# Unexpectedly strong effect of supergranulation on the detectability of Earth twins orbiting Sun-like stars with radial velocities

## TL;DR

Supergranulation significantly impacts the radial velocity signals of Sun-like stars, making the detection of Earth-like planets in habitable zones more challenging than previously thought.

## Contribution

This study quantifies the effect of supergranulation on exoplanet detectability and highlights its importance compared to other stellar surface flows.

## Key findings

- Detection rate is below 100% under realistic supergranulation levels.
- Supergranulation can obscure signals of Earth-mass planets.
- Current detection capabilities are limited by stellar surface flows.

## Abstract

Magnetic activity and surface flows at different scales pertub radial velocity measurements. This affects the detectability of low-mass exoplanets. In these flows, the effect of supergranulation is not as well characterized as the other flows, and we wish to estimate its effect on the detection of Earth-like planets in the habitable zone of Sun-like stars. We produced time series of radial velocities due to oscillations, granulation, and supergranulation, and estimated the detection limit for a G2 star and a period of 300 days. We also studied in detail the behavior of the power when the signal of a 1 Mearth planet was superposed on the signal from the stellar flows. We find that the detection rate does not reach 100% except for the supergranulation level we assume, which is still optimistic, and for an excellent sampling. We conclude that with current knowledge, it is a very challenging task to find Earth twins around Sun-like stars with our current capabilities.