With labels describing the surface features: https://www.esa.int/ESA_Multimedia/Images/2025/01/Mercury_s_...
11 comments
With labels describing the surface features: https://www.esa.int/ESA_Multimedia/Images/2025/01/Mercury_s_...
Absolutely love the ESA Like button in the article. Conveys the feeling it's designed by a flight instruments engineer rather than a social media frontend person (make sure to click it twice).
You tricked me
If you refresh the browser the button is unpressed, but when you press it again it gives a stern message about liking twice.
>M-CAM 1 took this long-exposure photograph of Mercury's north pole
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.
If you're thinking that long exposure automatically means something longer than 1 second, it might not mean long exposure to you.
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
Integration implies multiple pictures taken and stacked. This is how we do deep sky astrophotography on our back yards.
Integration over time and integration over bit fields are both ways we do deep sky astrophotography. Integration over time is used to collect more photons without saturating sensor wells and integrating bit fields (stacking) is used to increase signal to noise
I think this is their terminology for exposure time. The sensor is integrating charge from incident photons during this period. Of course the image could be stacked also!
Edit: the sensor is integrating CURRENT. Charge is the integral!
Wondering same. If my math is right, this was a 1/25 sec. exposure. (40/1000)
I would have expected a larger crater for Tolkien..