1 00:00:00,520 --> 00:00:03,600 Speaker 1: Welcome to brain Stuff from how stuff works dot com 2 00:00:03,600 --> 00:00:14,760 Speaker 1: where smart Happens. Hi, I'm Marshall Brain With today's question, 3 00:00:15,320 --> 00:00:18,640 Speaker 1: how are astronomers able to measure how far away a 4 00:00:18,800 --> 00:00:22,279 Speaker 1: star is? It turns out that measuring the distance to 5 00:00:22,400 --> 00:00:25,880 Speaker 1: a star is an interesting problem. Astronomers have come up 6 00:00:25,920 --> 00:00:29,200 Speaker 1: with two different techniques to estimate how far away any 7 00:00:29,240 --> 00:00:34,680 Speaker 1: given star might be. The first technique uses triangulation or parallax. 8 00:00:35,240 --> 00:00:38,040 Speaker 1: The Earth's orbit around the Sun has a diameter of 9 00:00:38,080 --> 00:00:41,640 Speaker 1: about a hundred eighty six million miles or three hundred 10 00:00:41,680 --> 00:00:45,120 Speaker 1: million kilometers. By looking at a star one day and 11 00:00:45,159 --> 00:00:48,800 Speaker 1: then looking at it again six months later, and astronomer 12 00:00:48,880 --> 00:00:51,800 Speaker 1: can see a difference in the viewing angle for the star. 13 00:00:52,400 --> 00:00:55,960 Speaker 1: With a little trigg, the different angles yield a distance. 14 00:00:56,400 --> 00:00:59,560 Speaker 1: This technique works for stars that are about four hundred 15 00:00:59,640 --> 00:01:03,600 Speaker 1: light is away from Earth or closer. There's no direct 16 00:01:03,680 --> 00:01:07,520 Speaker 1: method currently available to measure the distance two stars further 17 00:01:07,680 --> 00:01:11,959 Speaker 1: than four light years from Earth, so astronomers instead use 18 00:01:12,120 --> 00:01:16,280 Speaker 1: brightness measurements. It turns out that a star's color spectrum 19 00:01:16,400 --> 00:01:20,320 Speaker 1: is a good indication of its actual brightness. The relationship 20 00:01:20,400 --> 00:01:24,440 Speaker 1: between color and brightness has been proven using the several 21 00:01:24,480 --> 00:01:27,200 Speaker 1: thousand stars that are close enough to Earth to have 22 00:01:27,319 --> 00:01:31,320 Speaker 1: their distance measured directly. Astronomers can therefore look at a 23 00:01:31,400 --> 00:01:35,360 Speaker 1: distant star and determine its color spectrum. From the color, 24 00:01:35,480 --> 00:01:39,000 Speaker 1: they can determine the star's actual brightness, and then, by 25 00:01:39,080 --> 00:01:42,120 Speaker 1: knowing the actual brightness and comparing it to the apparent 26 00:01:42,200 --> 00:01:45,839 Speaker 1: brightness seen from Earth, that is, by looking at how 27 00:01:45,920 --> 00:01:49,160 Speaker 1: dim the star has become once it's light reaches Earth, 28 00:01:49,480 --> 00:01:54,400 Speaker 1: they can determine the distance to the star. For more 29 00:01:54,480 --> 00:01:57,000 Speaker 1: ONNS and thousands of other topics. Does that how stuff 30 00:01:57,000 --> 00:01:59,160 Speaker 1: works dot com and don't forget to check out the 31 00:01:59,160 --> 00:02:01,200 Speaker 1: brain stuff block on the house stuff works dot com 32 00:02:01,240 --> 00:02:04,080 Speaker 1: home page. You can also follow brain stuff on Facebook 33 00:02:04,160 --> 00:02:08,760 Speaker 1: or Twitter at brain stuff h s W. The house 34 00:02:08,800 --> 00:02:12,040 Speaker 1: Stuff Works iPhone app has arrived. Download it today on 35 00:02:12,080 --> 00:02:12,600 Speaker 1: iTunes