![]() The orbit before and after its 2018-flyby | |
Discovery[1] | |
---|---|
Discovered by | MLS |
Discovery site | Mount Lemmon Obs. |
Discovery date | 7 February 2018 |
Designations | |
2018 CF2 | |
NEO · Apollo[1][2] | |
Orbital characteristics[2] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 7 | |
Observation arc | 2 days |
Aphelion | 2.7662AU |
Perihelion | 0.9089 AU |
1.8375 AU | |
Eccentricity | 0.5054 |
2.49yr (910 days) | |
29.432° | |
0° 23m 44.52s / day | |
Inclination | 16.284° |
137.68° | |
320.19° | |
Earth MOID | 0.00077 AU (0.30 LD) |
Physical characteristics | |
4–15 m[3] 7 m(est. at0.20)[4] 14 m(est. at0.057)[4] | |
28.036[2] | |
2018 CF2 is a micro-asteroid andnear-Earth object of theApollo group on an eccentric orbit with has an estimated 4–15 meters (10–50 ft). It was first observed on 7 February 2018, by astronomers of theMount Lemmon Survey atMount Lemmon Observatory, Arizona, United States.[1] The discovery occurred the day after its sub-lunar passage as it approached the Earth from a sunward direction, and this flyby altered the asteroid's orbit slightly.
2018 CF2 belongs to theApollo asteroids, the largest group ofnear-Earth objects with nearly 10 thousand known members, whichcross the orbit of Earth.
Based on a highuncertainty, it orbits the Sun at a distance of 0.91–2.77 AU once every 2 years and 6 months (910 days;semi-major axis of 1.84 AU). Its orbit has aneccentricity of 0.51 and aninclination of 16° with respect to theecliptic.[2] With anaphelion of 2.77 AU, it is also aMars-crosser, as it crosses the orbit of the Red Planet at 1.666 AU. The body'sobservation arc begins at Mount Lemmon with its first observation on 7 February 2018.[1]
On 6 February 2018, 18:45 UTC, the day before its first observation, it had a flyby with the Earth at a nominal distance of 0.25lunar distances (LD).[3] Its next close approach to Earth is projected to occur on 23 January 2023, at 0.111 AU (43 LD).[2] After the 2018-passage, the body'sminimum orbital intersection distance with Earth increased to 0.30 LD (0.00077 AU).[2]
TheMinor Planet Center estimates a diameter of 4–15 meters (10–50 ft).[3] Based on a generic magnitude-to-diameter conversion using anabsolute magnitude of 28.036,[2] the body measures between 7 and 14 meters in diameter for an assumedalbedo of 0.057 and 0.20, which represent typical values forcarbonaceous andstony asteroids, respectively.[4]
As of 2018, no rotationallightcurve of2018 CF2 has been obtained from photometric observations. The body'srotation period,pole and shape remain unknown.[2]
Thisminor planet has not yet been numbered.[1]