Ancient light may point to where the cosmos’ missing matter hides | Science News for Students

Ancient light may point to where the cosmos’ missing matter hides

A new technique might have found the protons and neutrons unaccounted for in the universe
Nov 27, 2017 — 6:45 am EST
missing mass
Astronomers have been puzzled by the apparent absence of some ordinary matter throughout the cosmos. A new computer technique has now found hints at where it might be. It shows galaxies (pink) strung like beads along long filaments of dark matter (blue). Most of the ordinary matter is probably stored in gas (orange).
Illustris Collaboration/Illustris Simulation

There’s been a problem with the universe. Some matter has been missing — the ordinary type that makes up atoms. The good news: Astronomers say they may have found it.

Scientists think this missing matter is hot gas. It appears to be lurking in spaces between clusters of galaxies. Previous studies had hinted where this missing matter might be hiding. A new search technique now is helping home in on where it resides. Astronomers described online the technique they used in a pair of papers posted September 15 and 29 at

Finding this missing matter is important, says Dominique Eckert. He is an astronomer at the Max Planck Institute for Extraterrestrial Physics in Garching, Germany. He did not take part in the new work. He has, however, searched for the missing matter. It is made of protons, neutrons and other select subatomic particles. Scientists sometimes refer to these as baryons (BEAR-ee-ahns). “If you want to understand how galaxies form and how everything forms within a galaxy, you have to understand the evolution of the baryon content,” says Eckert. And that starts with knowing where those baryons are.

Astronomers know that about 85 percent of the matter in the universe is dark matter. This stuff is mysterious and elusive. And it’s not made of baryons. It doesn’t emit light (which is why it’s literally dark). It’s also different from ordinary matter.

In contrast, ordinary matter makes up only about 15 percent of the mass of the universe. It is what is in us and all around us. Weirdly, about half of even this  type of matter does not show up astronomers scan the skies. As they look at galaxies within the nearest few billion light-years from Earth, they find only about half the baryons that should have been produced in the Big Bang. (That’s the rapid expansion of dense matter in the universe. According to current theory, the Big Bang marked the origin of the universe. ) 

The rest of the ordinary matter is probably hiding in long strands, or filaments, of gas. These strands connect clusters of galaxies in a vast cosmic web. Previous attempts to find the missing baryons focused on X-rays emitted by the gas. Astronomers also looked at how the light coming out certain of bright, distant galaxies, called quasars, filtered through these cobwebby strands. Still, that missing ordinary matter had remained a no-show.

Now some scientists have scouted for the missing matter in a new way. Hideki Tanimura is a cosmologist at the Institute of Space Astrophysics in Orsay, France. He did this research while working at the University of British Columbia in Vancouver. Anna de Graaff is an astrophysicist in Scotland at the University of Edinburgh. She worked as part of another team.

Each group found a way to look through the gas. They peered all of the way back to the oldest light in the universe.

Accounting for cosmic clouds

That ancient light is known as the cosmic microwave background. It is residual heat that was emitted some 380,000 years after the Big Bang. As it beams through space, this light passes through clouds of electrons, which are negatively charged particles. Filaments of hot gas host these electron clouds. As the cosmic microwave background passes through these clouds, they deflect and distort the light in a particular way. In 2015, a satellite helped create an all-sky map of those distortions.

Tanimura and de Graaff separately figured that there should be more distortion along the filaments than in empty space. To locate the filaments, both teams focused on pairs of galaxies from a catalog known as the Sloan Digital Sky Survey. The galaxies they chose had to be at least 20 million light-years apart. De Graaff’s team chose roughly a million pairs of those galaxies. Tanimura’s team chose 262,864 pairs. Both groups assumed that the galaxies were not all part of some galaxy cluster. But they should be connected by a filament.

Individually, those filaments were too faint to see. To bring them into view, the teams used computer software. It layered all of the images. Then, each team subtracted out distortions that any clouds of electrons would have produced. This revealed a residual distortion in the cosmic microwave background. Both groups saw it and now link it to the presence of those filaments.

“Filamentary gas is very difficult to detect,” Tanimura says. “But now we have a technique to detect it.”

