If $U$ is a vector space then the function $d: \Omega^*(U) \rightarrow \Omega^*(U)$ has the following properties:
$df = \sum_{i= 1}^2 \dfrac{\partial f}{\partial x_i}$ if $f \in \Omega^0(U) $
$d(f\alpha) = df\cdot\alpha + f\cdot d\alpha$, $f\in \Omega^0(U), \alpha \in \Omega^*(U)$
$d \circ d = 0 \implies d \restriction_{\Omega^1(U)} = 0$
Now, I don't understand the implication in third property. For example, if you have $f\,dx \in \Omega^1(U)$ with $f \in \Omega^0(U) $ And you compute $d(f\,dx) = df\,dx \ne 0$