Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q2403963> ?p ?o }
Showing triples 1 to 41 of
41
with 100 triples per page.
- Q2403963 subject Q10649.
- Q2403963 subject Q7465903.
- Q2403963 subject Q8284795.
- Q2403963 subject Q8503558.
- Q2403963 abstract "HD 36960 is a B-type main-sequence star in the constellation Orion. At an apparent magnitude of +4.78 it is easily visible to the naked eye in many areas, though in most urban areas it cannot be seen due to light pollution. The star is also massive along with many other stars of Orion. At over 15 solar masses, it shines with nearly 40,000 times the Sun's luminosity due to its high surface temperature (29,000K). Due to its high mass, the star will expand into a blue supergiant in the next few million years and eventually a red supergiant after that. During this phase, the star will probably be a second or third magnitude star and easily viable to the naked eye (probably about as bright as Kappa Orionis (Saiph) is today). The ultimate fate of the star is most likely a Type II supernova. When it has fully exhausted its fuel, the core will produce heavier elements like Iron. Then, its core will become unstable and collapse with the rest of the star expanding outward in a luminous explosion. Such an event from this distance would shine brightly in Earth's sky. Assuming this event is identical to SN 1054, it would shine with an apparent magnitude of -8.71, about 1/40 as bright as the full moon despite its distance of over 1,800 light years.".
- Q2403963 thumbnail Orion_constellation_map.png?width=300.
- Q2403963 wikiPageExternalLink sim-id?Ident=HD+36960&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id.
- Q2403963 wikiPageWikiLink Q1048372.
- Q2403963 wikiPageWikiLink Q1049029.
- Q2403963 wikiPageWikiLink Q10649.
- Q2403963 wikiPageWikiLink Q111130.
- Q2403963 wikiPageWikiLink Q124313.
- Q2403963 wikiPageWikiLink Q14028.
- Q2403963 wikiPageWikiLink Q179600.
- Q2403963 wikiPageWikiLink Q180644.
- Q2403963 wikiPageWikiLink Q180892.
- Q2403963 wikiPageWikiLink Q2703.
- Q2403963 wikiPageWikiLink Q32037.
- Q2403963 wikiPageWikiLink Q3450.
- Q2403963 wikiPageWikiLink Q405.
- Q2403963 wikiPageWikiLink Q499138.
- Q2403963 wikiPageWikiLink Q531.
- Q2403963 wikiPageWikiLink Q555846.
- Q2403963 wikiPageWikiLink Q556.
- Q2403963 wikiPageWikiLink Q5898.
- Q2403963 wikiPageWikiLink Q677.
- Q2403963 wikiPageWikiLink Q7465903.
- Q2403963 wikiPageWikiLink Q8284795.
- Q2403963 wikiPageWikiLink Q8503558.
- Q2403963 wikiPageWikiLink Q8860.
- Q2403963 wikiPageWikiLink Q8928.
- Q2403963 type Place.
- Q2403963 type CelestialBody.
- Q2403963 type Location.
- Q2403963 type Place.
- Q2403963 type Star.
- Q2403963 type Thing.
- Q2403963 comment "HD 36960 is a B-type main-sequence star in the constellation Orion. At an apparent magnitude of +4.78 it is easily visible to the naked eye in many areas, though in most urban areas it cannot be seen due to light pollution. The star is also massive along with many other stars of Orion. At over 15 solar masses, it shines with nearly 40,000 times the Sun's luminosity due to its high surface temperature (29,000K).".
- Q2403963 label "HD 36960".
- Q2403963 depiction Orion_constellation_map.png.
- Q2403963 name "HD 36960".