Pitio la 19:26, 30 Machi 2019 tazama chanzo Kipala (majadiliano \| michango) Wanzilishaji wa akaunti, Watumiaji waliothibitishwa, IP block exemptions 52,022 edits No edit summary ← Badilisho lililopita		Pitio la 19:27, 30 Machi 2019 tazama chanzo Kipala (majadiliano \| michango) Wanzilishaji wa akaunti, Watumiaji waliothibitishwa, IP block exemptions 52,022 edits →‎Hali ya nyota Badilisho lijalo →
Mstari 16: [[Umri]] wa Ibuti la Jauza haukutimiza miaka [[milioni]] 10 lakini umeendelea haraka kutokana na [[masi]] yake kubwa. <ref>Levesque E.M. 2010. The physical properties of red supergiants. ''Astronomical Society of the Pacific''. 425 Hot and Cool: Bridging Gaps in Massive Star Evolution ASP Conference Series: '''103'''. [http://arxiv.org/abs/0911.4720]</ref> Ibuti la Jauza imeshaendelea kufikia ngazi za mwisho za [[mageuzi ya nyota]] (''[[:en:stellar evolution\|stellar evolution]]''). Katika kipindi cha miaka milioni 1 ijayo inakadiriwa kutimiza mageuzi yake hadi kulipuka kama [[nyota ya nova]]. <ref>{{cite web\|url=http://www.esa.int/Our_Activities/Space_Science/Betelgeuse_braces_for_a_collision \|title=Betelgeuse braces for a collision \|publisher=ESA \|date=2013-01-22 \|accessdate=2013-01-23 }}</ref> == Tazama pia ==

Ibuti la Jauza : Tofauti kati ya masahihisho