Apply Snell's law to find an angle of refraction, and apply the thin lens equation to find the location, orientation, and size of an image formed by a lens.
Refraction is the bending of light as it crosses into a medium where its speed changes -- light slows down entering a denser (higher-index) medium, like going from air into water or glass, and this bends the ray TOWARD the normal (the reverse happens moving into a less dense medium, bending AWAY from the normal). Snell's law makes this precise: n1*sin(theta1) = n2*sin(theta2), where n is each medium's index of refraction (about 1.00 for air, 1.33 for water, 1.5 for typical glass) and theta is measured from the normal.
Lenses use refraction at two curved surfaces to form images, and remarkably reuse the SAME equations as mirrors last week: 1/do + 1/di = 1/f and m = -di/do, with the same sign convention (converging lenses have positive f, diverging lenses have negative f). The key physical difference from a mirror is geometric: a lens's real image forms on the OPPOSITE side from the object (light passes all the way through), while a mirror's real image forms on the SAME side (light bounces back) -- but the numbers work out identically either way.
Mastery looks like: They apply Snell's law to find an angle of refraction, and apply the thin lens equation to find an image's location, orientation, and size for a converging or diverging lens.
Common stumbles: Forgetting that light bends AWAY from the normal when entering a LESS dense medium (the reverse of the worked example's case); mixing up which side of a lens a real image forms on compared to a mirror.