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Rare Venus Transit Across the Sun
Early evening sky watchers may have noticed that the brilliant planet Venus is now appearing lower in the dusk sky each evening; this is nothing to be concerned about. It happens because Venus is orbiting the sun and, within only a week or so, it …Read more.
Antares After Dark
"If you've seen one star, you've seen 'em all." How many times have I heard that phrase over my long stargazing career!
I suppose it's true to one who seldom peers at the nighttime sky. It's really too bad, though, because those of us who …Read more.
Solar Eclipse!
It's been quite a while since we in the United States have enjoyed an eclipse of the sun — about seven years, to be exact. But one is about to occur next Sunday, and you'll definitely not want to miss it.
A solar eclipse occurs when the moon …Read more.
The Celestial Water Snake
Here's a trivia question for you. Which is the largest of all constellations? If you answered "Hydra", you know more about the night sky than you admit.
At this time of year, we can find Hydra, the water snake, low in the southern sky …Read more.
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Week of June 28-July 4, 2009Try this fun experiment. Ask some friends which season of the year they think the Earth is closest to the sun. Unless your acquaintances are atypical, I'll bet most will guess that we're nearer the sun during our summertime. But this just isn't true. Like most celestial bodies, the Earth orbits the sun not in a circle, but along an ellipse. An ellipse is simply a circle that's been squashed. And, because we orbit along an elliptical path, our distance from the sun varies throughout the year. This was discovered some four centuries ago by the German mathematician Johannes Kepler. After struggling for many years to calculate a circular orbit for Mars, Kepler threw up his hands in disgust. All he had to show for his work was 900 pages of calculations and 70 worthless orbits. And then, around Easter 1605, he decided he had seen enough circles for one lifetime. He concluded that all he had left to try was an ellipse or, as he so eloquently described it: "a single cartful of dung". As Kepler drew his ellipse over the data, his eyes lit up. It fit beautifully. In a single moment of unrivalled genius, Kepler solved a problem that had confounded sky watchers for centuries. We now understand that the Earth, too, orbits the sun along an elliptical path.
Our planet's equator is tipped about 23.4 degrees to the plane of its orbit around the sun. This means that, during the months of June, July, and August, the Earth's Northern Hemisphere is tilted toward the sun and allows sunlight to beat directly down upon us. Six months and half an orbit later, our planet's tilt aims the Northern Hemisphere away from the sun, when solar rays shine down on us at a much shallower angle. This is what provides our seasonal temperature changes. It might surprise your friends to learn that the Earth actually reaches its farthest point from the sun during our summertime. This year, "aphelion" occurs around 7 p.m. PDT on July 3. We won't reach our nearest point to the sun — perihelion — until early January. 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. COPYRIGHT 2009 CREATORS SYNDICATE INC. ![]()
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