873 Mechthild

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873 Mechthild
Modelled shape of Mechthild from its lightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date21 May 1917
Designations
(873) Mechthild
Named after
unknown[2]
A917 KJ · 1917 CA
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc102.24 yr (37,343 d)
Aphelion3.0199 AU
Perihelion2.2346 AU
2.6273 AU
Eccentricity0.1495
4.26 yr (1,555 d)
48.264°
0° 13m 53.04s / day
Inclination5.2763°
150.00°
109.99°
Physical characteristics
  • 29.04±1.9 km[6]
  • 33.56±0.59 km[7]
  • 34.471±0.103 km[8]
11.006±0.001 h[9]
  • (249.0°, −52.0°) (λ11)[5]
  • (51.0°, −61.0°) (λ22)[5]
  • 0.040±0.004[8]
  • 0.041±0.002[7]
  • 0.0531±0.008[6]
11.4[1][3]

873 Mechthild (prov. designation: A917 KJ or 1917 CA) is a dark background asteroid from the central regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg Observatory on 21 May 1917.[1] The primitive P-type asteroid has a rotation period of 11.0 hours and measures approximately 34 kilometers (21 miles) in diameter. The origin of the asteroid's name remains unknown.[2]

Mechthild 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 central asteroid belt at a distance of 2.2–3.0 AU once every 4 years and 3 months (1,555 days; semi-major axis of 2.63 AU). Its orbit has an eccentricity of 0.15 and an inclination of 5° with respect to the ecliptic.[3] The body's observation arc begins with its first and official discovery observation at Heidelberg Observatory on 21 May 1917.[1]

Naming

This minor planet is named "Mechthild", a German feminine given name. Any reference of this name to a specific person or occurrence is unknown.[2]

Unknown meaning

Among the many thousands of named minor planets, Mechthild is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between 164 Eva and 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.[10]

Physical characteristics

References

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