What’s Proxima Centauri?

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Proxima Centauri is the closest star to the Sun, located in the Alpha Centauri system. It is a red dwarf star, one-seventh the diameter of the Sun, and is difficult to observe. It is a flare star and is not likely to sustain life due to extreme temperatures and brightness.

Proxima Centauri is a red dwarf star in the Alpha Centauri star system that is notable for being the closest star to the Sun. The discovery of the star’s close location was made in 1915 and it has been a topic of interest and frequent observation ever since. Some people think that when space travel develops to the point where humans can leave the solar system, the Alpha Centauri star system would be a logical place to visit and that Proxima Centauri would likely be the first stop, even though it seems unlikely that the star could sustain life.

Red dwarfs are stars much smaller and cooler than the Sun, with Proxima Centauri being about one-seventh the diameter of the Sun. Because of their size and relative coolness, they are extremely faint; Proxima Centauri can’t even be observed with the naked eye, although it can be captured with high-powered telescopes. This star is also classified as a flare star, meaning that it randomly experiences periods of increased brightness.

This star is located about 4.2 light-years from the Sun. Other stars in the Alpha Centauri system are much brighter, which can make Proxima Centauri difficult to observe. Equipment sensitive enough to observe the star and generate data that could be used to figure out where it was didn’t emerge until the early 20th century, and it wasn’t identified as a flare star until 1951. You can get some idea of where Proxima Centauri is if you happen to be in the Southern Hemisphere, as it appears in the constellation Centaurus, the Centaurus. The Alpha Centauri system appears as a single point of light to the naked eye, making it the brightest point in the constellation.

Because red dwarfs are much cooler than the Sun, they don’t provide much life expectancy. For a planet orbiting Proxima Centauri to support life, it would have to be extremely close to the star, creating a situation where it would be tidally locked. When planets are locked in rotation around stars, one side of the planet always faces the star, creating a situation where half the planet is always in darkness. In another example of tidal locking, Earth’s moon always faces Earth.

If Proxima Centauri supports the planets in a tidally locked orbit, it would be difficult for life to evolve on these planets, as it would have to contend with extreme temperatures on both sides of the planet. The planet’s organisms would also have to contend with periods of sudden and extreme brightness whenever the star shone, making life on the planet rather uncomfortable, in all likelihood.




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