De Graaff’s team calculates that those filaments must account for about three in every 10 baryons throughout the universe. And that’s likely an underestimate. After all, her team notes, it didn’t examine every filament in the universe.

Michael Shull is an astrophysicist at the University of Colorado Boulder. “Both groups here took the obvious first step,” he says. “I think they’re on the right track.” Still, he worries that the gas they see might come from another source. It could have been ejected from galaxies at high speeds. If true, he says, it might not be the missing matter after all.

Eckert also worries that the gas may belong more to the galaxies than to their intergalactic tethers. Future observations of what the gas is made from, he says, along with more sensitive X-ray observations, could help solve that part of the puzzle.

Power Words

(more about Power Words)

astronomy       The area of science that deals with celestial objects, space and the physical universe. People who work in this field are called astronomers.

astrophysics      An area of astronomy that deals with understanding the physical nature of stars and other objects in space. People who work in this field are known as astrophysicists.

baryons        Subatomic particles made from three smaller units called quarks. Protons and neutrons are the best known baryons.

Big Bang   The rapid expansion of dense matter that, according to current theory, marked the origin of the universe. It is supported by physics’ current understanding of the composition and structure of the universe.

cosmic microwave background    A type of radiation that fills the universe with a faint glow. It seems to flow in all directions and with an equal intensity. It's the heat left over from the Big Bang and that should exist throughout the universe. It is estimated to be about 2.725 degrees above absolute zero.

cosmology    The science of the origin and development of the cosmos, or universe. People who work in this field are known as cosmologists.

cosmos    (adj. cosmic) A term that refers to the universe and everything within it.

dark matter    Physical objects or particles that emit no detectable radiation of their own. They are believed to exist because of unexplained gravitational forces that they appear to exert on other, visible astronomical objects.

eject    (n. ejection) To suddenly remove or force something out of its container or current position.

filament    Something with a thin, thread-like shape. For instance, the fragile metal wire that heats up to emit light inside an incandescent light bulb is known as its filament.

galaxy    A massive group of stars bound together by gravity. Galaxies, which each typically include between 10 million and 100 trillion stars, also include clouds of gas, dust and the remnants of exploded stars.

galaxy cluster    A group of galaxies held together by gravity. Galaxy clusters are the largest known objects in the universe.

intergalactic    An adjective that describes some position between galaxies.

light-year    The distance light travels in one year, about 9.48 trillion kilometers (almost 6 trillion miles). To get some idea of this length, imagine a rope long enough to wrap around the Earth. It would be a little over 40,000 kilometers (24,900 miles) long. Lay it out straight. Now lay another 236 million more that are the same length, end-to-end, right after the first. The total distance they now span would equal one light-year.

neutron    A subatomic particle carrying no electric charge that is one of the basic pieces of matter. Neutrons belong to the family of particles known as hadrons.

proton    A subatomic particle that is one of the basic building blocks of the atoms that make up matter. Protons belong to the family of particles known as hadrons.

quasar    Short for quasi-stellar light source. This is the brilliant core of some galaxy (massive collections of stars) that contains a super-massive black hole. As mass from the galaxy is pulled into that black hole, a huge quantity of energy is released, giving the quasar its light.

subatomic    Anything smaller than an atom, which is the smallest bit of matter that has all the properties of whatever chemical element it is (like hydrogen, iron or calcium).

tether    A tie or cord that loosely anchors some object to a semi-fixed position. Or the process of tying some object to a cord that will keep it loosely affixed to that position. (Consider the child’s game tether ball, whereby a cord it attached to a ball on one end and an anchoring pole on the other end.)

universe    The entire cosmos: All things that exist throughout space and time. It has been expanding since its formation during an event known as the Big Bang, some 13.8 billion years ago (give or take a few hundred million years).

X-ray    A type of radiation analogous to gamma rays, but having somewhat lower energy.


Journal:​ ​​ H. Tanimura et al. A search for warm/hot gas filaments between pairs of SDSS luminous red galaxies. arXiv:1709:05024v1. Posted online September 15, 2017.

 Journal:​ A. de Graaff et al. Missing baryons in the cosmic web revealed by the Sunyaev-Zel’dovich effect. arXiv:1709.10378v1. Posted online September 29, 2017.