_Candy.png) Shape model of Candy from itslightcurve | |
| Discovery[1] | |
|---|---|
| Discovered by | E. Bowell |
| Discovery site | Anderson Mesa Stn. |
| Discovery date | 9 November 1980 |
| Designations | |
| (3015) Candy | |
Named after | Michael P. Candy (British astronomer)[2] |
| 1980 VN · 1974 VL2 1974 XC · 1984 HS | |
| main-belt · (outer)[1][3] | |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 52.17 yr (19,056 days) |
| Aphelion | 3.9747AU |
| Perihelion | 2.7983 AU |
| 3.3865 AU | |
| Eccentricity | 0.1737 |
| 6.23yr (2,276 days) | |
| 0.7451° | |
| 0° 9m 29.52s / day | |
| Inclination | 17.402° |
| 38.162° | |
| 300.96° | |
| Physical characteristics | |
| 24.517±0.470 km[4][5] 33.54 km(calculated)[3] | |
| 4.6249±0.0001 h[6] 4.625±0.001 h[7] 4.62501±0.00004 h[8] 4.62516 h[9][10] 4.625223 h[11] | |
| 0.057(assumed)[3] 0.1067±0.0173[4][5] | |
| C(assumed)[3] | |
| 11.1[1][3][5] · 11.14±0.34[12] | |
3015 Candy (prov. designation:1980 VN) is abackground asteroid from the outer regions of theasteroid belt, approximately 25 kilometers (16 miles) in diameter. It was discovered on 9 November 1980, by British-American astronomerEdward Bowell atAnderson Mesa Station in Flagstaff, Arizona.[13] The asteroid was named after British astronomerMichael P. Candy.[2]
Candy is a background asteroid that does not belong to any knownasteroid family. It orbits the Sun in theouter main-belt at a distance of 2.8–4.0 AU once every 6 years and 3 months (2,276 days). Its orbit has aneccentricity of 0.17 and aninclination of 17° with respect to theecliptic.[1] The body'sobservation arc begins with aprecovery taken atGoethe Link Observatory in May 1965, more than 15 years prior to its official discovery observation at Anderson Mesa.[13]
Thisminor planet was named afterMichael P. Candy (1928–1994) a British astronomer anddiscoverer of minor planets andcomets, who was a director of theRoyal Greenwich Observatory andPerth Observatory.[2] As a long-timeastrometrist and orbit computer, he discovered cometC/1960 Y1 (Candy) at Greenwich, as well as the minor planet3898 Curlewis,3893 DeLaeter and3894 Williamcooke. He was also president ofIAU's Commission VI.[2] The official naming citation was published by theMinor Planet Center on 22 June 1986 (M.P.C. 10845).[14]
Candy is an assumed carbonaceousC-type asteroid.[3]
Several rotationallightcurves of Candy were obtained from photometric observations by astronomer Maurice Clark. Lightcurve analysis gave a well-definedrotation period between 4.6249 and 4.62516 hours with a brightness variation between 0.50 and 1.05magnitude (U=3/3/3/3/3). (A high brightness amplitude typically indicates that a body has a non-spheroidal shape.)[6][7][8][9][10]
A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database (LPD), gave a concurring period of 4.625223 hours (U=2), as well as two spin axis of (142.0°, −26.0°) and (346.0°, −70.0°) inecliptic coordinates (λ, β).[11] Clark's spin modeling also suggests that Candy has aretrograde rotation, and a spin axis of (306.0°, 43.0.0°), that is nearly aligned with the body's shortest axis.[10]
According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Candy measures 24.517 kilometers in diameter and its surface has analbedo of 0.1067,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous of 0.057, and calculates a diameter of 33.54 kilometers based on anabsolute magnitude of 11.1.[3]
