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Here Be Dragons

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HERE BE DRAGONS<br />

Milky Way, our home galaxy. Its 300 billion stars merge into a broad<br />

river of light. Just a minute fraction of them, that happen to be close to<br />

us, form the myriad sparkling points that we call "the stars," yet even<br />

these few seem numberless. It's hard to doubt that, on a planet orbiting<br />

one of those stars, a living creature is gazing back at us.<br />

To tell whether any of the stars really do have planets, and whether<br />

any of these planets are inhabited, seemed for centuries an impossible<br />

task. Even today, the world's greatest telescopes, such as the Hale telescope<br />

at Palomar, the twin Keck telescopes on Hawaii, and the Hubble<br />

Space Telescope, are incapable of spotting planets around other stars:<br />

not because the planets are too faint, necessarily, but because they<br />

cling too close to their bright parent stars. Yet a series of brilliant innovations<br />

has allowed astronomers to detect a handful of such planets<br />

indirectly and even to describe their basic properties, such as their size<br />

and orbital characteristics, as we'll describe in the next chapter.<br />

Even more exciting than the detection of extrasolar planets, though,<br />

is our dawning understanding of the evolution of stars and their planetary<br />

systems, an evolution that may carry the seeds of life from the<br />

very beginning, even before a star and its planets are formed. Not<br />

many years ago, it was possible to believe that our Sun, with its nine<br />

planets—at least one of them inhabited—was a freak that might not<br />

be repeated within our galaxy. Now, though many details remain unresolved,<br />

we can speak of the birth of stars and their planets as one of<br />

the fundamental processes of the cosmos, and we can tentatively explain<br />

how the chemical building blocks of life take part in this process,<br />

making an extraordinary journey from deep space to end up in living<br />

creatures such as ourselves.<br />

As we look up into the night sky, the winter constellation of Orion<br />

dominates the scene. The mighty hunter, followed by his dogs (Canis<br />

Major and Minor), chases Taurus the bull eternally westward. Orion<br />

straddles the celestial equator—the circle, oblique to the ecliptic,<br />

which lies directly over the equator of the Earth. Almost everyone recognizes<br />

this dramatic constellation and its brilliant individual stars<br />

with their exotic names: <strong>Be</strong>telgeuse, the variable red giant in Orion's<br />

shoulder; <strong>Be</strong>llatrix, in Orion's other shoulder; and the blue-white giant<br />

Rigel, the sixth brightest star in the sky, in Orion's foot. Most striking,<br />

though, are the three close-set stars that form Orion's belt and the<br />

fainter line of stars that dangle from it, forming his sword.<br />

It wasn't till 1610, apparently, that anyone noticed something peculiar<br />

about the middle star in Orion's sword. A French lawyer,<br />

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