It has an estimated diameter of roughly 10 kilometers .

It is classified as a primitive, carbon-rich asteroid, a common type in the outer belt that often contains water and organic compounds.

A primary feature of 15008 Miruna is its (2,071 days), which characterizes its movement around the Sun. Key Characteristics

It maintains a semi-major axis of approximately 3.18 AU (astronomical units) from the Sun.

The asteroid was discovered on March 13, 1998 , by the Lowell Observatory Near-Earth-Object Search (LONEOS) at the Anderson Mesa Station.

is a carbonaceous (C-type) background asteroid located in the outer regions of the Main Asteroid Belt .