862 Franzia

862 Franzia (prov. designation: Template:Mp or Template:Mp) is a stony background asteroid from the central regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 28 January 1917. The common S-type asteroid has a rotation period of 7.5 hours and measures approximately in diameter. It was named after the discoverer's son, Franz Wolf.

Orbit and classification

Franzia 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 central asteroid belt at a distance of 2.6–3.0 AU once every 4 years and 8 months (1,715 days; semi-major axis of 2.8 AU). Its orbit has an eccentricity of 0.08 and an inclination of 14° with respect to the ecliptic. The body's observation arc begins with one of its first observations as Template:Mp at Heidelberg Observatory on 22 January 1903, or 14 years prior to its official discovery observation.

Naming

This minor planet was named in honor of Franz Wolf, son of the discoverer Max Wolf. The Template:MoMP was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 84). It also honors the discoverer's father, Franz Wolf, a physician and amateur astronomer who fostered his son's interest in astronomy by setting up a small observatory in the backyard when Max was sixteen.

Physical characteristics

In the Bus–Binzel SMASS classification, Franzia is a common, stony S-type asteroid.

Rotation period

Over the last two decades, numerous photometric observations of Franzia have been proven challenging to determine a well defined rotation period. In August 2018, a rotational lightcurve was obtained from observations by Christophe Demeautis and Raoul Behrend. Lightcurve analysis gave a period of hours with a brightness variation of magnitude (U=3−). This result supersedes previous observations.

Based on observations taken in September 2004, Brian Warner at his Palmer Divide Observatory Template:Obscode, Colorado, published an ambiguous period of and hours with an amplitude of and magnitude, respectively, depending on whether the period solution is derived from a monomodal or from a bimodal lightcurve (U=2/2). Alternatively, Warner also gave a revised period of hours and an amplitude of magnitude for his other observation taken in December 2000.Template:Efn

In February 2011, James W. Brinsfield at the Via Capote Observatory Template:Obscode in California measured a period of hours with an amplitude of magnitude (U=2). Observations by Nicolas Esseiva and Raoul Behrend in December 2014 gave a tentative period of hours and a weak amplitude of magnitude (U=2). A basically identical period of hours with a brightness variation of magnitude was determined by French amateur astronomer René Roy in February 2011 (U=2−). In March 2016, the Spanish group of asteroid observers, OBAS, measures a period of hours with an amplitude of magnitude (U=2).

Diameter and albedo

According to the surveys carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the Infrared Astronomical Satellite IRAS, and the Japanese Akari satellite, Franzia measures (), () and () kilometers in diameter and its surface has an albedo of (), () and (), respectively. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2700 and a diameter of 28.05 kilometers based on an absolute magnitude of 9.8.

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