| Discovery | |
|---|---|
| Discovered by | Paul Götz |
| Discovery site | Heidelberg |
| Discovery date | 28 May 1905 |
| Designations | |
| (566) Stereoskopia | |
| Pronunciation | /ˌstɛrioʊˈskoʊpiə/ |
| 1905 QO | |
| Orbital characteristics [1] | |
| Epoch 31 July 2016 ( JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 1,687.12 d (40,491 h) |
| Aphelion | 3.7804 AU (565.54 Gm) |
| Perihelion | 2.9908 AU (447.42 Gm) |
| 3.3856 AU (506.48 Gm) | |
| Eccentricity | 0.11662 |
| 6.23 yr (2,275.4 d) | |
| 177.298 ° | |
| 0° 9m 29.592s / day | |
| Inclination | 4.8864° |
| 79.644° | |
| 298.527° | |
| Physical characteristics | |
| 84.08±3.15 km | |
| 12.103 h (0.5043 d) [1] | |
| 0.0383±0.003 [1] | |
| 8.0 | |
Stereoskopia ( minor planet designation: 566 Stereoskopia) is a large, outer main-belt asteroid orbiting the Sun. [1] It was discovered on 28 May 1905 from Heidelberg by German astronomer Paul Götz. [2] The discovery was made from photographic plates with the use of a stereo-comparator that had been provided by Carl Pulfrich, a German physicist at the Carl Zeiss Company. [3] The asteroid name is a reference to this device. [2]
This object is a member of the Cybele group located beyond the core of the main belt. [1] It is orbiting at a distance of 3.39 AU with a period of 6.23 yr and an eccentricity of 0.12. The orbital plane is inclined at an angle of 4.9° to the plane of the ecliptic. [1] Light curve analysis based on photometric data collected during 2008 provide a rotation period of 12.103±0.002 h for this asteroid. [4] It spans a girth of approximately 167 km [1] and is classified as a carbonaceous C-type asteroid. [5]
- ^ a b c d e f g "JPL Small-Body Database Browser: 566 Stereoskopia (1905 QO)" (2010-06-24 last obs). Retrieved 7 May 2016.
- ^ a b Schmadel, Lutz (2003), Dictionary of minor planet names, vol. 1, Springer, p. 59, ISBN 9783540002383
- ^ Murdin, Paul (2016), Rock Legends: The Asteroids and Their Discoverers, Springer International Publishing, p. 51, Bibcode: 2016rlat.book.....M, ISBN 9783319318363.
- ^ Fauerbach, Michael; Marks, Scott A. (July 2009), "Lightcurve Analysis of 556 Stereoskopia and 823 Sisigambis", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 36 (3): 96–97, Bibcode: 2009MPBu...36...96F.
- ^ Vilas, F.; McFadden, L. A. (June 1987), "New CCD Reflectance Spectra of Outer Belt Asteroids", Bulletin of the American Astronomical Society, 19: 825, Bibcode: 1987BAAS...19Q.825V
- 566 Stereoskopia at AstDyS-2, Asteroids—Dynamic Site
- 566 Stereoskopia 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. |
| Discovery | |
|---|---|
| Discovered by | Paul Götz |
| Discovery site | Heidelberg |
| Discovery date | 28 May 1905 |
| Designations | |
| (566) Stereoskopia | |
| Pronunciation | /ˌstɛrioʊˈskoʊpiə/ |
| 1905 QO | |
| Orbital characteristics [1] | |
| Epoch 31 July 2016 ( JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 1,687.12 d (40,491 h) |
| Aphelion | 3.7804 AU (565.54 Gm) |
| Perihelion | 2.9908 AU (447.42 Gm) |
| 3.3856 AU (506.48 Gm) | |
| Eccentricity | 0.11662 |
| 6.23 yr (2,275.4 d) | |
| 177.298 ° | |
| 0° 9m 29.592s / day | |
| Inclination | 4.8864° |
| 79.644° | |
| 298.527° | |
| Physical characteristics | |
| 84.08±3.15 km | |
| 12.103 h (0.5043 d) [1] | |
| 0.0383±0.003 [1] | |
| 8.0 | |
Stereoskopia ( minor planet designation: 566 Stereoskopia) is a large, outer main-belt asteroid orbiting the Sun. [1] It was discovered on 28 May 1905 from Heidelberg by German astronomer Paul Götz. [2] The discovery was made from photographic plates with the use of a stereo-comparator that had been provided by Carl Pulfrich, a German physicist at the Carl Zeiss Company. [3] The asteroid name is a reference to this device. [2]
This object is a member of the Cybele group located beyond the core of the main belt. [1] It is orbiting at a distance of 3.39 AU with a period of 6.23 yr and an eccentricity of 0.12. The orbital plane is inclined at an angle of 4.9° to the plane of the ecliptic. [1] Light curve analysis based on photometric data collected during 2008 provide a rotation period of 12.103±0.002 h for this asteroid. [4] It spans a girth of approximately 167 km [1] and is classified as a carbonaceous C-type asteroid. [5]
- ^ a b c d e f g "JPL Small-Body Database Browser: 566 Stereoskopia (1905 QO)" (2010-06-24 last obs). Retrieved 7 May 2016.
- ^ a b Schmadel, Lutz (2003), Dictionary of minor planet names, vol. 1, Springer, p. 59, ISBN 9783540002383
- ^ Murdin, Paul (2016), Rock Legends: The Asteroids and Their Discoverers, Springer International Publishing, p. 51, Bibcode: 2016rlat.book.....M, ISBN 9783319318363.
- ^ Fauerbach, Michael; Marks, Scott A. (July 2009), "Lightcurve Analysis of 556 Stereoskopia and 823 Sisigambis", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 36 (3): 96–97, Bibcode: 2009MPBu...36...96F.
- ^ Vilas, F.; McFadden, L. A. (June 1987), "New CCD Reflectance Spectra of Outer Belt Asteroids", Bulletin of the American Astronomical Society, 19: 825, Bibcode: 1987BAAS...19Q.825V
- 566 Stereoskopia at AstDyS-2, Asteroids—Dynamic Site
- 566 Stereoskopia at the JPL Small-Body Database
|
| This article about an asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |