1 99:59:59,999 --> 99:59:59,999 What I want to do in this video is explain what parallax, what parallax actually is and then then 2 99:59:59,999 --> 99:59:59,999 try to visualize what the parallax would be like in the context of observing relatively nearby stars, and then in the next video 3 99:59:59,999 --> 99:59:59,999 we're going to think about how we can use the parallax of nearby stars to figure out how far they actually 4 99:59:59,999 --> 99:59:59,999 are away from us. So parallax really is just the apparent change in the position of something based on 5 99:59:59,999 --> 99:59:59,999 a different line of sight. So when you see that and you just look at, so while you are looking at a car 6 99:59:59,999 --> 99:59:59,999 you are going to see that depending on how far different things are from you it looks like they're moving 7 99:59:59,999 --> 99:59:59,999 relative to each other. Right now I am looking at my computer monitor and if I move my head around 8 99:59:59,999 --> 99:59:59,999 or shake my head around it looks like the wall behind the computer monitor is moving relative to the 9 99:59:59,999 --> 99:59:59,999 computer monitor. We've all experienced this. Let's think about what parallax means when looking at stars. 10 99:59:59,999 --> 99:59:59,999 So let me draw, let me draw the sun here, and obviously none of this is drawn to scale. So let me draw 11 99:59:59,999 --> 99:59:59,999 the sun here and let me draw the earth at some point in its orbit around the sun, and we're going to 12 99:59:59,999 --> 99:59:59,999 pretend that we're looking from above the solar system. The earth will be rotating, the earth will be 13 99:59:59,999 --> 99:59:59,999 rotating in this direction right over here; and let's say that the star we care about, the start that 14 99:59:59,999 --> 99:59:59,999 we care about is right over here. The star that we care about is right over here. Obviously, clearly not 15 99:59:59,999 --> 99:59:59,999 drawn to scale. And what we're going to do is we're going to wait until the point in the year, so the 16 99:59:59,999 --> 99:59:59,999 point in our orbit around the Earth, so that right at dawn, so we're sitting right here on the surface 17 99:59:59,999 --> 99:59:59,999 of the earth and to simplify things we're on the equator and let's say that this is the stars roughly 18 99:59:59,999 --> 99:59:59,999 in the plane of our solar system. So we're sitting right here, we're sitting right here, on the equator, and 19 99:59:59,999 --> 99:59:59,999 then right at dawn, right when the first light of the sun, right when the first light of the sun begins 20 99:59:59,999 --> 99:59:59,999 to reach me; remember that right now the sun is lighting up this side of the earth. So right when the 21 99:59:59,999 --> 99:59:59,999 first light of the sun is reaching me, I'm looking, I'm looking straight up. So if I look straight up