3671 Dionysus

3671 Dionysus
	Orbit of 3671 Dionysus
Discovery
Discovered by	C. S. Shoemaker; E. M. Shoemaker
Discovery site	Palomar Observatory
Discovery date	27 May 1984
Designations
MPC designation	(3671) Dionysus
Pronunciation	/daɪəˈnaɪsəs/[1]
Named after	Διόνυσος Dionȳsos
Alternative designations	1984 KD[2]
Minor planet category	PHA[2]
Adjectives	Dionysian /daɪəˈnɪsiən/[3]
Orbital characteristics[2]
	Epoch 13 January 2016 (JD 2457400.5)
	Uncertainty parameter 0
Observation arc	11629 days (31.84 yr)
Aphelion	3.389527126 AU (507.0660407 Gm)
Perihelion	1.00825538 AU (150.832858 Gm)
Semi-major axis	2.198891253 AU (328.9494493 Gm)
Eccentricity	0.54147101
Orbital period	3.26 yr (1191.0 d)
Mean anomaly	244.408078°
Mean motion	0° 18m 8.181s / day
Inclination	13.5346771°
Longitude of ascending node	82.1319934°
Argument of perihelion	204.217348°
Known satellites	1
Earth MOID	0.0199599 AU (2.98596 Gm)
Physical characteristics
Dimensions	1.5 km[2]
Mean density	1.6 g/cm3[4]
Rotation period	2.7053 h (0.11272 d)[2]
Geometric albedo	0.16[2]
Spectral type	B[2]
Absolute magnitude (H)	16.5[2]

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.

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

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

Webster (1884) A Practical Dictionary
"3671 Dionysus (1984 KD)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 14 April 2016.
"Dionysian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
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.
Johnston's Archive: (3671) Dionysus and S/1997 (3671) 1

External links

Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
3671 Dionysus at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
3671 Dionysus at ESA–space situational awareness
- Ephemerides · Observations · Orbit · Physical Properties · Summary
3671 Dionysus at the JPL Small-Body Database
- Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

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

[1] Webster (1884) A Practical Dictionary

[jpldata-2] "3671 Dionysus (1984 KD)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 14 April 2016.

[3] "Dionysian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)

[Survey-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.

[johnston-5] Johnston's Archive: (3671) Dionysus and S/1997 (3671) 1