Turning a Needle

A needle can turn around in as little area as you like, yet in 3D the set it sweeps can never be thin — proved by Hong Wang and Joshua Zahl in 2025

Turning a Needle

How much room do you need to turn a needle around? In the plane, as little area as you like. Yet in 2025 Hong Wang and Joshua Zahl proved that in three dimensions the set it sweeps can never be thin.

Two Ways to Turn

A unit needle makes a half-turn in a triangle and in a deltoid. Follow the white dot to see it end up reversed.

0.7854
disc of diameter 1
0.5774
triangle, height 1
0.3927
deltoid, π/8

The white dot marks one end of the needle: after a half-turn it is at the other end. Kakeya suspected the deltoid was optimal. Besicovitch showed in 1928 that the answer is: no minimum at all.

Go deeper:Kakeya’s Question

In 1917 Sōichi Kakeya asked for the smallest region in which a unit needle can be turned through 180°. A disc of diameter 1 works, with area π/4 ≈ 0.785. Gyula Pál showed in 1920 that among convex regions the best is the equilateral triangle of height 1, with area 1/√3 ≈ 0.577. The needle pivots at a corner, slides to the next corner, and repeats.

Without convexity you can do better. The deltoid, a three-cusped curve traced by a point on a circle rolling inside another three times its size, has area π/8 ≈ 0.393, and the needle glides round inside it, always touching the curve. Kakeya suspected this was optimal.

It is not, and in fact nothing is. Abram Besicovitch had already built a set of measure zero containing a unit segment in every direction, answering a question in integration theory, and in 1928 he adapted it to Kakeya’s problem. A needle can be turned around in a region of area less than any ε you name. The region becomes a thin tangle of spikes, and the needle has to travel a long way, but the area can be made as small as you like.

A Set With No Area

Raise the stage and watch the area fall. Then drag the direction: a full-height segment is always there.

0.4473
area at this stage
40%
lost since stage 0
0
area in the limit

The blue segment joins a Cantor point below to a Cantor point above, so it survives every stage. The pieces multiply by four each time while the area only creeps down, yet in the limit it is zero. The fan spans about 72°, so three copies turned by 60° cover every direction.

Go deeper:Small Area, Full Dimension

This construction is Jean-Pierre Kahane’s, from 1969. Take the Cantor set C of numbers whose base-4 digits are all 0 or 3. Put C on the bottom edge and a half-size copy on the top edge, and join every point below to every point above. The run of a segment from (x, 0) to (y/2, 1) is y/2 − x, and its base-4 digits are 1.5 times one of −2, −1, 0, 1. Four consecutive values are enough to fill an interval, so the runs cover all of [−1, 1/2].

Every horizontal slice of the limit set is a projection of the four-corner Cantor set C × C. That set is a scattered dust of total length zero in almost every direction, which is Besicovitch’s projection theorem. So almost every slice has length zero, and the set has area zero.

Measure zero is not the same as small in every sense. Roy Davies proved in 1971 that any set in the plane containing a segment in every direction has Hausdorff dimension 2: it is as large as the plane itself in the sense of dimension. The Kakeya conjecture says the same holds in every dimension: a set in ℝⁿ containing a unit segment in every direction has dimension n. It sits underneath some of the central open problems in harmonic analysis, including the restriction conjecture, which is why so much work has gone into it.

Kakeya Sets in a Finite World

Over a finite field every line is a row of q points. Step through the directions and compare the set’s size with Dvir’s bound.

133
points in the set
343
points in F_7³
39%
of the whole space
84
Dvir's lower bound

Every one of the 57 directions has a full line inside the orange set (the blue one is highlighted). As q grows this set fills about half of the plane and a quarter of space, and Dvir’s bound says no cleverer arrangement can fall below a fixed fraction.

Go deeper:Dvir in 2008, Wang and Zahl in 2025

In 1999 Thomas Wolff proposed a model problem: replace ℝⁿ by 𝔽_qⁿ, the n-dimensional space over a finite field with q elements, and ask how few points a set can have if it contains a full line in every direction. Zeev Dvir settled it in 2008 with an argument short enough to sketch here. If a set K has fewer than C(q + n − 1, n) points, some nonzero polynomial of degree at most q − 1 vanishes on all of K. Restricted to any line in K it vanishes at q points, more than its degree, so it vanishes on the whole line. Then its top-degree part vanishes at every direction vector, hence everywhere, and a nonzero polynomial of degree below q cannot vanish on the whole space. So K has at least C(q + n − 1, n) ≈ qⁿ/n! points, a fixed fraction of the space.

The real problem is much harder, because ℝ has no analogue of the counting that makes polynomials work so well over a finite field. In three dimensions Wolff proved in 1995 that a Kakeya set has dimension at least 5/2, and for thirty years the improvements came in tiny increments. The modern approach works with thickened tubes rather than segments: for each of about δ⁻² well-separated directions, take a tube of radius δ, and show that the union cannot be much smaller than the whole region however the tubes are arranged.

In February 2025 Hong Wang and Joshua Zahl posted a proof that every Kakeya set in ℝ³ has Hausdorff dimension 3 (arXiv:2502.17655), building on their earlier work on “sticky” Kakeya sets, where tubes pointing in nearby directions stay close together. The conjecture is still open in four dimensions and higher.

Key Takeaways

  • The best convex region for turning a unit needle is the triangle of height 1, with area 1/√3.
  • Besicovitch showed a needle can be turned in any positive area, however small.
  • Such sets still have full dimension: 2 in the plane (Davies 1971), 3 in space (Wang and Zahl 2025).
  • Over finite fields, Dvir’s polynomial method shows Kakeya sets fill a fixed fraction of space.

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