| Minorplanet: | yes |
| 4786 Tatiana | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 13 August 1985 |
| Mpc Name: | (4786) Tatianina |
| Alt Names: | 1948 GA 1970 KF |
| Named After: | Tatiana Somova  |
| Mp Category: | main-belt  background  |
| Orbit Ref: |   |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 47.10 yr (17,202 d) |
| Perihelion: | 1.9011 AU |
| Semimajor: | 2.3578 AU |
| Eccentricity: | 0.1937 |
| Period: | 3.62 yr (1,322 d) |
| Mean Motion: | / day |
| Inclination: | 7.2560° |
| Asc Node: | 115.77° |
| Arg Peri: | 118.27° |
| Mean Diameter: | 3.48 km |
| Rotation: | |
| Albedo: | |
| Spectral Type: | SMASS Xc E  |
| Abs Magnitude: | 13.3 13.76 |
4786 Tatianina, provisional designation, is a bright background asteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 3.4km (02.1miles) in diameter. It was discovered on 13 August 1985, by Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. It was named after Tatiana Somova, a friend of the discoverer. The E-/Xc-subtype has a short rotation period of 2.9 hours. Its sub-kilometer minor-planet moon was discovered on 20 March 2006 and announced the following month.
Tatianina 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 1.9–2.8 AU once every 3 years and 7 months (1,322 days; semi-major axis of 2.36 AU). Its orbit has an eccentricity of 0.19 and an inclination of 7° with respect to the ecliptic.
The asteroid was first observed as at the Algiers Observatory in April 1948. The body's observation arc begins at Nauchnij in May 1970 as, more than 15 years prior to its official discovery observation.
In the SMASS classification, Tatianina is a Xc-subtype that transitions from the X-type to the carbonaceous C-type asteroids. It has also been characterized as a bright E-type by the Wide-field Infrared Survey Explorer (WISE).
Several rotational lightcurves of Tatianina have been obtained from photometric observations since 2003 . Analysis of the best-rated lightcurve from March 2003, during which a satellite was also discovered (see below), gave a rotation period of 2.9227 hours with a brightness amplitude of 0.19 and 0.20 magnitude .
According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Tatianina measures between 3.282 and 3.475 kilometers in diameter and its surface has an exceptionally high albedo of 0.4763 to 0.514. The Collaborative Asteroid Lightcurve Link adopts the revised WISE-data by Petr Pravec, that is an albedo of 0.4763 and rounded diameter of 3.48 kilometers based on an absolute magnitude of 13.718.
During the photometric observations by Donald Pray, Petr Pravec and collaborators in March 2006, it was revealed that Tatianina is a synchronous binary asteroid with a minor-planet moon orbiting it every 21.67 hours at an estimated average distance of . The discovery was announced on 11 April 2006. The mutual occultation events suggest the presence of a satellite with an estimated diameter of meters or 19% the size of its primary.
This minor planet was numbered on 28 April 1991. It was named by the discoverer after Tatiana Aleksandrovna Somova, a nursery-school teacher in Saint Petersburg, Russia. The official naming citation was published by the Minor Planet Center on 5 March 1996 .