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Bad Astronomy: Misconceptions and Misuses Revealed, from ...

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A DASH OF SEASONS 49<br />

It’s true that the Earth orbits the Sun in an ellipse. We know it<br />

now through careful measurements of the sky, but it isn’t all that<br />

obvious. For thous<strong>and</strong>s of years it was thought that the Sun orbited<br />

the Earth. In the year 1530, the Polish astronomer Nicolaus Copernicus<br />

first published his idea that the Earth orbited the Sun. The<br />

problem is, he thought the Earth (<strong>and</strong> all the planets) moved in a<br />

perfectly circular path. When he tried to use that idea to predict<br />

the positions of the planets in the sky, things came out wrong. He<br />

had to really fudge his model to make it work, <strong>and</strong> it never really<br />

did do a good job predicting positions.<br />

In the very early part of the 1600s, Johannes Kepler came<br />

along <strong>and</strong> figured out that planets move in ellipses, not circles.<br />

Here we are 400 years later, <strong>and</strong> we still use Kepler’s discoveries to<br />

figure out where the planets are in the sky. We even use his findings<br />

to plan the path of space probes to those planets; imagine<br />

Kepler’s reaction if he knew that! (He’d probably say: “Hey! I’ve<br />

been dead 350 years! What took you so long?”)<br />

But there’s a downside to Kepler’s elliptical orbits; they play<br />

with our common sense <strong>and</strong> allow us to jump to the wrong conclusions.<br />

We know that planets, including our own, orbit the Sun<br />

in these oval paths, so we know that sometimes we’re closer to the<br />

Sun than at other times. We also know that distance plays a role<br />

in the heat we feel. We therefore come to the logical conclusion<br />

that the seasons are caused by our changing distance <strong>from</strong> the Sun.<br />

However, we have another tool at our disposal beside common<br />

sense, <strong>and</strong> that’s mathematics. Astronomers have actually measured<br />

the distance of the Earth to the Sun over the course of the year.<br />

The math needed to convert distance to temperature isn’t all that<br />

hard, <strong>and</strong> it is commonly assigned as a homework problem to<br />

undergraduate-level astronomy majors. I’ll spare you the details <strong>and</strong><br />

simply give you the answer. Surprisingly, the change in distance<br />

over the course of the seasons amounts to only a 4-degree Celsius<br />

(roughly 7 degrees Fahrenheit) change in temperature. This may<br />

not surprise people <strong>from</strong> tropical locations, where the local temperature<br />

doesn’t vary much over the year, but it may come as a shock<br />

to someone <strong>from</strong>, say, Maine, where the seasonal temperature<br />

change is more like 44 degrees Celsius (80 or so degrees Fahrenheit).

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