We have found the matter that was missing in the universe. I was hidden in the filaments of the cosmic network

Where is the dark matter is one of the great mysteries of the cosmos, but if someone thought we had all the barionic matter (the “conventional” matter) in the cosmos … it was wrong. At least until now. What was missing. A new study He has found in the cosmic network the barionic matter that remained hidden and that would represent about half of the “conventional” matter of the universe (matter which in turn only represents about 15% of the total matter). He has achieved it thanks to rapid radio (FRB) bursts, mysterious radio wave bursts that run the cosmos occasionally and have served to “illuminate” the subject of this intergalactic network. A network of “highways” in space. The cosmic network is a series of filaments of enormous size located in the intergalactic space in which a good part of the subject of the universe is distributed. These filaments are stretched clouds of gas and particles whose characteristics We discover little by little. Recent studies had documented the existence of this elusive network. The fact that the gas and particles that compose it are inert and do not give off light made their observation very difficult, which required hundreds of hours of dedication by powerful telescopes like VLT (Vary Large Telescope) of the European Observatory Austral (ESO). DSA-110. For study, the team had to build its own observatory in the California desert, in DSA (Deep synoptic array) -110. The name DSA-110 refers to the fact that this is a telescope composed of a network of 110 antennas. FRB The new Observatory was responsible for the detection of 39 of the 69 FRB thanks to which the deccovement was possible. These bursts are intense intriguing radio signals that we occasionally receive from the cosmos. We do not know exactly its cause or causes, but we suspect that they can be caused by supernovae or similar events. Some of these frb are repeated periodically while others are punctual; The origin of some can be located in a concrete galaxy, that of others does not. The frb used in the study They had their origin at points located at distances between 11.74 million light years and 9,100 million light years. This last distance, marked by the event FRB 20230521B, now marks a record: that of the most distant gust detected. Illuminating the highway. According to Explain the team itself Responsible for the study, the FRB “shine through the fog of the intergalactic medium.” When studying how this light stops when you meet matter, it is possible to measure this mist. When crossing the filaments, the frb light also separates in different wavelengths, such as when we see that a white light breaks down when crossing a prism, generating an rainbow. The measure to which the light decomposes also offers key information about the medium that is going through. The details of the study were published In an article In the magazine Nature Astronomy. Halos or networks. So far the cosmological models indicated that there was more barionic matter in the universe than we were able to observe. The new estimate of the mass of the huge filaments of the cosmic network allows us to fill in these holes. The new estimate indicates that 76% of the conventional matter of the cosmos is in the intergalactic environment, while 15% would be in the “halos” of the galaxies, while the rest, about 9% of this matter, would be the subject of which the interior of the galaxies is composed: planet stars and everything that lives are already vast cosmic structures. In Xataka | Dark matter has been one of the most fascinating mysteries of physics for years. Now we have a new theory Image | Vikram Ravi/Caltech/Ovro / Jack Madden, Illustristng, Ralf Konietzka, Liam Connor/CFA

There is a cosmic network of “roads” formed by gas and dark matter filaments. We have just captured it from Chile

We know well that matter is not distributed in a form of all homogeneous throughout the observable universe. The galaxies like the one we live are great clusters of matter in which the stars are born and died, and with them other objects such as planets and asteroids. However, that is only part of the story. In sight. A group of researchers has achieved Capture directly and in “high definition” an image of the so -called cosmic network, a network of gas filaments that extend throughout millions of light years in the intergalactic space. He has done it from the VLT, the large telescope that the Southern European Observatory has installed in Chile. A cosmic network. The subject in the universe is not only concentrated in the galaxies. Moreover, the subject distributed in intergalactic space plays a fundamental role in the structure of our cosmos. Physical interactions lead to this matter to be distributed in an interesting way. He does it In immense filamentsgas clouds that form an immense network that connects the galaxies around it. The gas that accumulates in this network of “cosmic highways” is the one that feeds the stars of the bright galaxies located at the intersections of this network. Huge, and almost invisible. In addition to the gas that feeds the stars, dark matter also plays an important role in the structuring of this network as indicated by the team responsible for this new image. Observing this dark matter is impossible today, but capturing the gas columns that accompany it, the “star fuel”, is possible. Hundreds of hours. Overcome this difficulty Requires dedicationeven for our most powerful telescopes. That is why capturing this image required hundreds of hours of observation by the VLT (Vary Large Telescope), The telescope of the European Observatory (ESO) installed in the Atacama desert, in Chile. The team resorted to the Muse instrument (Multi–Unit Spectroscopic Explorer), An advanced spectrograph installed in the Chilean telescope. The details of the process were published In an article In the magazine Nature Astronomy. In the image, in color, the diffuse gas that extends around and between the remarked galaxies can be seen. Davide Tornotti/University of Milano-Bicocca. Three million light years. The team used ultraprecisous data compiled by the telescope to create the most clear image ever achieved by one of the filaments that make up the cosmic network. The filament in question extends over three million light years and Connect two distant galaxieseach of them with its own supermassive black hole. “By capturing the dim light emitted by this filament, which has traveled for just under 12,000 million years to reach the Earth, we are able to accurately characterize its form,” Explain in a press release Davide Tornotti, co -author of the study. The team also highlights that the accuracy of the new data has allowed “Draw the border” between the gas of the galaxies themselves and all the subject that we associate with this cosmic web. And all through direct measurements. Validate the theory. In his study, the team used these direct observations to test the theoretical cosmological models. And with a positive result: “When comparing it to the new high definition image, we find a substantial agreement between theory and observations,” Tornotti indicated. Even so, the team also points out that they will continue working on the study of these structures. “One is none,” that is, with the image of one of these elements, it is not enough to draw generalizable conclusions about these key structures for our cosmos but as unknown as the filaments that make up the cosmic network. In Xataka | Is our Milky Way a zombie galaxy and we without knowing it? Image | Alejandro Benitez-Llambay/University of Milano-Bicocca/MPa/Davide Tornotti/University of Milano-Bicocca

Log In

Forgot password?

Forgot password?

Enter your account data and we will send you a link to reset your password.

Your password reset link appears to be invalid or expired.

Log in

Privacy Policy

Add to Collection

No Collections

Here you'll find all collections you've created before.