Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Resolved Stellar Populations Studies in M31 and its Satellites

TL;DR

A 30-meter class telescope in the Northern Hemisphere would revolutionize our understanding of M31 and its satellites by enabling detailed resolved stellar population studies, similar to those done for the Milky Way, thus addressing key questions in galaxy formation.

Contribution

Proposes the scientific potential and necessity of a 30-meter class telescope in the Northern Hemisphere for detailed studies of M31 and its satellites, filling a gap in current observational capabilities.

Findings

Enables detailed resolved stellar population studies of M31.

Facilitates comparison between the Milky Way and M31 systems.

Addresses fundamental questions in galaxy evolution.

Abstract

A 30 m class optical/near-IR telescope in the Northern Hemisphere, equipped for diffraction-limited imaging and high-resolution, multi-object spectroscopy of faint stars, would enable a transformational investigation of the formation and evolution of M31 and its satellite system - on par with what Gaia, the HST, and other major photometric and spectroscopic facilities have achieved for the Milky Way (MW) and its satellites. The unprecedented detail obtained for our home system has reshaped our understanding of the assembly of the MW disk, halo, and bulge, and that of its satellites, which now serve as a benchmark for galaxy formation and evolution models. Extending this level of insight to the M31 system - that of the nearest massive spiral and the only one for which such a comprehensive, resolved stellar population study is feasible - will allow us to address a fundamental question: how representative is the MW and its satellite system within the broader context of galaxy evolution?