4183 Cuno

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Cuno, imaged by radar
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Cuno, imaged by radar

4183 Cuno is an Apollo, Mars- and Venus-crosser asteroid. It was discovered in 1959 by Cuno Hoffmeister, from whom the asteroid takes its name.

Cuno is about 4-9 km in diameter and is an S-type asteroid, meaning that it is highly reflective and composed of nickel-iron mixed with iron- and magnesium-silicates.

In December 2000, Cuno was analysed by radar to determine its shape. The resultant images are lacking in detail, but indicate a rough sphere with some kind of concave depression 1-2 km in diameter.

4183 Cuno approaches the Earth to within 40 Gm six times in the 21st century. In 2012 it makes its closest pass, at 18 Gm, until 2093.

4183 Cuno
Discovery A
Discoverer Cuno Hoffmeister
Discovery date June 5, 1959
Alternate
designations
B
1959 LM
Category Apollo, Mars-crosser,
Venus-crosser
Orbital elements C
Epoch December 1, 2005 (JD 2453705.5)
Eccentricity (e) 0.636
Semi-major axis (a) 296.473 Gm (1.982 AU)
Perihelion (q) 107.872 Gm (0.721 AU)
Aphelion (Q) 485.073 Gm (3.243 AU)
Orbital period (P) 1019.031 d (2.790 a)
Mean orbital speed 18.827 km/s
Inclination (i) 6.750°
Longitude of the
ascending node
(Ω)
295.653°
Argument of
perihelion
(ω)
235.437°
Mean anomaly (M) 261.969°
Physical characteristics D
Dimensions 4.5 km
Mass
Density g/cm³
Surface gravity
Escape velocity 0.0002? km/s
Rotation period 3.6 h
Spectral class Sq
Absolute magnitude 14.4
Albedo (geometric)
Mean surface
temperature
K
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