3671 Dionysus

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3671 Dionysus
Orbit of 3671 Dionysus
Discovery and designation
Discovered by Carolyn and Gene Shoemaker
Discovery site Palomar Observatory
Discovery date May 27, 1984
Designations
MPC designation 3671
Named after Dionysus
Alternative names 1984 KD[1]
Orbital characteristics[1]
Epoch August 27, 2011 (JD 2455800.5
Aphelion 3.389130075 AU
Perihelion 1.00645923 AU
Semi-major axis 2.197794652 AU
Eccentricity 0.54205947
Orbital period 3.258283510 yr (1190.088052 d)
Mean anomaly 120.239711°
Inclination 13.547627°
Longitude of ascending node 82.15874°
Argument of perihelion 204.23906°
Known satellites 1
Physical characteristics
Dimensions 1.5 km[1]
Mean density 1.6 g/cm3[2]
Sidereal rotation period 2.7053 h[1]
Geometric albedo 0.16[1]
Spectral type B[1]
Absolute magnitude (H) 16.3[1]

    3671 Dionysus is a small binary Amor asteroid, orbiting between the Earth and the asteroid belt. It was discovered by Carolyn and Gene Shoemaker at Palomar Observatory on 27 May 1984. It is named after Dionysus, the Greek god of wine. Its provisional designation was 1984 KD. It is an outer Earth grazer because its perihelion is just within Earth's orbit.

    Near-Earth object

    Dionysus makes many close approaches to Earth. Its closest approach so far occurred in 1984, when Dionysus passed just 0.03047 astronomical units (4,558,000 km) from Earth.[1] Dionysus is expected to continue to make close approaches.

    Moon

    In 1997, a team of astronomers at the European Southern Observatory announced that lightcurve observations indicate the presence of a small moon orbiting Dionysus. Its provisional designation is S/1997 (3671) 1. This moon measures 300 meters in diameter, and orbits 3.6km from Dionysus with an eccentricity of 0.07 and an orbital period of 27.72 hours.[3] From the surface of Dionysus, S/1997 (3671) 1 would have an apparent diameter of roughly 3.02 degrees.[lower-alpha 1] For comparison, the Sun appears to be 0.5° from Earth.

    Notes

    1. Calculated by solving the equation \scriptstyle {{\mathrm  {tan}}\left({\frac  {\theta }{2}}\right)={\frac  {{\mathrm  {radius~of~moon}}}{{\mathrm  {distance~from~surface~of~asteroid~to~center~of~moon}}}}}.

    References

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