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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 107 Camilla is one of the largest main-belt asteroids. It orbits within the Cybele Group, beyond most of the main belt asteroids. It has a very dark surface and primitive carbonaceous composition. It was discovered by N. R. Pogson on November 17, 1868, and named after Camilla, Queen of the Volsci in Roman mythology. Lightcurve analysis indicates that Camilla's pole most likely points towards ecliptic coordinates ( , ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.…mehr

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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 107 Camilla is one of the largest main-belt asteroids. It orbits within the Cybele Group, beyond most of the main belt asteroids. It has a very dark surface and primitive carbonaceous composition. It was discovered by N. R. Pogson on November 17, 1868, and named after Camilla, Queen of the Volsci in Roman mythology. Lightcurve analysis indicates that Camilla's pole most likely points towards ecliptic coordinates ( , ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°.