433 Eros - Visibility From Earth

Visibility From Earth

On January 31, 2012, Eros passed the Earth at 0.17867 AU (26,729,000 km; 16,608,000 mi), about 70 times the distance to the Moon, with a visual magnitude of +8.1. During rare oppositions, every 81 years, such as in 1975 and 2056, Eros can reach a magnitude of +7.0, which is brighter than Neptune and brighter than any main-belt asteroid except 4 Vesta and, rarely, 2 Pallas and 7 Iris. Under this condition, the asteroid actually appears to stop, but unlike the normal condition for a body in heliocentric conjunction with the Earth, its retrograde motion is very small. For example, in January and February of 2137, it moves retrograde only 34 minutes in right ascension. Its synodic period of over 846 earth days is among the largest of any body in the Solar System.

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