FrancophonIA/Vikidia-EnFr huggingface dataset:
Proxima Centauri is a red dwarf star that is likely a part of the Alpha Centauri star system and is the closest star to the Sun at a distance of 
4.22 light-years (3.99×1013 km; 2.48×1013 mi). It is in the constellation of Centaurus.

Proxima Centauri was found to share the same proper motion as Alpha Centauri in 1915 by Robert Innes while he was Director of the Union Observatory in Johannesburg, South Africa.

In 1951, Harlow Shapley said that Proxima Centauri was a flare star. Recorded photographs showed that the star became measurably brighter about 8% of the time, making it the most active flare star then found.

Red dwarfs are usually far too faint to be seen with the naked eye, that means without a telescope. Proxima Centauri has an apparent magnitude of 11 while its absolute magnitude is a very dim 15.5. Even from Alpha Centauri A or B, Proxima would only be seen as a 5th magnitude star.

Proxima Centauri has been the closest star to the Sun for about the last 32,000 years. Barnard's Star will make its closest approach to the Sun around AD 11,700, when it approaches to within about 3.8 light-years.[1] However, at that time, it will not be the nearest star, since Proxima Centauri will then have moved even closer to the Sun.[2]

In 2016, a exoplanet was found by the European Southern Observatory around Proxima Centauri, Proxima Centauri b (or Proxima b). It was found in the habitable zone, and was thought to be Earth-like, with an ESI of 0.87.[3] While being Earth-like, it may not be habitable on the surface, since Proxima Centauri gives off strong solar flares and high solar winds, which could strip away parts of the atmosphere of the planet, making it less habitable.[4]

In October of 2016, scientists at France's CNRS research institute said that the planet may have oceans on its surface, and a thin atmosphere. If this idea is true or not is not known.[5]