The gas clouds are too diffuse to form stars and show virtually no signs of containing any “metals” — all elements heavier than hydrogen and helium, the two simplest and lightest elements in the universe. In fact, the only elements astronomers have detected in the clouds are hydrogen and its heavier isotope, deuterium.
The lack of metals strongly suggests that the gases are reservoirs of the pristine material left over from the Big Bang. Because stars fuse atoms to make heavier elements, these gases have never been involved in any star making. In other words, they are the remnant gases that are unchanged since they were created in the first few minutes after the Big Bang.
“Despite decades of effort to find anything metal-free in the universe, nature has previously set a limit to enrichment at no less than one-thousandth than that found in the Sun,” said J. Xavier Prochaska from the University of California (UC) Santa Cruz. “These clouds are at least 10 times lower than that limit and are the most pristine gas discovered in our universe.”
“We’ve searched carefully for oxygen, carbon, nitrogen, and silicon — the things that are found on Earth and the Sun in abundance,” Fumagalli said from UC Santa Cruz. “We don’t find a trace of anything other than hydrogen and deuterium.”
Exactly how they can detect dark, cold, diffuse gas about 12 billion light-years away is a story in itself.
“In this case we actually have to do a bit of a trick,” Prochaska said. “We study the gas in silhouette.” A more distant quasar provides the light for this. The quasar light shines though the gas, and the elements in the gas absorb specific wavelengths of light, which can only be found by splitting the light into detailed spectra to reveal the dark lines of missing light.
In other words, said Fumagalli, “all of the analysis is on the light we didn’t get.” The clouds absorb only a small fraction of the quasar light that makes it to Earth. “But the signatures of hydrogen absorption are obvious, so there’s no doubt there’s a lot of gas there.”
The blobs of pristine gas are good news to astronomers because they are confirmation of the theory of what the first elements were and how they were created in the Big Bang. Hydrogen, helium, lithium, and boron are the lightest elements on the periodic table of elements, and they were all created for the first time in what’s called the Big Bang nucleosynthesis (BBN).
“That theory has been very well tested at Keck as regards to hydrogen and its isotope deuterium,” said O’Meara from St. Michael’s College in Colchester, Vermont. “One of the conundrums of that previous work, however, is that the gas also showed at least trace amounts of oxygen and carbon. The clouds that we have discovered are the first to match the full predictions of BBN.”
The discovery also reveals how different the early universe was from today — where it’s very hard to find any place without some “metals” caused by generations of element-building fusion reactors, aka stars.
“What excites me about this discovery is that there is almost a range of 1,000,000 in the metallicity in gases at that time in the universe,” said Fumagalli. In other words, there were places like our solar system — where metals are very abundant — and there were also places very unlike today, where metals were still virtually nonexistent, and the gases were unchanged since almost the beginning of time.
The gas clouds are too diffuse to form stars and show virtually no signs of containing any “metals” — all elements heavier than hydrogen and helium, the two simplest and lightest elements in the universe. In fact, the only elements astronomers have detected in the clouds are hydrogen and its heavier isotope, deuterium.
The lack of metals strongly suggests that the gases are reservoirs of the pristine material left over from the Big Bang. Because stars fuse atoms to make heavier elements, these gases have never been involved in any star making. In other words, they are the remnant gases that are unchanged since they were created in the first few minutes after the Big Bang.
“Despite decades of effort to find anything metal-free in the universe, nature has previously set a limit to enrichment at no less than one-thousandth than that found in the Sun,” said J. Xavier Prochaska from the University of California (UC) Santa Cruz. “These clouds are at least 10 times lower than that limit and are the most pristine gas discovered in our universe.”
“We’ve searched carefully for oxygen, carbon, nitrogen, and silicon — the things that are found on Earth and the Sun in abundance,” Fumagalli said from UC Santa Cruz. “We don’t find a trace of anything other than hydrogen and deuterium.”
Exactly how they can detect dark, cold, diffuse gas about 12 billion light-years away is a story in itself.
“In this case we actually have to do a bit of a trick,” Prochaska said. “We study the gas in silhouette.” A more distant quasar provides the light for this. The quasar light shines though the gas, and the elements in the gas absorb specific wavelengths of light, which can only be found by splitting the light into detailed spectra to reveal the dark lines of missing light.
In other words, said Fumagalli, “all of the analysis is on the light we didn’t get.” The clouds absorb only a small fraction of the quasar light that makes it to Earth. “But the signatures of hydrogen absorption are obvious, so there’s no doubt there’s a lot of gas there.”
The blobs of pristine gas are good news to astronomers because they are confirmation of the theory of what the first elements were and how they were created in the Big Bang. Hydrogen, helium, lithium, and boron are the lightest elements on the periodic table of elements, and they were all created for the first time in what’s called the Big Bang nucleosynthesis (BBN).
“That theory has been very well tested at Keck as regards to hydrogen and its isotope deuterium,” said O’Meara from St. Michael’s College in Colchester, Vermont. “One of the conundrums of that previous work, however, is that the gas also showed at least trace amounts of oxygen and carbon. The clouds that we have discovered are the first to match the full predictions of BBN.”
The discovery also reveals how different the early universe was from today — where it’s very hard to find any place without some “metals” caused by generations of element-building fusion reactors, aka stars.
“What excites me about this discovery is that there is almost a range of 1,000,000 in the metallicity in gases at that time in the universe,” said Fumagalli. In other words, there were places like our solar system — where metals are very abundant — and there were also places very unlike today, where metals were still virtually nonexistent, and the gases were unchanged since almost the beginning of time.
