How has the solar wind evolved to become what it is today?
A. A. Vidotto (Leiden Observatory)

TL;DR
This paper reviews the long-term evolution of the solar wind, its properties, and implications for Earth, suggesting that studying exoplanetary systems can enhance understanding of solar wind evolution.
Contribution
It provides a concise overview of solar wind evolution and proposes exploring exoplanetary systems to advance knowledge in this area.
Findings
Solar wind mass-loss rate has evolved over time.
Evolution of solar wind properties affects Earth's environment.
Studying exoplanets offers new insights into solar wind history.
Abstract
In this contribution, I briefly review the long-term evolution of the solar wind (its mass-loss rate), including the evolution of observed properties that are intimately linked to the solar wind (rotation, magnetism and activity). I also briefly discuss implications of the evolution of the solar wind on the evolving Earth. I argue that studying exoplanetary systems could open up new avenues for progress to be made in our understanding of the evolution of the solar wind.
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Taxonomy
TopicsAstro and Planetary Science · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies
