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13003 Dickbeasley

13003 Dickbeasley, provisional designation 1982 FN, is a background asteroid from the central region of the asteroid belt, approximately 6 kilometers in diameter. It was discovered by American astronomer Edward Bowell at Lowell's Anderson Mesa Station on 21 March 1982.[2] The asteroid was named in memory of American NAU administrator Dick Beasley.[2]

13003 Dickbeasley
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date21 March 1982
Designations
(13003) Dickbeasley
Named after
Dick Beasley (NAU, artist)[2]
1982 FN · 1982 HJ2
main-belt · (inner)[3]
background
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc34.66 yr (12,661 days)
Aphelion3.0838 AU
Perihelion2.0332 AU
2.5585 AU
Eccentricity0.2053
4.09 yr (1,495 days)
227.37°
0° 14m 26.88s / day
Inclination26.560°
177.56°
33.358°
Physical characteristics
Mean diameter
5.41 km (calculated)[3]
8.240±0.119 km[4][5]
3.4992±0.0090 h[6]
3.4999±0.0005 h[7]
3.502±0.001 h[8]
0.074±0.011[4][5]
0.20 (assumed)[3]
S (assumed)[3]
13.7[1][3][4] · 14.402±0.008 (S)[6] · 14.25±0.89[9]

Orbit and classification edit

Dickbeasley is a non-family asteroid from the main belt's background population. It orbits the Sun in the central main-belt at a distance of 2.0–3.1 AU once every 4 years and 1 month (1,495 days). Its orbit has an eccentricity of 0.21 and an inclination of 27° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation, as no precoveries were taken, and no prior identifications were made.[2]

Naming edit

This minor planet was named in memory of American Richard "Dick" E. Beasley (1934–1992), a teacher and administrator at Northern Arizona University. He was also a multi-media artist and a preeminent figure in the calligraphic world.[2] The approved naming citation was published by the Minor Planet Center on 9 February 2009 (M.P.C. 65122).[10]

Physical characteristics edit

Rotation period edit

In April 2015, a rotational lightcurve of Dickbeasley was obtained from photometric observations made at the Phillips Academy Observatory (I12). It gave a rotation period of 3.502 hours with a brightness variation of 0.44 magnitude (U=3-).[8] One month later, in May 2015, observations at Texas Tech's Preston Gott Observatory gave a concurring period of 3.4999 hours with an amplitude of 0.30 magnitude (U=3-).[7]

These results supersede the first obtained lightcurve at the Palomar Transient Factory from September 2012, which gave a period of 3.4992 hours and an amplitude of 0.42 (U=2).[6]

Diameter and albedo edit

According to the surveys carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Dickbeasley measures 8.2 kilometers in diameter and its surface has an albedo of 0.07,[4][5] while he Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5.4 kilometers with an absolute magnitude of 13.7.[3]

References edit

  1. ^ a b c d "JPL Small-Body Database Browser: 13003 Dickbeasley (1982 FN)" (2016-11-18 last obs.). Jet Propulsion Laboratory. Retrieved 24 June 2017.
  2. ^ a b c d e "13003 Dickbeasley (1982 FN)". Minor Planet Center. Retrieved 23 May 2016.
  3. ^ a b c d e f "LCDB Data for (13003) Dickbeasley". Asteroid Lightcurve Database (LCDB). Retrieved 23 May 2016.
  4. ^ a b c d Mainzer, 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. Retrieved 23 May 2016.
  5. ^ a b c Masiero, 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. Retrieved 3 December 2016.
  6. ^ a b c Waszczak, 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. Retrieved 23 May 2016.
  7. ^ a b Clark, Maurice (January 2016). "Asteroid Photometry from the Preston Gott Observatory". The Minor Planet Bulletin. 43 (1): 2–5. Bibcode:2016MPBu...43....2C. ISSN 1052-8091. Retrieved 23 May 2016.
  8. ^ a b Odden, Caroline; Jenkins, Ravn; Nasser, Ravenne; Nix, Sabine; Dear, Anna (October 2015). "Finding the Lightcurve and Rotation Period of Minor Planet 13003 Dickbeasley". The Minor Planet Bulletin. 42 (4): 237. Bibcode:2015MPBu...42..237O. ISSN 1052-8091. Retrieved 23 May 2016.
  9. ^ 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. Retrieved 23 May 2016.
  10. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 23 May 2016.

