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2003-11-08, 08:14 PM
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[Ignore Me] #2 | ||
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First Sergeant
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I can see it, but its a little cloudy here
 . heres an article i found: By Joe Rao SPACE.COM PROBABLY NOT all of the phenomena mentioned will occur because no two eclipses are exactly the same. But many will, and those who know what to look for have a better chance of seeing the special effects of the eclipse. THE STAGES OF THE ECLIPSE 1. Moon enters penumbra (5:15 p.m. ET): Earth�s shadow cone has two parts: a dark, inner umbra, surrounding by a lighter penumbra. The penumbra is the pale outer portion of the Earth�s shadow. � Overview of the Nov. 8 Total Lunar Eclipse � Full Moon Fever � While You're Out, Take a Look at Venus � Fear and Awe: Eclipses Through the Ages � Next: The Meteor Show Although the eclipse begins officially at this moment, this is in essence an academic event. You won�t see anything unusual happening to the moon � at least not just yet. Earth�s penumbral shadow is so faint that it remains invisible until the moon is deeply immersed in it. We must wait until the penumbra has reached roughly 70 percent across the moon�s disk. For about the next hour the full moon will continue to appear to shine normally, although with each passing minute it is progressing ever deeper into Earth�s outer shadow. 2. Penumbral shadow begins to appear (6:14 p.m. ET): Now the moon has progressed far enough into the penumbra so that it should be evident on the moon�s disk. Start looking for a very subtle light shading to appear on the moon�s left portion. This will become increasingly more evident as the minutes pass, the shading appearing to spread and deepen. Just before the moon begins to enter the Earth�s dark umbral shadow the penumbra should appear as an obvious smudge or tarnishing of the moon�s left portion. 3. Moon enters umbra (6:33 p.m. ET): The moon now begins to cross into Earth�s dark central shadow, called the umbra. A small dark scallop begins to appear on the moon�s left-hand (eastern) limb. The partial phases of the eclipse begin; the pace quickens and the change is dramatic. The umbra is much darker than the penumbra and fairly sharp-edged. As the minutes pass the dark shadow appears to slowly creep across the moon�s face. At first, the moon�s limb may seem to vanish completely inside of the umbra, but much later, as it moves in deeper, you�ll probably notice it glowing dimly orange, red or brown. Notice also that the edge of Earth�s shadow projected on the moon is curved. Here is visible evidence that Earth is a sphere, as deduced by Aristotle from lunar eclipses he observed in the 4th century B.C. Almost as if a dimmer switch was slowly being turned down, the surrounding landscape on Earth and deep shadows of a brilliant moonlit night begin to fade away, at least for viewers away from bright lights. 4. 75 percent coverage (7:43 p.m. ET): With three-quarters of the moon�s disk now eclipsed, that part of it that is immersed in shadow should begin to very faintly light up, similar to a piece of iron heated to the point where it just begins to glow. Click through the highlights of the May 15-16 total lunar eclipse. It now becomes obvious that the umbral shadow does not involve complete darkness. Using binoculars or a telescope, its outer part is usually light enough to reveal lunar seas and craters, but the central part is much darker, and sometimes no surface features are recognizable. Colors in the umbra vary greatly from one eclipse to the next, Reds and grays usually predominate, but sometimes browns, blues and other tints are encountered. 5. Less than five minutes to totality (8:01 p.m. ET): Several minutes before (and after) totality, the contrast between the remaining pale-yellow sliver and the ruddy-brown coloration spread over the rest of the moon�s disk may produce a beautiful phenomenon known to some as the �Japanese Lantern Effect.� 6. Total eclipse begins (8:06 p.m. ET): When the last of the moon enters the umbra, the total eclipse begins. How the moon will appear during totality is not known. Some eclipses are such a dark gray-black that the moon nearly vanishes from view. At other eclipses it can glow a bright orange. The reason the moon can be seen at all when totally eclipsed is that sunlight is scattered and refracted around the edge of Earth by our atmosphere. To an astronaut standing on the moon during totality, the sun would be hidden behind a dark Earth outlined by a brilliant red ring consisting of all the world�s sunrises and sunsets. The brightness of this ring around Earth depends on global weather conditions and the amount of dust suspended in the air. A clear atmosphere on Earth means a bright lunar eclipse. If a major volcanic eruption has injected particles into the stratosphere during the previous couple of years, the eclipse is very dark. No such eruption has happened since our last total lunar eclipse in May of this year, so the betting is that this eclipse will be bright. A total lunar eclipse actually turns the moon red ... but why? Click to find out. 7. Middle of totality (8:19 p.m. ET): The moon is now shining anywhere from 10,000 to 100,000 times fainter than it was just a couple of hours ago. Since the moon is moving well to the south of the center of Earth�s umbra, the gradation of color and brightness across the moon�s disk should be such that its upper portion should appear darkest, with hues of deep copper