A vector-valued function r(t) = ⟨f(t), g(t), h(t)⟩ maps a scalar parameter to a vector in ℝ³, tracing a curve through space as t varies. Limits, continuity, and derivatives are defined component-wise: r′(t) = ⟨f′(t), g′(t), h′(t)⟩. The derivative r′(t) is the tangent vector to the curve at each point, and its magnitude |r′(t)| is the instantaneous speed. Integration of vector-valued functions is also component-wise.
Connect to parametric curves from single-variable calculus — a vector-valued function in ℝ³ is just a parametric curve with three components instead of two. Visualize the curve in 3D before computing derivatives. Emphasize that r′(t) gives direction (tangent) while |r′(t)| gives speed; these are distinct pieces of information.
You've worked with parametric curves in single-variable calculus — a curve traced by (x(t), y(t)) as t varies. A vector-valued function r(t) = ⟨f(t), g(t), h(t)⟩ is exactly that idea extended to three dimensions. The scalar parameter t can represent time, arc length, or any convenient variable. As t runs through its domain, the tip of the vector r(t) traces a space curve through ℝ³. Every point on the curve corresponds to a t-value, and the entire trajectory is encoded in a single vector expression.
Limits, continuity, and derivatives are defined component-wise, meaning all the machinery from single-variable calculus carries over directly: r′(t) = ⟨f′(t), g′(t), h′(t)⟩ just differentiates each component independently. All derivative rules apply component-wise as well — the product rule, quotient rule, and chain rule each work on individual components. The chain rule for r(s(t)) gives dr/dt = r′(s(t)) · s′(t), where the scalar s′(t) scales the entire output vector.
The geometric meaning of r′(t) is the tangent vector to the curve at r(t). It points in the direction of travel and its magnitude |r′(t)| is the instantaneous speed. Speed and velocity are distinct: velocity is the vector r′(t) (directional), speed is its scalar magnitude |r′(t)|. The unit tangent vector T(t) = r′(t)/|r′(t)| discards speed to preserve only direction — it will be essential when you study curvature and the Frenet-Serret frame for space curves.
Integration also works component-wise: ∫r(t)dt = ⟨∫f(t)dt, ∫g(t)dt, ∫h(t)dt⟩, producing a vector antiderivative. A definite integral ∫_a^b r(t)dt produces a single vector representing net displacement — where you end up minus where you started. This is distinct from arc length ∫_a^b |r′(t)|dt, which is a scalar measuring total distance traveled along the curve. Net displacement and arc length agree only for straight-line motion in one direction; in general, a winding curve travels far more distance than its net displacement suggests. Keeping these two quantities conceptually separate is one of the key organizational skills in this part of multivariable calculus.