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5316 Filatov

From Wikipedia, the free encyclopedia
Main-belt asteroid

5316 Filatov
Discovery[1]
Discovered byL. G. Karachkina
Discovery siteCrimean Astrophysical Obs.
Discovery date21 October 1982
Designations
(5316) Filatov
Named after
Vladimir Filatov
(ophthalmologist andsurgeon)[2]
1982 UB7 · 1982 XU3
1987 SF9 · 1991 LV3
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc34.44 yr (12,578 days)
Aphelion3.2253AU
Perihelion3.0919 AU
3.1586 AU
Eccentricity0.0211
5.61yr (2,050 days)
18.907°
0° 10m 32.16s / day
Inclination14.743°
230.22°
240.87°
Physical characteristics
Dimensions22.95 km(calculated)[3]
45.693±0.511 km[4]
1061.3756±76.36h[5]
0.019±0.003[4]
0.057(assumed)[3]
C[3]
11.474±0.002(R)[5] · 11.60[4] · 11.8[1] · 11.92[3] · 11.97±0.48[6]

5316 Filatov, provisional designation1982 UB7, is a carbonaceousasteroid and potentiallyslow rotator from the outer region of theasteroid belt, approximately 30 kilometers in diameter.

The asteroid was discovered on 21 October 1982, by Russian astronomerLyudmila Karachkina at theCrimean Astrophysical Observatory in Nauchnij on the Crimean peninsula.[7] It was later named for surgeonVladimir Filatov.[2]

Orbit and classification

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Filatov orbits the Sun in theouter main-belt at a distance of 3.1–3.2 AU once every 5 years and 7 months (2,050 days). Its orbit has aneccentricity of 0.02 and aninclination of 15° with respect to theecliptic.[1] The body'sobservation arc begins at Nauchnij, 2 days after its official discovery observation.[7]

Physical characteristics

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Potentially slow rotator

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In November 2010, a rotationallightcurve ofFilatov was obtained from photometric observations in the R-band at thePalomar Transient Factory in California. It gave an exceptionally longrotation period of 1061 hours with a brightness variation of 0.07magnitude (U=1).[5]

However, the fragmentary lightcurve has received a low quality rating by theCollaborative Asteroid Lightcurve Link which means that the result could be completely wrong(also seepotentially slow rotator).[3][5]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Filatov measures 45.69 kilometers in diameter, and its surface has analbedo of 0.019,[4] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous asteroids of 0.057 and calculates a diameter of 22.95 kilometers with anabsolute magnitude of 11.92.[3]

Naming

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Thisminor planet was named in honor ofVladimir Filatov (1875–1956), a Russian and Ukrainianophthalmologist andsurgeon.[2] The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22508).[8]

References

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  1. ^abcd"JPL Small-Body Database Browser: 5316 Filatov (1982 UB7)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved21 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(5316) Filatov".Dictionary of Minor Planet Names – (5316) Filatov.Springer Berlin Heidelberg. p. 456.doi:10.1007/978-3-540-29925-7_5131.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (5316) Filatov". Asteroid Lightcurve Database (LCDB). Retrieved16 December 2016.
  4. ^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. Retrieved16 December 2016.
  5. ^abcdWaszczak, 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. Retrieved16 December 2016.
  6. ^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. Retrieved16 December 2016.
  7. ^ab"5316 Filatov (1982 UB7)".Minor Planet Center. Retrieved16 December 2016.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved16 December 2016.

External links

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