| Minorplanet: | yes |
| 5026 Martes | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 22 August 1987 |
| Mpc Name: | (5026) Martes |
| Alt Names: | 1965 QE 1976 QL |
| Named After: | pine marten beech marten |
| Mp Category: | main-belt  |
| Orbit Ref: |   |
| Epoch: | 4 September 2017 (JD 2458000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 63.37 yr (23,145 days) |
| Perihelion: | 1.8020 AU |
| Semimajor: | 2.3780 AU |
| Eccentricity: | 0.2422 |
| Period: | 3.67 yr (1,339 days) |
| Mean Motion: | / day |
| Inclination: | 4.2831° |
| Asc Node: | 304.77° |
| Arg Peri: | 17.652° |
| Mean Diameter: | 4.93 km km |
| Albedo: | 0.20 |
| Spectral Type: | B–V = V–R = C S  |
| Abs Magnitude: | 13.8013.9 |
5026 Martes (prov. designation:) is a carbonaceous asteroid from the inner region of the asteroid belt, approximately 9km (06miles) in diameter. It was discovered on 22 August 1987, by Czech astronomer Antonín Mrkos at Kleť Observatory in the Czech Republic. It is named after the two weasel-like animal species: pine marten and beech marten.
Martes is the namesake member of a small asteroid family, named the Martes family. It orbits the Sun in the inner main-belt at a distance of 1.8–3.0 AU once every 3 years and 8 months (1,339 days). Its orbit has an eccentricity of 0.24 and an inclination of 4° with respect to the ecliptic.
A first precovery was taken at Palomar Observatory in 1953, extending the body's observation arc by 34 years prior to its official discovery observation at Klet.
This minor planet was named for the two species of the family Mustelidae, the pine marten and beech marten. They also live in the forests near the discovering Kleť Observatory. The official naming citation was published by the Minor Planet Center on 22 June 1999 .
Martes has been characterized as a carbonaceous C-type asteroid by PanSTARRS photometric survey.
Martes forms an asteroid pair with, and was part of the 35 sample asteroid pairs in Petr Pravec's study Formation of asteroid pairs by rotational fission, published in the journal Nature.
Between 2008 and 2010, several rotational lightcurves of Martes were obtained from photometric observations. Lightcurve analysis gave a well-defined rotation period of 4.4243 hours with a brightness amplitude of 0.69 magnitude .
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Martes measures 8.967 kilometers in diameter and its surface has an albedo of 0.066, which is typical for carbonaceous asteroids. The Collaborative Asteroid Lightcurve Link, however, assumes a standard albedo for stony asteroids of 0.20 and consequently calculates a much smaller diameter of 4.93 kilometers, due to the higher albedo.