or chocolate brown. Meanwhile, its lower portion � that part of the moon closest to the outer edge of the umbra � should appear brightest, with hues of reds, oranges and even perhaps a soft bluish-white. Observers away from bright city lights will notice a much greater number of stars than were visible before the eclipse began. The moon will be in the constellation of Aries the Ram, with the beautiful little Pleiades star cluster shining 15 degrees to the moon�s east (left). Your fist on an outstretched arm covers about 10 degrees of sky. More about eclipses The total phase of the lunar eclipse lasts from 8:06 to 8:31 p.m. ET Saturday, and is visible wherever the moon is above the horizon. � Show could be colorful � Guide to the eclipse � Why the moon turns red � 10 cool eclipse facts � Learn about the moon � MSNBC Live Video The darkness of the sky is impressive for those in the countryside. The surrounding landscape takes on a somber hue. Before the eclipse, the full moon looked flat and one-dimensional. During totality, however, it will look smaller and three-dimensional, like some weirdly illuminated ball suspended in space. Before the moon entered Earth�s shadow, the temperature on its sunlit surface hovered at 266 degrees Fahrenheit (130 degrees Celsius). Since the moon lacks an atmosphere, there is no way that this heat can be retained from escaping into space as the shadow sweeps by. Now, in shadow, the temperature on the moon has dropped to minus 146 degrees Fahrenheit (99 degrees below zero Celsius). That�s a drop of 412 degrees Fahrenheit (229 degrees Celsius) in less than 90 minutes! 8. Total eclipse ends (8:31 p.m. ET): The emergence of the moon from the shadow begins. The first small segment of the moon begins to reappear, followed again for the next several minutes by the Japanese Lantern Effect. 9. 75 percent coverage (8:55 p.m. ET ): Any vestiges of coloration within the umbra should be disappearing now. From here on, as the dark shadow methodically creeps off the moon�s disk it should appear black and featureless. 10. Moon leaves umbra (10:05 p.m. ET): The dark central shadow clears the moon�s right hand (western) limb. 11. Penumbra shadow fades away (10:24 p.m. ET): As the last, faint shading vanishes off the Moon�s right portion, the visual show comes to an end. 12. Moon leaves penumbra (11:22 p.m. ET): The eclipse �officially� ends, as it is completely free of the penumbral shadow. Joe Rao � a veteran of eleven total lunar eclipses � serves as an instructor and guest lecturer at New York�s Hayden Planetarium. He writes about astronomy for The New York Times and other publications, and he is also an on-camera meteorologist for News 12 Westchester, New York. � 2003 Space.com. All rights reserved. Source: http://msnbc.com/news/978686.asp#BODY
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sig-less Last edited by Blood_Knight; 2003-11-08 at 08:16 PM. |
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2003-11-08, 09:05 PM
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[Ignore Me] #4 | ||
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Contributor General
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Saw it. Anyone in the Northeast should have seen it. Rather wierd to see a red moon above you.
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Commanding Officer  To the next idiot who says the PS2 Devs do not listen: See this Thread |
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2003-11-08, 10:18 PM
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[Ignore Me] #11 | ||
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Lightbulb Collector
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No moon. Too many clouds. Any of you ever read "The Long Rain" by Ray Bradbury? That's Miami during summer and autumn nights.
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The gun katas. Through analysis of thousands of recorded gunfights, the Cleric has determined that the geometric distribution of antagonists in any gun battle is a statistically predictable element. The gun kata treats the gun as a total weapon, each fluid position representing a maximum kill zone, inflicting maximum damage on the maximum number of opponents while keeping the defender clear of the statistically traditional trajectories of return fire. By the rote mastery of this art, your firing efficiency will rise by no less than 120%. The difference of a 63% increase to lethal proficiency makes the master of the gun katas an adversary not to be taken lightly. |
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2003-11-08, 10:54 PM
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[Ignore Me] #15 | ||
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Lightbulb Collector
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The gun katas. Through analysis of thousands of recorded gunfights, the Cleric has determined that the geometric distribution of antagonists in any gun battle is a statistically predictable element. The gun kata treats the gun as a total weapon, each fluid position representing a maximum kill zone, inflicting maximum damage on the maximum number of opponents while keeping the defender clear of the statistically traditional trajectories of return fire. By the rote mastery of this art, your firing efficiency will rise by no less than 120%. The difference of a 63% increase to lethal proficiency makes the master of the gun katas an adversary not to be taken lightly. |
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will UL later
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