Start typing, then use the up and down arrows to select an option from the list.

Table of contents

Hey, guys, in this video, we're gonna talk about an equation for mirrors that will tell us pretty much everything that we need to know about the images produced by mirrors. Before we had to rely on ray diagrams, which are notoriously difficult to draw, then are really only good for qualitative information. With the mirror equation will be able to get definite quantitative information, such as the image, location, whether it's real or virtual, whether it's upright, inverted, etcetera. Okay, let's get to it. What? We're gonna focus on our spherical mirrors, and that's basically all that you ever see. Okay, what a spherical mirrors is is it's a mirror that's cut from a sphere. Okay, It's not really cut from a sphere thes air shaped to exist as if they had been part of a sphere. Okay, so you see the solid piece right here, the shaded in peace that's our actual mirror. What I've gone ahead and done is drawn with dashed lines. The sphere that this mirror appears to be part of okay, and that sphere has a radius R. Okay, now the mirror, because it's a piece of this imaginary sphere that doesn't actually exist it's still defined by that radius. And we call that for a curve. We call it the radius of curvature. That would be the radius of the sphere that that piece belonged to if it was part of this here. Okay, now the focal length Onley depends upon this radius of curvature, and it's just are divided by two. Okay, really easy to remember the focal length of a mirror half the radius of its curvature. Okay, Once you know the focal length for any spherical mirror, we have the mirror equation to determine where the image is located. Okay, we would say that one over the object distance how far the object is from the mirror, plus one over the image distance. How far the images from the mirror equals one over the focal length of that mirror. Right, which is just as we saw are over to In order to use the mirror equation properly, there are some sign conventions that we need to memorize. Okay. A con cave mirror, which is a converging mirror, right? It's a mirror that when column mated, light comes into it. That column aided like eventually focuses onto a single point that converging mirror. The con cave mirror has a positive focal length. Okay, always a positive focal length by convention, and it can produce images that have a positive image distance or a negative image distance. And we'll talk about what that means in a second. Convex mirrors, on the other hand, are diverging mirrors. When you have initially column aided light coming at it, that light is spread apart. That light is never focused, and by convention we assign convex mirrors negative focal lengths, and they can Onley produce negative image distances. Okay, for plain mirrors, which neither converge nor diverge light, we say by convention that the focal length is infinity. That's how we're gonna use it in the mirror equation. And it, too, can Onley produce negative image distances. So let's talk about these image distances and what it means. If we have a positive image. Distance this images riel and inverted. Okay, those two are always paired. All riel images are always inverted, okay, and they always have a positive image distance. If the image distances negative, this image is virtual and its upright. This always goes together. All virtual images air always upright, and they always have a negative image. Distance. Okay, so which of the three types of mirrors can produce a real image? The only one that could produce a real image is a con cave mirror, and this should have seemed obvious. A real images on Lee formed by a convergence of light and the Onley mirror that converge light is the con cave mirror. Any mirror that doesn't converge like cannot produce a real image. So the other two types of mirrors are stuck producing virtual images. Okay, lastly, straight as a result of the mirror equation, it's really easy to find the magnification of an image, which is how tall it is relative to the objects height, and this is given by this equation right here in this orange box. Now, the negative sign is a convention that may or may not be included in your textbooks and your lectures, and any other resource is you have what that negative sign is, therefore, is to tell you whether or not the images upright or inverted. Okay, if you have a positive magnification, the images upright. If you have a negative magnification, the images inverted. How do you get a positive magnification s I has to be negative. Which means the image has to be virtual. How do you get a negative magnification s? I has to be positive, Which means the image has to be inverted. Okay, Sorry. The image has to be riel because the information is already given right here. You don't actually need the negative sign of this equation is just a convention. But what the equation tells you is the size of the image relative to the object. If the magnification is to the objects twice as tall. But the magnification is half the objects, half is tall. Okay, Sorry. The image, if the magnification to the images twice as tall. If the magnification is half the images, half is tall. Okay, let's do a quick example. Ah, 1.4 m tall person stands 1 m in front of a plane mirror. Where is the person's image located? And how tall is it? Okay, so we have our mirror equation, which is always going to tell us where our image is located. Now, the thing here is that the focal length is actually infinity, right? And one divided it by infinity is zero. What this means is if I move the image distance to the other side, we have that one over. The image distances the negative off one over the object distance, or that the image distance is the negative of the object distance. So it's negative. 1 m, right? A person stands 1 m in front of a mirror. So if the object distances 1 m, the image instances negative 1 m. What does that mean about the images it riel? Or is it virtual? It's clearly virtual. And we knew this already that a plane mirror can only produce virtual images. Now, how tall is it? Well, to find the height, we need to use the magnification equation and I'll use the sign just to be proper about this. This is negative. S I over S O, which is negative. 1 m over 1 m, which is positive one. The positive means that this image is upright. This is why the sign is pretty much irrelevant in the magnification equation. We already knew that because this image distance was negative. This image was virtual and therefore it had to be upright. So we didn't gain any new information from the magnification or the sign of the magnification. But a magnification of one means that the height of the image has to equal the height of the object, which, as we're told, is 1.4 meters. Okay, this wraps up our discussion on the mirror equation. All right, guys, Thanks for watching.

Related Videos

Related Practice

04:55

03:23

05:35

09:03

05:21

11:00

11:27

05:25

04:11

© 1996–2023 Pearson All rights reserved.