The lunar phases of dust grains orbiting Fomalhaut

TL;DR

This paper explains the backward scattering of dust in the Fomalhaut ring by proposing the dominance of large grains, similar to micro-asteroids, which exhibit lunar-like phases and differ from solar system dust.

Contribution

It introduces a model where large grains dominate the Fomalhaut dust ring, explaining its backward scattering and lunar-like phases, contrasting with solar system dust properties.

Findings

Fomalhaut's dust grains are larger than solar system zodiacal dust.

The dust exhibits lunar-like phases due to large grain sizes.

The dust ring is dominated by micro-asteroids, not small dust particles.

Abstract

Optical images of the nearby star Fomalhaut show a ring of dust orbiting the central star. This dust is in many respects expected to be similar to the zodiacal dust in the solar system. The ring displays a clear brightness asymmetry, attributed to asymmetric scattering of the central starlight by the circumstellar dust grains. Recent measurements show that the bright side of the Fomalhaut ring is oriented away from us. This implies that the grains in this system scatter most of the light in the backward direction, in sharp contrast to the forward-scattering nature of the grains in the solar system. In this letter, we show that grains considerably larger than those dominating the solar system zodiacal dust cloud provide a natural explanation for the apparent backward scattering behavior. In fact, we see the phases of the dust grains in the same way as we can observe the phases of the Moon and other large solar system bodies. We outline how the theory of the scattering behavior of planetesimals can be used to explain the Fomalhaut dust properties. This indicates that the Fomalhaut dust ring is dominated by very large grains. The material orbiting Fomalhaut, which is at the transition between dust and planetesimals, can, with respect to their optical behavior, best be described as micro-asteroids.