Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:


Small but Plentiful: How the Faintest Galaxies Illuminated the Early Universe


Light from tiny galaxies more than 13 billion years ago played a larger role than previously thought in creating the conditions in the universe as we know it today, according to a new study by researchers at the Georgia Institute of Technology and the San Diego Supercomputer Center (SDSC) at the University of California, San Diego.

Ultraviolet (UV) light from stars in these faint dwarf galaxies helped strip interstellar hydrogen of electrons in a process called reionization, researchers said in a paper published this week in the journal Monthly Notices of the Royal Astronomical Society. The epoch of reionization began about 200 million years after the Big Bang and astrophysicists agree that it took about 800 million more years for the entire universe to become reionized. It marked the last major phase transition of gas in the universe, and it remains ionized today.

A view of the entire simulation volume that shows the large scale structure of the gas distribution in filaments and clumps. The red regions are heated by stellar UV light coming from the galaxies, highlighted in white. These galaxies are over 1000 times less massive than the Milky Way and contributed nearly one-third of the UV light during reionization. The field of view of this image is 400,000 light years across, when the universe was only 700 million years old. John Wise, Georgia Institute of Technology.

Astrophysicists aren’t in agreement when it comes to determining which type of galaxies played major roles in this epoch. Most have focused on larger, more luminous galaxies. However, this latest research, based on computer simulations, indicates scientists should also focus on the smallest ones. Specifically, these new simulations show that these tiny galaxies – despite being 1000 times smaller in mass and 30 times smaller in size than the Milky Way – contributed nearly 30 percent of the UV light during this process.

Reionization experts often ignored these dwarf galaxies because they didn’t think they formed stars. It was assumed that UV light from nearby galaxies was too strong and suppressed these tiny neighbors.

“It turns out they did form stars, usually in one burst, around 500 million years after the Big Bang,” said John H. Wise, a Georgia Tech assistant professor in the School of Physics who led the study. “The galaxies were small, but so plentiful that they contributed a significant fraction of UV light in the reionization process.”

The team’s simulations modeled 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 (more than 10 million solar masses) halos, or spheroidal collections of dark matter which is the site of galaxy formation. It was only 5 percent in larger halos (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 reionization.

“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 reionization 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 universe was fully ionized at 860 million years after its creation.

“That such small galaxies could contribute so much to reionization is a real surprise,” said Michael Norman, distinguished professor of physics at UC 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 reionization,” said Norman, who also is the director of SDSC, an Organized Research Unit of UC San Diego.

The term ‘reionized’ is used because the universe was ionized immediately after the fiery Big Bang. During that time, ordinary matter consisted mostly of hydrogen atoms with positively charged protons stripped of their negatively charged electrons. Eventually, the universe cooled enough for electrons and protons to combine and form neutral hydrogen. They didn’t give off any optical or UV light. Without the light, astrophysicists aren’t able to see traces of how the cosmos evolved during these Dark Ages using conventional telescopes. The light returned when reionization began, allowing experts such as Wise to pinpoint the youngest galaxies and study their features.

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.

In addition to Wise and Norman, the research team included Vasiliy G. Demchenko and

Martin T. Halicek (Center for Relativistic Astrophysics, Georgia Institute of Technology); Matthew J. Turk (Department of Astronomy, Columbia University); Tom Abel (Kavli Institute for Particle Astrophysics and Cosmology, Stanford University); and Britton D. Smith (Institute of Astronomy, University of Edinburgh). The research was supported by the National Science Foundation (NSF) under award numbers AST 1211626, AST 1333360, and AST 1109243.

Media Contact

Jan Zverina

Jan Zverina | Eurek Alert!
Further information:

Further reports about: Astrophysics Big Bang Dwarf galaxies Universe dark matter dwarf electrons galaxies protons telescopes

More articles from Physics and Astronomy:

nachricht Subaru Telescope helps pinpoint origin of ultra-high energy neutrino
16.07.2018 | National Institutes of Natural Sciences

nachricht Nano-kirigami: 'Paper-cut' provides model for 3D intelligent nanofabrication
16.07.2018 | Chinese Academy of Sciences Headquarters

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: First evidence on the source of extragalactic particles

For the first time ever, scientists have determined the cosmic origin of highest-energy neutrinos. A research group led by IceCube scientist Elisa Resconi, spokesperson of the Collaborative Research Center SFB1258 at the Technical University of Munich (TUM), provides an important piece of evidence that the particles detected by the IceCube neutrino telescope at the South Pole originate from a galaxy four billion light-years away from Earth.

To rule out other origins with certainty, the team led by neutrino physicist Elisa Resconi from the Technical University of Munich and multi-wavelength...

Im Focus: Magnetic vortices: Two independent magnetic skyrmion phases discovered in a single material

For the first time a team of researchers have discovered two different phases of magnetic skyrmions in a single material. Physicists of the Technical Universities of Munich and Dresden and the University of Cologne can now better study and understand the properties of these magnetic structures, which are important for both basic research and applications.

Whirlpools are an everyday experience in a bath tub: When the water is drained a circular vortex is formed. Typically, such whirls are rather stable. Similar...

Im Focus: Breaking the bond: To take part or not?

Physicists working with Roland Wester at the University of Innsbruck have investigated if and how chemical reactions can be influenced by targeted vibrational excitation of the reactants. They were able to demonstrate that excitation with a laser beam does not affect the efficiency of a chemical exchange reaction and that the excited molecular group acts only as a spectator in the reaction.

A frequently used reaction in organic chemistry is nucleophilic substitution. It plays, for example, an important role in in the synthesis of new chemical...

Im Focus: New 2D Spectroscopy Methods

Optical spectroscopy allows investigating the energy structure and dynamic properties of complex quantum systems. Researchers from the University of Würzburg present two new approaches of coherent two-dimensional spectroscopy.

"Put an excitation into the system and observe how it evolves." According to physicist Professor Tobias Brixner, this is the credo of optical spectroscopy....

Im Focus: Chemical reactions in the light of ultrashort X-ray pulses from free-electron lasers

Ultra-short, high-intensity X-ray flashes open the door to the foundations of chemical reactions. Free-electron lasers generate these kinds of pulses, but there is a catch: the pulses vary in duration and energy. An international research team has now presented a solution: Using a ring of 16 detectors and a circularly polarized laser beam, they can determine both factors with attosecond accuracy.

Free-electron lasers (FELs) generate extremely short and intense X-ray flashes. Researchers can use these flashes to resolve structures with diameters on the...

All Focus news of the innovation-report >>>



Industry & Economy
Event News

Leading experts in Diabetes, Metabolism and Biomedical Engineering discuss Precision Medicine

13.07.2018 | Event News

Conference on Laser Polishing – LaP: Fine Tuning for Surfaces

12.07.2018 | Event News

11th European Wood-based Panel Symposium 2018: Meeting point for the wood-based materials industry

03.07.2018 | Event News

Latest News

Subaru Telescope helps pinpoint origin of ultra-high energy neutrino

16.07.2018 | Physics and Astronomy

Barium ruthenate: A high-yield, easy-to-handle perovskite catalyst for the oxidation of sulfides

16.07.2018 | Life Sciences

New research calculates capacity of North American forests to sequester carbon

16.07.2018 | Earth Sciences

Science & Research
Overview of more VideoLinks >>>