Scientists have conducted a new census of the amount of matter in the cosmos, finding that the stuff makes up 31% of our universe.
“To put that amount of matter in context, if all the matter in the universe were spread out evenly across space, it would correspond to an average mass density equal to only about six hydrogen atoms per cubic meter [about 35 cubic feet],” Mohamed Abdullah, a graduate student in the Department of Physics and Astronomy at the University of California, Riverside (UCR), said in a statement.
“However, since we know 80% of matter is actually dark matter, in reality, most of this matter consists not of hydrogen atoms but rather of a type of matter which cosmologists don’t yet understand,” said Abdullah, who led a new study announcing the result.
The study, which was published online Friday (Sept. 25) in The Astrophysical Journal, suggests that 69% of the cosmos’ matter-energy budget is dark energy, a mysterious force thought to be responsible for our universe’s accelerating expansion.
That number is in rough agreement with previous estimates, which astronomers have calculated via a variety of methods. For example, the team behind Europe’s Planck satellite, which scrutinized the cosmic microwave background — the glow left over from the Big Bang — determined in 2013 that dark energy makes up 68.3% of the universe.
The new study also reaffirms the piddling 5% contribution of “normal” matter, the stuff that makes up stars, planets, trees, oceans and everything else that we can directly see and touch.
Abdullah and his colleagues arrived at their number by studying galaxy clusters. The researchers developed a tool that measures a cluster’s mass by examining the orbits of its member galaxies. They applied this tool to observations made by the Sloan Digital Sky Survey, a wide-ranging campaign that uses a telescope in New Mexico, creating a cluster catalog that the researchers then compared to numerical simulations.
Such comparison — observed cluster numbers and masses versus modeled predictions — is a proven technique for determining the universe’s total matter content, the study team explained. That’s because clusters, which take billions of years to form, are a sort of cosmological probe. Their observed numbers are sensitive to a number of variables, particularly the universe’s total matter content.
“We have succeeded in making one of the most precise measurements ever made using the galaxy cluster technique,” study co-author Gillian Wilson, a professor of physics and astronomy at UCR who leads the lab in which Abdullah works, said in the same statement.
“Moreover, this is the first use of the galaxy orbit technique, which has obtained a value in agreement with those obtained by teams who used noncluster techniques,” such as the Planck researchers’ cosmic microwave background method, she added.
Indeed, the 31% figure is a “best combined value,” at which Abdullah and his team arrived after combining their cluster results with previous calculations performed using a variety of techniques, the researchers said.