740 Cantabia
| Discovery | |
|---|---|
| Discovered by | Joel Hastings Metcalf |
| Discovery site | Winchester, Massachusetts |
| Discovery date | 10 February 1913 |
| Designations | |
| (740) Cantabia | |
| Pronunciation | /kænˈteɪbiə/[1] |
| 1913 QS | |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 103.10 yr (37,659 d) |
| Aphelion | 3.3892 AU (507.02 Gm) |
| Perihelion | 2.7145 AU (406.08 Gm) |
| 3.0519 AU (456.56 Gm) | |
| Eccentricity | 0.11053 |
| 5.33 yr (1,947.4 d) | |
| 133.938° | |
| 0° 11m 5.532s / day | |
| Inclination | 10.846° |
| 116.099° | |
| 47.844° | |
| Physical characteristics | |
| 45.45±0.85 km | |
| 64.453 h (2.6855 d) | |
| 0.0552±0.002 | |
| 9.1 | |
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 3.05 AU with a period of 5.33 years and an eccentricity (ovalness) of 0.11.[2] Between 2014 and 2021, 740 Cantabia has been observed to occult three stars.[citation needed]
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 64.453 hours (2.69 days) with a brightness variation of 0.16±0.03 in magnitude.[3] The spectrum is classified as type CX in the Tholen taxonomy.[4] It spans a girth estimated at ~91 km.[2]
See also
[edit]References
[edit]- ^ Per 'Cantabria' in Noah Webster (1884) A Practical Dictionary of the English Language
- ^ a b c "740 Cantabia (1913 QS)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
- ^ Stephens, Robert D.; et al. (January 2010), "Lightcurve Analysis of 740 Cantabia", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 37 (1): 17, Bibcode:2010MPBu...37...17S.
- ^ Lazzaro, D.; et al. (November 2004), "S3OS2: the visible spectroscopic survey of 820 asteroids", Icarus, 172 (1): 179–220, Bibcode:2004Icar..172..179L, doi:10.1016/j.icarus.2004.06.006.
External links
[edit]- Lightcurve plot of 740 Cantabia, Palmer Divide Observatory, B. D. Warner (2009)
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 740 Cantabia at AstDyS-2, Asteroids—Dynamic Site
- 740 Cantabia at the JPL Small-Body Database
_mathilde.jpg){kind=small} | This article about an asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |