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I swear, if you touch me, I’ll go Lorena Bobbitt on you.” Lorena Bobbitt? Why does that sound—oh my God, the lady that chopped off her husband’s dick? I busted out laughing and put my pillow over my face. “Oh my God! Princess! You’re my new favorite!” That’s it, that comment right there, and it was sealed. I would do anything to have this beautiful gray-eyed princess lying next to me, as mine. ↗
From the ruins, lonely and inexplicable as the sphinx, rose the Empire State Building. And just as it had been tradition of mine to climb to the Plaza roof to take leave of the beautiful city extending as far as the eyes could see, so now I went to the roof of that last and most magnificent of towers. Then I understood. Everything was explained. I had discovered the crowning error of the city. Its Pandora's box. Full of vaunting pride, the New Yorker had climbed here, and seen with dismay what he had never suspected. That the city was not the endless sucession of canyons that he had supposed, but that it had limits, fading out into the country on all sides into an expanse of green and blue. That alone was limitless. And with the awful realization that New York was a city after all and not a universe, the whole shining ediface that he had reared in his mind came crashing down. That was the gift of Alfred Smith to the citizens of New York. ↗
His laws changed all of physics and astronomy. His laws made it possible to calculate the mass of the sun and planets. The way it's done is immensely beautiful. If you know the orbital period of any planet, say, Jupiter or the Earth and you know its distance to the Sun; you can calculate the mass of the Sun. Doesn't this sound like magic? We can carry this one step further - if you know the orbital period of one of Jupiter's bright moons, discovered by Galileo in 1609, and you know the distance between Jupiter and that moon, you can calculate the mass of Jupiter. Therefore, if you know the orbital period of the moon around the Earth (it's 27.32 days), and you know the mean distance between the Earth and the moon (it's about 200,039 miles), then you can calculate to a high degree of accuracy the mass of the Earth. … But Newton's laws reach far beyond our solar system. They dictate and explain the motion of stars, binary stars, star clusters, galaxies and even clusters of galaxies. And Newton's laws deserve credit for the 20th century discovery of what we call dark matter. His laws are beautiful. Breathtakingly simple and incredibly powerful at the same time. They explain so much and the range of phenomena they clarify is mind boggling. By bringing together the physics of motion, of interaction between objects and of planetary movements, Newton brought a new kind of order to astronomical measurements, showing how, what had been a jumble of confused observations made through the centuries were all interconnected. ↗
When I looked, I knew I might never again see so much of the earth so beautiful, the beautiful being something you know added to something you see, in a whole that is different from the sum of its parts. What I saw might have been just another winter scene, although an impressive one. But what I knew was that the earth underneath was alive and that by tomorrow, certainly by the day after, it would be all green again. So what I saw because of what I knew was a kind of death with the marvellous promise of less than a three-day resurrection. ↗
I watched commercial ave. slide past and there in the distance were the lights of route 18. that was one of those moments that would always be Rutgers for me. ↗
