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3C295 in Context
3C295 is enveloped by a vast cloud of fifty million degree gas. The gas cloud, which is visible only with an X-ray telescope, contains more than a hundred galaxies and enough material to make a thousand more. The galaxies in most cases do not contain enough hot gas to be observed with an X-ray telescope, but they do show up in optical photographs. Because the galaxies were discovered before the hot gas cloud, these objects are called galaxy clusters, or clusters of galaxies.Galaxy clusters are formed through the merger of smaller groups and clusters over billions of years. The gas in clusters is thought to have been heated to fifty million degrees or more when the cloud collapsed about five to ten billion years ago. Galaxy clusters are the most massive gravitationally bound objects in the universe.
The gas in the central regions of the 3C295 cluster shows signs that it is cooling and settling onto the central galaxy. Astronomers think that the material falling onto 3C295 over the eons has caused it to grow into its present size and shape. It contains several times the mass of our Milky Way galaxy and resembles a giant glowing basketball.
The explosion that wracked 3C295 about a million years ago and produced the X-ray knots and radio lobes was probably due to the infall of gas onto the galaxy. In much the same way that a torrent of water pouring down a drain can produce a back pressure if the flow is more than the drain can handle, the enormous energy released by too much matter flowing into a supermassive black hole could trigger an explosion. Great quantities of matter and energy would be hurled back into the surrounding gas cloud, in a powerful payback for eons of being dumped on by a cosmic bully.
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