Originally posted by: Lalakai
Originally posted by: MisterJackson
Sorta on topic (maybe), but I've always wondered would a high powered telescope/obsevatory on Antarctica help us see what observatories on other area of the planet might not?
I'm a noob on this stuff, so don't laugh if that's stupid.
always a learning curve to everything we do; the real noobs are the ones that think they already know it all.
global positioning of the observatory has limited impacted on viewing area. of more importance is "light pollution" from nearby areas, clarity of the atmosphere (a plus for a polar station, and one of the reasons why Hubble is so successful), and simple accessibility. someone else had tried explaining why the polar areas seemed very suitable but in actuality they weren't; now i'm trying to push the grey matter to remember that conversation. hopefully someone else can expand a bit more.
Off the top of my head, I figure that maybe the wind would be a problem there, constantly depositing snow on the optics. And of course the temperature - new adaptive lenses use small motors to constantly reshape the mirror to adjust for atmospheric distortion. They'd have to be insulated and possibly heated to keep them going.
Then there's just the problem of staffing the place. Not many people say, "Yeah, I want to live in Antarctica, where I can take a casual stroll outside and be
dead in a few minutes!"
I think that these adaptive mirrors can actually produce images which rival Hubble's focal quality. However, Hubble, and other orbital telescopes, have some advantages, at least that I can think of:
- Long term exposures of a tiny point, such as its Ultra Deep Field image. It can point at the same spot very precisely, and be unaffected by any odd vibrations. Yes it does so during multiple orbits - the UDF took something around 1 million seconds of exposure time. 1 orbit takes about 90 minutes, so it'd be looking at one spot for maybe 45 minutes (2700 seconds), go around the planet, and look at the same spot again. At least that's how I think they did it.
- Ability to see wavelengths of light that the atmosphere filters out.
Link - scroll toward the bottom for some charts. They show the wavelengths that don't make it through the atmosphere. A lot gets filtered out before making it to the ground.