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24105 Broughton

24105 Broughton (provisional designation 1999 VE10) is a background asteroid from the inner regions of the asteroid belt, approximately 3.7 kilometers (2.3 miles) in diameter. The assumed S-type asteroid was discovered on 9 November 1999, by American amateur astronomer Charles W. Juels at the Fountain Hills Observatory (678) in Arizona, United States.[1] It has a rotation period of 15.9 hours and was named after Australian amateur astronomer John Broughton.[2][3]

24105 Broughton
Discovery [1]
Discovered byC. W. Juels
Discovery siteFountain Hills Obs.
Discovery date9 November 1999
Designations
(24105) Broughton
Named after
John Broughton
(Australian astronomer)[2]
1999 VE10 · 1997 BV6
main-belt[1][3] · (inner)
background[4][5]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc20.97 yr (7,659 d)
Aphelion2.4364 AU
Perihelion2.2457 AU
2.3410 AU
Eccentricity0.0407
3.58 yr (1,308 d)
340.18°
0° 16m 30.72s / day
Inclination7.3496°
310.72°
164.63°
Physical characteristics
Mean diameter
3.65 km (calculated)[6]
15.9442±0.0250 h[7]
0.24 (assumed)[6]
S[6]
13.907±0.005 (R)[7]
14.0[1][3]
14.36[6]

Orbit and classification edit

Broughton is non-family asteroid from the main belt's background population,[4][5] located near the region occupied by the Flora family, one of the largest clans of stony asteroids.[3] It orbits the Sun in the inner asteroid belt at a distance of 2.2–2.4 AU once every 3 years and 7 months (1,308 days; semi-major axis of 2.34 AU). Its orbit has an eccentricity of 0.04 and an inclination of 7° with respect to the ecliptic.[3]

The asteroid was first observed as 1997 BV6 at the Japanese Tajimi Observatory (901) in January 1997, where its observation arc begins in the following month, about 2 years prior to the asteroid's official discovery observation at Fountain Hills.[1]

Naming edit

This minor planet was named in honor of Australian amateur astronomer John Broughton (born 1952), a prolific discoverer of minor planets who received a "Shoemaker NEO Grant" in 2002.[2] The approved naming citation was published by the Minor Planet Center on 26 November 2004 (M.P.C. 53176).[8]

Physical characteristics edit

Lightcurves edit

In October 2013, a rotational lightcurve of Broughton was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 15.9442 hours with a brightness variation of 0.34 magnitude (U=2).[7]

Diameter and albedo edit

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the family's largest member and namesake – and calculates a diameter of 3.65 kilometers with an absolute magnitude of 14.36.[6]

References edit

  1. ^ a b c d e "24105 Broughton (1999 VE10)". Minor Planet Center. Retrieved 17 July 2018.
  2. ^ a b c Schmadel, Lutz D. (2006). "(24105) Broughton [2.34, 0.04, 7.3]". Dictionary of Minor Planet Names – (24105) Broughton, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 186. doi:10.1007/978-3-540-34361-5_2178. ISBN 978-3-540-34361-5.
  3. ^ a b c d e f "JPL Small-Body Database Browser: 24105 Broughton (1999 VE10)" (2016-07-07 last obs.). Jet Propulsion Laboratory. Retrieved 27 June 2017.
  4. ^ a b "Asteroid (24105) Broughton – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 17 July 2018.
  5. ^ a b "Asteroid 24105 Broughton". Small Bodies Data Ferret. Retrieved 17 July 2018.
  6. ^ a b c d e "LCDB Data for (24105) Broughton". Asteroid Lightcurve Database (LCDB). Retrieved 31 July 2016.
  7. ^ 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.
  8. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 31 July 2016.

External links edit

  • Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
  • Dictionary of Minor Planet Names, Google books
  • Asteroid 24105 Broughton, at the Small bodies Data Ferret
  • Discovery Circumstances: Numbered Minor Planets (20001)-(25000) – Minor Planet Center
  • 24105 Broughton at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 24105 Broughton at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

