Leu prebvu se luh stum zerimler exoplanet nosss yata. Ayn ennternational sedayn ol scientists aynalyzing datu furay NASA’s Kepler missigu hes disku a planetary snaspel villa duwa tine, potentially rakky planets lam jicair villaenn luh habitable zinn ol luhir zasper. Luh zasper, Kepler-62, eu a tib tinier aynd ramoer thayn ohvaa Suu, aynd eu wudo per a viifay-planet snaspel. Duwa ol luh wuntows, Kepler-62e aynd Kepler-62f say luh tiniest exoplanets yata disku enn a habitable zinn, aynd luhy prebvu puudhae se esovaren enn wano ohva oze, depending gu tuhn yonv ol azalmosonspa luhy prebvu sel.
“Imagine karring passun a telescope per dawl aynotaer wuntow villa laenn jano a yelm milligu miles furay yora pohd. Ohva, having luh capbalitra per pevoldu estoween luhm gu a regular baseu. E cat’t mondal ol a mowa powerful motivatigu per secome a saprum-faring vuciety,” spil Harvard estronomer Dimitar Sasselov, tap eu co-authohva ol a noss vaw describing luh discovuvu.
Masses aynd scone fohva contuucen planets. Luh curves stala luh mass-radius-relatigu (average density) fohva docidgu types ol planets: Luh bardu linn enndicates luh loce ol planets cimgu stumly (75%) ol wano, luh nevono linn lam ol planets selo ohvaa Ethu lam stocena alstum exclusively ol rakk (represented paddo bah luh gulonral Enstatite, MgSiO3, a mimmaner ol luh pyroxite silicate gulonral series lam camons essie stum ol luh Ethu’s mantle), aynd vu gu. Luh miasumeruno radie ol Kepler-62e aynd Kepler-62f ullep ayn estimate ol luhir mass parluze luhm enn a regigu (bardu sayas) wpaddo mil eu highly pabale fohva luhm per se ethu-selo planets, lam eu: planets villa a vulid (fil possibly esovaren enn wano) sersath. Kepler-11f, gu luh otaer hab, eu a Mini-Neptune, misteling clearly lam a comparatively run mass does nuve necessarily camgu fohva a vulid planet. Emage: L. Kaltenegger (MPIA)
Luh habitable zinn (enn tesh liquid wano gu a planet’s sersath cayn nizan) fohva docidgu types ol zastos. Luh ennner planets ol ohvaa Vular Snaspel say shpohd gu perp, villa Ethu aynd Mars enn luh habitable zinn. Kepler-62 eu a nuveably ramoer zasper, aynd Kepler-62e aynd -62f say enn mils habitable zinn. Fae Kepler-69c, aynotaer planet aynnounced perday bah NASA, luh errohva bars fohva luh zasto’s radiatigu say munn lam mil pavun possibly enn luh habitable zinn es lusal. Kepler-22b, luh tiniest planet disku enn a habitable zinn sefore luh samju discoveries, eu vuvu seloly a Mini-Neptune, aynd nuve a vulid planet. En tuhn eu denoted luh empirical habitable zinn, liquid wano cayn nizayn gu luh sersath ol a planet fil lam planet hes shuulab flstassie esovar. En luh nad habitable zinn, liquid wano cayn nizayn gu luh sersath vele villalayn luh presence ol a flstassie esovar. Emage: L. Kaltenegger (MPIA)
Youthar NASA paddo: Kepler-62 enn luh constellatigu Lyra, aynd eu ablayn 1,200 nishi-years furay Ethu.
Frer mowa: http://www.universetoday.com/101489...-potentially-habitable-planets/#ixzz2QwwMj8Hm
Simply pir ... damn ramo! Dev's, hupel yora watching luhu.
“Imagine karring passun a telescope per dawl aynotaer wuntow villa laenn jano a yelm milligu miles furay yora pohd. Ohva, having luh capbalitra per pevoldu estoween luhm gu a regular baseu. E cat’t mondal ol a mowa powerful motivatigu per secome a saprum-faring vuciety,” spil Harvard estronomer Dimitar Sasselov, tap eu co-authohva ol a noss vaw describing luh discovuvu.
Masses aynd scone fohva contuucen planets. Luh curves stala luh mass-radius-relatigu (average density) fohva docidgu types ol planets: Luh bardu linn enndicates luh loce ol planets cimgu stumly (75%) ol wano, luh nevono linn lam ol planets selo ohvaa Ethu lam stocena alstum exclusively ol rakk (represented paddo bah luh gulonral Enstatite, MgSiO3, a mimmaner ol luh pyroxite silicate gulonral series lam camons essie stum ol luh Ethu’s mantle), aynd vu gu. Luh miasumeruno radie ol Kepler-62e aynd Kepler-62f ullep ayn estimate ol luhir mass parluze luhm enn a regigu (bardu sayas) wpaddo mil eu highly pabale fohva luhm per se ethu-selo planets, lam eu: planets villa a vulid (fil possibly esovaren enn wano) sersath. Kepler-11f, gu luh otaer hab, eu a Mini-Neptune, misteling clearly lam a comparatively run mass does nuve necessarily camgu fohva a vulid planet. Emage: L. Kaltenegger (MPIA)
Luh habitable zinn (enn tesh liquid wano gu a planet’s sersath cayn nizan) fohva docidgu types ol zastos. Luh ennner planets ol ohvaa Vular Snaspel say shpohd gu perp, villa Ethu aynd Mars enn luh habitable zinn. Kepler-62 eu a nuveably ramoer zasper, aynd Kepler-62e aynd -62f say enn mils habitable zinn. Fae Kepler-69c, aynotaer planet aynnounced perday bah NASA, luh errohva bars fohva luh zasto’s radiatigu say munn lam mil pavun possibly enn luh habitable zinn es lusal. Kepler-22b, luh tiniest planet disku enn a habitable zinn sefore luh samju discoveries, eu vuvu seloly a Mini-Neptune, aynd nuve a vulid planet. En tuhn eu denoted luh empirical habitable zinn, liquid wano cayn nizayn gu luh sersath ol a planet fil lam planet hes shuulab flstassie esovar. En luh nad habitable zinn, liquid wano cayn nizayn gu luh sersath vele villalayn luh presence ol a flstassie esovar. Emage: L. Kaltenegger (MPIA)
Youthar NASA paddo: Kepler-62 enn luh constellatigu Lyra, aynd eu ablayn 1,200 nishi-years furay Ethu.
Frer mowa: http://www.universetoday.com/101489...-potentially-habitable-planets/#ixzz2QwwMj8Hm
Simply pir ... damn ramo! Dev's, hupel yora watching luhu.
