Small, But Plentiful: How The Faintest Galaxies Illuminated The Early Universe
Royal Astronomical Society (RAS)
Astronomers investigating behavior of the universe shortly after the Big Bang have made a surprising discovery: the properties of the early universe are determined by the smallest galaxies. The team report their findings in a paper published today in the journal Monthly Notices of the Royal Astronomical Society.
Shortly after the Big Bang, the universe was ionized: ordinary matter consisted of hydrogen with its positively charged protons stripped of their negatively charged electrons. Eventually, the universe cooled enough for electrons and protons to combine and form neutral hydrogen. This cool gas will eventually form the first stars in the universe but for millions of years, there are no stars. Astronomers therefore aren’t able to see how the cosmos evolved during these ‘dark ages’ using conventional telescopes. The light returned when newly forming stars and galaxies re-ionized the universe during the ‘epoch of re-ionization’.
Astronomers agree that the universe became fully re-ionized roughly one billion years after the Big Bang. About 200 million years after the birth of the cosmos, ultraviolet (UV) radiation from stars began to split neutral hydrogen into electrons and protons. It took another 800 million years to complete the process everywhere. This epoch of re-ionization marked the last major change to gas in the universe, and it remains ionized today, over 12 billion years later.
However, astronomers aren’t in agreement on which type of galaxies played the most important role in this process. Most have focused on large galaxies. The new study by researchers at the Georgia Institute of Technology and the San Diego Supercomputer Center indicates scientists should also focus on the smallest ones.
The researchers used computer simulations to demonstrate the faintest and smallest galaxies in the early universe were essential. These tiny galaxies – despite being 1000 times smaller in mass and 30 times smaller in size than our own Milky Way galaxy – contributed nearly 30 percent of the UV light during this process.
Other studies often ignore these small ‘dwarf’ galaxies as they weren’t thought to form stars, because the UV light from nearby larger galaxies was too strong and suppressed these tiny neighbors.
“It turns out these dwarf galaxies did form stars, usually in one burst, around 500 million years after the Big Bang,” said Prof. John Wise, of the Georgia Institute of Technology, who led the study. “The galaxies were small, but so plentiful that they contributed a significant fraction of UV light in the re-ionization process.”
The team’s simulations modelled the flow of UV stellar light through the gas within galaxies as they formed. They found that the fraction of ionizing photons escaping into intergalactic space was 50 percent in small galaxies (more than 10 million solar masses). It was only 5 percent in larger galaxies (300 million solar masses). This elevated fraction, combined with their high abundance, is exactly the reason why the faintest galaxies play an integral role during re-ionization.
“It’s very hard for UV light to escape galaxies because of the dense gas that fills them,” said Wise. “In small galaxies, there’s less gas between stars, making it easier for UV light to escape because it isn’t absorbed as quickly. Plus, supernova explosions can open up channels more easily in these tiny galaxies in which UV light can escape.”
The team’s simulation results provide a gradual timeline that tracks the progress of re-ionization over hundreds of millions of years. About 300 million years after the Big Bang, the universe was 20 percent ionized. It was 50 percent at 550 million years. The simulated universe was fully ionized at 860 million years after its creation.
“That such small galaxies could contribute so much to re-ionization is a real surprise,” said Prof. Michael Norman, of the University of California San Diego and one of the co-authors of the paper. “Once again, the supercomputer is teaching us something new and unexpected; something that will need to be factored into future studies of re-ionization.”
The research team expects to learn more about these faint galaxies when the next generation of telescopes is operational. For example, NASA’s James Webb Space Telescope, scheduled to launch in 2018, will be able to see them.
This research has been published in Wise J. el al., “The Birth of a Galaxy – III. Propelling reionization with the faintest galaxies“, Monthly Notices of the Royal Astronomical Society, in press, published by Oxford University Press.
This research was supported by the National Science Foundation (NSF) (AST 1211626, AST 1333360 and AST 1109243). Any conclusions expressed are those of the principal investigator and may not necessarily represent the official views of the NSF.
Image 2 (below): A zoomed-in view of the most massive dwarf galaxy in the simulation, seen when the universe was only 700 million years old. This galaxy only has 3 million solar masses of stars, compared to 60 billion solar masses in our Milky Way. The yellow points represent the older and cooler stars in the galaxy, and the blue points show the young and massive stars forming just before this snapshot of the simulation. The haze around the stars show the gas distribution in the galaxy with blue and red representing hot and cold temperatures, respectively. Credit: John Wise. [ Larger Image ]
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