The Farthest Galaxy ever Discovered.

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A team of researchers from California Institute of Technology [Caltech] has discovered a 13.2-billion-years old [the universe itself is about 13.8 billion years old] galaxy which may be the most distant galaxy ever found.

Earlier this year, EGS8p7 had been identified as a candidate for further investigation based on data gathered by NASA's Hubble Space Telescope and the Spitzer Space Telescope. Using the multi-object spectrometer for infrared exploration [MOSFIRE] at the W.M. Keck Observatory in Hawaii, the researchers performed a spectrographic analysis of the galaxy to determine its redshift.

Redshift results from the Doppler effect, the same phenomenon that causes the siren on a fire truck to drop in pitch as the truck passes. With celestial objects, however, it is light that is being "stretched" rather than sound; instead of an audible drop in tone, there is a shift from the actual color to redder wavelengths.

Redshift is traditionally used to measure distance to galaxies, but is difficult to determine when looking at the universe's most distant and thus earliest objects. 

Immediately after the Big Bang, the universe was a soup of charged particles, electrons, protons and photons [light]. Because these photons were scattered by free electrons, the early universe could not transmit light. 

By 380,000 years after the Big Bang, the universe had cooled enough for free electrons and protons to combine into neutral hydrogen atoms that filled the universe, allowing light to travel through the cosmos. Then, when the universe was just a half-billion to a billion years old, the first galaxies turned on and reionized the neutral gas. The universe remains ionized till today.

Prior to reionization, however, clouds of neutral hydrogen atoms would have absorbed certain radiation emitted by young, newly forming galaxies, including the so-called Lyman-alpha line, the spectral signature of hot hydrogen gas that has been heated by ultraviolet emission from new stars, and a commonly used indicator of star formation. Because of this absorption, it should not, in theory, have been possible to observe a Lyman-alpha line from EGS8p7.

"If you look at the galaxies in the early universe, there is a lot of neutral hydrogen that is not transparent to this emission," says Adi Zitrin, NASA Hubble postdoctoral scholar in astronomy. "We expect that most of the radiation from this galaxy would be absorbed by the hydrogen in the intervening space. Yet still we see Lyman-alpha from this galaxy."

They detected it using the MOSFIRE spectrometer, which captures the chemical signatures of everything from stars to the distant galaxies at near-infrared wavelengths [0.97-2.45 microns, or millionths of a meter].

The surprising aspect about the present discovery is that they have detected this Lyman-alpha line in an apparently faint galaxy at a redshift of 8.68, corresponding to a time when the universe should be full of absorbing hydrogen clouds. Prior to their discovery, the farthest detected galaxy had a redshift of 7.73.

One possible reason the object may be visible despite the hydrogen-absorbing clouds that the hydrogen reionization did not occur in a uniform manner. "Evidence from several observations indicate that the reionization process probably is patchy, some objects are so bright that they form a bubble of ionized hydrogen. But the process is not coherent in all directions." Zitrin told.

"The galaxy we have observed, EGS8p7, which is unusually luminous, may be powered by a population of unusually hot stars, and it may have special properties that enabled it to create a large bubble of ionized hydrogen much earlier than is possible for more typical galaxies at these times," says Sirio Belli, a Caltech graduate student who worked on the project.

The researchers are currently calculating more thoroughly the exact chances of finding this galaxy and seeing this emission from it, and to understand whether they need to revise the timeline of the reionization, which is one of the major key questions to answer in our understanding of the evolution of the universe.

Source:- caltech.edu
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