Habitable Worlds Observatory: The Nature of the Astrophysical r-process

Abstract

We present the science case for characterizing the origin of the heaviest elements on the periodic table, with a focus on those produced by the rapid neutron-capture process (r-process), using the Habitable Worlds Observatory (HWO). High-resolution ultraviolet (UV) spectroscopy can increase the number of r-process elements detectable in cool stars by more than 50% relative to optical and infrared spectra. These elements are key to characterizing the physical conditions that govern the r-process and identify the nature, sites, and environments where r-process events occurred. HWO has the potential to greatly expand the sample of stars where rarely studied heavy elements can be detected beyond the Solar neighborhood to the Galactic halo, globular clusters, and dwarf galaxies.