Matches in DBpedia 2015-10 for { <http://dbpedia.org/resource/Kombayashi–Ingersoll_limit> ?p ?o }
Showing triples 1 to 30 of
30
with 100 triples per page.
- Kombayashi–Ingersoll_limit abstract "In planetary science, the Kombayashi–Ingersoll limit represents the maximum solar flux a planet can handle without a runaway greenhouse effect setting in.For planets with temperature-dependent sources of greenhouse gases such as liquid water and optically thin atmospheres the outgoing longwave radiation curve (which indicates how fast energy can be radiated away by the planet) flattens at high temperatures, reaching a horizontal asymptote - the Kombayashi–Ingersoll limit itself. Since the equilibrium temperature is the intersection of this curve and a horizontal line representing solar flux, for fluxes above this point the planet heats up indefinitely. Kasting estimated the limit for Earth to 320 Watts per square meter.The limit is relevant for estimating the inner edge of the circumstellar habitable zone. However, the limit also depends on the surface gravity of the planet, making heavy worlds somewhat more resistant to the runaway effect.".
- Kombayashi–Ingersoll_limit wikiPageID "40545404".
- Kombayashi–Ingersoll_limit wikiPageLength "2154".
- Kombayashi–Ingersoll_limit wikiPageOutDegree "10".
- Kombayashi–Ingersoll_limit wikiPageRevisionID "653732919".
- Kombayashi–Ingersoll_limit wikiPageWikiLink Asymptote.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Category:Climate_feedbacks.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Category:Climatology.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Category:Planetary_science.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Circumstellar_habitable_zone.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Greenhouse_gas.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Greenhouse_gases.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Optical_depth.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Outgoing_longwave_radiation.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Planetary_science.
- Kombayashi–Ingersoll_limit wikiPageWikiLink Runaway_greenhouse_effect.
- Kombayashi–Ingersoll_limit wikiPageWikiLinkText "Kombayashi–Ingersoll limit".
- Kombayashi–Ingersoll_limit hasPhotoCollection Kombayashi–Ingersoll_limit.
- Kombayashi–Ingersoll_limit wikiPageUsesTemplate Template:Orphan.
- Kombayashi–Ingersoll_limit wikiPageUsesTemplate Template:Reflist.
- Kombayashi–Ingersoll_limit subject Category:Climate_feedbacks.
- Kombayashi–Ingersoll_limit subject Category:Climatology.
- Kombayashi–Ingersoll_limit subject Category:Planetary_science.
- Kombayashi–Ingersoll_limit comment "In planetary science, the Kombayashi–Ingersoll limit represents the maximum solar flux a planet can handle without a runaway greenhouse effect setting in.For planets with temperature-dependent sources of greenhouse gases such as liquid water and optically thin atmospheres the outgoing longwave radiation curve (which indicates how fast energy can be radiated away by the planet) flattens at high temperatures, reaching a horizontal asymptote - the Kombayashi–Ingersoll limit itself.".
- Kombayashi–Ingersoll_limit label "Kombayashi–Ingersoll limit".
- Kombayashi–Ingersoll_limit sameAs m.0x2fshd.
- Kombayashi–Ingersoll_limit sameAs Q17119447.
- Kombayashi–Ingersoll_limit sameAs Q17119447.
- Kombayashi–Ingersoll_limit wasDerivedFrom Kombayashi–Ingersoll_limit?oldid=653732919.
- Kombayashi–Ingersoll_limit isPrimaryTopicOf Kombayashi–Ingersoll_limit.