Changes

41:4.3 Cooling stars[http://en.wikipedia.org/wiki/Stars#Designations] can be [[physically]] [[gaseous]] and tremendously [[dense]] at the same time. You are not familiar with the [[solar]] supergases[?], but these and other [[unusual]] [[forms]] of [[matter]] explain how even nonsolid [[suns]] can [[attain]] a [[density]] [[equal]] to iron—about the same as [[Urantia]]—and yet be in a highly [[heated]] [[gaseous]] [[state]] and continue to [[function]] as [[suns]]. The [[atoms]] in these dense supergases are exceptionally small; they contain few [[electrons]]. Such suns have also largely lost their free [[ultimatonic]] stores of [[energy]].

41:4.3 Cooling stars[http://en.wikipedia.org/wiki/Stars#Designations] can be [[physically]] [[gaseous]] and tremendously [[dense]] at the same time. You are not familiar with the [[solar]] supergases[?], but these and other [[unusual]] [[forms]] of [[matter]] explain how even nonsolid [[suns]] can [[attain]] a [[density]] [[equal]] to iron—about the same as [[Urantia]]—and yet be in a highly [[heated]] [[gaseous]] [[state]] and continue to [[function]] as [[suns]]. The [[atoms]] in these dense supergases are exceptionally small; they contain few [[electrons]]. Such suns have also largely lost their free [[ultimatonic]] stores of [[energy]].

41:4.4 One of your near-by suns[http://en.wikipedia.org/wiki/Proxima_Centauri ?], which started life with about the same [[mass]] as yours, has now contracted almost to the size of [[Urantia]], having become sixty thousand times as dense as your sun. The [weight] of this hot-cold [[gaseous]]-[[solid]] is about one ton per cubic inch. And still this [[sun]] shines with a faint reddish [[glow]], the senile glimmer of a dying monarch of [[light]].

41:4.4 One of your near-by suns[http://en.wikipedia.org/wiki/Proxima_Centauri ?], which started life with about the same [[mass]] as yours, has now contracted almost to the size of [[Urantia]], having become sixty thousand times as dense as your sun. The [[weight]] of this hot-cold [[gaseous]]-[[solid]] is about one ton per cubic inch. And still this [[sun]] shines with a faint reddish [[glow]], the senile glimmer of a dying monarch of [[light]].

41:4.5 Most of the [[suns]], however, are not so dense. One of your nearer neighbors[http://en.wikipedia.org/wiki/Alpha_Centauri ?] has a [[density]] exactly [[equal]] to that of your [[atmosphere]] at sea level. If you were in the interior of this [[sun]], you would be unable to [[discern]] anything. And [[temperature]] permitting, you could penetrate the [[majority]] of the [[suns]] which twinkle in the [http://en.wikipedia.org/wiki/Night_sky night sky] and notice no more [[matter]] than you [[perceive]] in the air of your [[earthly]] living rooms.

41:4.5 Most of the [[suns]], however, are not so dense. One of your nearer neighbors[http://en.wikipedia.org/wiki/Alpha_Centauri ?] has a [[density]] exactly [[equal]] to that of your [[atmosphere]] at sea level. If you were in the interior of this [[sun]], you would be unable to [[discern]] anything. And [[temperature]] permitting, you could penetrate the [[majority]] of the [[suns]] which twinkle in the [http://en.wikipedia.org/wiki/Night_sky night sky] and notice no more [[matter]] than you [[perceive]] in the air of your [[earthly]] living rooms.