How Are Planets Detected Through Transit Method?

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The transit method for detecting planets involves observing the dimming of a star's light when a planet passes in front of it, primarily using visible-light photometry. This technique can be performed with small amateur telescopes, provided the planet's orbital plane is aligned favorably for observation. The size ratio of the planet to its star affects detection, with noise creating a lower limit on the size of detectable planets. The method relies on precise measurements to distinguish the slight changes in brightness caused by the transit. Overall, the transit method is a viable way to discover extrasolar planets, especially when conditions are optimal.
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How exactly is this done? Is it done in the visible wavelengths or in the radio? Also, how small can the (planet size)/(sun size) ratio be. I'd expect that given noise especially, there's a definite lower limit.
 
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Just do a Google search on the relevant terms (extrasolar, planet, transit, etc) and you will get all the information you need. It's possible to discover extrasolar planets through visible-light photometry with small amateur telescopes. The trick is that the plane of the planets' orbits have to be pointed pretty much at us, so we can see the planet superimposed over its star.
 
UC Berkely, December 16, 2025 https://news.berkeley.edu/2025/12/16/whats-powering-these-mysterious-bright-blue-cosmic-flashes-astronomers-find-a-clue/ AT 2024wpp, a luminous fast blue optical transient, or LFBOT, is the bright blue spot at the upper right edge of its host galaxy, which is 1.1 billion light-years from Earth in (or near) a galaxy far, far away. Such objects are very bright (obiously) and very energetic. The article indicates that AT 2024wpp had a peak luminosity of 2-4 x...

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