Twice a day, seven days a week, from February to November for the 
past four years, two researchers have layered themselves with thermal 
underwear and outerwear, with fleece, flannel, double gloves, double 
socks, padded overalls and puffy red parkas, mummifying themselves until
 they look like twin Michelin Men. Then they step outside, trading the 
warmth and modern conveniences of a science station (foosball, fitness 
center, 24-hour cafeteria) for a minus-100-degree Fahrenheit featureless
 landscape, flatter than Kansas and one of the coldest places on the 
planet. They trudge in darkness nearly a mile, across a plateau of snow 
and ice, until they discern, against the backdrop of more stars than any
 hands-in-pocket backyard observer has ever seen, the silhouette of the 
giant disk of the South Pole Telescope, where they join a global effort 
to solve possibly the greatest riddle in the universe: what most of it 
is made of.
For thousands of years our species has studied the night sky and 
wondered if anything else is out there. Last year we celebrated the 
400th anniversary of Galileo’s answer: Yes. Galileo trained a new 
instrument, the telescope, on the heavens and saw objects that no other 
person had ever seen: hundreds of stars, mountains on the Moon, 
satellites of Jupiter. Since then we have found more than 400 planets 
around other stars, 100 billion stars in our galaxy, hundreds of 
billions of galaxies beyond our own, even the faint radiation that is 
the echo of the Big Bang.
Now scientists think that even this extravagant census of the 
universe might be as out-of-date as the five-planet cosmos that Galileo 
inherited from the ancients. Astronomers have compiled evidence that 
what we’ve always thought of as the actual universe—me, you, this 
magazine, planets, stars, galaxies, all the matter in space—represents a
 mere 4 percent of what’s actually out there. The rest they call, for 
want of a better word, dark: 23 percent is something they call dark 
matter, and 73 percent is something even more mysterious, which they 
call dark energy.
“We have a complete inventory of the universe,” Sean Carroll, a 
California Institute of Technology cosmologist, has said, “and it makes 
no sense.”
Scientists have some ideas about what dark matter might be—exotic and
 still hypothetical particles—but they have hardly a clue about dark 
energy. In 2003, the National Research Council listed “What Is the 
Nature of Dark Energy?” as one of the most pressing scientific problems 
of the coming decades. The head of the committee that wrote the report, 
University of Chicago cosmologist Michael S. Turner, goes further and 
ranks dark energy as “the most profound mystery in all of science.”
The effort to solve it has mobilized a generation of astronomers in a
 rethinking of physics and cosmology to rival and perhaps surpass the 
revolution Galileo inaugurated on an autumn evening in Padua. They are 
coming to terms with a deep irony: it is sight itself that has blinded 
us to nearly the entire universe. And the recognition of this blindness,
 in turn, has inspired us to ask, as if for the first time: What is this
 cosmos we call home?
Scientists reached a consensus in the 1970s that there was more to 
the universe than meets the eye. In computer simulations of our galaxy, 
the Milky Way, theorists found that the center would not hold—based on 
what we can see of it, our galaxy doesn’t have enough mass to keep 
everything in place. As it rotates, it should disintegrate, shedding 
stars and gas in every direction. Either a spiral galaxy such as the 
Milky Way violates the laws of gravity, or the light emanating from 
it—from the vast glowing clouds of gas and the myriad stars—is an 
inaccurate indication of the galaxy’s mass.
But what if some portion of a galaxy’s mass didn’t radiate light? If 
spiral galaxies contained enough of such mystery mass, then they might 
well be obeying the laws of gravity. Astronomers dubbed the invisible 
mass “dark matter.”
“Nobody ever told us that all matter radiated,”Vera Rubin, an 
astronomer whose observations of galaxy rotations provided evidence for 
dark matter, has said. “We just assumed that it did.”
WOW!!
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