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Leveraging Pierre Paquette's excellent answer and reference to Hilton and Mallama, the magnitude of Saturn can be estimated by: $$ V = 5 \log_{10} (rd) - 8.95 - 3.7\times10^{-4} \alpha + 6.16\times10^{-4} \alpha^2 $$ Here, $r\approx9.5$ AU is the distance from Saturn to the Sun, $d$ is the distance from Saturn to the observer, and $\alpha$ is the angle of ...


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It would be dark. Titan in eclipse can be dimly lit by refracted sunlight and light scattered by Saturn's rings. The refracted light would be reddened, but the scattered light would be white. But there isn't much light that far out, and so the brightness would be very low. It has been imaged in eclipse: See https://solarsystem.nasa.gov/resources/14528/...


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Because of the much greater distance from the sun, and the much greater size of Saturn compared to Earth, while there may be a brief period when Titan goes into eclipse where there will still be some refracted sunlight, as well as some reflected light from the rings, for the majority of the eclipse Titan will be effectively dark. And this assumes you have an ...


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