• Source: 974 Lioba

974 Lioba (prov. designation: A922 FC or 1922 LS) is a stony background asteroid from the central regions of the asteroid belt, approximately 25 kilometers (16 miles) in diameter. It was discovered on 18 March 1922, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southern Germany. The S-type asteroid has a longer than average rotation period of 38.7 hours. It was named after missionary Saint Leoba (Lioba).




Orbit and classification


Lioba 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 2.3–2.8 AU once every 4.04 years (1,474 days; semi-major axis of 2.53 AU). Its orbit has an eccentricity of 0.11 and an inclination of 5° with respect to the ecliptic. The asteroid was first observed as A906 FG (1906 FG) at the Heidelberg Observatory in March 1906, where the body's observation arc begins 16 years later, with its official discovery observation in March 1922.




Naming


This minor planet was named after Saint Leoba (also Lioba) (c. 710–782), abbess in Tauberbischofsheim, Germany, who helped Saint Boniface spreading Christianity throughout Germany. In 782, she was buried near Bonifatius in Fulda, Germany. The author of the Dictionary of Minor Planet Names confirmed the naming from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.




Physical characteristics


In the Tholen classification, Lioba is a common stony S-type asteroid.




= Rotation period

=
In May 1984, a rotational lightcurve of Lioba was obtained from photometric observations by American astronomer Richard Binzel during a survey of 130 asteroids at the University of Texas McDonald Observatory and Cerro Tololo Inter-American Observatory. Lightcurve analysis gave a well-defined, longer-than average rotation period of 38.7 hours with a brightness amplitude of 0.37 magnitude (U=3). In April 2007, a poorly rated period determination by French amateur astronomer René Roy gave 15.6 hours (0.65000 days) or more (U=1).




= Diameter and albedo

=
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's WISE telescope, Lioba measures between 18.39±2.6 and 28.71±0.91 kilometers in diameter and its surface has a high albedo between 0.16 and 0.40. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.3609 from the IRAS results, and calculates a diameter of 18.23 kilometers based on an absolute magnitude of 11.8.




References






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
974 Lioba at AstDyS-2, Asteroids—Dynamic Site
Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
974 Lioba at the JPL Small-Body Database

Kata Kunci Pencarian:

• 974 Lioba
• Lioba
• List of minor planets: 1–1000
• Meanings of minor-planet names: 1–1000
• Karl Wilhelm Reinmuth
• List of named minor planets: L
• List of named minor planets: 1–999
• 973 Aralia
• 975 Perseverantia