The space launch system, our large rocket under development, obviously has the characteristics to lift heavy weights, but almost as important to science is that it has a very broad launch path and therefore a future telescope that will have the ability to collect light. The ability to detect and measure biosciences, if you like, a very, very faint planet around a very bright star would require a large collection area and advanced instrumentation, and a telescope of this size if you think of James It's like the Webb Space Telescope here -that will be launched, and I know President Smith, you saw a model in which everything is folded like origami and turned into a launch route for a very large Orion V rocket. Then, besides that, the New World telescope - just like it was described in the Decade Review - will be a very large telescope in which the James Webb Space Telescope has a diameter of 6-1 / 2 meters, about 20 feet, for In fact, by detecting signs of life, if any, on a planet around a relatively nearby star, we should probably travel 16 or 20 meters in diameter, which is what you mean in your question about a space launch system. 

The telescope also explores every object in our solar system, from Mars to frozen objects outside Pluto. Over the course of his life, Webb will search for hundreds, if not thousands, of planets orbiting distant stars. 

One of the first planetary systems that Weber will show is the TRAPPIST-1 system, which is 39 light years away. It has seven planets, three of which are located in the blonde zone and orbit a dwarf star. Its light is not too bright, making it easier to determine the composition of the atmosphere. As a bonus, the instrument will also use gravitational microlenses-tiny changes in the background light of stars-to potentially detect millions of exoplanets. 

The new James Webb Space Telescope will collect infrared light from distant corners of space, allowing scientists to see farther than ever. The James Webb Space Telescope, years behind schedule and billions of euros over budget and 100 times more powerful than the famous Hubble, is finally ready for a crucial mission to observe the near-Big Bang that space has created. 

The revolutionary rookie space observatory is ready to search for exoplanets, which are unprecedented exoplanets. So far, we have discovered more than 4,000 exoplanets, and it is estimated that there are billions of them in the Milky Way galaxy alone. It will also enable scientists to understand the various characteristics of exoplanets, from climate and seasons to atmospheric composition. 

Equipped with a powerful set of tools, it will allow you to see farther than any other telescope, and will be used to unlock the mysteries of our solar system, explore the origin of the universe, and push the boundaries of scientific knowledge. Under the leadership of the European Space Agency, it will target sources of gravitational waves that are not available to Earth probes, such as the collision of supermassive black holes and the merging of dense objects in our galaxy. The telescope is scheduled to launch in 2027 and will explore millions of galaxies by mapping our cosmic environment. 



As the first general-purpose infrared telescope, Weber will take us into the universe of the first stars and galaxies that formed only 100 million years ago. Pierre Ferruy, a researcher on the European Space Agency’s Webb project, explained that when a planet passes in front of a star, MIRI will be able to read the infrared signature of light filtered through various substances in the planet’s atmosphere. We don’t know how many habitable planets there are, let alone the Earth, but Weber will be able to use spectroscopy to knock down the starlight that passes through these atmospheres and study the chemical composition of the atmospheres of nearby exoplanets.