The left-hand image is a Dawn FC (framing camera) brightness image, which shows the brightness/ darkness of Vesta’s surface. The right-hand image is based on this brightness image.
Image Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA
This Dawn FC (framing camera) image shows the sun illuminating the landscape of Vesta during a Vestan ‘sunrise’. When this image was obtained the sun had a low angle relative to Vesta’s surface, just as the sun has a low angle in the sky in the morning on Earth.
Image Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA
This Dawn FC (framing camera) image shows impact ejecta deposits dominating Vesta’s landscape. This impact ejecta material was ejected from an impact crater located outside the imaged area.
Image Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA
This Dawn FC (framing camera) image shows two overlapping impact craters. The large crater is roughly 20 kilometers (12 miles) in diameter and the smaller crater is roughly 6 kilometers (4 miles) in diameter.
Image Credit: NASA/ JPL-Caltech/ UCLA/ MPS/ DLR/ IDA
This mosaic shows the location of the data acquired by VIR (visible and infrared spectrometer) during the HAMO (high-altitude mapping orbit) phase of the Dawn mission.