Feralia Planitia

[5][6] The feature was then named after the ancient Roman public festival of Feralia, where citizens would place offerings at the tombs of the dead.

[7]: 91 [2]: 116  The surrounding cratered highlands likely represent ejecta blasted out by the impact event(s) that created Feralia Planitia.

[2]: 116–118  However, a precise date for Feralia Planitia's formation cannot be determined through crater counting, as the basin underwent a resurfacing event roughly 3.62 billion years ago.

[7]: 99  Feralia Planitia's surface is partially composed of eucrites, a type of basaltic rock containing anorthite, calcium-poor pyroxene, and augite.

This is in contrast to the older northern and northeastern highlands, whose mineralogy is dominated by howardite, a mixture of eucrite and diogenite.

Feralia Planitia (green, top) is large enough to be visible from Earth, here as seen in a model of Vesta constructed from Hubble Space Telescope images taken in May 1996. The much larger crater at the bottom is Rheasilvia
An image of the Lepida Quadrangle on Vesta, including the far northwestern corner of Feralia Planitia. Lepida is located at right, whilst Vestalia Terra is located at lower left