| Minorplanet: | yes |
| 2018 CC | |
| Background: |
|
| Discovered: | 4 February 2018 |
| Mpc Name: | 2018 CC |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 65 |
| Observation Arc: | 17 days |
| Perihelion: | 0.8358 AU |
| Semimajor: | 1.2841 AU |
| Eccentricity: | 0.3491 |
| Period: | 1.46 yr (531 days) |
| Mean Motion: | / day |
| Inclination: | 8.4577° |
| Asc Node: | 317.50° |
| Arg Peri: | 245.91° |
| Moid: | 0.0002 AU (0.078 LD) |
| Mean Diameter: | |
| Abs Magnitude: | 26.541 |
is a micro-asteroid, classified as a near-Earth object of the Apollo group, approximately 20sigfig=1NaNsigfig=1 in diameter. Its official first observation was made by the Catalina Sky Survey at Mount Lemmon Observatory, Arizona, United States, on 4 February 2018. Two days later, the asteroid crossed the orbit of the Moon and made a very close approach to Earth.
belongs to the Apollo asteroids, which cross the orbit of Earth. Apollo's are the largest group of near-Earth objects with nearly 10 thousand known members. It orbits the Sun at a distance of 0.84–1.73 AU once every 18 months (531 days; semi-major axis of 1.28 AU). Its orbit has an eccentricity of 0.35 and an inclination of 8° with respect to the ecliptic. With an aphelion of 1.73 AU, it is also a Mars-crosser, as it crosses the orbit of the Red Planet at 1.66 AU.
The body's observation arc begins with its first recorded observation by Pan-STARRS on 20 January 2018.
The object has a low minimum orbital intersection distance with Earth of 0.0002AU, which corresponds to 0.078 lunar distances (LD). On 8 February 2034, it will approach Earth to a distance of 0.0212AU or 8.2 LD.
On 6 February 2018, it passed at a nominal distance of 0.001264AU from Earth (0.49 LD). One hour earlier, it passed the Moon at 0.0038564AU.
The body's physical parameter remain largely unknown. Based on a generic magnitude-to-diameter conversion, and for an absolute magnitude of 26.541, the asteroid measures 15 and 40 meters in diameter, assuming a carbonaceous and stony albedo of 0.057 and 0.20, respectively. No rotational lightcurve has been obtained from photometric observations, and no rotation period, shape or pole has been determined.
As of 2018, this minor planet has not been numbered or named.