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Planetary News: Mercury (2006)Mercury Transit on November 8 -- Watching our Solar System at Workby Melanie Melton Knocke
It's one thing to understand intellectually the forces at work in our solar system. It's another thing to see immediate, physical proof of those forces. On November 8, 2006, you will get your chance to do just that when Mercury passes between Earth and the Sun. Now, given the nature of this event -- known as a Mercury transit -- the forces at work are going to be a little difficult to see. In fact, while it is occurring, most people on our planet won't have a clue that anything special is going on. Even those who know about the transit will require specialized observing equipment to see it. Even so, it will be worth the effort. Below are some examples of solar system forces you will be able to observe firsthand during this five-hour transit, as well as tips on when, where, and how to observe Mercury's passage across the Sun's disk. Our Solar System at Work1. During this transit, you
will see that Mercury is actually moving. During this transit, the Sun will provide an excellent (though bright) backdrop that will allow you to see Mercury's motion clearly. The planet will be visible as a tiny black dot moving slowly and steadily across the bright solar disk. Though the entire transit will take five hours to complete (see exact times below) it will still be moving fast enough for you to notice changes in its position in just a few minutes. 2. You will
notice that Mercury is round. 3. You will
see just how small Mercury is. Keep in mind these numbers: the diameter of the Sun is 1,392,000 kilometers (864,400 miles) and the diameter of Mercury is 4,880 kilometers (3,030 miles). In other words, Mercury will cover a mere 0.06% of the Sun's surface. 4. As
you watch the transit progress, you will notice that the orbit of Mercury
is tilted with respect to the Sun. If the face of the Sun were a clock with its top (north) representing 12:00, Mercury would first cross in front of the Sun at the 4:30 position and exit the Sun at the 9:00 position. NOTE: These are not actual event times, merely position markers! Transit Facts1. When does the transit take place? The halfway point of the transit will be at 1:41 p.m. (PST). The transit will end when Mercury moves away from the Sun at 4:10 p.m. (PST). 2. Who can
see it? Viewers in North and South America will get to see the beginning of the transit. The Sun will set before the transit is complete (although the west coast of the U.S will be able to see the transit in its entirety). For viewers in eastern Asia, Australia, and New Zealand, the transit will already be underway when the Sun rises above your horizon on November 9. You will get to see the end of the transit. The entire transit will be visible over most of the Pacific Ocean, southern Alaska and along the western coast of the United States. People in Europe, Africa, western Asia, the Middle East, and India are out of luck this time around. 3. How to Safely Observe
It. It is extremely important to use filters that were designed specifically for solar viewing. Though Mercury transits are fairly rare (only 13-14 occur each century), they are not worth losing your sight over. If you are not absolutely sure of the safety of your solar filter, DON'T RISK IT! 4. Viewing Without Equipment Hassles. Whether or not you get a chance to view this month's Mercury transit, you've now had a little refresher course on the workings of our solar system, courtesy of its smallest planet.. |
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