SIGHTINGS


 
Hubble Shows We Are
Only A 'Chevy' Of A Galaxy
By Mark Ward
Milwaukee Journal Sentinel
From Scripps Howard News Service
8-18-98
 
 
 
The more astronomers learn about the universe, the less exalted our place in it seems.
 
Ever since Nicolaus Copernicus in the 1540s demonstrated that the Earth revolves around the Sun, and so is not the center of the universe, the prominence of our blue-green planet has faded quickly.
 
In studying the stars, astronomers came to realize that the sun is a garden-variety specimen -- not especially large or small -- and that our solar system resides in a galactic backwater out toward the end of one of the spiral arms of the Milky Way.
 
In the 1920s, astronomers discovered that the fuzzy smudges they spotted beyond the stars were not clouds of gas, but separate galaxies, each containing billions of stars. Still, their initial measurements suggested that among galaxies, the Milky Way was unusually large: perhaps the biggest, at least in its class of spiral galaxies.
 
Now astronomers from Great Britain, using the Hubble Space Telescope to measure distances to other galaxies, have burst that bubble too.
 
Calculating the diameters of galaxies based on new, more accurate measurements of their distance from Earth, astronomers Simon Goodwin, John Gribbin and Martin Hendry declared that the Milky Way is not especially big. In fact, the average size for spiral galaxies now appears to be slightly bigger than the diameter of the Milky Way.
 
As astronomer Jay Gallagher of the University of Wisconsin-Madison put it: "It looks like we're kind of a Chevy of a galaxy."
 
The measurements were made possible by Hubble's ability to resolve more clearly than ever before individual stars called Cepheid variables in distant galaxies. Cepheids are special kinds of stars that vary in brightness in regular pulses that astronomers have come to use as astronomical measuring rods.
 
Mostly, they have been used to measure distances within the Milky Way. In recent years, astronomers have spotted Cepheid variables in other galaxies, but the measurements derived from them have been relatively crude because of the limited resolving power of Earth-based telescopes.
 
"It's as if you were sitting on the moon looking at the Earth and you detected a glow along Lake Michigan, but you couldn't detect whether it was Milwaukee, Racine or Chicago," said Gallagher.
 
The same applies to Cepheids in distant galaxies. "With Hubble," Gallagher said, "you can separate them. You can pick out the individual Cepheid stars. That's important in judging distance."
 
The British astronomers selected 17 spiral galaxies where astronomers working on Hubble had identified Cepheids and measured their diameters. They found two that were at least twice as big as the Milky Way and others that were smaller.
 
The findings, they wrote, support the notion that "there is nothing special about where or when we live or observe from. We seem to live on an ordinary planet, orbiting an ordinary star, and it is natural to infer that the Solar System resides in an ordinary galaxy."
 
Gallagher said that assessment may be a little generous.
 
Residing as we do near the outer edge of a middling spiral galaxy, we are probably a little bit further out of the action than most. Closer to average, he said, likely would be a star in the midst of a massive elliptical galaxy 100 times bigger than the Milky Way.
 
It may seem a little deflating to have our place in the universe reduced to sub-par. For astronomers, though, it's actually a good sign. It means that our astronomical neighborhood is fairly typical, which means that what we learn here probably applies to most of the rest of the universe.





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