The second-largest body in the Main Belt and the only protoplanet whose surface rocks have fallen to Earth as HED meteorites.
Its Rheasilvia impact basin holds one of the tallest mountains in the solar system (~22 km).

The brightest asteroid in the sky — at its best it skirts naked-eye visibility from a dark rural site, and is an easy binocular target anywhere.
Vesta is a 525-km differentiated protoplanet — a survivor from the first few million years of the solar system, with an iron–nickel core, a rocky mantle and a basaltic crust. It is less a typical asteroid than a tiny planet that never finished forming.
Its south pole is dominated by Rheasilvia, a ~500-km impact basin whose central peak rises ~20–22 km — among the tallest mountains in the solar system. The giant impact that carved it flung out the 'Vestoid' family of fragments.
Discovered on 29 March 1807 by Heinrich Olbers — the fourth asteroid ever found — and named by Carl Friedrich Gauss for Vesta, the Roman goddess of the hearth.
NASA's Dawn orbited Vesta from July 2011 to September 2012, mapping it from as close as 210 km and confirming it as a differentiated protoplanet and the parent body of the HED meteorites.
Sources: NASA — Dawn at Vesta · in-the-sky.org — Vesta 2026