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Using a bit of mathematics i have been looking into degrees,
arcseconds and so on. Having verified the moon to be .5 degrees, and the sun to be about the same - and this agreeing with books - i was happy that i was doing the right thing. When getting say x2 magnification does that mean we see the moon as if it was 1 whole degree? it ought to follow. I used the same calculations on nearby stars to fully appreciate why we just can't see them as disks through telescopes, i roughly estimated that seeing Sirius A as a disc roughly the size of the moon would require x300,000 magnification (but i may have that wrong): 360 / 2Pi =57.3 (used later) Moon degrees = 57.3 * arctan(diameter/distance) (thats roughly 3476/384000) = just over 0.5 degrees Sirius A degrees = 57.3 * arctan(1390000km/8.6ly) (ly=9,460,530,000,000km) = 0.000001645 degrees multiply that by 300,000 to get just under .5 degrees! but please do correct any errors, it's a first bash at this. What is the highest magnification realistically available to amateurs and the best amatuer scope in realistic seeing. A really huge mirror in space, or an even bigger one built on the moon, would perhaps get to the point of being able to see nearby stars as discs. I'm still impressed by the idea of seeing something at x80 ! I understand that the HST saw a red giant (betelguese?) as a tiny disk. btw, i hadn't appreciated how big in the sky andromedia is - i guess it's because we generally only see the smaller central part. |
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