960 Birgit

960 Birgit (prov. designation: Template:Mp or Template:Mp) is a background asteroid, approximately Template:Convert in diameter, located in the Florian region of the inner asteroid belt. It was discovered on 1 October 1921, by astronomer Karl Reinmuth at the Heidelberg Observatory in southern Germany. The possibly S-type asteroid has a rotation period of 8.9 hours. It was named after Birgit Asplind, daughter of Swedish astronomer Bror Asplind (1890–1954).

Orbit and classification

Located in the Florian region, Birgit is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,232 days; semi-major axis of 2.25 AU). Its orbit has an eccentricity of 0.17 and an inclination of 3° with respect to the ecliptic. The body's observation arc begins at Heidelberg on 25 October 1925, three weeks after its official discovery observation.

Naming

This minor planet was named after Birgit Asplind, daughter of Swedish astronomer Bror Ansgar Asplind (1890–1954). Asteroids 958 Asplinda, 959 Arne and 961 Gunnie are named after him and his other two children, respectively. The Template:MoMP was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 92).

Physical characteristics

Based on its determined albedo, Birgit is an assumed S-type asteroid. The albedo determined by the Wide-field Infrared Survey Explorer (WISE) for this asteroid agrees with that assumption (see below).

Rotation period

In February 2007, a rotational lightcurve of Birgit was obtained from photometric observations by Agnieszka Kryszczyńska at Poznań Observatory, Poland, and international collaborators. Lightcurve analysis gave a rotation period of Template:Val hours with a brightness variation of Template:Val magnitude (U=2+).Template:Efn The result supersedes observations by Federico Manzini, Roberto Crippa, and Pierre Antonini from August 2005, who determined a poorly rated period of Template:Val hours with an amplitude of Template:Val magnitude (U=1+).

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Birgit measures Template:Val kilometers in diameter and its surface has an albedo of Template:Val. Another published measurement by the WISE team gives a mean diameter of Template:Val with an albedo of Template:Val. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 9.40 kilometers based on an absolute magnitude of 12.5.

External links

• Lightcurve Database Query (LCDB), at www.minorplanet.info
• Dictionary of Minor Planet Names, Google books
• Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
• Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
• Template:AstDys
• Template:JPL small body