Physical Characteristics
Angelina is an uncommon form of E-type asteroid; it is the third largest E-type after 44 Nysa and 55 Pandora, and has an exceptionally high albedo. As of 1991, it is thought to have an average radius of about 30 kilometers (19 mi). Back when asteroids were generally assumed to have low albedos, Angelina was thought to be the largest of this class, but modern research has shown that its diameter is only a quarter of what was previously assumed, an error caused by its exceptional brightness. Traditional calculations had suggested that since Angelina has an absolute magnitude of 7.7 and an albedo of 0.15, its diameter would have been around 100 km. However, a 2004 occultation showed a cross-sectional profile of only 48x53 km. Angelina was observed by Arecibo radar in January 2010.
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