Hydrogen and deuterium survey of minor bodies: transformative science with a purpose-built CubeSat

Introduction

The advent of standardized small satellites called CubeSats has made astronomical research from space more accessible than ever before. The proposed ERC project directly derives from the vast research possibilities offered by this platform, and aims at the construction of a miniature UV space telescope designed specifically to detect hydrogen and deuterium around comets and asteroids through the ultra-luminous Lyman alpha transition.

Objectives

Thanks to the unparalleled sensitivity to these atoms, the envisioned satellite will provide definite answers to some of the most profound problems of the near Universe.

Investigation of Interstellar Objects

1. It will enable ultra-sensitive investigation of future interstellar objects passing through the Solar System in search of their hydrogen clouds.
2. This has direct implications for our understanding of orbital anomalies in the absence of detectable dust, such as seen in ‘Oumuamua, as well as their physical nature in general.

Study of Main-Belt Comets

The satellite will allow for deep investigation of hydrogen content around main-belt comets, probing water-ice outgassing from these bodies with a better sensitivity than the best present-day limits.

• The high level of sensitivity will be routinely achieved for all known objects of this class, including new main-belt comets discovered by LSST.
• This will transform our knowledge of the ice reservoir in the outer Main Belt.

D/H Ratio Measurements

Finally, the satellite will provide homogeneous, model-independent, and self-consistent measurements of the D/H ratio for dozens of comets from different dynamical classes down to 12 mag of total brightness.

• This represents a factor-of-hundred improvement in sensitivity over the state-of-the-art methods and a major leap in measurement reliability.
• The D/H measurements will ultimately resolve the puzzle of the cometary origin of water on Earth and unveil the link between present-day cometary reservoirs and their original place of formation in the solar nebula.