Changes

[[File:lighterstill.jpg]][[File:The_eye_of_all_ur60.jpg|right|frame]]

[[File:lighterstill.jpg]][[File:The_eye_of_all_ur60.jpg|right|frame]]

41:8.1 In those [[suns]] which are encircuited in the [[space]]-[[energy]] [[channels]], [[solar energy]] is liberated by various [[complex]] [http://en.wikipedia.org/wiki/Nuclear_Reaction nuclear-reaction] chains, the most common of which is the hydrogen-carbon-helium reaction. In this [[metamorphosis]], carbon [[acts]] as an [[energy]] [[catalyst]] since it is in no way actually changed by this [[process]] of converting hydrogen into helium. Under certain conditions of high [[temperature]] the hydrogen penetrates the carbon [[nuclei]]. Since the [http://en.wikipedia.org/wiki/Carbon carbon] cannot hold more than four such protons, when this saturation state is [[attained]], it begins to emit protons as fast as new ones arrive. In this [[reaction]] the ingoing hydrogen [[particles]] come forth as a [http://en.wikipedia.org/wiki/Helium helium] [[atom]].

41:8.1 In those [[suns]] which are encircuited in the [[space]]-[[energy]] [[channels]], [[solar energy]] is liberated by various [[complex]] [https://en.wikipedia.org/wiki/Nuclear_Reaction nuclear-reaction] chains, the most common of which is the hydrogen-carbon-helium reaction. In this [[metamorphosis]], carbon [[acts]] as an [[energy]] [[catalyst]] since it is in no way actually changed by this [[process]] of converting hydrogen into helium. Under certain conditions of high [[temperature]] the hydrogen penetrates the carbon [[nuclei]]. Since the [https://en.wikipedia.org/wiki/Carbon carbon] cannot hold more than four such protons, when this saturation state is [[attained]], it begins to emit protons as fast as new ones arrive. In this [[reaction]] the ingoing hydrogen [[particles]] come forth as a [https://en.wikipedia.org/wiki/Helium helium] [[atom]].

41:8.2 Reduction of hydrogen content increases the [[luminosity]] of a [[sun]]. In the suns [[destined]] to burn out, the height of [[luminosity]] is [[attained]] at the point of hydrogen exhaustion. Subsequent to this point, [[brilliance]] is [[maintained]] by the resultant [[process]] of [[gravity]] contraction. Eventually, such a [[star]] will become a so-called [http://en.wikipedia.org/wiki/White_dwarf white dwarf], a highly condensed [[sphere]].

41:8.2 Reduction of hydrogen content increases the [[luminosity]] of a [[sun]]. In the suns [[destined]] to burn out, the height of [[luminosity]] is [[attained]] at the point of hydrogen exhaustion. Subsequent to this point, [[brilliance]] is [[maintained]] by the resultant [[process]] of [[gravity]] contraction. Eventually, such a [[star]] will become a so-called [https://en.wikipedia.org/wiki/White_dwarf white dwarf], a highly condensed [[sphere]].

41:8.3 In large [[suns]]—small circular [[nebulae]]—when hydrogen is exhausted and [[gravity]] contraction ensues, if such a [[body]] is not sufficiently [[opaque]] to retain the internal [[pressure]] of [[support]] for the outer [[gas]] regions, then a sudden collapse occurs. The [[gravity]]-[[electric]] [[changes]] give origin to vast [[quantities]] of tiny [[particles]] devoid of [[electric]] [[potential]], and such [[particles]] readily escape from the [http://en.wikipedia.org/wiki/Sun#Core solar interior], thus bringing about the collapse of a gigantic sun within a few days. It was such an emigration of these "runaway [[particles]]" that occasioned the collapse of the giant [http://en.wikipedia.org/wiki/Nova nova] of the [http://en.wikipedia.org/wiki/Andromeda_%28constellation%29 Andromeda] [[nebula]] about fifty years ago. This vast [[stellar]] body collapsed in forty minutes of [[Urantia]] time.

41:8.3 In large [[suns]]—small circular [[nebulae]]—when hydrogen is exhausted and [[gravity]] contraction ensues, if such a [[body]] is not sufficiently [[opaque]] to retain the internal [[pressure]] of [[support]] for the outer [[gas]] regions, then a sudden collapse occurs. The [[gravity]]-[[electric]] [[changes]] give origin to vast [[quantities]] of tiny [[particles]] devoid of [[electric]] [[potential]], and such [[particles]] readily escape from the [https://en.wikipedia.org/wiki/Sun#Core solar interior], thus bringing about the collapse of a gigantic sun within a few days. It was such an emigration of these "runaway [[particles]]" that occasioned the collapse of the giant [https://en.wikipedia.org/wiki/Nova nova] of the [https://en.wikipedia.org/wiki/Andromeda_%28constellation%29 Andromeda] [[nebula]] about fifty years ago. This vast [[stellar]] body collapsed in forty minutes of [[Urantia]] time.

41:8.4 As a rule, the vast extrusion of [[matter]] [[continues]] to exist about the residual cooling [[sun]] as extensive clouds of [[nebula]]r [[gases]]. And all this explains the [[origin]] of many types of irregular [[nebulae]], such as the [http://en.wikipedia.org/wiki/Crab_nebula Crab nebula], which had its [[origin]] about nine hundred years ago, and which still exhibits the [[mother]] [[sphere]] as a lone star near the [[center]] of this irregular nebular [[mass]].

41:8.4 As a rule, the vast extrusion of [[matter]] [[continues]] to exist about the residual cooling [[sun]] as extensive clouds of [[nebula]]r [[gases]]. And all this explains the [[origin]] of many types of irregular [[nebulae]], such as the [https://en.wikipedia.org/wiki/Crab_nebula Crab nebula], which had its [[origin]] about nine hundred years ago, and which still exhibits the [[mother]] [[sphere]] as a lone star near the [[center]] of this irregular nebular [[mass]].

<center>[https://nordan.daynal.org/wiki/index.php?title=Paper_41 Go to Paper 41]</center>

<center>[https://nordan.daynal.org/wiki/index.php?title=Paper_41 Go to Paper 41]</center>