The weak-star topology is pointwise convergence of functionals on . If is nonreflexive, it is strictly weaker than the weak topology on .
If for a bounded operator on a separable Banach space, and is a nonempty weak-star closed convex subset of the dual unit ball with , then has a fixed point in . The Cesàro averages of the orbit remain in , and minus the identity sends those averages to vectors of norm at most . Weak-star compactness supplies a cluster point, and the adjoint action is weak-star continuous. The corresponding assertion with only weak closedness is false for the right shift on the probability simplex in , the dual of .
The continuous dual of a separable Banach space is separable in its weak-star topology, even when it is not norm separable. Banach-Alaoglu theorem and weak-star metrizability of the dual ball make the dual unit ball a separable compact metric space. The countable union of positive integer multiples of a countable dense subset of that ball is dense in the whole dual. This does not imply global weak-star metrizability.
For an infinite-dimensional normed space, the weak-star open unit ball of its dual is not a Baire space. The smaller closed norm balls are weak-star closed and have empty relative interior: a nonzero functional annihilating any finitely many tested vectors can move the norm beyond the smaller radius while remaining below one. Their countable union is the open norm ball. Thus this topology is not topologically complete, regardless of separability.
A countable local base at zero would give countably many finite sets of evaluation vectors. Any other evaluation must lie in the span of one of those finite sets: otherwise a bounded functional vanishing on that set but not on the evaluation vector, supplied by Hahn-Banach theorem, contradicts inclusion of neighbourhoods after scalar rescaling. Thus the predual has countable Hamel dimension, impossible for an infinite-dimensional Banach space by the Baire category theorem. This concerns the entire dual, unlike weak-star metrizability of the dual ball.
A linear functional on is continuous for the weak-star topology exactly when it is evaluation at an element of . Continuity makes it vanish on the common kernel of finitely many evaluations, so it is a linear combination of those evaluations. The canonical embedding into the bidual identifies this dual with .
In , the sequence converges weak-star to zero by the Riemann-Lebesgue lemma, while converges weak-star to the constant . Nonlinear pointwise operations therefore need not preserve weak-star limits.
If is separable, the weak-star topology on is metrizable. For a dense sequence in , a compatible metric is obtained by summing bounded multiples of .
The dual unit ball is weak-star metrizable if and only if is separable. For the converse direction, Banach-Alaoglu theorem makes a metrizable dual ball a compact metric space, and the evaluation map embeds isometrically into the separable space .
A Banach space is a Grothendieck space when every weak-star convergent sequence in is weakly convergent. Every reflexive Banach space has this property, and every separable Grothendieck space is reflexive.
For a weak-star compact set , its Szlenk derivation at scale is
It removes points having a relatively weak-star open neighbourhood of norm diameter at most .
Transfinite iteration of this operation defines the Szlenk index; one derivation step is not itself the index.
If is separable and is a nonempty weak-star closed subset of , then is a proper subset of for every . Metrizability produces sequences witnessing membership in the derivative, while a Baire-category argument applied to a universal weakly null sequence yields the strict inclusion.

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