 Orbital diagram | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 21 March 1893 |
| Designations | |
| (365) Corduba | |
| Pronunciation | /ˈkɔːrdjʊbə/ [1] [2] |
Named after | Possibly Córdoba, Spain [3] |
| 1893 V | |
| Main belt | |
| Orbital characteristics [4] | |
| Epoch 31 July 2016 ( JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 117.96 yr (43084 d) |
| Aphelion | 3.2417 AU (484.95 Gm) |
| Perihelion | 2.36078 AU (353.168 Gm) |
| 2.80122 AU (419.057 Gm) | |
| Eccentricity | 0.15723 |
| 4.69 yr (1712.5 d) | |
| 233.78 ° | |
| 0° 12m 36.792s / day | |
| Inclination | 12.792° |
| 185.196° | |
| 216.45° | |
| Physical characteristics | |
| Dimensions | 105.92±3.0
km
[4] 104.51 ± 2.42 km [5] |
| Mass | (5.84 ± 0.95) × 1018 kg [5] |
Mean
density | 9.76 ± 1.73 g/cm3 [5] |
| 12.705 h (0.5294 d) | |
| 0.0335±0.002 | |
| C | |
| 9.2 | |
Corduba ( minor planet designation: 365 Corduba) is a very large main-belt asteroid that was discovered by the French astronomer Auguste Charlois on 21 March 1893 from Nice. It is classified as a C-type asteroid and is probably composed of carbonaceous material.
Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007 gave a light curve with a period of 6.551 ± 0.002 hours and a brightness variation of 0.05 in magnitude. This differs somewhat from a 2004 study that gave a period of 6.354 hours, but this difference may be explained by the small magnitude variation which tends to increase the randomizing effect of noise in the data. [6]
References
- ^ Walker (1830) A Key to the Classical Pronunciation of Greek, Latin, and Scripture Proper Names
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
- ^ Schmadel, L. (2003:45). Dictionary of minor planet names. Germany: Springer.
- ^ a b Yeomans, Donald K., "365 Corduba", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 11 May 2016.
- ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv: 1203.4336, Bibcode: 2012P&SS...73...98C, doi: 10.1016/j.pss.2012.03.009. See Table 1.
- ^ Warner, Brian D. (June 2008), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory - June - October 2007", The Minor Planet Bulletin, vol. 35, no. 2, pp. 56–60, Bibcode: 2008MPBu...35...56W.
External links
- Lightcurve plot of 365 Corduba, Palmer Divide Observatory, B. D. Warner (2007)
- 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
- 365 Corduba at AstDyS-2, Asteroids—Dynamic Site
- 365 Corduba at the JPL Small-Body Database
_mathilde.jpg){kind=small} | This article about a C-type asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |
|
Orbital diagram | |
| Discovery | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery date | 21 March 1893 |
| Designations | |
| (365) Corduba | |
| Pronunciation | /ˈkɔːrdjʊbə/ [1] [2] |
Named after | Possibly Córdoba, Spain [3] |
| 1893 V | |
| Main belt | |
| Orbital characteristics [4] | |
| Epoch 31 July 2016 ( JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 117.96 yr (43084 d) |
| Aphelion | 3.2417 AU (484.95 Gm) |
| Perihelion | 2.36078 AU (353.168 Gm) |
| 2.80122 AU (419.057 Gm) | |
| Eccentricity | 0.15723 |
| 4.69 yr (1712.5 d) | |
| 233.78 ° | |
| 0° 12m 36.792s / day | |
| Inclination | 12.792° |
| 185.196° | |
| 216.45° | |
| Physical characteristics | |
| Dimensions | 105.92±3.0
km
[4] 104.51 ± 2.42 km [5] |
| Mass | (5.84 ± 0.95) × 1018 kg [5] |
Mean
density | 9.76 ± 1.73 g/cm3 [5] |
| 12.705 h (0.5294 d) | |
| 0.0335±0.002 | |
| C | |
| 9.2 | |
Corduba ( minor planet designation: 365 Corduba) is a very large main-belt asteroid that was discovered by the French astronomer Auguste Charlois on 21 March 1893 from Nice. It is classified as a C-type asteroid and is probably composed of carbonaceous material.
Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado, during 2007 gave a light curve with a period of 6.551 ± 0.002 hours and a brightness variation of 0.05 in magnitude. This differs somewhat from a 2004 study that gave a period of 6.354 hours, but this difference may be explained by the small magnitude variation which tends to increase the randomizing effect of noise in the data. [6]
References
- ^ Walker (1830) A Key to the Classical Pronunciation of Greek, Latin, and Scripture Proper Names
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
- ^ Schmadel, L. (2003:45). Dictionary of minor planet names. Germany: Springer.
- ^ a b Yeomans, Donald K., "365 Corduba", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 11 May 2016.
- ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv: 1203.4336, Bibcode: 2012P&SS...73...98C, doi: 10.1016/j.pss.2012.03.009. See Table 1.
- ^ Warner, Brian D. (June 2008), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory - June - October 2007", The Minor Planet Bulletin, vol. 35, no. 2, pp. 56–60, Bibcode: 2008MPBu...35...56W.
External links
- Lightcurve plot of 365 Corduba, Palmer Divide Observatory, B. D. Warner (2007)
- 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
- 365 Corduba at AstDyS-2, Asteroids—Dynamic Site
- 365 Corduba at the JPL Small-Body Database
|
| This article about a C-type asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |