Astronomers have identified the point where the Universe moved from heating to cooling - 11 billion years ago, when the temperature was an astonishing 13,000 degrees Celsius, hotter than the surface of the Sun.
An international team, led by researchers from Swinburne University of Technology, found evidence that the Universe broke its rising 'fever' about 11 billion years ago.
They measured the temperature of the Universe when it was 3 to 4 billion years old by studying the gas in between galaxies - the intergalactic medium.
"However, 11 billion years ago, this fever seems to have broken and the Universe began cooling down again," lead researcher Elisa Boera, a PhD student from Swinburne's Centre for Astrophysics and Supercomputing, said.
"The intergalactic medium is an excellent recorder of the Universe's history. It retains memory of the big events that affected its properties, such as temperature and composition, during its different phases of evolution," said Boera.
In the study, Boera collected the bluest light that Earth's atmosphere transmits - harsh ultraviolet (UV) light from 60 quasars.
This UV light comes from slightly later in the Universe's development, allowing the new temperature measurement.
"The quasar light suggests that the Universe had cooled by about 1000 degrees C within 1 billion years after reaching its maximum of 13,000 degrees," Boera said.
"This cooling trend has probably continued to the present day," said Boera.
"We think the answer is helium," co-author of the study, Swinburne Associate Professor Michael Murphy said.
"Fourteen per cent of the intergalactic gas is helium and, 12 billion years ago, it was absorbing the intense radiation from active galaxies, losing electrons in the process," Murphy said.
"The electrons whizz around, heating up the gas. It's similar to the greenhouse effect on Earth: Carbon dioxide gas absorbs infrared radiation and heats our atmosphere.
"Once all the helium was ionised, the radiation would simply pass through the gas without heating it. Then, as the Universe expands the gas cools down, just like the cold gas sprayed from an aerosol can - it quickly cools as it expands out of the can," said Murphy.
The study has been published in the Monthly Notices of the Royal Astronomical Society.
An international team, led by researchers from Swinburne University of Technology, found evidence that the Universe broke its rising 'fever' about 11 billion years ago.
They measured the temperature of the Universe when it was 3 to 4 billion years old by studying the gas in between galaxies - the intergalactic medium.
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During these early years of the Universe's development, many extremely active galaxies were 'switching on' for the first time and heating their surroundings.
"However, 11 billion years ago, this fever seems to have broken and the Universe began cooling down again," lead researcher Elisa Boera, a PhD student from Swinburne's Centre for Astrophysics and Supercomputing, said.
"The intergalactic medium is an excellent recorder of the Universe's history. It retains memory of the big events that affected its properties, such as temperature and composition, during its different phases of evolution," said Boera.
In the study, Boera collected the bluest light that Earth's atmosphere transmits - harsh ultraviolet (UV) light from 60 quasars.
This UV light comes from slightly later in the Universe's development, allowing the new temperature measurement.
"The quasar light suggests that the Universe had cooled by about 1000 degrees C within 1 billion years after reaching its maximum of 13,000 degrees," Boera said.
"This cooling trend has probably continued to the present day," said Boera.
"We think the answer is helium," co-author of the study, Swinburne Associate Professor Michael Murphy said.
"Fourteen per cent of the intergalactic gas is helium and, 12 billion years ago, it was absorbing the intense radiation from active galaxies, losing electrons in the process," Murphy said.
"The electrons whizz around, heating up the gas. It's similar to the greenhouse effect on Earth: Carbon dioxide gas absorbs infrared radiation and heats our atmosphere.
"Once all the helium was ionised, the radiation would simply pass through the gas without heating it. Then, as the Universe expands the gas cools down, just like the cold gas sprayed from an aerosol can - it quickly cools as it expands out of the can," said Murphy.
The study has been published in the Monthly Notices of the Royal Astronomical Society.