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The Long Climb from the Sun's CoreWeek of July 21, 1997It has been said that our Solar System really consists of only three things: the Sun, Jupiter, and assorted rubble. With that in mind, we'll start our snacking tour of the Solar System with the part of it that gives it its name: the Sun. You may have noticed that the Sun has two overwhelmingly obvious characteristics: it's bright, and it's hot. These two things are related. The source of the Sun's heat wasn't understood until the middle of the 20th century, when nuclear fusion was first being mathematically analyzed. Although even today we do not completely understand what is happening inside the Sun, we have a pretty good grasp of it. Basically, the nuclei of hydrogen atoms are compressed together so hard that they fuse to form helium atoms (the actual process is quite a bit more complicated, but fusion to helium is the end result). This releases a tiny bit of energy. At least, tiny when you only do it once. But the Sun converts millions of tons of hydrogen into helium in its core every second, and so a lot of energy is released. This energy is in the form of photons, or light.
* In this Snack, I originally said it takes a million years for a photon to get out. Since then, I have found more recent papers that show that it takes far less, perhaps even as little as 17,000 years. 40,000 is a number that seems to me to be the best supported, but who knows? Maybe future papers will refine the time even more. Would you like to know more about the Sun? Bill Arnett's "The Nine Planets" page is the definitive guide to our Solar System.
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