1125 China

Orbit and classification

China 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 2.4–3.8 AU once every 5 years and 6 months (2,019 days; semi-major axis of 3.13 AU). Its orbit has an eccentricity of 0.22 and an inclination of 3° with respect to the ecliptic. The asteroid was first observed as at Heidelberg Observatory in January 1909, where the body's observation arc begins three week later in February 1909, or more than 48 years prior to its official discovery observation at Nanking, China.

Naming

This minor planet was named after People's Republic of China where the asteroid was discovered. The official naming citation was published by the Minor Planet Center on 31 May 1988 (M.P.C. 13179).

Accidentally usurped designation

Main article: 3789 Zhongguo

While studying in Chicago in 1928, Zhang Yuzhe discovered an asteroid that was given the provisional designation , and later the number 1125. He named it "China" or "中華" (Zhōnghuá). However, this asteroid was not observed beyond its initial appearance and a precise orbit could not be calculated. In 1957, the Purple Mountain Observatory in China discovered a new asteroid, and with Zhang Yuzhe's agreement the new object was reassigned the official designation 1125 China in place of the lost . However, in 1986, the newly discovered object was confirmed to be a rediscovery of the original , and this object was named 3789 Zhongguo. Zhongguo is the Chinese word for China.

Physical characteristics

China is an assumed carbonaceous C-type asteroid.

Rotation period and poles

In February 2009, a rotational lightcurve of China was obtained from photometric observations by Kenneth T. Menzies at the Tigh Speuran Observatory in Massachusetts, United States. Lightcurve analysis gave a well-defined rotation period of 5.367 hours with a brightness variation of 0.38 magnitude (). In October 2013, Robert Stephens measured a similar period of 5.45 hours and an amplitude of 0.62 magnitude at the Center for Solar System Studies in California ().

Published in 2016, an additional lightcurve was modeled from photometric data obtained by a large international collaboration of astronomers. Modelling gave a concurring sidereal rotation period of hours, as well as two spin axes of (132.0°, −46.0°) and (305.0°, −49.0°) in ecliptic coordinates.

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, China measures between 21.86 and 30.49 kilometers in diameter and its surface has an albedo between 0.057 and 0.0860.

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 26.64 kilometers based on an absolute magnitude of 11.6.

Notes

References