An Ultrasound Portrait of the Embryonic Universe by an Dre W E, Lange
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\'1t han~ a cle" \,ICW. ha c k to that moment turn", , ransparcn!. By analog In cosmic h"'StofY when lh·e Ulll,-. .. rSIe y !O a human lifetime .. afler concepdon_b. rh,s IS about six hours r t,orc tht· l Yt;ore• has di"idt-d r:or t IIt fnst. time. ,. H~I~i!lI~G & \ { I E Nt E ... J !OOO An Ultrasound Portrait of the Embryonic Universe by An dre w E, Lange I've been working wirh relescopes carried aloft In fact, the woodcut is preny accurate-there by balloons since I was a graduate studem, We'd is a beyond, and in order to lead yo u to it, [ 'II have launch chern from Palestine, Texas , and my job to take you on a brief and rarher Caltech·cemric was to dri ve like a bat Oll[ of hell all night long tOur of modern cosmology. (That's nor hard to do, to Tuscaloosa, Alabama, to sec up rhe downrange beclluse Gltech has played a remarkably impor srarion, Then, when che balloon lost mdio coman ram role,) ['II talk llbom three seminal observa with Texas, I could receive rhe data in Alabama, tions. The fiTS[ was made by Edwin H ubble L ~ft: What would w~ s~e if And, as will nor surprise my wife, I was frequeml y at the t.k Wilson Observatory, which overlooks we (ould look beyond the scoPlx·d for spel1:ling--once in Louisiana, which is Pasadena, in 1929, Seveml people, narably Vesco visible heavens? something you never, ever want to have happen to Melvin Slipher, had noticed that the galaxies out you. The sheriff, who looked a lot like Jackie side our immediate neighborhood are moving Right: Th e Hubble Deep Gleason, was actually weMing pe ~ I r!. h~mdled away from us ac various speeds, bur H ubble Fi eld (overs a one· revolvers, He took mt· to the sheriff's stlltion. plon ed their velocities as 1\ func tion of thcir arcminute speck of sky and I was ra mbling on and on about how wt' d istance from us. He found that the f:mher about the size of a dime were crying co cake pinures of [he earl y universe, Hway rhey are, the FJster they afe re<eding, He didn't say a word for (Iui n.· a whil e. Then he so he concluded rhat the universe is exp.1 nding. se ~n 'rom 15 '~e t away, or looked me in the eye and sllid, "Now whadya wam Furthermore. we're not ar the cemer of the 1/10th the diameu r of the co do a thing like that for ?" \'{fe ll, I chink tim e)(pansion-there is no "cemer." The universe is full moon-ntar the pan of being human is a fu ndllmenral desire co expanding in all directions from every poine, It's handle of the Big Dipper, look beyond rhe limit of ou r vision, be<:ll use anoth· much like sitting on one raisin in a raisin bread as {'r ve ry human instincr tells us [hac if we do (and it b.'lkes-no matter which misin you choose, rhe Th is region was specifically this applies to the microscopic scale a~ wel l), others are moving away from you. H is actual dam cho s ~n to ~. dud~ bright we're },;oing to find something wonderful. And stars, nearby galaxies and the project I'm },;oing to tell you about, called BOOMERANG, for Balloon Observations Of galaxy dusters, and bright Millimetric Exrragalanic Rad iation ANd Geo radio sour(u that might physics, has done JUSt thar. obsture the view of dim· The artisr who made rh e woodcut at left had mer, more distant objeds, the sa me idea-if we could somehow look beyond the stars, there would be some wonderful, mag ical T h ~ dimmes t galaxies here world "outside," The most powerful C<luivalcm of are nearly four billion our eyes these days is the H ubble Space Tel~scope , times fainter than the which is sensiri ... e to the same wavelengrhs we see, At riglu is a piece of the so·called Hubble Deep human eye (an se~ , Fidd. in which rhe H ubble stared at a riny corner of rll(: sky for 10 days straight in order to see as far as it could possibl}' see, Of all the objects in [his image, onl y nvo are scars-the rest are g:llaxies. But our artist would have been deeply disllp, IXli nred by rhis picture, because if you look between the galaxies, it's just dark, There's no glowing. otherworldly "beyond" Out there. lO O O 00 Hubble's data, as pub1i shed in the Proceedings of the • /. National Academy of Sciences (Volume IS, pagO! 172) . • ~ Distance equals time In usmology. betause the farther o . ""/0' ..... away something is. the longer its light takes to ruth us. • /~ h ' The oldest, fartheU galaxies are also moYing away from us • , the fasust, which implies that the aye"'ge separation j between galuin _assuming our place in the uni verse is , r 0 • ~;<• typical--is incnasing over time. In a static universe, whe~ • • • the galaxies remain at find distances from one another, ! the line wOLild be horizonta l. T....... • ..