I'm curious how this works. The dynamic range between the sunlit parts and the dark portions must be huge at that distance from the Sun. Anyone have the technical details on the camera or post processing they use to achieve this? Is it really a long exposure or is it a series of photos at different exposures stitched together?
Edit: details at the bottom seem to imply a single photo, but that "long exposure" really isn't that long
>This image of Mercury's surface was taken by M-CAM 1 [...] using an integration time of 40 milliseconds.
Edit: the sensor is integrating CURRENT. Charge is the integral!
I'd guess this is a fixed aperture system where the main way to control the exposure is with shutter speed. But for images taken in bright sunlight, you can use shutter speeds 1/250, 1/1000, 1/2000, or even higher type numbers. In those terms, 40 milliseconds is 10 times slower/longer than 1/250.
So for the M-CAM 1 system, 40 milliseconds could be an extremely long exposure