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ed theory。
neither hubble nor einstein would be much of a part of that big story。 though no onewould have guessed it at the time； both men had done about as much as they were ever goingto do。
in 1936 hubble produced a popular book called the realm of the nebulae； whichexplained in flattering style his own considerable achievements。 here at last he showed thathe had acquainted himself with einstein’s theory—up to a point anyway： he gave it four pagesout of about two hundred。
hubble died of a heart attack in 1953。 one last small oddity awaited him。 for reasonscloaked in mystery； his wife declined to have a funeral and never revealed what she did withhis body。 half a century later the whereabouts of the century’s greatest astronomer remainunknown。 for a memorial you must look to the sky and the hubble space telescope；launched in 1990 and named in his honor。
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9THE MIGHTY ATOM
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while einstein and hubble were productively unraveling the large…scale structure ofthe cosmos； others were struggling to understand something closer to hand but in its way justas remote： the tiny and ever… mysterious atom。
the great caltech physicist richard feynman once observed that if you had to reducescientific history to one important statement it would be “all things are made of atoms。” theyare everywhere and they constitute every thing。 look around you。 it is all atoms。 not just thesolid things like walls and tables and sofas； but the air in between。 and they are there innumbers that you really cannot conceive。
the basic working arrangement of atoms is the molecule （from the latin for “little mass”）。
a molecule is simply two or more atoms working together in a more or less stablearrangement： add two atoms of hydrogen to one of oxygen and you have a molecule of water。
chemists tend to think in terms of molecules rather than elements in much the way thatwriters tend to think in terms of words and not letters； so it is molecules they count； and theseare numerous to say the least。 at sea level； at a temperature of 32 degrees fahrenheit； onecubic centimeter of air （that is； a space about the size of a sugar cube） will contain 45 billionbillion molecules。 and they are in every single cubic centimeter you see around you。 thinkhow many cubic centimeters there are in the world outside your window—how many sugarcubes it would take to fill that view。 then think how many it would take to build a universe。
atoms； in short； are very abundant。
they are also fantastically durable。 because they are so long lived； atoms really get around。
every atom you possess has almost certainly passed through several stars and been part ofmillions of organisms on its way to being you。 we are each so atomically numerous andso vigorously recycled at death that a significant number of our atoms—up to a billion foreach of us； it has been suggested—probably once belonged to shakespeare。 a billion moreeach came from buddha and genghis khan and beethoven； and any other historical figureyou care to name。 （the personages have to be historical； apparently； as it takes the atomssome decades to bee thoroughly redistributed； however much you may wish it； you arenot yet one with elvis presley。）so we are all reincarnations—though short…lived ones。 when we die our atoms willdisassemble and move off to find new uses elsewhere—as part of a leaf or other human beingor drop of dew。 atoms； however； go on practically forever。 nobody actually knows how longan atom can survive； but according to martin rees it is probably about 1035years—a numberso big that even i am happy to express it in notation。
above all； atoms are tiny—very tiny indeed。 half a million of them lined up shoulder toshoulder could hide behind a human hair。 on such a scale an individual atom is essentiallyimpossible to imagine； but we can of course try。
start with a millimeter； which is a line this long： …。 now imagine that line divided into athousand equal widths。 each of those widths is a micron。 this is the scale of microorganisms。
a typical paramecium； for instance； is about two microns wide； 0。002 millimeters； which isreally very small。 if you wanted to see with your naked eye a paramecium swimming in adrop of water； you would have to enlarge the drop until it was some forty feet across。
however； if you wanted to see the atoms in the same drop； you would have to make the dropfifteen miles across。
atoms； in other words； exist on a scale of minuteness of another order altogether。 to getdown to the scale of atoms； you would need to take each one of those micron slices and shaveit into ten thousand finer widths。 that’s the scale of an atom： one ten…millionth of amillimeter。 it is a degree of slenderness way beyond the capacity of our imaginations； but youcan get some idea of the proportions if you bear in mind that one atom is to the width of amillimeter line as the thickness of a sheet of paper is to the height of the empire statebuilding。
it is of course the abundance and extreme durability of atoms that makes them so useful；and the tininess that makes them so hard to detect and understand。 the realization that atomsare these three things—small； numerous； practically indestructible—and that all things aremade from them first occurred not to antoine…laurent lavoisier； as you might expect； or evento henry cavendish or humphry davy； but rather to a spare and lightly educated englishquaker named john dalton； whom we first encountered in the chapter on chemistry。
dalton was born in 1766 on the edge of the lake district near cockermouth to a family ofpoor but devout quaker weavers。 （four years later the poet william wordsworth would alsojoin the world at cockermouth。） he was an exceptionally bright student—so very brightindeed that at the improbably youthful age of twelve he was put in charge of the local quakerschool。 this perhaps says as much about the school as about dalton’s precocity； but perhapsnot： we know from his diaries that at about this time he was reading newton’s principia in theoriginal latin and other works of a similarly challenging nature。 at fifteen； stillschoolmastering； he took a job in the nearby town of kendal； and a decade