24105, broughton, provisional, designation, 1999, ve10, background, asteroid, from, inner, regions, asteroid, belt, approximately, kilometers, miles, diameter, assumed, type, asteroid, discovered, november, 1999, american, amateur, astronomer, charles, juels, . 24105 Broughton provisional designation 1999 VE10 is a background asteroid from the inner regions of the asteroid belt approximately 3 7 kilometers 2 3 miles in diameter The assumed S type asteroid was discovered on 9 November 1999 by American amateur astronomer Charles W Juels at the Fountain Hills Observatory 678 in Arizona United States 1 It has a rotation period of 15 9 hours and was named after Australian amateur astronomer John Broughton 2 3 24105 BroughtonDiscovery 1 Discovered byC W JuelsDiscovery siteFountain Hills Obs Discovery date9 November 1999DesignationsMPC designation 24105 BroughtonNamed afterJohn Broughton Australian astronomer 2 Alternative designations1999 VE10 1997 BV6Minor planet categorymain belt 1 3 inner background 4 5 Orbital characteristics 3 Epoch 23 March 2018 JD 2458200 5 Uncertainty parameter 0Observation arc20 97 yr 7 659 d Aphelion2 4364 AUPerihelion2 2457 AUSemi major axis2 3410 AUEccentricity0 0407Orbital period sidereal 3 58 yr 1 308 d Mean anomaly340 18 Mean motion0 16m 30 72s dayInclination7 3496 Longitude of ascending node310 72 Argument of perihelion164 63 Physical characteristicsMean diameter3 65 km calculated 6 Synodic rotation period15 9442 0 0250 h 7 Geometric albedo0 24 assumed 6 Spectral typeS 6 Absolute magnitude H 13 907 0 005 R 7 14 0 1 3 14 36 6 Contents 1 Orbit and classification 2 Naming 3 Physical characteristics 3 1 Lightcurves 3 2 Diameter and albedo 4 References 5 External linksOrbit and classification editBroughton is non family asteroid from the main belt s background population 4 5 located near the region occupied by the Flora family one of the largest clans of stony asteroids 3 It orbits the Sun in the inner asteroid belt at a distance of 2 2 2 4 AU once every 3 years and 7 months 1 308 days semi major axis of 2 34 AU Its orbit has an eccentricity of 0 04 and an inclination of 7 with respect to the ecliptic 3 The asteroid was first observed as 1997 BV6 at the Japanese Tajimi Observatory 901 in January 1997 where its observation arc begins in the following month about 2 years prior to the asteroid s official discovery observation at Fountain Hills 1 Naming editThis minor planet was named in honor of Australian amateur astronomer John Broughton born 1952 a prolific discoverer of minor planets who received a Shoemaker NEO Grant in 2002 2 The approved naming citation was published by the Minor Planet Center on 26 November 2004 M P C 53176 8 Physical characteristics editLightcurves edit In October 2013 a rotational lightcurve of Broughton was obtained from photometric observations in the R band by astronomers at the Palomar Transient Factory in California Lightcurve analysis gave a rotation period of 15 9442 hours with a brightness variation of 0 34 magnitude U 2 7 Diameter and albedo edit The Collaborative Asteroid Lightcurve Link assumes an albedo of 0 24 derived from 8 Flora the family s largest member and namesake and calculates a diameter of 3 65 kilometers with an absolute magnitude of 14 36 6 References edit a b c d e 24105 Broughton 1999 VE10 Minor Planet Center Retrieved 17 July 2018 a b c Schmadel Lutz D 2006 24105 Broughton 2 34 0 04 7 3 Dictionary of Minor Planet Names 24105 Broughton Addendum to Fifth Edition 2003 2005 Springer Berlin Heidelberg p 186 doi 10 1007 978 3 540 34361 5 2178 ISBN 978 3 540 34361 5 a b c d e f JPL Small Body Database Browser 24105 Broughton 1999 VE10 2016 07 07 last obs Jet Propulsion Laboratory Retrieved 27 June 2017 a b Asteroid 24105 Broughton Proper elements AstDyS 2 Asteroids Dynamic Site Retrieved 17 July 2018 a b Asteroid 24105 Broughton Small Bodies Data Ferret Retrieved 17 July 2018 a b c d e LCDB Data for 24105 Broughton Asteroid Lightcurve Database LCDB Retrieved 31 July 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 MPC MPO MPS Archive Minor Planet Center Retrieved 31 July 2016 External links editAsteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroid 24105 Broughton at the Small bodies Data Ferret Discovery Circumstances Numbered Minor Planets 20001 25000 Minor Planet Center 24105 Broughton at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 24105 Broughton 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 24105 Broughton amp oldid 1197016736, wikipedia, wiki, book, books, library,

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