1 00:00:00,000 --> 00:00:04,080 Thanks, Jen. 2 00:00:04,080 --> 00:00:09,600 A Venus transit occurs when Venus crosses the disk of the Sun as seen by an observer. 3 00:00:09,600 --> 00:00:13,720 It's like a solar eclipse in that Venus is located on the line between the Sun and the 4 00:00:13,720 --> 00:00:17,240 Earth and therefore blocks some of the Sun's light. 5 00:00:17,240 --> 00:00:21,680 However, in a Venus transit, the amount of sunlight blocked is very small compared to 6 00:00:21,680 --> 00:00:26,440 a solar eclipse, and so the observer who is unaware will never notice it. 7 00:00:26,440 --> 00:00:30,240 Venus's circular shadow is much, much smaller than our Moon's shadow. 8 00:00:30,240 --> 00:00:34,720 Even though Venus is nearly the size of the Earth, it is much farther away than the Moon. 9 00:00:34,720 --> 00:00:39,960 In clear weather, Venus transits are visible with the naked eye or with a small telescope, 10 00:00:39,960 --> 00:00:43,560 which is why they became popular in the 1600s. 11 00:00:43,560 --> 00:00:48,160 Before the advent of radar, Venus transits were used mainly for the measurement of the 12 00:00:48,160 --> 00:00:52,440 astronomical unit, or the Sun-Earth distance, as you've heard earlier. 13 00:00:52,440 --> 00:00:57,280 The biggest activity surrounding the June 2004 Venus transit will be the International 14 00:00:57,280 --> 00:01:00,320 Network of Amateur Astronomers. 15 00:01:00,320 --> 00:01:04,560 These astronomers will measure the astronomical unit with the Venus transit using the same 16 00:01:04,560 --> 00:01:07,000 techniques as used by the early observers. 17 00:01:07,000 --> 00:01:12,360 An innovative aspect this time, however not available in 1882, is the widespread use of 18 00:01:12,360 --> 00:01:17,600 the Internet to organize international participation and the ease of access to the tools needed 19 00:01:17,600 --> 00:01:19,900 to make the parallax calculations. 20 00:01:19,900 --> 00:01:24,940 There also will be a few astronomical researchers who will try to exploit state-of-the-art observing 21 00:01:24,940 --> 00:01:29,540 tools to see what can be learned about the use of transits to investigate planets around 22 00:01:29,540 --> 00:01:31,100 other stars. 23 00:01:31,100 --> 00:01:34,260 Transits are currently being used to search for such planets. 24 00:01:34,260 --> 00:01:38,300 Perhaps this Venus transit will lead to some new technique or measurement that will allow 25 00:01:38,300 --> 00:01:44,420 future researchers to further study the terrestrial planets during long-range planet-finding missions. 26 00:01:44,420 --> 00:01:49,060 The Venus transit will also serve to remind us of Earth's place in the cosmos. 27 00:01:49,060 --> 00:01:53,340 The tiny dot crossing the solar disk is a terrestrial planet with an atmosphere, and 28 00:01:53,340 --> 00:01:55,020 yet it is far from an Earth. 29 00:01:55,020 --> 00:01:59,780 Venus was once called a twin Earth, in part because of its similar size and distance from 30 00:01:59,780 --> 00:02:00,960 the Sun. 31 00:02:00,960 --> 00:02:05,300 It is now known to be a place that is extremely hostile to life for reasons that are still 32 00:02:05,300 --> 00:02:06,300 under study. 33 00:02:06,300 --> 00:02:10,900 One can speculate how our own pale blue dot would look to some distant alien astronomer 34 00:02:10,900 --> 00:02:15,820 as it passed across the Sun in transit, and whether it has ever been so observed. 35 00:02:15,820 --> 00:02:18,980 Maybe one day humans will be able to observe the Earth transit. 36 00:02:18,980 --> 00:02:23,740 To learn more about the planet Venus and the Venus transit, check out the Sun-Earth Connection 37 00:02:23,740 --> 00:02:25,980 Education Forum website. 38 00:02:25,980 --> 00:02:27,060 Take it away, Jennifer!