![]() Orbital diagram | |
Discovery | |
---|---|
Discovered by | Auguste Charlois |
Discovery date | 8 March 1893 |
Designations | |
(358) Apollonia | |
Pronunciation | /æpəˈloʊniə/ [1] [2] |
Named after | Possibly Apollonia (Illyria) [3] |
1893 K | |
Main belt | |
Orbital characteristics [4] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 118.08 yr (43129 d) |
Aphelion | 3.31497 AU (495.912 Gm) |
Perihelion | 2.43597 AU (364.416 Gm) |
2.87547 AU (430.164 Gm) | |
Eccentricity | 0.15284 |
4.88 yr (1781.0 d) | |
179.300° | |
0° 12m 7.682s / day | |
Inclination | 3.55411° |
172.161° | |
253.343° | |
Physical characteristics | |
Dimensions | 89.45±2.7 km |
50.6 h (2.11 d) | |
0.0506±0.003 | |
9.1 | |
Apolonia (minor planet designation: 358 Apolonia) is a large Main belt asteroid. [4] It was discovered by Auguste Charlois on 8 March 1893 in Nice.
Pierretta is a 46 km main-belt asteroid discovered on 28 Aug 1891 by Auguste Charlois at Nice.
Rosalia is a large Main belt asteroid. It was discovered by Auguste Charlois on 1 September 1891 in Nice.
353 Ruperto-Carola is a background asteroid from the central region of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg Observatory on 16 January 1893. It is named after the Ruprecht Karls University, whose Latin name is Ruperto Carola Heidelbergensis.
Gabriella is a typical Main belt asteroid.
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Bohemia is a sizeable Main belt asteroid. It was discovered by Auguste Charlois on 16 July 1893 in Nice.
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Burgundia is a typical main belt asteroid that was discovered by Auguste Charlois on 18 September 1893 in Nice. It was named for the former French region of Burgundy. It is one of seven of Charlois's discoveries that was expressly named by the Astromomisches Rechen-Institut.
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662 Newtonia is a minor planet orbiting the Sun.
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875 Nymphe is a minor planet orbiting the Sun. It is a member of the Maria family of asteroids.
829 Academia is a minor planet orbiting the Sun. The asteroid is roughly 44 km in diameter and has a low albedo. Photometric measurements of the asteroid made in 2005 at the Palmer Divide Observatory showed a light curve with a period of 7.891 ± 0.005 hours and a brightness variation of 0.44 ± 0.02 in magnitude.