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

Here the ‘calm’ neutron observatory was installed

In a corner of the Guadalajara Science and Technology Park, far from large telescopes and space agencies, there are A 40 -ton mole dedicated to detecting high -energy particles that constantly bombard the earth. It’s called calm. “Castilla-La Mancha Neutron Monitor”. And for more than a decade it is the first and only installation of its kind in Spain. His work: monitor the attacks of the sun and understand how cosmic rays affect our planet. From space to Guadalajara. The origin of calm is intrinsically linked to the mission Solar orbiter of the European Space Agency. Scientists from the University of Alcalá designed one of the key instruments of the probe, the energy particle detector. Following that experience, an idea arose: build an instrument on land. “We thought of a system that would allow us He explained to Eldiario.es Juan José Blanco, head of the project. Running since 2011. What began almost as a support project for a space mission of ESA has become an international reference in neutron monitoring. Financed with funds from the European Union and the Board of Communities of Castilla-La Mancha, Calm is integrated into the World Network of Neutron Monitorswhere you pour your data in real time. Today is a distributed project. Calm has a twin node called orca which detects both neutrons and muons. It is at the Antarctic base Juan Carlos I of Livingston Island, a magnetically privileged location. The project also has a mobile detector called Mini-Calma which has traveled aboard the Hesperides ship to measure the flow of cosmic rays throughout the journey to Antarctica. The last node to join the project is called Icaro and is installed in the Izaña Atmospheric Observatory (in Tenerife). It measures neutron of solar origin from 2,000 meters of altitude. What exactly measures. When Cosmic rays (High energy particles from deep space) collide with the atoms of our atmosphere, generate a cascade of secondary particles. Among them, neutrons that reach the surface. The sun, with its magnetic field, acts as a modulating shield: the greater solar activity, less galactic cosmic rays reach the earth, and vice versa. Measuring neutron flow, calm can infer solar activity. In addition, it is able to directly detect the arrival of solar energy particles that have been expelled during large eruptions. How a neutron monitor works. The detector consists of gas full of gas surrounded by several layers that alternate lead and polyethylene. This structure allows to reject neutrons that are not very energetic, that is, the environmental ones, letting those who come from space pass, after reducing their speed, to be able to analyze them. With 12 of its 15 active tubes, this 40 -ton machine is a particle filter of amazing precision. What is the use of calm. All this technology has a very practical purpose: to protect us from spatial meteorology. Solar eruptions and coronal mass ejections can be spectacular and create intense northern norter, but also They are extremely dangerous For our technological civilization. The Operators of the Electricity use this data to protect their facilities. Airlines and space agencies need them to assess radiation levels on high altitude routes. And the space industry to protect astronauts and satellites in orbit. It even has applications for interplanetary trips. After having already measured a complete solar cycle of 11 years, calm can be used in the missions to Mars to know which is the best time to start the trip, minimizing Astronaut’s exhibition to radiation. Image | Uah In Xataka | The biggest study in mice sows doubts about travel to Mars: the space shrinks the kidneys

The Chandra X-ray Observatory shows us how a neutron star has “fractured a bone” to our galaxy

As if it were the radiography of a broken bone, the last image that has come to us from NASA shows us the image of a whitish structure whose natural silhouette has been “fractured” by the passage of a mysterious object. An object in whose nature we have been able to investigate thanks precisely to the recent observations. The fracture. The new image It was captured Combining captures of different astronomical observatories and shows us the fracture in G359.13142-0.20005 (abbreviated as G359.13) as well as the object that would have caused this fracture: a neutron star or pulsar. The “bone.” G359.13, the “bone” of this photo, is a cosmic structure called sometimes also as “snake.” This cosmic filament expands over about 230 light years and is about 26,000 light years from the earth, near the core of our galaxy. Filaments that emit radio waves that make them detectable from our planet. These structures are directed, NASA explainsby magnetic fields that run in parallel to them. The radio waves that come to us are caused by particles loaded with energy that form spirals along these magnetic fields. Joint work. The image has been possible Thanks to the combination of observations taken in different segments of the electromagnetic spectrum. As we pointed out, the “bone” of the photo is a visible structure in radio lengths, and its observation has been possible thanks to the Radiolescopes of the Merkat Observatory. When “diagnosing” the cause of this fracture, however, resort to X -rays. Those of Chandra Space Observatoryto be more exact. The reason is that the main suspect of causing this fracture is hidden in the structure itself. Fortunately, this mysterious object also emits in the frequency of X -rays, since what is hidden after this “fracture” seems to be a neutron star or, probably, a pulsar. According to NASA, this object would be emitting light both in the form of radio waves and X -ray, to which an additional x -ray source caused by electrons and positrons (its antiparticles) accelerated to large energies should be added. To millions of km/h. The fracture itself would have been caused by the irruption of the pulsar at exorbitant speeds. According to astronomer estimation, this speed would be between 1.6 million and 3.2 million kilometers per hour. A study linked to this image was published last year In an article In the magazine Monthly Notices of the Royal Astronomical Society, Change perspective. The image is a memory that sometimes things are not what they seem. The light that our eyes perceive is a tiny fraction of the emissions that exist in the cosmos. Sometimes the invisible to our eyes can be made visible using the correct instruments, while other times the opaque may not be so much if we change perspective. In Xataka | One of the objectives of the Webb Space Telescope was to look for signs of life on other planets. He just found them Image | NASA/CXC/Northwestern Univ./f. Yusef-Zadeh et al; RF/Sarao/Meerkat; NASA/CXC/SAO/N. Wolk

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