The cosmic web is an elaborate network of interconnected hydrogen filaments that have given shape to the universe since the early years following the Big Bang.
“This is a key period because the universe was very active back then,” astrophysicist Roland Bacon, who spearheaded the research, told RFI.
“A lot of stars and galaxies were being formed … and the gas was the fuel for this formation.”
Deepest images of space
The cosmic web was mostly the stuff of cosmological simulations until it was observed by the European Southern Observatory's Very Large Telescope, which was pointed at a single region of the sky for some 140 hours, over eight months.
This focus point forms part of the Hubble Ultra-Deep Field, a section of the cosmos that was, until now, the deepest part of the universe ever observed.
Using 3D spectrograph technology, known as MUSE, scientists led by Bacon’s team at the Lyon Astrophysical Research Centre were able to produce stunning images some 12 billion light years away.
So far indirect glimpses of the cosmic web have been achieved only through studying the light of quasars, massive galactic objects that emit superhot radiation.
However this latest research, published Thursday in the journal Astronomy & Astrophysics, marks the first time light emitted from the cosmic web itself has been observed.
“Even though we know it’s there, we need to actually observe it to measure it,” says Bacon, adding that quasars are located in a very specific part of the cosmic web where the filaments cross paths.
Surprise galaxies
The biggest surprise to result from the research was the discovery that UV light from the filaments was coming from a previously invisible population of billions of dwarf galaxies.
These tiny galaxies – which produce a huge amount of light because they are so numerous – may be responsible for “reionising” the universe and ending the “dark age” that followed the Big Bang.
“For 500 million or a billion years, there was no light, no stars, no galaxies – and then there was the first emission of light,” Bacon explains.
“What was the source of this sort of reionisation? Black holes, micro black holes, special stars? I think it was this population of dwarf galaxies.”
