The short video above clearly describes how the tilt of the Earth’s axis causes the seasons.
We’ve come to the end of February and tomorrow will tiptoe into March. Traveling at 66,487 miles per hour aboard spaceship Earth, you and I have traveled over 110 million miles around the sun since the first day of winter. That’s far enough to see a new set of constellations surge into the eastern sky as well as to change our hemisphere’s orientation with respect to the sun. No longer is the northern hemisphere pointed directly away from the sun as in December. Spring, the time of equality of light for both hemispheres, is just three weeks away. You’ve probably already noticed that the sun is considerably higher now at noon; it also rises and sets further north. We’ve gained a full hour of daylight in the morning and an hour and a half in the evening. Even with bright moonlight, I could still see the blue tint of twilight in the west yesterday at 7 o’clock.

The star Sirius sparkled in the southeastern sky when I photographed it at 7 p.m. in moonlight last night. Details: 35mm lens at f/2.8. 15-second exposure at ISO 800. Photo: Bob King
Speaking of twilight, two people asked me this week what that bright star is in the south just as the sky gets dark. Although we’ve visited with this star several times over the winter, it doesn’t hurt to return to it again in case you’ve forgotten. It’s Sirius in the constellation Canis Major and the brightest star in the entire night sky. No photo can quite capture its searing, magnesium-white flame. Sirius is 1.75 times the sun’s diameter and about 25 times brighter. Combined with its relative proximity to Earth of just 8.6 light years, it’s no wonder it shines so brightly. Sirius remains prominent in the southern sky throughout March.
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Face the moon to find Saturn over the next couple evenings. Created with Stellarium
The moon will be full tonight and conveniently positioned midway between Leo the Lion’s brightest star Regulus and the planet Saturn. Tomorrow night it’s even closer to Saturn. If you’ve been wondering just how to find the ringed planet, let the moon be your guide.

Supernova (SN) 2010Y is an exploding star in the galaxy NGC 3392 not far from the bowl of the Big Dipper. The light from the stellar explosion is so intense it shines as brightly as the galaxy’s entire nucleus which is packed with millions of stars. NGC 3394 is another spiral galaxy in the same field of view. Credit: William Wiethoff
Champion supernova photographer William Wiethoff of Port Wing, Wisconsin sent me some photos of recent supernovas he photographed with his 14-inch telescope Friday night. At any particular time, there might be a dozen or so supernovas visible in galaxies beyond the Milky Way. Most are very faint and difficult to see visually but show up well in long time exposure photography. 2010Y was the 25th supernova discovered this year and was found by amateur supernova hunter Giancarlo Cortini of Italy on February 8. The host galaxy, NGC 3392 is located about 150 million light years from Earth. This one is bright enough to see at high power through larger amateur telescopes. Supernovas come in two basic varieties: supergiant stars that run out of nuclear fuel in their cores which leads to collapse, implosion and then explosion or white dwarf stars that "put on" too much weight and explode like titantic thermonuclear bombs.
Early this week spacecraft will make close flybys of three planetary moons. On March 2, Cassini will take closeup photos and "sniff" Saturn’s moon Rhea for unusual particles it might be giving off, while on the 3rd it will photograph the small moon Helene. Also the 3rd, the European Mars Express craft will take the closest pictures ever of Mars’ moon Phobos. We’ll have images to share as they arrive.
I was a just a boy of 10 or 11 when I first got interested in astronomy. I still can’t recall exactly what spurred my interest — was it the space program, a total lunar eclipse or did I just decide to look up for the first time and wonder? From suburban Chicago I followed the motions of the planets and still have meticulous notes of lunar conjunctions, ice halos and interesting clouds. At age 13 I decided it was time to start an astronomy club. It went by the somewhat overblown name "The Organization of Amateur Astronomers" and garnered a few of my grade school friends. We hung out talking about astronomy … and girls.
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Aristarchus brilliant idea lives on with his namesake crater. It measures 28 miles across, modest by moon standards, and is located in a vast, relatively smooth lunar "sea" called the Ocean of Storms. This is the moon’s largest sea, and it stretches across some 1500 miles. Most lunar craters are more than three billion years old but Aristarchus’ age is estimated to be only 450 million, a teenager in comparison. That’s why it’s so bright. When the asteroid hit that excavated the crater, it exposed fresh lunar soil from beneath the surface. Over time the soil, or regolith as it’s called, weathers to darker greys under the influence of the sun’s radiation. The crater’s relative youth gives it that fresh-faced look and also makes it an easy target for binoculars..jpg)





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Mountains on Earth generally form as a result of moving tectonic plates that "bump" into one another. On the moon, many of the most prominent mountain chains like the Apennines were formed from rock uplifted during enormous impacts long ago. One of the largest dark spots that forms part of the "man in the moon’s" face is Mare Imbrium or the Sea of Rains. This 700-mile diameter basin was formed formed by a colossal asteroid impact about 3.7 billion years ago which later filled up with lava. Several mountain ranges define its perimeter including the Apennines..jpg)


Because the moon is less than half-lit tonight (40 percent), the boundary separating the bright, daylit part from the part still not in sunlight will be slightly curved. This boundary is called the terminator. Sunday night the moon will be seven days old, exactly half-lit and the terminator will run straight up and down. Try to visualize the terminator as the advancing edge of sunrise on the moon’s surface. The moon never sits still but is always moving apace in its orbit around Earth. Before full moon, the terminator advances toward the east (left) and reveals a new slice of lunar landscape each night. After full moon, the moon’s phase lessens or "wanes" and the terminator becomes the advancing line of lunar sunset. When the sun has set over most of the moon, we see it as a thin crescent in the morning sky at dawn. The moon disappears for a day or two around new moon phase because it’s lost in the glare of the daytime sun. When it reappears as an evening crescent, the terminator once again becomes the advancing line of lunar sunrise. The changing phases and shifting terminator of the moon are ultimately caused by the ever-changing angle between Earth, sun and moon during the moon’s monthly orbital cycle. Use the illustration below to help guide you through the phases.
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