Summary

This document appears to be notes on astronomy, specifically about the solar system and stars. It includes diagrams and descriptions of different objects like planets, stars, and celestial bodies. The information could be used for educational purposes.

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massive Likethelowertaperfadememe Our Solar System 8 oanoQQQQmeiiiiiimsisiies.it c tt iai e.gravity.ana TerrestrialPlanets...

massive Likethelowertaperfadememe Our Solar System 8 oanoQQQQmeiiiiiimsisiies.it c tt iai e.gravity.ana TerrestrialPlanets m.i i i ii Gas planets liFe surroundsthecores EE ee a eee.ee e in g siiim a ai e aintn anrasi esis.it tn nito it into have mass bepulled enough stable a spherebygravit units dominateitsownorbit e featsts Astronomical unit thedistancebetween thesunandEarthUsedforobjectswithin Earth i sismasismaonm.ua celestialobjects EEEijiisiii'stem Lightyear thedistancelighttravels if in avacuum in 1yearusedfor uvoras GÉ c our solar system f aroraBorealis iitieioitinmeransigncausing m nm ftp.spqiaymtiojggenf um mixtooo luminosity brightness thetotal amountofenergyproduced Earth'smagneticforce a starpersecond Eu's in qiriitaer gnfingw colour temperature colourindicatessurfacetempHo bsolutemagnetude thebrightnessofstarsas iftheywerelocated stars areblueishcoolerstarsarered 3319awayfromEarth in colour thelowerthenumberthebrighter mass astar'smass determines its lumino pparentMagnetude thebrightness ofstars astheyappearfrom coloursizeandlifespan Earth asram more massivethestaris.tn cycles of stars fastertherate offusionis starts w a nebula meansshorterlifespa nebulacollapsesonitself 2 5 thisisovermillionsofyearsgasesanddustget pulledintothemoredenseregions Pittstyamities't s an his allformsaprotostar 35 theprotostarskeepspullinginmorematter starsdon'tmovethrough All of thispullingofmattercauses it tobesodense thediagram astheyage the E.siiIucs9iIsorenergy thatrushesoutwards e death of a star f f massisequal orsmallerthanthesun itbecomes initoquare largerandredder verses regiant Planetarya f f eyestrain f astarwhichhas a massbigger A m'assister bula than theSun sedergiant supernova Phil at'starstartstodie thecoreleftbehindcouldbecome a nuclearfusion when pggsiymsstagsnesntqitstyafyseoheahiu.mu.si to neutronstar Pso or theouterlayersslowlydriftaway hydrogen planetarynebula theykeepfusingmakingeven if thesupernovawassuperdensetheco allthatremains is thecore heavierelements mightalsocollapseunderitsowngravit whitedwarf stopsatiron ocausingablackholetofor onceitgetstoiron.itcollapsesto itsown gravity thiscauses a supernova TypesofGalaxies aims ellipiffinary saff ioflengtiik.gr ftp.iigaidlyar omasphere havelongarms central bulge surroundedby a flattened don'thave aregularshape 1 19 jasaaimasat.gelotsof disc madeofnewandoldstar gquatginssomeoftheoldest nospira arm In S.iereohfaiistnormoia'stars yqygt.tobespiralgalaxies that lost LocalGroup olderredstars smallgroupofgalaxies GalaxySupercluster BigBangTheory gianticsuperclusterof 4 25clusters ofgalaxies it statesthatapproximately13.7billionyearsago webelongtotheVirgosupercluster all matterwaspackedintoonesmalldensenot mass Butthenit allmovedapartintheBigBang eversincetheBigBangtheuniversehasbeen expanding

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