External links edit

  • Richard E. Beasley, Biography
  • Richard E. Beasley (1934–1992), The Art of the Letter
  • Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
  • Dictionary of Minor Planet Names, Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
  • 13003 Dickbeasley at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 13003 Dickbeasley at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

13003, dickbeasley, provisional, designation, 1982, background, asteroid, from, central, region, asteroid, belt, approximately, kilometers, diameter, discovered, american, astronomer, edward, bowell, lowell, anderson, mesa, station, march, 1982, asteroid, name. 13003 Dickbeasley provisional designation 1982 FN is a background asteroid from the central region of the asteroid belt approximately 6 kilometers in diameter It was discovered by American astronomer Edward Bowell at Lowell s Anderson Mesa Station on 21 March 1982 2 The asteroid was named in memory of American NAU administrator Dick Beasley 2 13003 DickbeasleyDiscovery 1 Discovered byE BowellDiscovery siteAnderson Mesa Stn Discovery date21 March 1982DesignationsMPC designation 13003 DickbeasleyNamed afterDick Beasley NAU artist 2 Alternative designations1982 FN 1982 HJ2Minor planet categorymain belt inner 3 backgroundOrbital characteristics 1 Epoch 4 September 2017 JD 2458000 5 Uncertainty parameter 0Observation arc34 66 yr 12 661 days Aphelion3 0838 AUPerihelion2 0332 AUSemi major axis2 5585 AUEccentricity0 2053Orbital period sidereal 4 09 yr 1 495 days Mean anomaly227 37 Mean motion0 14m 26 88s dayInclination26 560 Longitude of ascending node177 56 Argument of perihelion33 358 Physical characteristicsMean diameter5 41 km calculated 3 8 240 0 119 km 4 5 Synodic rotation period3 4992 0 0090 h 6 3 4999 0 0005 h 7 3 502 0 001 h 8 Geometric albedo0 074 0 011 4 5 0 20 assumed 3 Spectral typeS assumed 3 Absolute magnitude H 13 7 1 3 4 14 402 0 008 S 6 14 25 0 89 9 Contents 1 Orbit and classification 2 Naming 3 Physical characteristics 3 1 Rotation period 3 2 Diameter and albedo 4 References 5 External linksOrbit and classification editDickbeasley is a non family asteroid from the main belt s background population It orbits the Sun in the central main belt at a distance of 2 0 3 1 AU once every 4 years and 1 month 1 495 days Its orbit has an eccentricity of 0 21 and an inclination of 27 with respect to the ecliptic 1 The body s observation arc begins with its official discovery observation as no precoveries were taken and no prior identifications were made 2 Naming editThis minor planet was named in memory of American Richard Dick E Beasley 1934 1992 a teacher and administrator at Northern Arizona University He was also a multi media artist and a preeminent figure in the calligraphic world 2 The approved naming citation was published by the Minor Planet Center on 9 February 2009 M P C 65122 10 Physical characteristics editRotation period edit In April 2015 a rotational lightcurve of Dickbeasley was obtained from photometric observations made at the Phillips Academy Observatory I12 It gave a rotation period of 3 502 hours with a brightness variation of 0 44 magnitude U 3 8 One month later in May 2015 observations at Texas Tech s Preston Gott Observatory gave a concurring period of 3 4999 hours with an amplitude of 0 30 magnitude U 3 7 These results supersede the first obtained lightcurve at the Palomar Transient Factory from September 2012 which gave a period of 3 4992 hours and an amplitude of 0 42 U 2 6 Diameter and albedo edit According to the surveys carried out by the NEOWISE mission of NASA s space based Wide field Infrared Survey Explorer Dickbeasley measures 8 2 kilometers in diameter and its surface has an albedo of 0 07 4 5 while he Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0 20 and calculates a diameter of 5 4 kilometers with an absolute magnitude of 13 7 3 References edit a b c d JPL Small Body Database Browser 13003 Dickbeasley 1982 FN 2016 11 18 last obs Jet Propulsion Laboratory Retrieved 24 June 2017 a b c d e 13003 Dickbeasley 1982 FN Minor Planet Center Retrieved 23 May 2016 a b c d e f LCDB Data for 13003 Dickbeasley Asteroid Lightcurve Database LCDB Retrieved 23 May 2016 a b c d Mainzer 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 Retrieved 23 May 2016 a b c Masiero 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 Retrieved 3 December 2016 a b c Waszczak 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 Retrieved 23 May 2016 a b Clark Maurice January 2016 Asteroid Photometry from the Preston Gott Observatory The Minor Planet Bulletin 43 1 2 5 Bibcode 2016MPBu 43 2C ISSN 1052 8091 Retrieved 23 May 2016 a b Odden Caroline Jenkins Ravn Nasser Ravenne Nix Sabine Dear Anna October 2015 Finding the Lightcurve and Rotation Period of Minor Planet 13003 Dickbeasley The Minor Planet Bulletin 42 4 237 Bibcode 2015MPBu 42 237O ISSN 1052 8091 Retrieved 23 May 2016 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 Retrieved 23 May 2016 MPC MPO MPS Archive Minor Planet Center Retrieved 23 May 2016 External links editRichard E Beasley Biography Richard E Beasley 1934 1992 The Art of the Letter Asteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Observatoire de Geneve Raoul Behrend Discovery Circumstances Numbered Minor Planets 10001 15000 Minor Planet Center 13003 Dickbeasley at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 13003 Dickbeasley at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 13003 Dickbeasley amp oldid 1183347874, wikipedia, wiki, book, books, library,

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