| Minorplanet: | yes |
| 19848 Yeungchuchiu | |
| Background: |
|
| Discovered: | 2 October 2000 |
| Mpc Name: | (19848) Yeungchuchiu |
| Alt Names: | |
| Named After: | Chu Chiu Yeung |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 34.82 yr (12,718 days) |
| Perihelion: | 2.7768 AU |
| Semimajor: | 3.0070 AU |
| Eccentricity: | 0.0766 |
| Period: | 5.21 yr (1,905 days) |
| Mean Motion: | / day |
| Inclination: | 11.061° |
| Asc Node: | 54.759° |
| Arg Peri: | 350.16° |
| Mean Diameter: | 12.90 km km |
| Rotation: | h |
| Albedo: | 0.14 |
| Abs Magnitude: | 12.211.7 |
19848 Yeungchuchiu (provisional designation) is a stony Eos asteroid from the outer region of the asteroid belt, approximately 12km (07miles) in diameter. It was discovered on 2 October 2000 by Canadian amateur astronomer William Yeung at the Desert Beaver Observatory in Arizona, United States. It is the largest object found by the discoverer, just 1°.2 west of Jupiter, who named it after his father, Chu Chiu Yeung.
Yeungchuchiu is a member of the Eos family, an orbital group of more than 4,000 asteroids, which are known for mostly being of stony composition. It orbits the Sun in the outer main-belt at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,905 days). Its orbit has an eccentricity of 0.08 and an inclination of 11° with respect to the ecliptic. The first precovery was taken at the Australian Siding Spring Observatory in 1982, extending the asteroid's observation arc by 18 years prior to its discovery.
This minor planet was named by the discoverer after his father, Chu Chiu Yeung (born 1925), in gratitude for his unconditional support. The approved naming citation was published by the Minor Planet Center on 9 March 2001 .
In November 2005, a rotational lightcurve of Yeungchuchiu was obtained from photometric observations by the discoverer at the Desert Eagle Observatory in Arizona. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of 0.70 magnitude . The large amplitude suggests that the body is of non-spherical shape and that the long axis is almost twice as long as the short axis. It is likely that the rotational axis was almost perpendicular to the observation's line-of-sight. A second lightcurve was obtained at the Palomar Transient Factory in September 2010, and gave a concurring period of hours with an amplitude of 0.63 in magnitude .
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission, the asteroid measures 11.7 and 13.2 kilometers in diameter with an albedo for its surface of 0.17 and 0.21, respectively. The Collaborative Asteroid Lightcurve Link assumes an albedo for stony asteroids of 0.21 and calculates a diameter of 12.9 kilometers with an absolute magnitude of 12.2.