970 Primula

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970 Primula (prov. designation: Template:Mp or Template:Mp) is a stony background asteroid from the central regions of the asteroid belt, approximately Template:Convert in diameter. It was discovered on 29 November 1921, by astronomer Karl Reinmuth at the Heidelberg Observatory in southern Germany.[1] The S-type asteroid has a short rotation period of 2.8 hours. It was named after the genus of flowering plants, Primula, which are also known as "primroses".[2]

Orbit and classification

Primula is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[3][4] It orbits the Sun in the central asteroid belt at a distance of 1.9–3.3 AU once every 4 years and 1 month (1,496 days; semi-major axis of 2.56 AU). Its orbit has an eccentricity of 0.27 and an inclination of 5° with respect to the ecliptic.[5] The body's observation arc begins with its official discovery observation at Heidelberg observatory in November 1921.[1]

Naming

This minor planet was named after the genus of flowering plants, Primula, also known as "primroses". These perennial herbs belong to the family Primulaceae (primrose family) and have large tufted basal leaves and variously colored flowers. The Template:MoMP was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 93Script error: No such module "Check for unknown parameters".).[2]

Physical characteristics

In the SMASS classification (Bus–Binzel 2000), Primula is a common stony S-type asteroid.[5]

Rotation period

In November 2003, a rotational lightcurve of Primula was obtained from photometric observations by Pedro Sada, Eder Canizales and Edgar Armada using a remotely controlled commercial telescope at Tenagra Observatories Template:Obscode. Lightcurve analysis gave a well-defined, short rotation period of Template:Val hours with a brightness variation of Template:Val magnitude (U=3Script error: No such module "Check for unknown parameters".).[6] Astronomer Maurice Clark at the Preston Gott Observatory confirmed the period in September 2011, measuring Template:Val hours and a somewhat higher amplitude of Template:Val (U=3Script error: No such module "Check for unknown parameters".)[7]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Primula measures Template:Val kilometers in diameter and its surface has an albedo of Template:Val.[8] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 10.30 kilometers based on an absolute magnitude of 12.3.[9]

References

Template:Reflist

External links

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