The southern entrance to the A5 underground is already 80% excavated, and there is a culprit that has speeded up the work: the soil

Allow me, if you don’t mind, to use an expression that I have been wanting to use for a long time: there is already light in the tunnel. That’s right, then the burial of the A5 Move against the clock to meet deadlines. And the goal is to open traffic in November. The southern tunnel of the Extremadura highway has already exceeded four fifths of its route under Madrid. There is less left, largely due to the technical innovations that have made it possible. The largest work in Madrid right now. The burial of the A-5 is, today, the largest infrastructure under construction of the capital. Under the streets that connect Madrid with the exit to Extremadura, two tunnel boring machines work in parallel to bury one of the historic entrances to the city and thus free up surface space for urban use. Where is each tunnel. The work runs in two independent galleries. The southern tunnel, through which vehicles entering Madrid will circulate, has been excavated for approximately 80% of its length. The northern tunnel, the exit, is advancing at a slower pace and has completed about half of the route. Although the asphalt has not yet been laid, the interior appearance of the most advanced gallery already allows a fairly clear idea of ​​what the final infrastructure will look like, according to transfer to Telemadrid the technical teams that supervise the work. The key to acceleration: the ground. As the media points out, a new construction system applied to the tunnel floor has made it possible to speed up both the excavation and the consolidation of the infrastructure. For this reason, and because of the work that is being put into the work every day, it has been possible to reach 80% without major delays, maintaining the schedule. 14 emergency exits. Parallel to the main gallery, the work includes the construction of 14 emergency exits, one every approximately 200 meters. Each of them is accompanied by technical rooms where the systems necessary for the operation of the tunnel will be housed, including geothermal installations that will improve its energy efficiency. Jump to the surface. Starting in September is planned that the works also extend abroad, with urbanization actions in the area around the A-5. The idea in this phase will be to definitively integrate the infrastructure into the surface, with the aim of reducing traffic outside and taking advantage of the area for new public spaces. November, the date marked on the calendar. With the tunnel boring machines still in operation, the goal is for vehicles to be able to travel through the new tunnel before the end of the year. November is the date currently managed by those responsible for the work. So we just have to wait a few more months to call it a day. one of the heaviest works of these years in the capital. Cover image | Madrid City Council In Xataka | Portugal had to choose where to take its AVE first. And between Madrid and Galicia, it is very clear

Who or what excavated the ravines on Mars? The answer is even stranger than we always thought

For years, we have seen images of strange grooves in the dunes of Mars that seemed to have been carved by liquid water, feeding the hopes of finding conditions for life. But the reality, as often happens in these fields, is much stranger and fascinating as shown a new study published in Geophysical Research Letters which not only confirms that the culprit is carbon dioxide ice, but has discovered a completely new mechanism that seems straight out of science fiction. The study. Dr. Lonneke Roelofs of Utrecht University, lead author of the study, described it in a way that will be familiar to many of us: “I felt like I was watching the sandworms from the movie Dune.” And it’s no wonder. In his experiments, he saw blocks of dry ice not only slide, but literally burrow and dig into the sand with explosive force, a phenomenon never before observed. Recreating Mars. To solve the mystery, the research team used the martian simulation chamber ‘George’. Inside this two-meter cylinder, they recreated the conditions of Mars’ thin atmosphere, which has a pressure of only 700 pascals compared to Earth’s 100,000 pascals. The experiment was simple: place a tray with dune sand, adjust the inclination and drop blocks of CO₂ ice from the top. Here the process that was being sought was that of sublimationthe direct passage from solid to gas. On Earth, this is a calm process, but on Mars it is extremely violent. The enormous temperature difference between the ice and the sand on which it is located, combined with the low pressure, causes the CO₂ to expand explosively and generate immense force. Results. In this case, the team discovered that the ice blocks moved very differently depending on the steepness of the slope. On steep slopes (>22.5º) the ice block slid rapidly, at about 0.8 m/s, over a layer of gas, almost floating. This movement created straight, shallow channels with almost imperceptible ridges. This is something that coincides with the channels seen in the highest parts of the Martian dunes. In the case of gentle slopes is where the real magic happened. The block moved very slowly, at about 0.0003 m/s, and instead of sliding it was partially buried in the sand. Explosive sublimation threw grains of sand ballistically in all directions, carving a deep channel beneath the block and with high ridges on its sides. This ‘digging’ movement perfectly explains the deep channels, high ridges and sinuous curves that for so long They baffled scientists. But finally, when the block finally stops at the foot of the dune, the sublimation effect continues to occur and generates the characteristic pits. The importance. These findings are very relevant to understanding Mars as a planet. First of all, the results confirm that one of the most active and striking phenomena is driven by CO₂ processes, without the need for have liquid water. In addition, it gives us a physical model that explains all the strange characteristics of the ravines. Sharp curves, for example, are not due to the flow of liquid, but to an excavating block that changes course due to small irregularities in the terrain. Finally, the formation of these ravines requires very specific conditions, such as sufficient accumulation of CO₂ ice in winter and sufficient solar radiation in spring to heat the sand and cause violent sublimation. In short, the mystery of the grooves in the Martian dunes has been solved, and the answer is not the water we long to find, but a violent and exotic physical process, more typical of an alien planet. Images | Daniele Colucci POT In Xataka | NASA has a plan to speed up our arrival on Mars: crash things into its surface

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