.9683±0.0001 hours, and it has a lightcurve brightness variation of 0.15 magnitude, indicating a nearly spheroidal shape. Mutual eclipse/occultation events suggest a lower limit on secondary-to-primary mean-diameter ratio of 0.29.Central Bureau for Astronomical Telegrams No. 1716
    Reported by: D. Pray, Carbuncle Observatory, W. Brookfield, MA, U.S.A.; P. Kusnirak and P. Pravec, Ondrejov Observatory; J. Gross, W. Cooney, and D. Terrell, Sonoita Research Observatory, Sonoita, AZ; and R. Durkee, Minneapolis, MN.
  2. ^abcPravec (2009) web: rotation period3.9683±0.0001 hours with a brightness amplitude of0.15 mag, as well as Pravec (2014) web: rotation period3.9681±0.0002 hours with a brightness amplitude of0.17 mag. Quality Code for both observations: U=3 (denotes a secure result within the precision given and no ambiguity). Summary figures for (4607) Seilandfarm atCollaborative Asteroid Lightcurve Link (CALL)

References

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  1. ^abcdef"JPL Small-Body Database Browser: 4607 Seilandfarm (1987 WR)" (2017-06-06 last obs.).Jet Propulsion Laboratory. Retrieved4 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4607) Seilandfarm".Dictionary of Minor Planet Names – (4607) Seilandfarm.Springer Berlin Heidelberg. p. 396.doi:10.1007/978-3-540-29925-7_4532.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4607) Seilandfarm". Asteroid Lightcurve Database (LCDB). Retrieved3 August 2016.
  4. ^abcPray, D.; Brookfield, W.; Kusnirak, P.; Pravec, P.; Gross, J.; Cooney, W.; et al. (March 2009)."(4607) Seilandfarm".Central Bureau Electronic Telegrams.1716 (1716): 1.Bibcode:2009CBET.1716....1P. Retrieved3 January 2016.
  5. ^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. Retrieved3 August 2016.
  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. Retrieved3 August 2016.
  7. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved5 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. Retrieved3 August 2016.
  9. ^ab"4607 Seilandfarm (1987 WR)".Minor Planet Center. Retrieved3 August 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 August 2016.

External links

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Distant minor planet
Comets
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