Note: Mariner 10 (1974-75) imaged only one hemisphere of Mercury.

1st flyby (January 2008)
2nd flyby (October 2008)
By October 2008, Messenger had flown past Mercury 2 times on its way to being
the first spacecraft to orbit the planet by 2011.
A large part of the previously un-imaged surface has already been revealed.

Mariner 10 image
Messenger image

Mariner 10 image
Messenger image

Mariner 10 image
Messenger image
Smooth bottomed craters, flood basalts (lava) filled after impacts.
Other evidence for internal tectonic forces acting after the initial high
impact rate subsided include many high cliffs formed by contraction of
the planet as it cooled. Note the long scarp (cliff face) cutting
through the right of the Messenger image. (Images are not the same scale.)
Caloris Basin (ringed impact basin), Mariner 10 image (Caloris Basin not
yet imaged by Messenger).


Craters on Mercury (left-Mariner 10, middle-Messenger) and the Moon (right-HST) compared.