Astronomy:24105 Broughton

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Short description: Background asteroid
24105 Broughton
Discovery [1]
Discovered byC. W. Juels
Discovery siteFountain Hills Obs.
Discovery date9 November 1999
Designations
(24105) Broughton
Named afterJohn Broughton
(Australian astronomer)[2]
1999 VE10 · 1997 BV6
Minor planet categorymain-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)
|{{{apsis}}}|helion}}2.4364 AU
|{{{apsis}}}|helion}}2.2457 AU
2.3410 AU
Eccentricity0.0407
Orbital period3.58 yr (1,308 d)
Mean anomaly340.18°
Mean motion0° 16m 30.72s / day
Inclination7.3496°
Longitude of ascending node310.72°
164.63°
Physical characteristics
Mean diameter3.65 km (calculated)[6]
Rotation period15.9442±0.0250 h[7]
Geometric albedo0.24 (assumed)[6]
S[6]
Absolute magnitude (H)13.907±0.005 (R)[7]
14.0[1][3]
14.36[6]


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]

Orbit and classification

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

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

Lightcurves

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 ({{{1}}}).[7]

Diameter and albedo

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

  1. 1.0 1.1 1.2 1.3 1.4 "24105 Broughton (1999 VE10)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=24105. Retrieved 17 July 2018. 
  2. 2.0 2.1 2.2 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. 3.0 3.1 3.2 3.3 3.4 3.5 "JPL Small-Body Database Browser: 24105 Broughton (1999 VE10)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2024105. Retrieved 27 June 2017. 
  4. 4.0 4.1 "Asteroid (24105) Broughton – Proper elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?n=24105&pc=1.1.6. Retrieved 17 July 2018. 
  5. 5.0 5.1 "Asteroid 24105 Broughton". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=24105+Broughton. Retrieved 17 July 2018. 
  6. 6.0 6.1 6.2 6.3 6.4 "LCDB Data for (24105) Broughton". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=24105%7CBroughton. Retrieved 31 July 2016. 
  7. 7.0 7.1 7.2 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. doi:10.1088/0004-6256/150/3/75. Bibcode2015AJ....150...75W. 
  8. "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. Retrieved 31 July 2016. 

External links