Solar-like stars observed by Kepler: an incredible adventure

TL;DR

The paper discusses the groundbreaking potential of Kepler's high-quality light curves for ensemble asteroseismology of solar-like stars, enabling new insights into stellar properties across diverse types.

Contribution

It introduces the first large-scale asteroseismic analysis of solar-like stars using Kepler data, expanding the scope of stellar studies.

Findings

Successful ensemble asteroseismology with Kepler data

Identification of stellar characteristics across diverse stars

Enhanced understanding of solar-like star properties

Abstract

The NASA Kepler mission -in flight since March 2009- is producing an enormous number of high-quality continuous light curves. Now, and for the first time ever, we are able to do ensemble asteroseismology, i.e., to do an asteroseismic analysis with a statistically significant sub-sample of solar-like stars covering a wide range of stellar characteristics. In the present work, I highlight some of the most recent studies carried out using these data.