The Urantia Book

Settings

Reading
Theme
Text size
Line spacing

Typeface

Width
Alignment
Show
Listening

Kept in this browser only.

Paper 41

Physical Aspects of the Local Universe

Archangel

3. Our Starry Associates

41:3.1There are up­ward of two thou­sand bril­liant suns pour­ing forth light and en­ergy in Sa­ta­nia, and your own sun is an av­er­age blaz­ing orb. Of the thirty suns near­est yours, only three are brighter. The Uni­verse Power Di­rec­tors ini­ti­ate the spe­cial­ized cur­rents of en­ergy which play be­tween the in­di­vid­ual stars and their re­spec­tive sys­tems. These so­lar fur­naces, to­gether with the dark gi­ants of space, serve the power cen­ters and phys­i­cal con­trol­lers as way sta­tions for the ef­fec­tive con­cen­trat­ing and di­rec­tion­iz­ing of the en­ergy cir­cuits of the ma­te­rial cre­ations.

41:3.2The suns of Neb­a­don are not un­like those of other uni­verses. The ma­te­rial com­po­si­tion of all suns, dark is­lands, plan­ets, and satel­lites, even me­te­ors, is quite iden­ti­cal. These suns have an av­er­age di­am­e­ter of about one mil­lion miles, that of your own so­lar orb be­ing slightly less. The largest star in the uni­verse, the stel­lar cloud Antares, is four hun­dred and fifty times the di­am­e­ter of your sun and is sixty mil­lion times its vol­ume. But there is abun­dant space to ac­com­mo­date all of these enor­mous suns. They have just as much com­par­a­tive el­bow room in space as one dozen or­anges would have if they were cir­cu­lat­ing about through­out the in­te­rior of Uran­tia, and were the planet a hol­low globe.

41:3.3When suns that are too large are thrown off a neb­u­lar mother wheel, they soon break up or form dou­ble stars. All suns are orig­i­nally truly gaseous, though they may later tran­siently ex­ist in a semiliq­uid state. When your sun at­tained this quasi-liq­uid state of super­gas pres­sure, it was not suf­fi­ciently large to split equa­to­ri­ally, this be­ing one type of dou­ble star for­ma­tion.

41:3.4When less than one tenth the size of your sun, these fiery spheres rapidly con­tract, con­dense, and cool. When up­wards of thirty times its size—rather thirty times the gross con­tent of ac­tual ma­te­rial—suns read­ily split into two sep­a­rate bod­ies, ei­ther be­com­ing the cen­ters of new sys­tems or else re­main­ing in each other’s grav­ity grasp and re­volv­ing about a com­mon cen­ter as one type of dou­ble star.

41:3.5The most re­cent of the ma­jor cos­mic erup­tions in Or­von­ton was the ex­traor­di­nary dou­ble star ex­plo­sion, the light of which reached Uran­tia in A.D. 1572. This con­fla­gra­tion was so in­tense that the ex­plo­sion was clearly vis­i­ble in broad day­light.

41:3.6Not all stars are solid, but many of the older ones are. Some of the red­dish, faintly glim­mer­ing stars have ac­quired a den­sity at the cen­ter of their enor­mous masses which would be ex­pressed by say­ing that one cu­bic inch of such a star, if on Uran­tia, would weigh six thou­sand pounds. The enor­mous pres­sure, ac­com­pa­nied by loss of heat and cir­cu­lat­ing en­ergy, has re­sulted in bring­ing the or­bits of the ba­sic ma­te­rial units closer and closer to­gether un­til they now closely ap­proach the sta­tus of elec­tronic con­den­sa­tion. This pro­cess of cool­ing and con­trac­tion may con­tinue to the lim­it­ing and crit­i­cal ex­plo­sion point of ul­ti­ma­tonic con­den­sa­tion.

41:3.7Most of the gi­ant suns are rel­a­tively young; most of the dwarf stars are old, but not all. The col­li­sional dwarfs may be very young and may glow with an in­tense white light, never hav­ing known an ini­tial red stage of youth­ful shin­ing. Both very young and very old suns usu­ally shine with a red­dish glow. The yel­low tinge in­di­cates mod­er­ate youth or ap­proach­ing old age, but the bril­liant white light sig­ni­fies ro­bust and ex­tended adult life.

41:3.8While all ado­les­cent suns do not pass through a pul­sat­ing stage, at least not vis­i­bly, when look­ing out into space you may ob­serve many of these younger stars whose gi­gan­tic res­pi­ra­tory heaves re­quire from two to seven days to com­plete a cy­cle. Your own sun still car­ries a di­min­ish­ing legacy of the mighty up­swellings of its younger days, but the pe­riod has length­ened from the for­mer three and one-half day pul­sa­tions to the pres­ent eleven and one-half year sun­spot cy­cles.

41:3.9Stel­lar vari­ables have nu­mer­ous ori­gins. In some dou­ble stars the tides caused by rapidly chang­ing dis­tances as the two bod­ies swing around their or­bits also oc­ca­sion pe­ri­odic fluc­tu­a­tions of light. These grav­ity vari­a­tions pro­duce reg­u­lar and re­cur­rent flares, just as the cap­ture of me­te­ors by the ac­cre­tion of en­ergy-ma­te­rial at the sur­face would re­sult in a com­par­a­tively sud­den flash of light which would speed­ily re­cede to nor­mal bright­ness for that sun. Some­times a sun will cap­ture a stream of me­te­ors in a line of less­ened grav­ity op­po­si­tion, and oc­ca­sion­ally col­li­sions cause stel­lar flare-ups, but the ma­jor­ity of such phe­nom­ena are wholly due to in­ter­nal fluc­tu­a­tions.

41:3.10In one group of vari­able stars the pe­riod of light fluc­tu­a­tion is di­rectly de­pen­dent on lu­mi­nos­ity, and knowl­edge of this fact en­ables as­tron­o­mers to uti­lize such suns as uni­verse light­houses or ac­cu­rate mea­sur­ing points for the fur­ther ex­plo­ration of dis­tant star clus­ters. By this tech­nique it is pos­si­ble to mea­sure stel­lar dis­tances most pre­cisely up to more than one mil­lion light-years. Bet­ter meth­ods of space mea­sure­ment and im­proved tele­scopic tech­nique will some­time more fully dis­close the ten grand di­vi­sions of the super­uni­verse of Or­von­ton; you will at least rec­og­nize eight of these im­mense sec­tors as enor­mous and fairly sym­met­ri­cal star clus­ters.