783 Nora

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783 Nora
Discovery[1]
Discovered byJ. Palisa
Discovery siteVienna Obs.
Discovery date18 March 1914
Designations
(783) Nora
Named after
Character of Nora Helmer in the play A Doll's House
(By poet Henrik Ibsen)[2]
A914 FB · A911 QG
1914 UL
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc108.44 yr (39,607 d)
Aphelion2.8811 AU
Perihelion1.8046 AU
2.3429 AU
Eccentricity0.2297
3.59 yr (1,310 d)
136.94°
0° 16m 29.28s / day
Inclination9.3410°
142.09°
154.70°
Physical characteristics
  • 38.719±0.105 km[7]
  • 39.58±0.62 km[8]
  • 40.02±0.8 km[9]
55.53±0.08 h[10]
  • 0.0635±0.003[9]
  • 0.065±0.002[8]
  • 0.068±0.012[7]
SMASS = C[3]

783 Nora (prov. designation: A914 FB or 1914 UL) is a dark background asteroid from the inner regions of the asteroid belt. It was discovered by Austrian astronomer Johann Palisa at the Vienna Observatory on 18 March 1914.[1] The carbonaceous C-type asteroid has a longer-than average rotation period of 55.5 hours and measures approximately 40 kilometers (25 miles) in diameter. It was likely named after Nora Helmer, principal character in the play A Doll's House by Norwegian poet Henrik Ibsen.[2]

Nora 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][6] It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.9 AU once every 3 years and 7 months (1,310 days; semi-major axis of 2.34 AU). Its orbit has an eccentricity of 0.23 and an inclination of 9° with respect to the ecliptic.[3] The body's observation arc begins with its first observation as A911 QG at Heidelberg Observatory on 28 August 1911, more than two years prior to its official discovery observation at Vienna Observatory.[1]

Naming

This minor planet was likely named after Nora Helmer, the heroine in the play A Doll's House (1879) by Norwegian poet Henrik Ibsen (1828–1906). The name was given by the discoverer's friends. The naming was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 78).[2]

Physical characteristics

References

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