I know very little about astronomy, but I'm preparing a talk for a class that will involve Betelgeuse. Assume that we could cool Betelgeuse so that it wouldn't burn us up and "freeze" its size at its mean size and then place its closest "surface" 384,400 km from Earth directly "above" a viewing position (ignore other factors like gravity). If it was generating enough light to be clearly seen (rather than blackening the sky), how much of the sky would it fill?
I realize that at this distance its opposite "edge" would be far past the sun and most of the planets in our solar system.
I've seen comparisons of the size of a period (Earth) to a 20-story building (Betelgeuse), but I'm trying to think of some other ways of visualizing the size of these immense objects which are visible without a telescope.
Please feel free to mention other ways of getting our brains around how big these objects we're seeing actually are.
Thanks.
2007-02-05
07:07:32
·
3 answers
·
asked by
Gary D
1
in
Science & Mathematics
➔ Astronomy & Space
If Betelgeuse would completely fill the sky from horizon to horizon at the moon's distance, how far away would we have to push it until we could start to see some "sky" at each horizon?
2007-02-05
07:13:34 ·
update #1
Some great answers here, thanks. That "amount of area outside the airplane window" example is especially helpful.
I'm still surprised that it wouldn't take up more than half the sky looking straight up and I'm sure it's because of faulty logic on my part.
Here is what I thought: A full moon directly overhead occupies about .52 degrees of the sky. If you doubled the size of the moon, wouldn't you *nearly* double this amount? I realize a law of diminishing returns here because the moon doesn't wrap around the earth, but since Betelgeuse is 270,000 times the size of the moon, I would think that there would just be a small amount of visible sky (much less than 45 degrees) at each horizon. Feel free to help me see where I'm off-base here.
2007-02-05
11:30:47 ·
update #2