Europe and China are at risk in the race for the first gravitational wave observatory in space

Terrestrial gravitational wave detectors, such as the famous LIGO, have made very interesting discoveries in the last decade. However, there is a great consensus that it would be very useful to detect this cosmic phenomenon directly from space. For this reason, some space agencies are already getting to work to launch their own projects. One of them is the Taiji mission, of the Chinese Academy of Sciences, with which, in fact, a great step forward has just been taken. Everything ready for Taiji 2. The Taiji mission consists of three phases. The first was already launched in 2019. For the second, a piece called the full-function interferometer optical core had to be tested. The tests carried out on Earth have gone perfectlyso it is considered that the second phase could be launched as soon as possible. In fact, its launch It was initially scheduled in 2024but it has been suffering delays. Luckily, it seems that now all the pieces are ready. Three ships in total. The Taiji mission is made up of three ships, strategically placed in space millions of kilometers away. They will all be connected to each other through laser interferometry, so that slight changes in these distances that could be associated with gravitational waves can be detected. The first phase of the mission, in which the interferometry system was analyzed, was launched in 2019. It is expected to send the second part as soon as possible, in which the first two ships will be put into space. As for the third, in principle the established calendar places its launch in the 2030s. Better in space than on Earth. Gravitational waves are waves produced in space-time as a result of a catastrophic event. These types of events could be, for example, the merger of neutron stars or the collision of black holes. When this occurs, space-time experiences a disturbance similar to that produced when a stone is thrown into a pond. Those are gravitational waves. The terrestrial observatories, like LIGOthey can detect them, but they have a small limitation. And there could be confusion with seismic noise and other terrestrial interference. In space, that problem disappears. Taiji to the rescue. According to the tests that have been carried out on Earth and the analyzes of the interferometry system that have already been carried out in space with Taiji-1, this mission is capable of greatly reducing interference. Furthermore, the optical core that has just been tested is capable of detecting disturbances on the order of picometers. That is, on Earth you can discern displacements equivalent to one ten-thousandth of the diameter of a human hair. Although those distances would change under spatial conditions, it is still highly accurate. Therefore, it is expected to detect even gravitational waves caused by intermediate mass black holes. Other similar missions. The European Space Agency It also has its own mission aimed at detecting gravitational waves in space. This is LISAa project with which it is planned to do something similar: launch three ships connected by laser interferometry into space. In this case, the launch of all ships is scheduled for 2035, so China could have some advantage. Of course, until the complete triangle is in space, the mission cannot be considered completed. Perhaps Europe will be able to overtake the Asian country. Image | NOIRLab In Xataka | What happens if you fall into a black hole, explained simply in an overwhelming NASA simulation

The most detailed gravitational waves in history have just confirmed the great prediction of Stephen Hawking

After ten years Perfecting the detection of gravitational wavesLigo sensors achieved such a precise observation which has allowed physicists to confirm one of Stephen Hawking’s most famous predictions: the black holes area theorem. Ten years. A decade has passed since the scientists of the Ligo Observatory The universe listened for the first time in a completely new way: by detecting gravitational waves. On September 14, 2015, wrinkles in spacetime tissue Predicts by Albert Einstein a century earlier inaugurated a new era in astronomy. What was then an almost imperceptible cosmic whisper, today has become a symphony that sensors can clearly hear. And on the tenth anniversary of that milestone, the Ligo-Virgo-Kagra (LVK) collaboration has captured the most clear gravitational wave signal to date. GW250114. Detected on January 14, 2025, physicists believe that these gravitational waves were caused by the collision and subsequent fusion of two black holes to about 1.3 billion light years from the earth. Interestingly, the event is almost a twin that ended using Ligo’s physicists the 2017 Nobel PrizeGW150914. In both cases, it was two black holes with masses between 30 and 40 times that of our sun. But there is an abysmal difference: the signal quality. An unprecedented sharpness. Thanks to a decade of technological improvements and advances in quantum engineering, Ligo detectors are now almost four times more sensitive. While the first signal had a signal/noise ratio of 26, that of GW250114 has a 80. “We can hear it high and clear, and that allows us Physical Review Letters. This sharpness has been key to unraveling the secrets that were hidden in the vibrations of the black hole resulting from the merger. Hawking theorem. In 1971, Stephen Hawking proposed that the total area of ​​the event horizon of a black hole can never be reduced. It can increase or remain the same, but never shrink. This, which is known as the Hawking area theorem, is analogous to the second law of thermodynamics, which says that the entropy (the disorder) of an isolated system always increases. Therefore, the area of ​​a black hole is a measure of its entropy. Trying it is complicated. When two black holes merge, part of their mass becomes an enormous amount of energy in the form of gravitational waves (the famous E = mc²). In addition, the new black hole can turn much faster, and a larger turn implies a minor area for the same dough. Does the increase in mass compensate for these losses so that the final area is always greater? The analysis of GW250114 has been settled by the matter bluntly. Hawking was right. In this case, the two initial black holes had a combined area of ​​about 240,000 square kilometers. After the merger, the new black hole, with a mass of about 63 times that of the sun, it had an area of ​​400,000 square kilometers. If in 2021 a first test with the 2015 signal showed a 95%confidence, the new data raises that certainty to 99,999%. As Kip Thorne recalls, one of Ligo’s parents and Hawking personal friend, the British physicist called him right after the first detection in 2015 to ask if they could try his theorem. Hawking died in 2018but today his theory has been verified in a way that would have left him very satisfied. Einstein too. Thanks to this new signal, scientists have been able to analyze the moment just after the merger in which the new black hole vibrates like a newly hit bell before stabilizing. The frequencies and speed with which these tones are attenuated. It is the most solid test to the date that black holes are seemingly simple objects that can be completely described with only three properties: mass, spin and electric charge. All other information of the material that formed them is lost. But each detection of gravitational waves is one more piece in the puzzle of the cosmos. And as GW250114 demonstrates, to understand them we travel on the shoulders of giants such as Einstein and Hawking. Image | Aurore Simonnet (SSU/edeon)/LVK/URI In Xataka | Everything to know about gravitational waves: what they are, where are they and why we will not stop talking about them

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