On the rotation rates and axis ratios of the smallest known near-Earth asteroids—The archetypes of the Asteroid Redirect Mission targets

•We examine the data available on the smallest near-Earth asteroids.•We characterize the sample from which the Asteroid Redirect Mission target will be chosen.•The average rotation period of the sample is 40 min.•The mean and median axis ratios are 1.43 and 1.29, respectively.•The spectral types are dominated by S types (>90%) with a few C and X types.

NASA's Asteroid Redirect Mission (ARM) has been proposed with the aim to capture a small asteroid a few meters in size and redirect it into an orbit around the Moon. There it can be investigated at leisure by astronauts aboard an Orion or other spacecraft. The target for the mission has not yet been selected, and there are very few potential targets currently known. Though sufficiently small near-Earth asteroids (NEAs) are thought to be numerous, they are also difficult to detect and characterize with current observational facilities. Here we collect the most up-to-date information on near-Earth asteroids in this size range to outline the state of understanding of the properties of these small NEAs. Observational biases certainly mean that our sample is not an ideal representation of the true population of small NEAs. However our sample is representative of the eventual target list for the ARM mission, which will be compiled under very similar observational constraints unless dramatic changes are made to the way near-Earth asteroids are searched for and studied.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%>90%), with only a handful of C and X types known.