6882 Sormano

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6882 Sormano
Shape model of Sormano from its lightcurve
Discovery[1]
Discovered byP. Sicoli
V. Giuliani
Discovery siteSormano Obs.
Discovery date5 February 1995
Designations
(6882) Sormano
Named after
Sormano Observatory
(discovering observatory)[2]
1995 CC1 · 1986 XM2
1989 OW · 1993 OQ
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc27.85 yr (10,173 days)
Aphelion2.8043 AU
Perihelion2.2997 AU
2.5520 AU
Eccentricity0.0989
4.08 yr (1,489 days)
327.31°
0° 14m 30.48s / day
Inclination14.390°
284.19°
16.030°
Physical characteristics
6.69 km (calculated)[4]
7.665±0.101 km[5]
8.096±0.040 km[6]
3.6901±0.0006 h[7]
3.998344±0.000001 h[8]
0.21 (assumed)[4]
0.269±0.034[6]
0.3003±0.0545[5]
S (family-based)[4]
12.5[5] · 12.7[3] · 12.736±0.003 (R)[7] · 13.19[4]

6882 Sormano (prov. designation: 1995 CC1) is an stony Eunomia asteroid from the middle region of the asteroid belt, approximately 7 kilometers (4.3 miles) in diameter. It was discovered on 5 February 1995, by Italian amateur astronomers Piero Sicoli and Valter Giuliani at Sormano Astronomical Observatory in northern Italy.[1] The asteroid was named for the Italian mountain-village of Sormano and its discovering observatory.[2]

Sormano is a member of the Eunomia family, a large group of S-type asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun at a distance of 2.3–2.8 AU once every 4 years and 1 month (1,489 days). Its orbit has an eccentricity of 0.10 and an inclination of 14° with respect to the ecliptic.[3] The asteroid's observation arc begins 6 years prior to its discovery, as it had previously been observed as 1989 OW at Palomar Observatory in 1989.[1]

Naming

This minor planet was named in honor of the Italian mountain-village of Sormano and its discovering nearby observatory. It is funded, built and operated by the "Gruppo Astrofili Brianza", a group of Italian amateur astronomers who have discovered numerous minor planets.[2] The official naming citation was published by the Minor Planet Center on 3 May 1996 (M.P.C. 27130).[9]

Physical characteristics

References

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