1 00:00:00,040 --> 00:00:09,050 [Music] 2 00:00:09,070 --> 00:00:13,080 Carolyn Crow: So far we've found more than 400 planets around other stars. 3 00:00:13,100 --> 00:00:17,110 Unfortunately, for many years to come, we won't be able to see them as anything more than dim 4 00:00:17,130 --> 00:00:21,180 points of light. If only the planets that we know best could help us 5 00:00:21,200 --> 00:00:25,250 learn more about the real worlds behind those dim points of light. 6 00:00:25,270 --> 00:00:29,430 Well it turns out they can. Remember the Deep Impact mission? 7 00:00:29,450 --> 00:00:33,460 The NASA spacecraft that slammed a probe into a comet in 2005? 8 00:00:33,480 --> 00:00:37,480 Well now it's headed for another comet. While on its way we used its 9 00:00:37,500 --> 00:00:41,500 instruments to study the amount of red, green, and blue light reflected 10 00:00:41,520 --> 00:00:45,540 by Earth, the Moon, and Mars. Combining this color information 11 00:00:45,560 --> 00:00:49,560 with similar studies of the other planets in our solar system, we found an interesting 12 00:00:49,580 --> 00:00:53,590 pattern. These crosshairs mark the spot where 13 00:00:53,610 --> 00:00:57,620 a planet would perfectly reflect all the light from the Sun. The more 14 00:00:57,640 --> 00:01:01,640 red light a planet reflects, the farther it moves to the right on this chart. 15 00:01:01,660 --> 00:01:05,660 The more blue light it reflects, the higher it goes. And if the 16 00:01:05,680 --> 00:01:09,840 planet reflects relatively little blue and red light, it falls in the dark 17 00:01:09,860 --> 00:01:13,850 section. Viewed in this way, here's 18 00:01:13,870 --> 00:01:17,870 where the planets lie. 19 00:01:21,920 --> 00:01:25,920 Not surprisingly, Mars, the reddest planet, occupies the reddest spot. 20 00:01:25,940 --> 00:01:29,960 Mercury is also nearby on the plot because neither planet has a large 21 00:01:29,980 --> 00:01:33,980 atmosphere that scatters blue light. Venus has a thick cloudy atmosphere 22 00:01:34,000 --> 00:01:38,020 that reflects most of the red light and only a little bit 23 00:01:38,040 --> 00:01:42,050 of the blue light, so it stays near the bottom. Jupiter and Saturn fall in the darkest 24 00:01:42,070 --> 00:01:46,100 region of the plot. Their atmospheres have methane and ammonia in it, which 25 00:01:46,120 --> 00:01:50,110 absorbs red light and other gasses that absorb blue light. 26 00:01:50,130 --> 00:01:54,270 Here's what's really interesting. In this chart, Earth stands apart 27 00:01:54,290 --> 00:01:58,290 from all the other planets. Earth is 28 00:01:58,310 --> 00:02:02,320 really blue. Not because of its oceans, but because it has an atmosphere that reflects 29 00:02:02,340 --> 00:02:06,350 a lot of blue light. It makes sense, that's why the sky is blue. 30 00:02:06,370 --> 00:02:10,380 At the same time, Earth does reflect a little bit of red light. 31 00:02:10,400 --> 00:02:14,420 Long before we have telescopes that will show us what extrasolar 32 00:02:14,440 --> 00:02:18,460 planets really look like, we'll be able to measure their colors and put them on the plot. 33 00:02:18,480 --> 00:02:22,500 This means we'll be able to tell the difference between alien 34 00:02:22,520 --> 00:02:26,550 versions of Mars, Jupiter, and even Earth. And that's