(7722) Firne ice
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Asteroid (7722) Firneis |
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| Properties of the orbit ( animation ) | |
| Orbit type | Main belt asteroid |
| Major semi-axis | 2.3516 AU |
| eccentricity | 0.0770 |
| Perihelion - aphelion | 2.1705 AU - 2.5326 AU |
| Inclination of the orbit plane | 7.0894 ° |
| Length of the ascending node | 16.2526 ° |
| Argument of the periapsis | 174.8772 ° |
| Sidereal period | 3.61 a |
| Mean orbital velocity | 19.42 km / s |
| Physical Properties | |
| Absolute brightness | 14.0 mag |
| history | |
| Explorer |
Cornelis Johannes van Houten , Ingrid van Houten-Groeneveld , Tom Gehrels |
| Date of discovery | 29th September 1973 |
| Another name | 2240 T-2 , 1997 GV 17 |
| 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. | |
(7722) Firneis is an asteroid of the main belt that was discovered on September 26, 1960 by the Dutch astronomer couple Cornelis Johannes van Houten and Ingrid van Houten-Groeneveld . The discovery happened during the second Trojan survey , during which Tom Gehrels surveyed field plates recorded at the University of Leiden with the 120 cm Oschin Schmidt telescope of the Palomar observatory ( IAU code 675) .
The asteroid was named on February 11, 1998 after the Austrian astronomer and university professor Maria G. Firneis (* 1947), who founded the University Observatory Museum in Vienna and has been giving lectures on astronomy-historical topics at various universities in Austria since 1979 .
See also
Web links
- Asteroid Lepaute: Discovery Circumstances according to the Minor Planet Center of the International Astronomical Union at the Harvard-Smithsonian Center for Astrophysics, Cambridge, USA
- Asteroid Lepaute in the Small-Body Database of NASA's Jet Propulsion Laboratory at the California Institute of Technology, Pasadena, USA
- (7722) Firneis in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).