Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q7783074> ?p ?o }
Showing triples 1 to 20 of
20
with 100 triples per page.
- Q7783074 subject Q7033720.
- Q7783074 subject Q7476780.
- Q7783074 abstract "In astrophysics, the thermal time scale or Kelvin-Helmholtz time scale is the approximate time it takes for a star to radiate away its total kinetic energy content at its current luminosity rate. Along with the nuclear and dynamical time scales, it is used to estimate the length of time a particular star will remain in a certain phase of its life and its lifespan if hypothetical conditions are met. In reality, the lifespan of a star is greater than what is estimated by the thermal time scale because as one fuel becomes scarce, another will generally take its place--hydrogen burning gives way to helium burning, which is replaced by carbon burning.".
- Q7783074 wikiPageWikiLink Q1057093.
- Q7783074 wikiPageWikiLink Q105902.
- Q7783074 wikiPageWikiLink Q1075685.
- Q7783074 wikiPageWikiLink Q11423.
- Q7783074 wikiPageWikiLink Q173817.
- Q7783074 wikiPageWikiLink Q18373.
- Q7783074 wikiPageWikiLink Q336225.
- Q7783074 wikiPageWikiLink Q37547.
- Q7783074 wikiPageWikiLink Q46276.
- Q7783074 wikiPageWikiLink Q462926.
- Q7783074 wikiPageWikiLink Q523.
- Q7783074 wikiPageWikiLink Q525.
- Q7783074 wikiPageWikiLink Q7033720.
- Q7783074 wikiPageWikiLink Q7068201.
- Q7783074 wikiPageWikiLink Q7476780.
- Q7783074 comment "In astrophysics, the thermal time scale or Kelvin-Helmholtz time scale is the approximate time it takes for a star to radiate away its total kinetic energy content at its current luminosity rate. Along with the nuclear and dynamical time scales, it is used to estimate the length of time a particular star will remain in a certain phase of its life and its lifespan if hypothetical conditions are met.".
- Q7783074 label "Thermal time scale".