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- ...en-Institut Heidelberg | date=March 4, 1998 | work=ARI Database for Nearby Stars |url=http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c01453.h ...wo-Tenths catalogue|LTT]] 15309, Munich 15040, [[List of nearest stars|Proxima Ophiuchi]], [[Variable star designation|V2500 Ophiuchi]], ''[[Latin ...30 KB (4,146 words) - 19:05, 17 August 2009
- | title =SIMBAD query result: V* V645 Cen -- Flare Star | variable=[[Flare star]] ...43 KB (6,190 words) - 12:18, 5 February 2010
- ...ght|300px|The [[Pleiades (star cluster)|Pleiades]], an [[open cluster]] of stars in the [[constellation]] of [[Taurus (constellation)|Taurus]]. ''[[NASA]] p ...ghtest stars gained proper names. Extensive [[star catalogue|catalogues of stars]] have been assembled by astronomers, which provide standardized [[star des ...96 KB (14,170 words) - 15:20, 20 August 2009
- ...he [[Milky Way]] at the time and was thus moving against a denser field of stars. Neptune's next occultation, on 12 September 1983, resulted in a possible d ..." /> Courage, a very faint arc found during the Voyager flyby, was seen to flare in brightness in 1998, while more recently it was back to its usual dimness ...29 KB (4,327 words) - 19:38, 16 August 2009
- ...G.; McLean, B.; Spagna, A. |title=The Second Guide Star Catalogue and Cool Stars |work=Perkins Observatory |url=http://adsabs.harvard.edu/abs/2001udns.conf. ...d be enriched with these atoms. The oldest stars contain few metals, while stars born later have more. This high metallicity is thought to have been crucial ...82 KB (12,276 words) - 02:46, 16 June 2010
- ...these caverns may be protected from micrometeoroids, UV radiation, [[solar flare]]s and high energy particles that bombard the planet's surface.<ref>{{cite {{cite web | title = MIRA's Field Trips to the Stars Internet Education Program ...105 KB (15,836 words) - 04:41, 17 August 2009