Bridging stellar evolution and planet formation: from birth, to survivors of the fittest, to the second generation of planets

TL;DR

This paper discusses the interconnected processes of star and planet formation, evolution, and death, emphasizing the importance of dust physics in various stellar environments and proposing future observational and imaging advancements to better understand these phenomena.

Contribution

It bridges stellar evolution and planet formation fields by highlighting the role of dust dynamics and macrostructure in diverse dusty environments throughout stellar lifecycles.

Findings

Dust physics influences star and planet evolution stages.

Future telescopes will enable detailed study of exoplanets and dusty environments.

Imaging capabilities are crucial for testing theories of dust and planet interactions.

Abstract

Stars and planets form, live, and evolve in unison. Throughout the life of a star, dusty circumstellar discs and stellar outflows influence the further evolution of both the star(s) and their orbiting planet(s). Planet-forming discs, winds of red giant branch (RGB) or asymptotic giant branch (AGB) stars, and post-RGB/post-AGB discs are examples of such host environments where dust physics plays a key role. The physical processes that occur during each of these stages establishes how the Solar System as well as exoplanetary systems were formed, are evolving, and will eventually die. This White Paper aims to bridge the fields of stellar evolution and planet formation by peering into the dust kinematics and macrostructure formation, and its effect on planet-host interaction, in dusty environments from stellar birth to death. Near-future advancements in the 2030s will enable the detection, orbital monitoring and atmospheric/mineralogical characterisation of close-in (proto)planets across diverse stages of stellar evolution. To take full advantage of these developments by the 2040s, we should develop the capabilities required to image the varied dusty environments in which planets are entrained over their lifetime. This will enable extensive testing of current theoretical understandings - from the micro-scales of dust assembly to the deeply interlinked macro-scales of planet-host interactions - across diverse settings often too small, distant, and faint to be resolved in the next decade, simultaneously providing valuable constraints on the two-way interplay of dusty host environments and planetary formation/evolution.