889 Erynia

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889 Erynia
Modelled shape of Erynia from its lightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date5 March 1918
Designations
(889) Erynia
Pronunciation/ɛˈrniə/
Named after
Erinyes, or Furies
(Greek mythology)[2]
A918 EN · 1929 BG
A912 PA · 1912 PA
1918 DG
main-belt[1][3] · (inner)
background[4][5]
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc101.81 yr (37,187 d)
Aphelion2.9428 AU
Perihelion1.9500 AU
2.4464 AU
Eccentricity0.2029
3.83 yr (1,398 d)
342.62°
0° 15m 27.36s / day
Inclination8.1064°
132.53°
278.52°
Physical characteristics
9.89±0.01 h[8]
  • (187.0°, −60.0°) (λ11)[5][9]
  • (335.0°, −74.0°) (λ22)[5][9]
  • 0.196±0.014[7]
  • 0.230±0.042[6]
11.0[1][3]

889 Erynia /ɛˈrniə/ is a highly elongated background asteroid from the inner regions of the asteroid belt. It was discovered on 5 March 1918, by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory, and given the provisional designations A918 EN and 1918 DG.[1] The stony S-type asteroid (Sl) has a rotation period of 9.89 hours and measures approximately 17 kilometers (11 miles) in diameter. It was named from Greek mythology, after the Erinyes, also known as Furies.[2]

Erynia is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in the inner asteroid belt at a distance of 2.0–2.9 AU once every 3 years and 10 months (1,398 days; semi-major axis of 2.45 AU). Its orbit has an eccentricity of 0.20 and an inclination of 8° with respect to the ecliptic.[3] The asteroid was first observed as A912 PA (1912 PA) at the Johannesburg Observatory on 7 August 1912. The body's observation arc begins at Heidelberg Observatory on 16 March 1918, or eleven nights after its official discovery observation.[1]

Naming

This minor planet was named after one of the Erinyes from Greek mythology, also known as Furies in Roman mythology. The female deities of vengeance have snakes for hair, dog's heads, coal black bodies, bat's wings, and blood-shot eyes. They tortured their victims with brass-studded scourges and inflicted plagues. The naming was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 86).[2]

Physical characteristics

References

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