Debris disks are tenuous, dust-dominated disks commonly observed around stars over a
wide range of ages. Those around main sequence stars are analogous to the Solar System's …

This review presents our understanding of cometary dust at the end of 2017. For decades,
insight about the dust ejected by nuclei of comets had stemmed from remote observations …

Before Rosetta, the space missions Giotto and Stardust shaped our view on cometary dust,
supported by plentiful data from Earth based observations and interplanetary dust particles …

In this work, we present results that simultaneously constrain the dust size distribution, dust-
to-gas ratio, fraction of dust re-deposition, and total mass production rates for comet …

Context. The scattering properties of the dust originating from debris discs are still poorly
known. The analysis of scattered light is however a powerful remote-sensing tool to …

Here we describe the novel, multi-point Comet Interceptor mission. It is dedicated to the
exploration of a little-processed long-period comet, possibly entering the inner Solar System …

ABSTRACT Comet 67P/Churyumov–Gerasimenko (67P) become observable for the first
time in 2021 since the Rosetta rendezvous in 2014–2016. Here, we present pre-perihelion …

We present an update to the Granada–Amsterdam Light Scattering Database
(https://scattering. iaa. es/), which includes experimental data from both the IAA-Cosmic Dust …

Exocomets are small bodies releasing gas and dust which orbit stars other than the Sun.
Their existence was first inferred from the detection of variable absorption features in stellar …

Context. The process of gas-driven ejection of refractory materials from cometary surfaces
continues to pose a challenging question in cometary science. The activity modeling of …