24105 Broughton

24105 Broughton
Discovery[1]
Discovered by C. W. Juels
Discovery site Fountain Hills Obs.
Discovery date 9 November 1999
Designations
MPC designation 24105 Broughton
Named after
John Broughton
(astronomer)[2]
1999 VE10 · 1997 BV6    
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 19.36 yr (7,070 days)
Aphelion 2.4369 AU
Perihelion 2.2453 AU
2.3411 AU
Eccentricity 0.0409
3.58 yr (1,308 days)
230.11°
 16m 30.72s / day
Inclination 7.3498°
310.73°
164.63°
Physical characteristics
Dimensions 3.65 km (calculated)[3]
15.9442±0.0250 h[4]
0.24 (assumed)[3]
S[3]
13.9[1]
13.907±0.005 (R)[4]
14.07±0.50[5] · 14.36[3]

    24105 Broughton, provisional designation 1999 VE10, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 9 November 1999, by American amateur astronomer Charles W. Juels at the U.S. Fountain Hills Observatory in Arizona.[6]

    The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 2.2–2.4 AU once every 3 years and 7 months (1,308 days). Its orbit has an eccentricity of 0.04 and an inclination of 7° with respect to the ecliptic.[1] Identified as 1997 BV6 at the Japanese Tajimi Observatory, the first used observation was a precovery obtained at Steward Observatory 13 days later, and extending Broughton's observation arc by more than 2 years prior to the official discovery observation.[6]

    In October 2013, a rotational light-curve for this asteroid was obtained from photometric observations at the U.S. Palomar Transient Factory in California. It gave a longer-than-average rotation period of 15.9442±0.0250 hours with a brightness variation of 0.34 in magnitude (U=2).[4] 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, based on an absolute magnitude of 14.36.[3]

    The minor planet is named in honor of Australian amateur astronomer John Broughton (b.1952), a prolific discoverer of minor planets who received a "Shoemaker NEO Grant" in 2002.[2] Naming citation was published on 26 November 2004 (M.P.C. 53176).[7]

    References

    1. 1 2 3 4 "JPL Small-Body Database Browser: 24105 Broughton (1999 VE10)" (2016-06-13 last obs.). Jet Propulsion Laboratory. Retrieved 2 December 2016.
    2. 1 2 Schmadel, Lutz D. (2006). Dictionary of Minor Planet Names – (24105) Broughton, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 186. ISBN 978-3-540-34361-5. Retrieved 31 July 2016.
    3. 1 2 3 4 5 6 "LCDB Data for (24105) Broughton". Asteroid Lightcurve Database (LCDB). Retrieved 31 July 2016.
    4. 1 2 3 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. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75. Retrieved 31 July 2016.
    5. 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:1506.00762Freely accessible. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 31 July 2016.
    6. 1 2 "24105 Broughton (1999 VE10)". Minor Planet Center. Retrieved 31 July 2016.
    7. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 31 July 2016.

    External links

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