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- S0–102 abstract "S0–102 is a star that is located very close to the centre of the Milky Way, near the radio source Sagittarius A*, orbiting it with an orbital period of 11.5 years. As of 2012 it is the star with the shortest known period orbiting the black hole at the centre of the Milky Way. This now beats the record set by S0–2 of 16 years. The star was identified by a University of California, Los Angeles team headed by Andrea M. Ghez. At its perihelion, its speed exceeds 1% of the speed of light.Its position in the sky has been monitored from 2000 to 2012 using the W. M. Keck telescope. One complete orbit has been observed. From Earth's current perspective, it travels in a clockwise direction. Having observed two stars orbiting through complete periods around the centre, the gravitational potential of SgrA* can be established. Possibly there is a great deal of dark matter around the orbits of these stars. Also general relativistic effects due to gravitational redshift should become observable.".
- S0–102 wikiPageID "37240862".
- S0–102 wikiPageLength "3382".
- S0–102 wikiPageOutDegree "12".
- S0–102 wikiPageRevisionID "678484953".
- S0–102 wikiPageWikiLink Andrea_M._Ghez.
- S0–102 wikiPageWikiLink Category:Sagittarius_(constellation).
- S0–102 wikiPageWikiLink File:SO-102_Orbital_Plot.jpg.
- S0–102 wikiPageWikiLink Gravitational_potential.
- S0–102 wikiPageWikiLink Gravitational_redshift.
- S0–102 wikiPageWikiLink Perihelion.
- S0–102 wikiPageWikiLink Perihelion_and_aphelion.
- S0–102 wikiPageWikiLink S2_(star).
- S0–102 wikiPageWikiLink Sagittarius_(constellation).
- S0–102 wikiPageWikiLink Sagittarius_A*.
- S0–102 wikiPageWikiLink Speed_of_light.
- S0–102 wikiPageWikiLink University_of_California,_Los_Angeles.
- S0–102 wikiPageWikiLink W._M._Keck_Observatory.
- S0–102 wikiPageWikiLink W._M._Keck_telescope.
- S0–102 wikiPageWikiLinkText "S0–102".
- S0–102 appmagK "17.2".
- S0–102 constell Sagittarius_(constellation).
- S0–102 distLy "25900".
- S0–102 distPc "7940".
- S0–102 eccentricity "0.68".
- S0–102 hasPhotoCollection S0–102.
- S0–102 inclination "151".
- S0–102 name "Sagittarius A*".
- S0–102 node "175".
- S0–102 periarg "185".
- S0–102 periastron "2009.5".
- S0–102 period "11.5".
- S0–102 wikiPageUsesTemplate Template:Cite_web.
- S0–102 wikiPageUsesTemplate Template:Reflist.
- S0–102 wikiPageUsesTemplate Template:Starbox_astrometry.
- S0–102 wikiPageUsesTemplate Template:Starbox_begin.
- S0–102 wikiPageUsesTemplate Template:Starbox_catalog.
- S0–102 wikiPageUsesTemplate Template:Starbox_character.
- S0–102 wikiPageUsesTemplate Template:Starbox_end.
- S0–102 wikiPageUsesTemplate Template:Starbox_observe.
- S0–102 wikiPageUsesTemplate Template:Starbox_reference.
- S0–102 wikiPageUsesTemplate Template:Starbox_visbin.
- S0–102 wikiPageUsesTemplate Template:Stars_of_Sagittarius.
- S0–102 subject Category:Sagittarius_(constellation).
- S0–102 type CelestialBody.
- S0–102 type Place.
- S0–102 type Star.
- S0–102 type Location.
- S0–102 type Place.
- S0–102 type Thing.
- S0–102 comment "S0–102 is a star that is located very close to the centre of the Milky Way, near the radio source Sagittarius A*, orbiting it with an orbital period of 11.5 years. As of 2012 it is the star with the shortest known period orbiting the black hole at the centre of the Milky Way. This now beats the record set by S0–2 of 16 years. The star was identified by a University of California, Los Angeles team headed by Andrea M. Ghez.".
- S0–102 label "S0–102".
- S0–102 sameAs S0-102.
- S0–102 sameAs S0-102.
- S0–102 sameAs m.0n53nth.
- S0–102 sameAs S0-102.
- S0–102 sameAs Q4387860.
- S0–102 sameAs Q4387860.
- S0–102 sameAs S0-102.
- S0–102 wasDerivedFrom S0–102?oldid=678484953.
- S0–102 isPrimaryTopicOf S0–102.
- S0–102 name "S0–102".