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I made this Content/video using Wondershare Filmora 14 & Adobe Audition with Shure SM58 & Behringer C-1. Please do not upload anywhere else without my permission. You will receive a Copyright Strike if it is uploaded without my permission. Music : YouTube Audio Library Image : Google Exoplanets are discovered using several methods, most commonly through the transit method, which detects the slight dimming of a star's light as a planet passes in front of it. Other key methods include the radial velocity method, which detects a star's gravitational "wobble," and direct imaging, where a telescope directly photographs the exoplanet. Less common techniques involve gravitational microlensing and astrometry. Common discovery methods Transit Method: Astronomers monitor a star's brightness and look for a repeating, periodic dip in light that indicates a planet is passing in front of it. The size of the planet and its orbital period can be determined from the amount of light blocked and the time between transits. Radial Velocity Method: This technique detects the tiny "wobble" in a star's position caused by the gravitational pull of an orbiting planet. By measuring the change in the star's velocity (using a Doppler shift), scientists can infer the mass and orbital period of the planet. Other discovery methods Direct Imaging: This involves using advanced telescopes, often with a coronagraph to block the overwhelming light of the host star, to capture a direct image of the exoplanet itself. This method is most effective for large, hot planets that are far from their stars. Gravitational Microlensing: This method uses the gravity of a foreground star to act as a gravitational lens, magnifying the light of a more distant star behind it. If the foreground star has a planet, its gravity can cause a temporary, unique spike in the background star's brightness. On the morning of 30 June 1908, a massive explosion shook the sparsely-populated Eastern Siberian taiga. It was a visitor from outer space: a comet or asteroid explosively disintegrated in the atmosphere and caused a great amount of damage locally. The Tunguska event caused dust to be thrown high into the atmosphere where it remained for some time. As far away as the UK and Ireland there were reports of bright nigh-time lights caused by sunlight reflecting off the dust. It also affected the climate around the world for several days, as our records show. Some newspaper cuttings are included in the gallery at the bottom of the page Eyewitness Testimony Early in the morning – a little after 7am local time – in the plains of central Siberia populated only by a handful of natives and some Russian settlers, “the sky split in two and fire appeared high and wide over the forest. The split in the sky grew larger, and the entire northern side was covered with fire.” This is an account from an eyewitness who was at Vanavara trading post, some 65 km (40 miles) south of the epicentre. He went on to say that his shirt felt as if it were on fire, the ground shook, and shortly afterwards a great blast pushed him off his chair and threw him a few metres away. Soon after, a hot rushing wind came, “which left traces in the ground like pathways, and it damaged some crops. Later we saw that many windows were shattered, and in the barn, a part of the iron lock snapped.”