Cosmic phylogeny: reconstructing the chemical history of the solar neighbourhood with an evolutionary tree

TL;DR

This study applies phylogenetic methods from biology to stellar chemical data, reconstructing the evolutionary history of stars in the solar neighborhood and revealing insights into their populations and formation processes.

Contribution

It introduces a novel application of phylogenetic clustering to stellar chemical data, providing a new perspective on stellar populations and their evolutionary relationships.

Findings

Identified three main stellar populations: thin disk, thick disk, and an intermediate group.

Quantified the chemical enrichment rates for different stellar populations.

Estimated the impact of dynamical processes like radial migration on chemical distributions.

Abstract

Using 17 chemical elements as a proxy for stellar DNA, we present a full phylogenetic study of stars in the solar neighbourhood. This entails applying a clustering technique that is widely used in molecular biology to construct an evolutionary tree from which three branches emerge. These are interpreted as stellar populations which separate in age and kinematics and can be thus attributed to the thin disk, the thick disk, and an intermediate population of probable distinct origin. We further find six lone stars of intermediate age that could not be assigned to any population with enough statistical significance. Combining the ages of the stars with their position on the tree, we are able to quantify the mean rate of chemical enrichment of each of the populations, and thus show in a purely empirical way that the star formation rate in the thick disk is much higher than in the thin disk. We are also able to estimate the relative contribution of dynamical processes such as radial migration and disk heating to the distribution of chemical elements in the solar neighbourhood. Our method offers an alternative approach to chemical tagging methods with the advantage of visualising the behaviour of chemical elements in evolutionary trees. This offers a new way to search for `common ancestors' that can reveal the origin of solar neighbourhood stars.