description 31 Euphrosyne Overview
31 Euphrosyne is a large, dark, carbonaceous asteroid orbiting in the outer region of the main asteroid belt. It was discovered in 1854 by American astronomer James Ferguson and named after Euphrosyne, a figure from Greek mythology representing joy or mirth. As a C-type asteroid, its surface is highly primitive and reflects very little sunlight, making it one of the darkest large bodies in the solar system. It also serves as the namesake for the Euphrosyne family of asteroids, which share a similar orbital path and composition.
help 31 Euphrosyne FAQ
Where is 31 Euphrosyne located?
31 Euphrosyne is in the outer region of the main asteroid belt, beyond the central belt population closer to Mars. Its dark surface makes it difficult to observe compared with brighter rocky asteroids.
Who discovered 31 Euphrosyne?
American astronomer James Ferguson discovered it in 1854. It was later named after Euphrosyne, a figure from Greek mythology associated with joy and mirth.
What type of asteroid is 31 Euphrosyne?
It is classified as a dark, carbonaceous C-type asteroid. Its low reflectivity and carbon-rich composition are typical of primitive outer-belt bodies.
Why is 31 Euphrosyne scientifically interesting?
Its large size and dark composition make it an important representative of the outer main belt. The Euphrosyne family also includes numerous smaller bodies believed to be related through a past collisional event.
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