A planet has just disappeared. NASA’s Hubble telescope has captured a violent cosmic event that changes everything

Investigating the universe beyond the Solar System we know sometimes brings up more questions than answers. The search for exoplanets has left findings so different from what we know as fascinating. Thus, more than a decade ago the Kepler space telescope identified the Kepler-16ba planet with “two suns” along Star Wars Tatooine and the James Webb telescope stumbled upon a world of boiling lava that paradoxically it’s colder what the theory says. In the process of investigating the universe you can witness the disappearance of a planet, as NASA’s Hubble has monitored, to discover that there was nothing like a planet: they were in front of a violent cosmic phenomenon. First they detected a bright point of light and assumed that it was a planet covered in dust where the brightness of its star was reflected. Then the object disappeared and a different bright source appeared nearby. Finally, this international research team realized that they were not seeing planets at all: the light came from incandescent debris generated by violent collisions, as they later published in Science. A planetesimal collision that changes everything In their observations in time, they captured two different and very powerful impacts that generated large amounts of dust in the same planetary system, which constitutes a magnificent opportunity to understand how planets are formed and what type of materials they are made of. Their main hypothesis: they have glimpsed not one, but two extremely rare events: one (two) planetesimal collisionthat is, a collision between small rocky objects similar to asteroids. Northwestern University astrophysicist Jason Wang explains that it is the first time they have seen a planetesimal collision outside the solar system and that its study is “key to understanding how planets form and can also provide information about the structure of asteroids, something important for planetary defense programs such as the DART test.” Paul Kalas, an astronomer at the University of California at Berkeley and lead author, insists on the exceptionality of the event: “It is not present in any of our previous Hubble images, which means that we have just witnessed a violent collision between two massive objects and a huge cloud of debris, something that has no parallel in our current solar system.” By NASA, ESA, P. Kalas, J. Graham, E. Chiang, E. Kite (University of California, Berkeley), M. Clampin (NASA Goddard Space Flight Center), M. Fitzgerald (Lawrence Livermore National Laboratory), and K. Stapelfeldt and J. Krist (NASA Jet Propulsion Laboratory) These collisions occurred in the planetary system surrounding the star Fomalhautwhich is larger than the Sun, is surrounded by an extensive and dense set of dusty debris belts and located about 25 light years from Earth, in the constellation Pisces Austrinus. That dust belt is so large that it is a real candy for research. Planet it seems, cloud of dust it is In 2008 they detected Fomalhaut b, a bright object of unknown nature that some researchers thought was a planet and others believed it was an expanding cloud of dust from a collision. Back in 2023, a new Hubble observation gave an unexpected twist to everything: the original light source was no longer there and another bright object had appeared in a slightly different area. As explains Wang, first They assumed it was Fomalhaut b, but they got a surprise: “We assumed the bright light was Fomalhaut b because it was the known source of the system. But by carefully comparing the new images with the old ones, we realized that it couldn’t be the same source. It was exciting, but also perplexing” So they had to change perspective and nomenclature: the original object was renamed Fomalhaut cs1 and its disappearance supports the idea that it was a cloud of dust that was slowly dispersing after a collision. They called the second bright source Fomalhaut cs2 and its behavior reinforces the conclusion that neither of the two objects was a planet: everything indicates that they are clouds of debris created when large planetesimals collide with each other. Investigating Fomalhaut cs2 they concluded that it looked very similar to the beginnings of cs1 from two decades ago, both in brightness and location. So the team already estimates the frequency of collisions in this guy in the system: every 100,000 years or even less. After all, in 20 years they have already seen two. Kalas explains that “if you took a movie of the last 3,000 years and sped it up so that each year lasted a fraction of a second, imagine how many flashes you would see. The Fomalhaut planetary system would be full of these crashes.” Fomalhaut cs1 no longer exists, but the research team wants to continue monitoring the system and has its eyes on cs2, which could hide more valuable information about how collisions develop in young planetary systems. Of course, in addition to the old Hubble, they will use the near-infrared camera of the James Webb Space Telescope since the NIRCam can capture detailed information about color, so they can determine the size and composition of dust grainsfor example if they contain water or ice. The confirmation of these collisions put a warning on the table for hunters of planets outside the Solar System: the gLarge clouds of dust can very well imitate the appearance of an exoplanetto by reflecting light from its star, which can lead to error using the reflected light detection system. Kalas sums it up: “What we learned from studying cs1 is that a large dust cloud can masquerade as a planet for many years.” As new observatories point to the sky to obtain direct images of Earth-like planets, differentiating between real planets and temporary dust clouds seems providential. In Xataka | Poland and Spain are the European countries that have increased their contribution to space the most. For very different reasons In Xataka | China reveals its cards for 2030: it will go in search of an “Earth 2.0” on its own Cover | Javier Miranda By ESA, NASA, and L. … Read more

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

Almost 20 years ago a telescope captured a “cosmic tornado.” Now, thanks to James Webb, we know he hid a galaxy behind

Appearances often deceive. A unbridled eye could well confuse one of the planets in our solar neighborhood, such as Venus, with a distant star. We could also see an image taken by a telescope and think that the two objects that most attract attention on it are part of the same cosmic phenomenon. This is precisely what happens in the last image of the James Webb space telescope (JWST). A cosmic tornado. While the new image seems to show a huge nebula filled by a star on the tip; What we really see It is the combination of the emanations expelled by a nascent star, called Herbig-Haro 49/50, and a galaxy located far behind in the plane. Herbig-Haro. The calls Herbig-Haro objects They are produced by the form of a star formation, specifically they are the result of the expulsion of matter during this process, matter that can accumulate in regions several light years away from the birthplace of the star. This matter “cools” emitting light both in the visible spectrum and infrared. Herbig-Haro 49/50 (HH 49/50) It is one of these objects. The appellation of “cosmic tornado” received it after the Spitzer space telescope observed it in 2006. The image did not allow to distinguish with certainty what type of object we saw at the tip of this cosmic tornado. A distant galaxy. The new image of James Webb allows us to see this luminous object with great definition, showing us the small details of a distant spiral galaxy. In its bluish center are the oldest stars. In its spirals of more reddish tones the galactic dust and areas of intense star formation would be concentrated. Comparison between the image of the Spitzer Space Telescope taken in 2006, and the last Inagen captured by the James Webb. NASA, ESA, CSA, STSCI, NASA-JPL, SSC Back to the foreground. But, let’s return to Herbig-Haro 49/50, the foreground of the image. The cloud of matter we see is within our galaxy, about 625 light years from our solar system. What we see are waves of bright hydrogen molecules, carbon dioxide and dust grains loaded with energy, red and orange tints in this false color photo. This formation is found in the Chamaeleon I cloudy complex, one of the regions with the formation activity of closer stars in our galaxy. Experts estimate that this “jet” of matter moves between 100 and 300 kilometers per second. And what about the star you are emanating? Astronomers believe that it is about cederblad 110 IRS4, a protoestrella Located at 1.5 light years From this cloud and visible in the image of the JWST, below right. Cederblad 110 IRS4 is a class I protoestrel, that is, it is in a rapid accumulation phase of matter. A combined image. The new image captured by the JWST is a combination of several snapshots taken by this telescope fruit of international collaboration. To create it Observations were combined of two of the instruments of James Webb, Nircam (Near-Infrared Camera), And Miri (MID-INFRAED INSTRUMENT). In Xataka | These real images were unthinkable before the Webb Telescope: they are planets orbiting other stars to 130 light years Image | NASA, ESA, CSA, STSCI

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

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