• ........U t ... • .... UO'L .. is shown above, and in cosmology, the way the points fit that straight line is considNl~ perfect. You rarely get such a good correhJ(ion. The slope of that line is now ca!led che Hubble constant, and it tells us the rate at which the universe is ex.pand ing. (The numerical value H ubble derived was off by abour a facror of 10 , bur, being cosmology, rhar was O K too.) Before moving on ro rhe next discovery, I Einstein (Idt); Walter have ro tell you another thing about cosmology: Adams, director of the MI. !lawre is consistendy more interesting than we can imagine. When Albert Einstein was working OUt Wilson Observatory, and his field-theory ('(Iuations fo r Seneral relativity 12 Hubble on the catwalk of years before Hubble's discovery, they refused ro the obseroatory's lOO . inch ag ree with what Einstei n 's common sense told Hooker telenope. at the him-namely, that the universe had been around forever in pretty much the Slime fo rm that it is time the world's largest, today, He fixlx! that by sticking in II little thing which Hubble used to called the cosmol08ical constant, or Einstein's muslin galactic distances. constant, such chat when he plorted the se paration between any twO galaxies as a function of rime, he gOt a horizontal line. But H ubble showed Einstein (har his common sense was wrong. Einstein visited Caltech and met Hubble in 193 1, and the campus was abuzz abom whether Einstein would disavow his cosmological consrant. He stayed mum while he was here, but he laeer called il the "greatest blunder of my life." More about thll[ later; it's come back [0 haunt us in rhe last couple of years. If the universe is ex panding, it follows that it must hllve been smaller in the past, and [hat if you play the movie backward all the way [0 the begin ning, it all collapses down to nothing. And now, if you run the movie forward again, you h:lve the so-called BiS Ban8- the birth of the uni verse. So people speculated dun the universe was much hotter when rhe matter was all crammed rogether, because if yOll le t a gas expand, it cools. Our second major discovery was made at Caltl"Ch III (he 19505, when the late Nobel laureare Willie Fow ler (PhD '36) and others m(-as urecl what """'""c.pIo ........"h ,.,. ~ , OOJ 1""''" '''''''' 0("" II<I>n- Uo, •• f> " f 0( J...... I,,,, ,oJ ",. R""... Rocf,,.... "II<""'}'. I.., " 2000 atomic nuclei do in a very hot, dense environment. I won't go into detail, but at the very high temperarures and densities presem in the early universe, promns and neutrons playa strange game of musical chairs from which come the light elemenrs-hydrogen. deuterium, tritium, helium- Temperature (kel vins) 3, helium, and tiny amounts of lithium and beryl 10' lium. (The heavier srufT gets made later, in stars and supernovas.) Each elemenr (-ml'rges in a fixed 10- 1 proportion to th(- others-for example, about one 9 'He 10-1 helium atOm fo r every 16 hydrogen aroms-and rhese rarios agree with what we see throughou t 10- 3 ~ the universe. That's a key reason why we believe u c 10~ in the Big Bang. ~ -0 5 The third discovery was made in 1964 and C 10- ~ involv«l a Caltech graduate, but it was nor made 10~ at Cahech. If was made in Holmdel, New Jersey, "'"-< 10- 7 which had nor previously been known as a great > " 10- 8 astronomical site, at a big radio dish owmxl by ."~ Bell Labs. Nobel laureates Arno Peozi3s and u 10"" Robert Wilson (PhD '62) were working on dle "' 10- 10 Tclstar project, which was the first full-fledged 10-11 communications satellite, and they found that wherever they looked, the sky was aglow with 10- 12 , , , microwaves. This is now called the cosmic micro min 3 mins I hour wave background, or CMB, and it's the fossilizl'(l primcval fireball. These microwaves are litl'rally Age oFthe Uni verse the heat left over from the Big Bang. The total amount of energy em itted by all the Stars thar have ever burned in the whole history of rhe MLlsic .