
About Vesta
Vesta is the second-largest asteroid in the main belt and a protoplanet: it grew large enough to differentiate into core, mantle, and crust before the formation of Jupiter truncated its growth. NASA’s Dawn spacecraft orbited Vesta from July 2011 to September 2012. Its surface features the Rheasilvia impact basin — 500 km across and 19 km deep in the south polar region — whose ejecta have been traced on Earth as the HED (howardite-eucrite-diogenite) meteorite class.
Physical Properties
Orbit
Gallery
Hand-picked mission imagery of Vesta sourced from NASA and partner archives. Click any photo for full resolution and source attribution.
Imagery on this page is provided by the original mission teams. Full attribution terms: Image Rights & Credits.
Sources & Further Reading
- NASA — official mission / factsheet page
- Wikipedia — extensive cross-referenced article
- NASA Dawn Mission
Numerical values (radius, mass, orbital elements, temperatures) are drawn from NASA NSSDC Planetary Fact Sheets, JPL Horizons, and the JPL Small-Body Database. Last refreshed: 2026-06-08 01:37:02.