(1826) Miller
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Asteroid (1826) Miller |
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|---|---|
| Properties of the orbit ( animation ) | |
| Orbit type | Main belt asteroid |
| Asteroid family | Eos family |
| Major semi-axis | 2.995 AU |
| eccentricity | 0.0819 |
| Perihelion - aphelion | 2.750 AU - 3.241 AU |
| Inclination of the orbit plane | 9.232 ° |
| Sidereal period | 5.18 a |
| Mean orbital velocity | 17.20 km / s |
| Physical Properties | |
| Medium diameter | 24.41 km |
| Dimensions | ? kg |
| Albedo | 0.1294 |
| Medium density | ? g / cm³ |
| Rotation period | ~ 6,776 h |
| Absolute brightness | 10.90 likes |
| Spectral class | ? |
| history | |
| Explorer | Indiana Asteroid Program |
| Date of discovery | September 14, 1955 |
| Another name | 1955 RC, 1929 RV, 1940 WF, 1950 TD, 1952 BL |
| Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items. | |
(1826) Miller (provisional name 1955 RC ) is an asteroid that was discovered in the Goethe Link Observatory near Brooklyn, Indiana as part of the Indiana Asteroid Program . It was discovered on September 14, 1955, but was later found to be the same object as 1929 RV , 1940 WF , 1950 TD, and 1952 BL , which were sighted before the official discovery.
(1826) Miller is an asteroid of the outer main belt and has an average diameter of 15 miles. Differences in light reflected from the asteroid suggest that the period of rotation is approximately 6 hours and 46 minutes, but this is an assumption with great uncertainty.
The asteroid was involved in an occultation of a star of size 10 in the constellation Cancer in April 2004 .
swell
- (1826) Miller in the Small-Body Database of the Jet Propulsion Laboratory (English).
Individual evidence
- ↑ ipa.nw.ru: Table of Minor planet lightcurve parameters , accessed on March 12, 2011
- ↑ netstevepr.com: Apr 2004 Asteroid Occultation Path Predictions. Archived from the original on December 2, 2008 ; accessed on March 15, 2011 (English).