Pagbabago noong 17:53, 20 Oktubre 2020 baguhin SeñorPastel (usapan \| ambag) 6 edits m typo, dagdag na impormasyon Tatak: Pagbabagong biswal Binago sa mobile Pagbabago sa web gamit mobile ← Nakaraang pagkakaiba		Pagbabago noong 02:44, 6 Agosto 2021 baguhin i-undo InternetArchiveBot (usapan \| ambag) 31,924 edits Rescuing 2 sources and tagging 0 as dead.) #IABot (v2.0.8 Susunod na pagkakaiba →
Linya 5: \| title=Latin Resources \| publisher =Joint Association of Classical Teachers \| accessdate=2007-07-15}}</ref> ay isang [[pulang duwende]] na may layong 4.24 [[sinag-taon]] mula sa Araw, na nasa loob ng ''[[G-cloud]]'', sa [[konstelasyon]] ng [[Centaurus]].<ref>{{cite web \| url=http://interstellar.jpl.nasa.gov/interstellar/probe/introduction/neighborhood.html \| title=Our Local Galactic Neighborhood \| publisher=NASA \| date=February 8, 2000 \| accessdate=2013-03-22 \| archive-date=2013-11-21 \| archive-url=https://web.archive.org/web/20131121061128/http://interstellar.jpl.nasa.gov/interstellar/probe/introduction/neighborhood.html \| url-status=dead }}</ref><ref>{{cite web \| first=Paul \| last=Glister \| date=September 1, 2010 \| url=http://www.centauri-dreams.org/?p=14203 \| title=Into the Interstellar Void \| publisher=Centauri Dreams \| accessdate=2013-03-22 }}</ref> Natuklasan ito noong 1915 ng isang [[Suwiso (tao)\|Suwisong]] [[astronomo\|astrónomo]] na si [[Robert Innes]], ang Direktor ng [[Union Observatory]] sa Timog Aprika, at naging [[List of nearest stars\|pinakamalapit]] na natuklasang bituin mula sa [[Araw]],<ref name="ESO2003">{{cite news \| author=Kervella, Pierre; Thevenin, Frederic \| title=A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars \| publisher=ESO \| date=2003-03-15 \| url=http://www.eso.org/public/outreach/press-rel/pr-2003/pr-05-03.html \| accessdate=2007-07-09 \| accessdate=2007-07-09 }}</ref> kahit na malabo itong makita ng mga mata, na may [[maliwanag na kalakhan]] na 11.05. May layo itong 0.237 ± 0.011 ly (15,000 ± 700 [[yunit na pang-astronomiya\|AU]] sa ikalawa at ikatlong pinakamalapit na bituin, na kung saan ay bumubuo sa [[dalawang bituin\|dalawahang]] [[Alpha Centauri]].<ref name="apj132">{{cite journal▼ \| archive-date=2008-06-16 \| archive-url=https://web.archive.org/web/20080616125016/http://www.eso.org/public/outreach/press-rel/pr-2003/pr-05-03.html \| url-status=dead ▲ ~~\| accessdate=2007-07-09~~ }}</ref> kahit na malabo itong makita ng mga mata, na may [[maliwanag na kalakhan]] na 11.05. May layo itong 0.237 ± 0.011 ly (15,000 ± 700 [[yunit na pang-astronomiya\|AU]] sa ikalawa at ikatlong pinakamalapit na bituin, na kung saan ay bumubuo sa [[dalawang bituin\|dalawahang]] [[Alpha Centauri]].<ref name="apj132">{{cite journal \| author=Wertheimer, Jeremy G.; Laughlin, Gregory \| title=Are Proxima and α Centauri Gravitationally Bound?

Proxima Centauri: Pagkakaiba sa mga binago