Ellipses are one of the biggest topics on Exam 4, and the techniques here โ reading standard form, completing the square, finding foci โ carry over directly to hyperbolas. Nail this section and hyperbolas will feel like a remix, not a new song.
Think of an ellipse as a squished circle โ like an oval or the shape of a running track. Here's a fun way to picture it: stick two thumbtacks into a board (these are the foci), loop a piece of string around them, and pull it tight with a pencil. As you drag the pencil around, you'll trace an ellipse. The total length of string stays the same, which is why the *sum* of the distances from any point on the ellipse to the two foci is always constant.
Center (h, k), vertices at (h ยฑ a, k), co-vertices at (h, k ยฑ b)
Center (h, k), vertices at (h, k ยฑ a), co-vertices at (h ยฑ b, k)
Tap any item if you need a refresher:
Think of an ellipse as a squished circle โ like an oval or the shape of a running track. Here's a fun way to picture it: stick two thumbtacks into a board (these are the foci), loop a piece of string around them, and pull it tight with a pencil. As you drag the pencil around, you'll trace an ellipse. The total length of string stays the same, which is why the *sum* of the distances from any point on the ellipse to the two foci is always constant.
Every ellipse has a longer direction (the major axis) and a shorter direction (the minor axis). The number is always the bigger measurement โ it tells you how far the ellipse stretches along its longer side. The number is the shorter measurement. When you look at the equation, whichever fraction has the bigger denominator โ that's , and the variable underneath it tells you whether the ellipse is wider (horizontal) or taller (vertical).
The two foci are special points inside the ellipse, always sitting on the major axis. You find how far they are from the center using (subtract โ not add!). The eccentricity tells you how squished the ellipse is: if is close to 0 it's nearly a circle, and if is close to 1 it's very long and thin. Earth's orbit around the Sun is an ellipse with โ almost a perfect circle!
When a problem gives you a messy equation (not already in neat fraction form), you'll need to complete the square to rewrite it. The goal is to get it looking like two fractions that equal 1. Once it's in that standard form, everything โ center, , , vertices, foci โ can be read right off the equation.
Center (h, k), vertices at (h ยฑ a, k), co-vertices at (h, k ยฑ b)
Center (h, k), vertices at (h, k ยฑ a), co-vertices at (h ยฑ b, k)
c = distance from center to each focus; foci lie on the major axis
e near 0 โ nearly circular; e near 1 โ elongated