4 Vesta

573 kmmaximum extent

Updated

573km
Visual creditDawn 2011 / NASA / JPL / MPS / DLR / IDA / Björn Jónsson / Public domainSource: Wikimedia Commons

Details

Vesta is one of the largest bodies in the asteroid belt and was mapped in detail by NASA's Dawn spacecraft. Unlike most asteroids, it separated into crust, mantle, and core early in Solar System history, making it a surviving protoplanetary world rather than a simple leftover rock.

Vesta formed early enough for heat from short-lived radioactive elements to separate it into a basaltic crust, rocky mantle and metal-rich core—differentiation more often associated with planets than with small asteroids. NASA estimates that this happened within the first one or two million years of Solar System history.

Dawn mapped Vesta’s gravity, minerals and giant south-polar Rheasilvia basin. Those measurements strengthened the link between Vesta and the howardite–eucrite–diogenite meteorites found on Earth, allowing laboratory samples and spacecraft observations to describe the same differentiated body.

Key facts

Category
Asteroids
Object class
Protoplanetary asteroid
Mass
~257 quadrillion metric tons
Scale fact
573 kmmaximum extent
Estimated age
~4.56 billion years
Composition
Basaltic crust, rocky mantle, nickel-iron core
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Size neighbors

Objects near 4 Vesta on the scale

On the logarithmic size axis, 4 Vesta falls between Enceladus and Ceres. The band uses nearby Asteroids records.

Shared physical scale
438km

Sources

References for 4 Vesta

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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