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Another advantage of the Moon is that it takes 28 days to rotate on its axis, meaning that it has 28 times longer than an Earthbound telescope to gather light from faint sources. The key to astronomical photography is exposure - the fainter the object, the longer you need to leave the aperture open. For example, the original Hubble Deep Field (the deepest exposure of the Universe to date) was created by combining 342 separate exposures, taken across 10 consecutive days. Using lunar telescope arrays, we could see even deeper into space, analysing the structure of the universe right back to the time when it first became transparent to electromagnetic radiation. Before we get too carried away with the possibilities of lunar astronomical observatories, it's important to recognise that even though astronomy is a perfectly good reason to return to the Moon, it's going to cost money - a lot of it. Even a relatively modest array, involving just a handful of telescopes, would cost significantly more than the HST. And being located on the far side, it would require the support of at least one satellite in lunar orbit, in order to relay the data back to Earth. Also, the shuttle missions to repair and upgrade the HST have shown us the value of in-orbit servicing. A similar mission to service one or more lunar telescopes would be both problematic and extremely expensive. The truth is that investment in astronomy is rewarded with knowledge, not hard cash, so science alone won't be enough of an incentive to return to the Moon. POSTSCRIPT: A note to Pink Floyd fans and readers of bad sci-fi: I avoid using the expression "dark side of the Moon". Just because we can't see it directly doesn't mean that it's dark. The far side receives just as much sunlight as the near side. In fact, if you take lunar eclipses into consideration, it actually receives more. |
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Page created & maintained by Mark Kilner | Last Updated: |
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