Last time | Next time |
You also have a homework for 5.2 due Wednesday, 3/4.
Before we leave, however, I need to issue a correction that Grant brought to my attention:
For my final example, I neglected to square a term (#5), so I want to fix that.
Then I'd like to revisit the computation of Earth's mass from last time, which I did via a method of "spherical shells". In that case we have a sphere, which has a mass density function
I saw that graph and decided to
The shells look like this (imagine an onion). At left is a "dV", a little chunk of volume. We'd multiply that dV times the mass density at that radius, to get a .
Then we add up the in an integral:
where is the radius of the Earth.
independent | dependent |
oC | oF |
0 | 32 |
100 | 212 |
create a nice graph of (Fahrenheit as a function of Celsius). Compute .
Then write the linear function g that converts C to F.
As soon as we answer that question, we'll probably want to know: how do we convert between Celsius and Fahrenheit? That's the inverse function!
Write the linear function that converts F to C.
Now: would we want to carry out stage three of the three-step process of computing an inverse function? That is, would you want to exchange the variable names of the dependent and independent variables?
Now you made nice graphs: criticize my graphs in the Mathematica summary.