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Sažetak
OpisArtist’s impression of Proxima Centauri b shown hypothetically as an arid rocky super-earth.jpg
English: Artist's impression of the exoplanet Proxima Centauri b shown as of a arid (but not completely water-free) rocky Super-Earth. This appearance is one of several possible outcomes of current theories regarding the development of this exoplanet, while the actual look and structure of the planet is known in no ways at this time. Proxima Centauri b is the closest exoplanet to the Sun and also the closest potentially habitable exoplanet as well. It orbits Proxima Centauri, a red dwarf with a surface temperature of 3040 K (thus hotter than light bulbs and therefore whiter, as depicted here). The Alpha Centauri binary system is shown in the background.
Ovo je retuširana slika, što znači da je digitalno izmjenjena u odnosu na svoju izvornu inačicu. Izmjene: The hue of the star was adjusted to the real color of Proxima Centauri as it would appear to a human eye, as well as matching the white areas on the planet from which it is shown to be reflected. Izmjene je napravio: Karl432. Izvornik se može vidjeti [ESO ovdje].
Licencija
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הדמיה של פרוקסימה קנטאורי b מקיף את פרוקסימה קנטאורי.
Reverted to version as of 20:47, 26 August 2016 (UTC). Sorry, the original version is PLAIN WRONG and violates https://commons.wikimedia.org/wiki/Commons:Project_scope : "Must be realistically useful for an educational purpose". We are no talking about...