6498 Ko
| Discovery | |
|---|---|
| Discovered by |
K. Endate K. Watanabe |
| Discovery site | Kitami Obs. |
| Discovery date | 26 October 1992 |
| Designations | |
| MPC designation | (6498) Ko |
|
Named after
|
Ko Nagasawa (Japanese scientist) |
|
1992 UJ4 · 1964 PM 1971 QK3 · 1994 CD4 |
|
| main-belt · Flora | |
| Orbital characteristics | |
| Epoch 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 61.97 yr (22,634 days) |
| Aphelion | 2.6661 AU |
| Perihelion | 1.8960 AU |
| 2.2810 AU | |
| Eccentricity | 0.1688 |
| 3.45 yr (1,258 days) | |
| 91.902° | |
| 0° 17m 9.96s / day | |
| Inclination | 7.9907° |
| 149.64° | |
| 156.76° | |
| Physical characteristics | |
| Dimensions | 3.99 km (calculated) |
| 500 h | |
| 0.24 (assumed) | |
| S | |
| 13.5 · 13.71 · 13.92±0.47 · 14.16 | |
6498 Ko, provisional designation 1992 UJ4, is a stony Flora asteroid and exceptionally slow rotator from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 26 October 1992, by Japanese amateur astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory on eastern Hokkaidō, Japan.
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 1.9–2.7 AU once every 3 years and 5 months (1,258 days). Its orbit has an eccentricity of 0.17 and an inclination of 8° with respect to the ecliptic. The first precovery was taken at Palomar Observatory in 1954, extending the asteroid's observation arc by 38 years prior to its discovery.
Although the asteroid does not cross the orbit of any planet, it does make close approaches to other large asteroids, such as 29 Amphitrite, which it approached within 0.038 AU in 1915. Further close approaches will take place in 2025 and 2135 at a distance of 0.012 and 0.009 AU, respectively. On 14 November 2009, the asteroid also made a close encounter with 3 Juno at a distance of about 0.047 AU.
A rotational light-curve for this asteroid was obtained from photometric observations by Czech astronomer Petr Pravec at the Ondřejov Observatory in June 2012. It rendered an exceptionally long rotation period of 500 hours with a brightness amplitude of 0.6 in magnitude (U=2). The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24, derived from the Flora family's largest member and namesake, the asteroid 8 Flora, and calculates a diameter of 4.0 kilometers based on an absolute magnitude of 14.16.
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