3671 Dionysus

3671 Dionysus is a small binary Amor asteroid, orbiting between 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.

3671 Dionysus
Orbit of 3671 Dionysus
Discovery
Discovered byC. S. Shoemaker
E. M. Shoemaker
Discovery sitePalomar Observatory
Discovery date27 May 1984
Designations
(3671) Dionysus
Pronunciation/daɪəˈnaɪsəs/[1]
Named after
Διόνυσος Dionȳsos
1984 KD[2]
PHA[2]
AdjectivesDionysian /daɪəˈnɪsiən/[3]
Orbital characteristics[2]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc11629 days (31.84 yr)
Aphelion3.389527126 AU (507.0660407 Gm)
Perihelion1.00825538 AU (150.832858 Gm)
2.198891253 AU (328.9494493 Gm)
Eccentricity0.54147101
3.26 yr (1191.0 d)
244.408078°
0° 18m 8.181s / day
Inclination13.5346771°
82.1319934°
204.217348°
Known satellites1
Earth MOID0.0199599 AU (2.98596 Gm)
Physical characteristics
Dimensions1.5 km[2]
Mean density
1.6 g/cm3[4]
2.7053 h (0.11272 d)[2]
0.16[2]
B[2]
16.5[2]

    Potentially hazardous object

    3671 Dionysus is a potentially hazardous asteroid (PHA) because its minimum orbit intersection distance (MOID) is less than 0.05 AU and its diameter is greater than 150 meters. The Earth-MOID is 0.01989 AU (2,976,000 km; 1,849,000 mi).[2] Its orbit is well-determined for the next several hundred years.

    Dionysus makes modestly close approaches to Earth. On 19 June 1984 Dionysus passed 0.0305 AU (4,560,000 km; 2,840,000 mi) from Earth.[2] On 18 June 2085 it will pass 0.028 AU (4,200,000 km; 2,600,000 mi) from Earth.[2]

    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 3.6 km from Dionysus with an eccentricity of 0.07 and an orbital period of 27.72 hours.[5] 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 .
    gollark: This isn't really better than an "options" struct with a bunch of defaults.
    gollark: The function way also does not have a possible inconsistent state (in its external API).
    gollark: What if you `.build()` twice?
    gollark: Which I think is a better API.
    gollark: A lot of things will just let you create a "listener" with a callback.

    References
    1. Webster (1884) A Practical Dictionary
    2. "3671 Dionysus (1984 KD)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 14 April 2016.
    3. "Dionysian". Oxford English Dictionary (3rd ed.). Oxford University Press. September 2005. (Subscription or UK public library membership required.)
    4. Pravec, P.; Scheirich, P.; Kusnirak, P.; Sarounova, L.; Mottola, S.; Hahn, G.; Brown, P.; Esquerdo, G.; Kaiser, N.; Krzeminski, Z.; Pray, D. P.; Warner, B. D.; Harris, A. W.; Nolan, M. C.; Howell, E. S.; Benner, L. A. M.; Margot, J. -L.; Galád, A.; Holliday, W.; Hicks, M. D.; Krugly, Yu. N.; Tholen, D.; Whiteley, R.; Marchis, F.; Degraff, D. R.; Grauer, A.; Larson, S.; Velichko, F. P.; Cooney, W. R.; et al. (March 2006). "Photometric survey of binary near-Earth asteroids". Icarus. 181 (1): 63–93. Bibcode:2006Icar..181...63P. doi:10.1016/j.icarus.2005.10.014.
    5. Johnston's Archive: (3671) Dionysus and S/1997 (3671) 1

    This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.