965 Angelica

965 Angelica (prov. designation: Template:Mp or Template:Mp), is a large background asteroid from the outer regions of the asteroid belt, approximately in diameter. It was discovered on 4 November 1921, by astronomer Johannes F. Hartmann at the La Plata Astronomical Observatory in Argentina. The dark X-type asteroid (Xc) with a low T_Jupiter has a rotation period of 26.8 hours and is likely spherical in shape. It was named after the discoverer's wife, Angelica Hartmann.

Orbit and classification

Angelica 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 outer asteroid belt at a distance of 2.3–4.0 AU once every 5 years and 7 months (2,049 days; semi-major axis of 3.16 AU). Its orbit has an eccentricity of 0.28 and an inclination of 21° with respect to the ecliptic. Due to this relatively high inclination and eccentricity, Angelica has a Jupiter Tisserand's parameter just barely above 3, which is commonly used as the threshold to distinguish between the populations of asteroids and Jupiter-family comets. The body's observation arc begins at Heidelberg Observatory in December 1927, or six years after its official discovery observation at the La Plata Astronomical Observatory.

Naming

This minor planet was named after Angelica Hartmann, wife of German astronomer Johannes F. Hartmann, who discovered this asteroid. The Template:MoMP was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 92).

Physical characteristics

In the Bus–Binzel SMASS classification, Angelica is a Xc subtype, that transitions from the X-types to the carbonaceous C-type asteroids.

Rotation period

During five nights in December 2017, a rotational lightcurve of Angelica was obtained from photometric observations by Tom Polakis at the Command Module Observatory Template:Obscode in Tempe, Arizona. Lightcurve analysis gave a rotation period of hours with a very low brightness variation of magnitude (U=3−), which is indicative of regular, spherical shape.

Another observation from January 2018, by Brigitte Montminy and Katherine McDonald at Minnetonka High School, and Russell Durkee at the Shed of Science Observatory Template:Obscode in Minnetonka, Minnesota, determined a concurring period of hours with an amplitude of magnitude (U=2+). Federico Manzini at the Sozzago Astronomical Station Template:Obscode obtained the object's first lightcurve in December 2006, measuring a period of hours and an amplitude magnitude (U=2).

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), and the Japanese Akari satellite, Angelica measures , and kilometers in diameter, and its surface has an albedo of , and , respectively. Earlier published measurements by the WISE team gives larger mean diameter of and . The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0515 and a diameter of 53.39 km based on an absolute magnitude of 10.2.

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:PAGENAMEBASE at the JPL Small-Body DatabaseTemplate:EditAtWikidata