959 Arne

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959 Arne
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date30 September 1921
Designations
(959) Arne
Named after
Arne Asplind
(son of Bror Asplind)[2]
A921 SE · 1927 YD
1952 DD2 · 1960 OF
A916 YB · 1921 KF
main-belt[1][3] · (outer)
background[4][5]
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc103.03 yr (37,630 d)
Aphelion3.8813 AU
Perihelion2.4752 AU
3.1782 AU
Eccentricity0.2212
5.67 yr (2,070 d)
86.935°
0° 10m 26.4s / day
Inclination4.4967°
58.521°
333.57°
Physical characteristics
  • 45.176±0.350 km[6]
  • 53.09±0.75 km[7]
  • 57.42±1.5 km[8]
123.7±0.1 h[9][10]
  • 0.0446±0.002[8]
    0.054±0.002[7]
  • 0.067±0.004[6]
X (SDSS-MOC)[11]
10.8[1][3]

959 Arne (prov. designation: A921 SE or 1921 KF) is a background asteroid and slow rotator, approximately 52 kilometers (32 miles) in diameter, located in the outer region of the asteroid belt. It was discovered by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory on 30 September 1921.[1] The X-type asteroid has an exceptionally long rotation period of 123.7 hours. It was named after Arne Asplind, son of Swedish astronomer Bror Asplind (1890–1954).[2]

Arne 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 outer asteroid belt at a distance of 2.5–3.9 AU once every 5 years and 8 months (2,070 days; semi-major axis of 3.18 AU). Its orbit has an eccentricity of 0.22 and an inclination of 4° with respect to the ecliptic.[3] The body's observation arc begins with its first observation as A916 YB (1916 YB) at Heidelberg Observatory on 27 December 1916, almost 5 years prior to its official discovery observation on 30 September 1921.[1]

Naming

This minor planet was named after Arne Asplind, son of Swedish astronomer Bror Ansgar Asplind (1890–1954). Asteroids 958 Asplinda, 960 Birgit and 961 Gunnie are named after him and his two daughters, respectively. The naming was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 92).[2]

Physical characteristics

References

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