Stellar Flares from the First TESS Data Release: Exploring a New Sample of M Dwarfs

Maximilian N. Günther, Zhuchang Zhan, Sara Seager, Sara Seager, Paul B. Rimmer, Paul B. Rimmer, Paul B. Rimmer, Sukrit Ranjan, Keivan G. Stassun, Ryan J. Oelkers, Tansu Daylan, Elisabeth Newton, Elisabeth Newton, Martti H. Kristiansen, Martti H. Kristiansen, Katalin Olah, Edward Gillen, Saul Rappaport, George R. Ricker, Roland K. VanderspekDavid W. Latham, Joshua N. Winn, Jon M. Jenkins, Ana Glidden, Ana Glidden, Michael Fausnaugh, Alan M. Levine, Jason A. Dittmann, Samuel N. Quinn, Akshata Krishnamurthy, Eric B. Ting

Research output: Contribution to journalArticle

10 Scopus citations

Abstract

We perform a study of stellar flares for the 24,809 stars observed with 2 minute cadence during the first two months of the TESS mission. Flares may erode exoplanets' atmospheres and impact their habitability, but might also trigger the genesis of life around small stars. TESS provides a new sample of bright dwarf stars in our galactic neighborhood, collecting data for thousands of M dwarfs that might host habitable exoplanets. Here, we use an automated search for flares accompanied by visual inspection. Then, our public allesfitter code robustly selects the appropriate model for potentially complex flares via Bayesian evidence. We identify 1228 flaring stars, 673 of which are M dwarfs. Among 8695 flares in total, the largest superflare increased the stellar brightness by a factor of 16.1. Bolometric flare energies range from 1031.0 to 1036.9 erg, with a median of 1033.1 erg. Furthermore, we study the flare rate and energy as a function of stellar type and rotation period. We solidify past findings that fast rotating M dwarfs are the most likely to flare and that their flare amplitude is independent of the rotation period. Finally, we link our results to criteria for prebiotic chemistry, atmospheric loss through coronal mass ejections, and ozone sterilization. Four of our flaring M dwarfs host exoplanet candidates alerted on by TESS, for which we discuss how these effects can impact life. With upcoming TESS data releases, our flare analysis can be expanded to almost all bright small stars, aiding in defining criteria for exoplanet habitability.

Original languageEnglish (US)
Article number60
JournalAstronomical Journal
Volume159
Issue number2
DOIs
StatePublished - Feb 2020

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Günther, M. N., Zhan, Z., Seager, S., Seager, S., Rimmer, P. B., Rimmer, P. B., Rimmer, P. B., Ranjan, S., Stassun, K. G., Oelkers, R. J., Daylan, T., Newton, E., Newton, E., Kristiansen, M. H., Kristiansen, M. H., Olah, K., Gillen, E., Rappaport, S., Ricker, G. R., ... Ting, E. B. (2020). Stellar Flares from the First TESS Data Release: Exploring a New Sample of M Dwarfs. Astronomical Journal, 159(2), [60]. https://doi.org/10.3847/1538-3881/ab5d3a