| Minorplanet: | yes |
| 970 Primula | |
| Background: |
|
| Discovery Ref: |   |
| Discovered: | 29 November 1921 |
| Mpc Name: | (970) Primula |
| Alt Names: | A921 WK1929 RN 1966 TG1921 LB |
| Named After: | Primula  |
| Mp Category: | background  |
| Orbit Ref: |   |
| Epoch: | 31 May 2020 (JD 2459000.5) |
| Uncertainty: | 0 |
| Observation Arc: | 98.11 yr (35,834 d) |
| Perihelion: | 1.8644 AU |
| Semimajor: | 2.5598 AU |
| Eccentricity: | 0.2717 |
| Period: | 4.10 yr (1,496 d) |
| Mean Motion: | / day |
| Inclination: | 5.0331° |
| Asc Node: | 310.77° |
| Arg Peri: | 95.564° |
| Spectral Type: | SMASS S  |
| Abs Magnitude: | 12.3 |
970 Primula (prov. designation: or) is a stony background asteroid from the central regions of the asteroid belt, approximately 9.2km (05.7miles) in diameter. It was discovered on 29 November 1921, by astronomer Karl Reinmuth at the Heidelberg Observatory in southern Germany. The S-type asteroid has a short rotation period of 2.8 hours. It was named after the genus of flowering plants, Primula, which are also known as "primroses".
Primula 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 central asteroid belt at a distance of 1.9–3.3 AU once every 4 years and 1 month (1,496 days; semi-major axis of 2.56 AU). Its orbit has an eccentricity of 0.27 and an inclination of 5° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Heidelberg observatory in November 1921.
This minor planet was named after the genus of flowering plants, Primula, also known as "primroses". These perennial herbs belong to the family Primulaceae (primrose family) and have large tufted basal leaves and variously colored flowers. The was mentioned in The Names of the Minor Planets by Paul Herget in 1955 .
In the SMASS classification (Bus–Binzel 2000), Primula is a common stony S-type asteroid.
In November 2003, a rotational lightcurve of Primula was obtained from photometric observations by Pedro Sada, Eder Canizales and Edgar Armada using a remotely controlled commercial telescope at Tenagra Observatories . Lightcurve analysis gave a well-defined, short rotation period of hours with a brightness variation of magnitude . Astronomer Maurice Clark at the Preston Gott Observatory confirmed the period in September 2011, measuring hours and a somewhat higher amplitude of
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Primula measures kilometers in diameter and its surface has an albedo of . The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 10.30 kilometers based on an absolute magnitude of 12.3.