| Minorplanet: | yes |
| Background: |
|
| 740 Cantabia | |
| Mpc Name: | (740) Cantabia |
| Alt Names: | 1913 QS |
| Pronounced: | [1] |
| Discovered: | 10 February 1913 |
| Epoch: | 31 July 2016 (JD 2457600.5) |
| Eccentricity: | 0.11053 |
| Semimajor: | 3.0519AU |
| Perihelion: | 2.7145AU |
| Aphelion: | 3.3892abbr=onNaNabbr=on |
| Period: | 1947.4days |
| Inclination: | 10.846° |
| Asc Node: | 116.099° |
| Arg Peri: | 47.844° |
| Mean Motion: | / day |
| Observation Arc: | 37659days |
| Uncertainty: | 0 |
| Abs Magnitude: | 9.1 |
| Rotation: | 64.453abbr=onNaNabbr=on |
| Mean Radius: | km |
740 Cantabia is a minor planet orbiting the Sun. It was discovered on 10 February 1913 at Winchester, Massachusetts by American amateur astronomer J. H. Metcalf. Cantabia is a contraction of Cantabrigia, Latin for Cambridge, named in honor of Cambridge, Massachusetts. It is orbiting at a distance of with a period of 1947.4days and an eccentricity (ovalness) of 0.11. Between 2014 and 2021, 740 Cantabia has been observed to occult three stars.
This asteroid shows an exceptionally slow rate of spin. Photometry observations from two independent teams during 2009 were combined to generate a light curve showing a rotation period of 64.4532NaN2 with a brightness variation of in magnitude. The spectrum is classified as type CX in the Tholen taxonomy. It spans a girth estimated at ~91 km.