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 [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. |