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IUT Michel de Montaigne

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ASTRONOMICAL DISCOVERIES Internet watch Thomas KERAMPRAN- 2A GIDO

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Education Material about Astronomy Presentation Template If you want to buy this presentation template, please visit http://madlis.com Good design gets out of the way of the content you are sharing. It helps your audience focus on the content itself instead of the design. But, it's no secret that most people dislike giving presentations. The dread of public speaking consistently ranks among the greatest fears in public surveys. This presentation slides can help you reduce the anxiety involved with giving a presentation. Well-designed slides not only build your own confidence, they make your key points clearer to the audience.

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Exploring Exoplanets and Extraterrestrial Atmospheres: An Introduction Exoplanets" are planets outside of our Solar System, and their atmospheres can provide invaluable information about the formation and evolution of distant worlds. This article discusses the scientific methods used to investigate exoplanet atmospheres, and the implications of our findings for astrobiology. Exoplanets, or planets that orbit stars outside of our solar system, are studied by astronomers using a variety of methods. One popular method is called the radial velocity method, which measures the wobble of a star caused by the gravitational pull of an orbiting planet. Another method is the transit method, which detects a planet when it crosses in front of its star and causes a temporary dip in the star's brightness. Once a planet is detected, scientists can study its atmosphere by analyzing the light that passes through it as the planet transits its star. By studying the planet's spectrum, scientists can determine the composition of its atmosphere, including the presence of gases such as water vapor, methane, and carbon dioxide. In some cases, scientists can also use this method to study the planet's temperature and weather patterns. Another way to study exoplanet atmospheres is direct imaging. This method involves using telescopes to directly observe the planet as it orbits its star. This method is more challenging because the planet is much fainter than the star, but it allows scientists to study the planet's surface features and atmospheric conditions in more detail. The study of exoplanet atmospheres is a rapidly growing field with many new discoveries being made. This can help us understand the potential habitability of other planets and the possibility of life existing beyond our solar system. What is an Exoplanets? Exoplanets are planets that orbit stars outside of our solar system. They come in a wide variety of sizes and orbits, from large gas giants like Jupiter to small, rocky planets like Earth. Some exoplanets orbit their stars very closely, while others orbit at much greater distances. Some exoplanets are even in a binary star systems, where two stars orbit around each other and the exoplanet orbits both of them. The study of exoplanets is a rapidly growing field that has seen many new discoveries and advancements in recent years. This is due to the development of new technologies and instruments that have made it possible to detect and study exoplanets in greater detail. For example, the radial velocity method and transit method are two common techniques that have been used to detect exoplanets. The radial velocity method measures the wobble of a star caused by the gravitational pull of an orbiting planet, while the transit method detects a planet when it crosses in front of its star and causes a temporary dip in the star's brightness. As technology continues to improve, scientists will be able to study the exoplanet's atmosphere in more detail, and

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This article aims to present the contribution of astronomy and, in particular, the James Webb telescope to the advancement of knowledge about the Universe. Astronomy is the study of the Universe that exists beyond Earth's atmosphere. This includes objects that can be seen with the naked eye, such as the Sun, Moon, planets and stars. It also includes celestial bodies that can only be observed with telescopes or other instruments, such as distant galaxies and small particles, and it also includes things we cannot see, such as dark matter and dark energy. The main goal of the James Webb Telescope is to peer into the past, looking back a few hundred thousand years after the Big Bang. One of the James Webb Telescope's key abilities is its ability to look back through time to the beginning of the Universe, observing the first galaxies and stars. The telescope, which is 1.5 million kilometers from Earth, has already spotted the most distant and oldest galaxy found so far. The James Webb Telescope also made the first detection of a “molecule of life”. The James Webb super telescope, with its great discoveries, shows the importance of the telescope by revealing, with unexpected speed, a series of information that can call cosmological theories into question.

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