Originally posted by stevebrot Thanks for this very useful suggestion, though the fact remains that live view focus at 1:1 (direct pixel mapping to the rear LCD) is a true representation of the state of focus for capture. Assuming adequate focus lock, secure support, accurate/precise tracking, and stable atmosphere, live view should be WYSIWYG. For sure, more accurate focus (so-called sub-pixel focus) may be attained with a Bahtinov mask when coupled with appropriate focus mechanism, but such cannot overcome focus drift, atmospheric instability or vibration.
FWIW, focus failure on Venus (~ 0.5 degrees of arc) using live view is somewhat unexpected, even without a mask.
Steve
In my experience, the Bahtinov mask beats live view 1:1 for high-magnification imaging. I find the live view to be a good starting point. Steady atmosphere is still needed, focus drift must be accounted for (redo focus, but the automated way is better (I don't have it
)), vibration is inadequate equipment ,etc.
At the end of January, Venus only gets up to 30.4 arc-seconds in diameter (Sky & Telescope). This is rather high magnification territory. The moon is ~ 0.5 degrees in diameter.
I suspect that the OP was imaging Venus at night, as Venus is about 3 hours behind the sun in January. If so, a problem of the extreme contrast between the sun-illuminated very bright clouds of Venus and the black sky surrounding is "irradiation", a bleeding of the brightness into the dark. Always a problem for our eyes, it is also present in optical systems, and the sharp line between light and dark is not adequately represented in the final image. Many viewers and imagers of Venus prefer the daytime for their operations, as the much brighter daytime sky reduces the extreme contrast and provides for much better, sharper viewing and imaging. The contrast between the planet and the blackness is much greater for Venus than any astronomical object (leaving out the Sun). Could be a problem here.