"Quite a controversy had erupted as to whether theres so much dust in galaxies that it completely blocks our view and we dont see even half of whats there, or whether theres a lot less," said Keel. "So we decided to start looking for pairs of overlapping galaxies [to find out]. We went through every galaxy catalog we could find, and we found about a dozen pairs that were big enough to learn something from."
Of the dozen galaxy pairs, Keel and White were able to image three in detail with the Hubble Space Telescope. As it turns out, the overlap between the foreground and background galaxies in NCG 3314 is the most exact ever seen. This exactness has allowed astronomers to measure the amount of dust there is near the center of the foreground galaxy, a feat that is normally impossible to accomplish with solo galaxies due to the black background of space behind them.
The dust of the foreground galaxy, NGC 3314-A, is easily visible to astronomers because it absorbs light emanating from the background galaxy, which lies somewhere between 15 million and 25 million light-years behind NGC 3314-A. "You can see this very red splotch, which is the light from the center of the background galaxy filtering through this huge amount of dust on the way," said Keel. "It turns out that only about 1 percent of the blue light makes it through."
"We desperately hope theres nothing special about [these two] galaxies," added Keel. Thats because he hopes to someday use observations about the dust in NGC 3314-A to describe galaxies the universe over.
But before that can happen, more research in the way of overlapping galaxies must be done. Yet already, some of Keel and Whites observations about this particular pair have proved quite valuable. "Already, weve shown that the dust in the backlit galaxy is very similar to the dust in our galaxy," said Keel.