(no title)
hajola
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1 year ago
Figuring out the optimal placement of CCDs on Plato's 24(+2) cameras. Due to the way CCDs are fabricated, their properties vary a bit, they are not identical. For example, they can vary how much light they can hold before they become saturated. Given the high cost of fabricating these CCDs, and the fact that for each camera 4 CCDs are used, and all these 4 have to share front-end electronics, it was prudent to optimize their grouping to we maximise the dynamic range we get. More dynamic range means that we can tell more about the planets we find with higher confidence.
ziddoap|1 year ago
I think this is "Charge-Coupled Device"?
"an electronic sensor that converts light to digital signals through charges generated by bouncing photons on a thin silicon wafer"
Is that correct? Not familiar with the acronym.
UltraSane|1 year ago
This is a picture of the CCD array for the Gaia space observatory that used parallax to measure precise distances and slightly less precise angular velocities of billions of objects
http://www.bo.astro.it/~altavilla/FTP/GAIA/IMAGES/The%20comp...
hajola|1 year ago
fragmede|1 year ago
hajola|1 year ago
However they won't be photos of planets really. It will be countless photos of the same stars over and over again, it's just that sometimes they will be slightly less bright than other times. Directly imaging exoplanets is incredibly difficult, but humans have managed it: https://en.wikipedia.org/wiki/List_of_directly_imaged_exopla...