Sunday, September 07, 2008 | 6:18 p.m.

Stargazers by Dennis Mammana

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Dennis Mammana

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  • Week of Sept. 7-13, 2008
    It was nearly four centuries ago that the great Italian astronomer Galileo Galilei first aimed his telescope toward the heavens. Over time his new optical tube revealed to him mountains, valleys and craters on the moon, spots on the sun and the …

  • Week of Aug. 31-Sept. 6, 2008
    As summers go, I guess this one hasn't been too terribly hot. But it's not over yet. We've still got a few weeks before the official onset of autumn and, hopefully, cooler temperatures. In the meantime, however, pay close attention and I'll bet you …

  • Week of Aug. 24-30, 2008
    As the months of summer slowly give way to those of autumn, stargazers peering due south after dark can spot one of the great celestial icons of the season: the zodiacal constellation of Sagittarius. Sagittarius, the archer, is often imagined as a …

  • Week of Aug. 17-23, 2008
    It's baaack! The glistening planet Venus has been noticeably absent from our early evening sky since last summer. It has spent most of that time on the opposite side of its orbit, rising and setting before the sun. But now it's back in the evening …

Week of Sept. 14-20, 2008

Autumn is nearly here.

This year, the season officially begins on Sept. 22 at 8:45 a.m. PDT (11:45 a.m. EDT). Many people think that the beginning of autumn occurs when the sun rises due east and sets due west, and when the length of our day and night are equal. And, as long as we don't concern ourselves with fine details, those are both reasonably true statements.

So why, then, do we often cite the exact time for the beginning of autumn?

That's because astronomers know the beginning of autumn , the autumnal equinox, to be not actually a day, but rather a moment in time. It's marked by the sun's passage in the heavens from the Northern Hemisphere sky into the Southern Hemisphere sky; in fact, it's the moment when the sun's center crosses the celestial equator on its journey from north to south.

Confused? Well, try to imagine what's going on.

During summertime, we in the Northern Hemisphere see the sun cross our daytime sky high overhead; in our wintertime it crosses relatively low in the southern sky. This perspective comes from the fact the Earth's axis is tilted and, as we orbit the sun, our summertime sun shines more directly onto our planet's Northern Hemisphere, while the wintertime sun shines more directly onto the Southern Hemisphere.

At some point during the year, the sun — traveling along its orbit called the "ecliptic" — must cross the equator on its way southward, and that defines the moment known as the autumnal equinox.
When this occurs, our sun lies directly over the Earth's equator.

Now try to imagine standing on the Earth's equator. On the first day of autumn you'd see the sun pass directly overhead. A few days or weeks earlier, the sun would have crossed your northern sky, and a few days or weeks later it would cross your southern sky. But on that day, the sun stands directly over the equator so you would watch it pass directly overhead.

Another way of thinking about it is to visualize a projection of the Earth's equator into the starry heavens. This would create in the sky what astronomers call the "celestial equator." The moment the sun crosses this great circle on its way south marks the autumnal equinox, and the onset of autumn in the Earth's Northern Hemisphere.

To find out more about Dennis Mammana and read features by other Creators Syndicate writers and cartoonists, visit the Creators Syndicate website at www.creators.com.

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Originally Published on Thursday September 04, 2008

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