Andthat's theamazingthingthatthingsthat a fewyearsagowecouldonlyevenhopetoseeyoubyactuallygoingandseeingthem, youknow, sending a spaceprobeonactuallygoingupclosetohave a look.
Sothesekindofwavelengths, theinfraredis a verygoodplacetolook.
You'rereallyseeingthatbright, hotambition.
What?
It's anamazingthingwiththisideathatactuallyweaken, takesensiblepicturesofgeologicalphenomenaon a moonofJupiterfromthegroundisanamazingthatthesharpnessoftheimageyouneedtobeabletopickoutthiskindofdetailonsomethingsotinysofarawayisabsolutelyoutstanding.
There's a coupleoflimitationstohowsharpandimageyoucouldtakefromtheground.
Bothgetridoftheeffectsoftheatmosphereandtodealwiththislimitationoffhowsharpandimageyoucantakewith a finitesizeoftelescopeOkay, so I haveanotherpictureforyou.
Thisisthetelescopethatdidthejob.
It's a thingcalledtheLargeBinocularTelescopeortheLbgt.
Soyouhaveseenmanythings, buttheneedtotrickhereisactuallyyoucancombinethelightfromthetwoin a coherentfashion, which, intermsofthissharpnesslimitthisdiffractionlimitfor a telescopemeansthateffectively, you'vegot a singletelescopethat's kindofthethedistancebetweenthetwoofthem, ratherthanthediameterofeach, eachoneindividually.
Sotheeffectivediameterofthetwowhenthey'reworkingtogether, I thinkit's about 22 or 23 meters.
Figuringouttheangularresolutionofthesimageis a very, verysharpimage.
Professor, ifyoustood 60 milesawayfromthetelescopeinArizonaand I swungaroundandpointedit, I suspect I probablydon't emitbrightlyenoughintheinfraredforittoactuallybeabletorecordmyadmission.
Butcertainlyintermsoftheresolutionoftheimages, yes, itwillbeabletotellthat, but I wouldhavetobeglowingfairlybrightlyintheafraidforthattowork, sothat's actinglikeonemirror.
Sothere's a coupleofagain a coupleoftricksyoucanplay, whichis, ifyouthinkaboutitasyoutraceanobjectifyouthinkabout a kindofanextendedobject.
Sohere I amwithmytelescopelookingthisway, andit's followingthisextendedobjectwhenanobjectwhathappenstoitisastimegoesonastheearthrotatedwillriseandthenit'llsetagain.
Andso, bycombiningimagesthatyou'vetaken a differenttimesasanobjecttracksacrossthesky, youcanactuallyusethatextraresolutioninalldirectionstoget a sharpanimagewhichissharpinallaspects, ratherthanbeingsquashedonewayandverysharpinonedirectionandblurredintheotherdirection.
Youcouldcombineallthoseimagestogethertocreate a singleimageoftheobject, whichis a sharp, asifyouhad a a singletelescope, effectivelykindofthiskindofsizeandround.
Whydid I evenmakebigmirrors?
Whydon't theymakeeverytelescopelikethat?
Becauseit's actuallyhardtogetthistowork.
Thisis a youknow, it's a verysophisticatedtechnique.