| Discovery[1] | |
|---|---|
| Discovered by | C. W. Juels |
| Discovery site | Fountain Hills Obs. |
| Discovery date | 9 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 arc | 20.97yr (7,659 d) |
| Aphelion | 2.4364AU |
| Perihelion | 2.2457 AU |
| 2.3410 AU | |
| Eccentricity | 0.0407 |
| 3.58 yr (1,308 d) | |
| 340.18° | |
| 0° 16m 30.72s / day | |
| Inclination | 7.3496° |
| 310.72° | |
| 164.63° | |
| Physical characteristics | |
| 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] | |
24105 Broughton (provisional designation1999 VE10) is a backgroundasteroid from the inner regions of theasteroid belt, approximately 3.7 kilometers (2.3 miles) in diameter. The assumedS-type asteroid was discovered on 9 November 1999, by American amateur astronomerCharles W. Juels at the Fountain Hills Observatory (678) in Arizona, United States.[1] It has arotation period of 15.9 hours and was named after Australian amateur astronomerJohn Broughton.[2][3]
Broughton is non-family asteroid from the main belt'sbackground population,[4][5] located near the region occupied by theFlora family, one of the largestclans ofstony asteroids.[3] It orbits the Sun in theinner 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 aneccentricity of 0.04 and aninclination of 7° with respect to theecliptic.[3]
The asteroid was first observed as1997 BV6 at the Japanese Tajimi Observatory (901) in January 1997, where itsobservation arc begins in the following month, about 2 years prior to the asteroid's official discovery observation at Fountain Hills.[1]
Thisminor planet was named in honor of Australian amateur astronomerJohn Broughton (born 1952), a prolificdiscoverer of minor planets who received a "Shoemaker NEO Grant" in 2002.[2] The approved naming citation was published by theMinor Planet Center on 26 November 2004 (M.P.C. 53176).[8]
In October 2013, a rotationallightcurve of Broughton was obtained from photometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of15.9442 hours with a brightness variation of 0.34magnitude (U=2).[7]
TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the family's largest member and namesake – and calculates a diameter of 3.65 kilometers with anabsolute magnitude of 14.36.[6]
