| Minorplanet: | yes |
| 4789 Sprattia | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 20 October 1987 |
| Mpc Name: | (4789) Sprattia |
| Named After: | |
| Mp Category: | main-belt  background  |
| Orbit Ref: |   |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 41.82 yr (15,276 d) |
| Perihelion: | 1.9596 AU |
| Semimajor: | 2.2386 AU |
| Eccentricity: | 0.1246 |
| Period: | 3.35 yr (1,223 d) |
| Mean Motion: | / day |
| Inclination: | 1.2760° |
| Asc Node: | 209.73° |
| Arg Peri: | 152.92° |
| Mean Diameter: | 4.22 km |
| Albedo: | |
| Abs Magnitude: | 13.80 13.9 14.24 |
4789 Sprattia, provisional designation, is a stony background asteroid from the inner regions of the asteroid belt, approximately 4km (02miles) in diameter. It was discovered on 20 October 1987, by Canadian astronomer David Balam at the Climenhaga Observatory in Victoria, Canada. The S-type asteroid has a rotation period of 3.1 hours and was named after Canadian amateur astronomer Christopher E. Spratt.
Sprattia is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner asteroid belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,223 days; semi-major axis of 2.24 AU). Its orbit has an eccentricity of 0.12 and an inclination of 1° with respect to the ecliptic. The body's observation arc begins with its first observation as at the Félix Aguilar Observatory in April 1976, more than 11 years prior to its official discovery observation at Victoria.
Sprattia has been characterized as a common, stony S-type asteroid by Pan-STARRS and the Sloan Digital Sky Survey.
In December 2011, a rotational lightcurve of Sprattia was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 3.136 hours with a brightness amplitude of 0.17 magnitude .
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Sprattia measures between 3.54 and 4.172 kilometers in diameter and its surface has an albedo between 0.28 and 0.44.
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20, and calculates a diameter of 4.22 kilometers based on an absolute magnitude of 14.24.
This minor planet was named after Canadian amateur astronomer Christopher E. Spratt (born 1942), a long-time member of the Royal Astronomical Society of Canada, whose interests involve comets, minor planets, meteors and variable stars. The official naming citation was published by the Minor Planet Center on 27 June 1991 .