https://padlet.com/corra_flanagan/lgfix4d0c3f6 By Corra Flanagan en-us 2016-12-11 17:08:13 UTC 2024-11-16 09:59:09 UTC hello@padlet.com corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143002003 What is a Dark Nebula ]]> 2016-12-11 17:22:22 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143002003 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003022 Stars form inside relatively dense concentrations of interstellar gas and dust known as molecular clouds. These regions are extremely cold. At these temperatures, gases become molecular meaning that atoms bind together. CO and H2 are the most common molecules in interstellar gas clouds. The deep cold also causes the gas to clump to high densities. When the density reaches a certain point, stars form.]]> 2016-12-11 17:38:25 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003022 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003225 contain dense cosmic dust and gas where star formation takes pace.]]> 2016-12-11 17:41:22 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003225 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003435 small patches of nebulosity associated with newly born stars, and are formed when narrow jets of gas ejected by those stars collide with nearby clouds of gas and dust at speeds of several hundred kilometres per second.]]> 2016-12-11 17:44:32 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003435 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003703  two continuous flows of gas from the poles of a star. ]]> 2016-12-11 17:48:15 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143003703 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004048 they use infrared to stud the heat energy the object in space give off. ]]> 2016-12-11 17:53:29 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004048 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004208 Stars form inside relatively dense concentrations of interstellar gas and dust known as molecular clouds.]]> 2016-12-11 17:56:04 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004208 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004364 Energy flows from the hot core to the cooler surface as radiation or as convection.]]> 2016-12-11 17:58:35 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004364 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004704 stars use the proton-proton chain]]> 2016-12-11 18:03:19 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143004704 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143005312  Massive stars evolve quicker than light stars. he relationship between the luminosity and mass was explained using basic principles of how compressed gases behave. Slight increases in mass produce large increases in the luminosities of stars.]]> 2016-12-11 18:12:01 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143005312 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143103551 jets of gas in the eagle nebula]]> 2016-12-12 13:29:10 UTC https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143103551 corra_flanagan https://padlet.com/corra_flanagan/lgfix4d0c3f6/wish/143105967

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