Decoding the Magnification Graph
Finding the Focal Length
Graphs in physics are not just lines on a grid; they are visual stories of mathematical relationships. In this problem, we are given a graph showing how the magnification m of a thin lens varies with the image distance v. Our goal is to extract the focal length f from this visual data.
The Math Behind the Graph
To understand the graph, we first need to establish the mathematical relationship between m and v. We start with the fundamental thin lens formula:
We know that magnification m is defined as the ratio of image distance to object distance, m=uv. To introduce m into our equation, we can multiply the entire lens formula by v:
Rearranging this to solve for m, we get:
This equation is beautifully simple. It is in the form of a straight line, y=mx+c, where our y-axis is m and our x-axis is v. The slope of this line is exactly −f1.
Extracting Data from the Graph
Now, let's turn our attention to the provided graph. We need to find the slope of the line using the given points.
The graph highlights two distinct points. The horizontal distance between these two points on the v-axis is given as b. This represents our change in x, or Δv=b.
The vertical distance between these same two points on the m-axis is given as c. This represents our change in y, or Δm=c.
The slope of any straight line is the 'rise over run', or the change in y divided by the change in x:
The Grand Finale
We now have two expressions for the slope of the line: one from our theoretical derivation and one from the graphical data. By equating them, we can solve for the focal length f:
The negative sign indicates the nature of the lens (in this case, a concave lens, since the slope c/b is positive, making f negative). However, the question asks for the magnitude of the focal length, which is simply:
And there we have it! By bridging the gap between algebraic formulas and graphical geometry, we've successfully decoded the focal length.