We collect here information on 88 near-Earth asteroids with diameters less than 60 m and with high quality light curves. We find that the typical rotation period is 40 min. Relatively few axis ratios are available for such small asteroids, so we also considered the 92 smallest NEAs with known axis ratios. This sample includes asteroids with diameters up to 300 m. The mean and median axis ratios were 1.43 and 1.29, respectively.
Rotation rates much faster than the spin barrier are seen, reaching below 30 s, and implying that most of these bodies are monoliths. Non-principal axis rotation is uncommon. Axial ratios often reach values as high as two, though no undisputed results reach above three. We find little correlation of axis ratio with size. The most common spectral type in the sample of small NEAs is S-type (>90%), with only a handful of C and X types known.