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Green Pea Galaxy Provides Insights to Early Universe Evolution

Jan 19, 2016 |
A Hubble Space Telescope image of the compact green pea galaxy J0925+1403. The diameter of the galaxy is approximately 6,000 light years, and it is about twenty times smaller than the Milky Way.

Newly formed dwarf galaxies were likely the reason that the universe heated up about 13 billion years ago, according to new work by an international team of scientists that included a University of Virginia researcher. The finding opens an avenue for better understanding the early period of the universe’s 14 billion year history.

In the period of several hundred thousand years after the Big Bang, the universe was so hot and dense that matter was ionized instead of being in a neutral form. But 380,000 years later, the expansion of the universe had cooled it enough for matter to become neutral and for the first structures of the universe to form – gas clouds of hydrogen and helium. Gravity then made these gas clouds grow in mass and collapse to form the first stars and galaxies. Then, about one billion years after the Big Bang, another important transformation occurred: the universe reheated, and hydrogen – the most abundant element – became ionized for a second time, as it had shortly after the Big Bang, an event which astronomers call “cosmic re-ionization.” How this happened is still debated.

Astronomers have long thought that galaxies were responsible for this transformation.

An international team of scientists, organized by University of Virginia astronomer Trinh Thuan in the United States, has largely validated that hypothesis in a paper published Thursday in the journal Nature. Trinh’s research colleagues on the paper are at institutions in Ukraine, the Czech Republic, Switzerland, France and Germany.

Trinh Thuan, Professor of Astronomy
Dan Addison / University Communications

Using data from an ultraviolet spectrometer aboard the Hubble Space Telescope, the team discovered a nearby compact dwarf galaxy emitting a large number of ionizing photons into the intergalactic medium, or the space between galaxies. Scientists believe those photons are responsible for the universe’s re-ionization.

“This galaxy appears to be an excellent local analog of the numerous dwarf galaxies thought to be responsible for the reionization of the early universe,” Trinh said. “The finding is significant because it gives us a good place to look for probing the reionization phenomenon, which took place early in the formation of the universe that became the universe we have today.”

Normal matter in the early universe consisted mostly of gas. Stars and star clusters are born from clouds of gas, forming the first galaxies. Ultraviolet radiation emitted by these stars contains numerous ionizing photons. For this reason, scientists have long suspected that galaxies were responsible for cosmic reionization. However, for reionization to occur, galaxies must eject these photons into the intergalactic medium; otherwise, they are easily absorbed by the gas and dust before they can escape. Despite 20 years of intensive searching, no galaxy emitting sufficient ionizing radiation had been found, and the mechanism by which the universe became re-ionized remained a mystery.

To solve this problem, the international research team proposed to observe “green pea” galaxies. Discovered in 2007, these galaxies represent a special and rare class in the nearby universe. They appear green to light sensors and are round and compact, like a pea. They are believed to host stellar explosions or winds strong enough to eject ionizing photons.

The team examined data from the Sloan Digital Sky Survey – a database of more than a million galaxies. From this survey, they identified approximately 5,000 galaxies that match their criteria: very compact galaxies emitting very intense UV radiation. Researchers selected five galaxies for observation with the Hubble Space Telescope.

Using Hubble’s UV radiation detecting capabilities, the research team found that the “green pea” galaxy J0925+1403, located at a distance of three billion light-years from Earth, was “ejecting” ionizing photons, with an intensity never seen before – about an 8 percent ejection. This fundamental discovery shows that galaxies of this type could explain cosmic reionization, confirming the most commonly made hypothesis for this phenomenon.

“As we make additional observations using Hubble, we expect to gain a much better understanding of the way photons are ejected from this type of galaxy, and the specific galaxy types driving cosmic reionization,” Trinh said. “These are crucial observations in the process of stepping back in time to the early universe. They paved the way to future observations with the successor of Hubble, the James Webb Space Telescope, planned for launch in 2018, which is expected to revolutionize the field with updated capabilities for detailing the first galaxies and sources of cosmic re-ionization.”

The research team on the Nature paper includes:

Y. I. Izotov and N. G. Guseva of the National Academy of Sciences of Ukraine; I. Orlitova of the Czech Academy of Sciences; D. Schaerer of the University of Geneva and the French National Center for Scientific Research; T. X. Thuan of the University of Virginia; A. Verhamme of the University of Geneva; and G. Worseck of the Max Planck Institute for Astronomy.