November 2, 2010
Evidence Found Of Cosmic Climate Change
A team of astronomers has found evidence that the universe may have gone through a warming trend early in its history. They measured the temperature of the gas that lies in between galaxies, and found a clear indication that it had increased steadily over the period from when the universe was one tenth to one quarter of its current age. This cosmic climate change is most likely caused by the huge amount of energy output from young, active galaxies during this epoch. The researchers publish their results in a forthcoming paper in the journal Monthly Notices of the Royal Astronomical Society.
"Early in the history of the universe, the vast majority of matter was not in stars or galaxies", University of Cambridge astronomer George Becker explains. "Instead, it was spread out in a very thin gas that filled up all of space." The team, led by Becker, was able to measure the temperature of this gas using the light from distant objects called quasars. "The gas, which lies between us and the quasar, adds a series of imprints to the light from these extremely bright objects," Becker continues, "and by analyzing how those imprints partly block the background light from the quasars, we can infer many of the properties of the absorbing gas, such as where it is, what it's made of, and what its temperature is."
"ËOf course, the temperatures we measured are a bit different from what you find on Earth," commented Becker. "One billion years after the Big Bang, the gas we measured was a 'cool' 8,000 degrees Celsius. By three and a half billion years the temperature had climbed to at least 12,000 degrees Celsius."
The warming trend is believed to run counter to normal cosmic climate patterns. Normally the universe is expected to cool down over time. As the cosmos expands, the gas should get colder, much like gas escaping from an aerosol can. To create the observed rise in temperature, something substantial must have been heating the gas.
"The likely culprits in this intergalactic warming are the quasars themselves", explains fellow team member Martin Haehnelt, who is also at Cambridge University's newly-established Kavli Institute for Cosmology. "Over the period of cosmic history studied by the team, quasars were becoming much more common. These objects, which are thought to be giant black holes swallowing up material in the centers of galaxies, emit huge amounts of energetic ultraviolet light. These UV rays would have interacted with the intergalactic gas, creating the rise in temperature we observed."
One of the lightest and most abundant elements in these intergalactic clouds, helium, played a vital role in the heating process. Ultraviolet light stripped the electrons from a helium atom, freeing the electrons to collide with other atoms and heat up the gas. Once the supply of fresh helium was exhausted, the universe started to cool down again. Astronomers believe this probably occurred after the cosmos was one quarter of its present age.
The team's discovery was made possible by data taken with the 10-meter Keck telescopes in Hawaii, aided by advanced simulations run on a supercomputer at the University of Cambridge. Along with Becker and Haehnelt, the team included James Bolton at the University of Melbourne, and Wallace Sargent at the California Institute of Technology.
The results will appear in, "Detection of Extended He II Reionization in the Temperature Evolution of the Intergalactic Medium", Monthly Notices of the Royal Astronomical Society, Becker G. D., Bolton J. S., Haehnelt G. M., Sargent W. L. W., in press.
Image Caption: A graph showing the temperature of the all-pervasive intergalactic medium when the universe was between one and three billion years old, overlaid on an artist's impression of the emergence of galaxies over the same period. The shaded region shows the range of possible temperatures measured from the team's data. The warming occurred at a time when the growth of galaxies was in full swing. Credit: Amanda Smith / IoA
On the Net:
- Royal Astronomical Society (RAS)
- A preprint of the paper can be seen at http://arxiv.org/abs/1008.2622