MadSci Network: Astronomy |
People with the most acute eyesight, under the darkest of skies on Earth, can see down to the apparent brightness of the planet Uranus. The brightest supergiant stars, placed at a comparison distance of 10 parsecs (approximately 32 light-years) would intrinsically shine about 160,000 times brighter than Uranus. Thus it could be seen as similar to Uranus in brightness if it were 400 times farther than 32 light-years, or about 13,000 light-years away. (400 is the square root of 160,000.) So, a supergiant star at about 13,000 light-years defines the distance limit for humans spotting the light of a single star. This distance isn't even half-way to the center of our own Milky Way! How do we then see the outlines of our own Galaxy, or any of the Galaxies much farther away? The answer is simple: we see the combined light of many bright stars, in regions which appear too small for our eyes to resolve. If a typical galaxy contains 1 billion supergiant stars, it's a billion times brighter than one star and appears as bright as that star even if it's 30,000 times more distant (30,000 is approximately the square root of a billion). Thus, the limits to human vision lie at about 30,000 x 13,000 light-years, or roughly half a billion light-years distance. Even so, we can't see most of the galaxies within that limit, with the unaided human eye. Their light is too spread out (unlike stars). Moreover, this limit is only about 1/25th of the way to the farthest galaxy known via telescopic observations. Telescopes can see objects much farther than human eyes can, since they collect a lot more light than the pupil entrance to our eyes can. Right now, the biggest telescope mirrors are about 10 meters, or 1 million times larger in area than our eyes. They can thus see objects 1,000 times more distant - single stars in galaxies 13 million light years away; entire distant galaxies to the known edge of the universe. Now, while it is true that the whole universe is expanding, gravity is fighting against that expansion and actually wins on the scale of a galaxy, and even in clusters of galaxies. For instance, the Andromeda Galaxy, and several other members of our Local Group of galaxies, are moving toward the Milky Way. Thus, we won't have the problem of stars in our Galaxy becoming too distant for us to see them unaided - as long as our Galaxy keeps on producing stars. Likewise for other galaxies in our local, gravity-bound cluster. What would our Galaxy need to keep on doing that? It would need an unlimited supply of hydrogen and helium. OK, its supply is not endless, so eventually stars will use up all their hydrogen and helium fuel and there won't be enough to ignite baby stars. When, in the distant future, the night sky appears completely black, it won't be due to the light being too distant, but due to visible light not being emitted at all.
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