Difference between revisions 716502 and 763764 on astwiki[[Archivu:Sirius A and B artwork.jpg|right|thumb|300px|Recreación artística de Sirius A (estrella grande) y Sirius B (Credit:NASA).]] '''Sirius''' (tamién conocida como [[estrella]] del Can, grupu estelar ''Canis maior'') ye la más rellumante del cielu nocherniegu (-1,43m). Esta estrella ye posible vela dende cada rexón poblada de la [[Tierra]], nel hemisferiu norte, ye un vértiz del [[Hexágonu ivernal]]. Ye un astru blancu que ta asitiáu a 8,7 años lluz, si(contracted; show full) == Enllaces Esternos == * [http://www.astro.uiuc.edu/~kaler/sow/sirius.html Professor Kaler's webpage on Sirius] * [http://apod.nasa.gov/apod/ap001006.html APOD of Sirius B in x-ray] * [http://chandra.harvard.edu/chronicle/0400/sirius_part2.html Discussion on Dogon issue] [[Categoría:Estrelles]] ⏎ ⏎ {{Enllaz AD|de}} {{Enllaz AD|en}} {{Enllaz AD|tr}} All content in the above text box is licensed under the Creative Commons Attribution-ShareAlike license Version 4 and was originally sourced from https://ast.wikipedia.org/w/index.php?diff=prev&oldid=763764.
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