《原理》的核心是牛頓的三大運(yùn)動(dòng)定律(定律非常明確地指出,物體朝著推力的方向運(yùn)動(dòng);它始終做直線運(yùn)動(dòng),直到某種別的力起了作用,使它慢下來(lái)或改變它的方向;每個(gè)作用都有相等的反作用)以及他的萬(wàn)有引力定律。這說(shuō)明,宇宙里的每個(gè)物體都吸引每個(gè)別的物體。這似乎不大可能,但當(dāng)你在這里坐著的時(shí)候,你在用你自己小小的(的確很小)引力場(chǎng)吸引你周圍的一切事物--墻壁、天花板、燈、寵物貓。而這些東西也在吸引你。
It was Newton who realized that the pull of any two objects is, to quote Feynman again, "proportional to the mass of each and varies inversely as the square of the distance betweenthem." Put another way, if you double the distance between two objects, the attraction betweenthem becomes four times weaker. This can be expressed with the formula F = Gmm/R^2
which is of course way beyond anything that most of us could make practical use of, but at leastwe can appreciate that it is elegantly compact. A couple of brief multiplications, a simpledivision, and, bingo, you know your gravitational position wherever you go. It was the firstreally universal law of nature ever propounded by a human mind, which is why Newton isregarded with such universal esteem.
是牛頓認(rèn)識(shí)到,任何兩個(gè)物體的引力,再用費(fèi)曼的話來(lái)說(shuō),“與每個(gè)物體的質(zhì)量成正比,以兩者之間距離的平方反比來(lái)變化”。換一種說(shuō)法,要是你將兩個(gè)物體之間的距離翻一番,兩者之間的引力就弱4倍。這可以用下面的公式來(lái)表示: F=Gmm/(R^2) 這個(gè)公式對(duì)我們大多數(shù)人來(lái)說(shuō)當(dāng)然是根本沒(méi)有實(shí)際用途的,但至少我們欣賞它的優(yōu)美,它的簡(jiǎn)潔。無(wú)論你走到哪里,只要做兩個(gè)快速的乘法,一個(gè)簡(jiǎn)單的除法,嘿,你就知道你的引力狀況。這是人類提出的第一個(gè)真正有普遍意義的自然定律,也是牛頓到處深受人們尊敬的原因。