Let be a regular surface. Its first fundamental form at is the positive definite quadratic form on
where
Examples
Example 19.14 (Angles between coordinate curves)
The first fundamental form also measures angles: the coordinate curves and meet at the angle with
the single coefficient decides orthogonality of the parameter net. For the sphere chart and the helicoid, : meridians cut parallels, and helices cut the horizontal rulings, at right angles — which is why their area integrands collapsed to . For a graph chart, vanishes only where a partial derivative does: the coordinate net of a tilted graph is not orthogonal, even though the -net downstairs is. When computations on a surface look heavy, the first move is to seek a chart with .
Example 19.17 (Why airliners fly over the pole)
Two airports sit at latitude and opposite longitudes: and on the sphere of radius . Along the parallel (), the length is . Along the route over the pole (up the meridian , down the meridian ), it is . At latitude (sixty degrees): parallel route , polar route — a third shorter. In fact on (the function vanishes at both ends and its derivative changes sign once, so it is first increasing then decreasing, hence nonnegative): the polar route never loses. The first fundamental form turned a navigation question into two one-line integrals; Exercise 19.6 pushes the idea to a genuine minimality proof for meridians.
Example 19.22 (Two different graphs, one area)
Over the unit disk, compare the bowl and the saddle . Their area integrands (Exercise 19.5) are
identical. The two surfaces — one curving the same way in all directions, the other saddle-shaped — have exactly equal areas over every domain, over the unit disk. The area element only sees the length of the gradient, not the arrangement of the bending; telling the bowl from the saddle requires second-order data (the sign structure exhibited in Figure 19.1), which no amount of area measurement detects. First fundamental form: metric, blind to shape; the shape-seeing second form belongs to Year 3.