Skip to main content
Log in

Activity of M-dwarf L 98-59 and Atmospheric Escape of its Exoplanets

  • Published:
Astrophysical Bulletin Aims and scope Submit manuscript

Abstract

A study of the activity of a bright M-dwarf L 98-59, located at a distance of 10.6 pc from Earth is reported. The star has a multiplanetary system, where one of the planets, L 98-59 b, is a rocky planet with a mass not exceeding the mass of Venus. It was found that the level of chromospheric activity of L 98-59 does not exceed the average value characteristic of other cold dwarfs with similar color index values \((B-V)\). This level is below solar, the mean \(\log R{{}^{\prime}}_{\textrm{HK}}\) parameter for L 98-59 is equal to \(-\)5.297 dex. The data about the parent star and its activity was used to estimate the magnitude of the atmospheric escape of five planets (including the planet candidate 05). To calculate the loss of matter from the planetary atmospheres (without a detailed modeling of the processes in the ‘‘star–planet’’ system), we applied an approximation formula corresponding to the energy-limited atmospheric loss model. Estimates of the XUV photon flux—extreme ultraviolet (EUV) and X-ray photons for the medium and high activity levels, as well as the estimates of the tidal parameter \(K_{\textrm{tide}}(\xi)\) were found. Variations of the \(\dot{M}\) parameter have been specified for five planets of the L 98-59 system, taking into account the possible activity level variations of the star. The \(\dot{M}\) parameter variations for planets c–e range from \(7.6\times 10^{6}\) g s\({}^{-1}\) to \(3.8\times 10^{7}\) g s\({}^{-1}\) (average activity level) and \(1.2\)\(5.7\times 10^{7}\) g s\({}^{-1}\) (high activity level). For the planet L 98-59 b, the an analogue of Venus, we got the following estimates: \(1.3\times 10^{7}\) and \(2.0\times 10^{7}\) g s\({}^{-1}\) (for the intermediate and high activity levels, respectively). It can be assumed that the relatively modest outflow of matter from their atmospheres \(\dot{M}\), despite the proximity of the planets to their star, is due to a small flux of XUV photons from the star due to the low level of its activity.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1
Fig. 2

Notes

  1. https://exoplanetarchive.ipac.caltech.edu/

REFERENCES

  1. S. Boro Saikia, C. J. Marvin, S. V. Jeffers, et al., Astron. and Astrophys. 616, id. A108 (2018).

  2. R. Cloutier, N. Astudillo-Defru, X. Bonfils, et al., Astron. and Astrophys. 629, id. A111 (2019).

  3. O. D. S. Demangeon, M. R. Zapatero Osorio, Y. Alibert, et al., Astron. and Astrophys. 653, id. A41 (2021).

  4. N. V. Erkaev, Y. N. Kulikov, H. Lammer, et al., Astron. and Astrophys. 472 (1), 329 (2007).

    Article  ADS  CAS  Google Scholar 

  5. E. S. Kalinicheva, V. I. Shematovich, and I. S. Savanov, Astronomy Reports 66 (12), 1318 (2022).

    Article  ADS  Google Scholar 

  6. E. M. R. Kempton, J. L. Bean, D. R. Louie, et al., Publ. Astron. Soc. Pacific 130 (993), 114401 (2018).

  7. T. T. Koskinen, P. Lavvas, C. Huang, et al., Astrophys. J. 929 (1), id. 52 (2022).

  8. V. B. Kostov, J. E. Schlieder, T. Barclay, et al., Astron. J. 158 (1), article id. 32 (2019).

  9. K. Ment, D. Charbonneau, J. Irwin, et al., arXiv e-prints astro/ph:2304.01920 (2023).

  10. I. S. Savanov and V. I. Shematovich, Astrophysical Bulletin 76 (4), 450 (2021).

    Article  ADS  Google Scholar 

  11. A. G. Sreejith, L. Fossati, A. Youngblood, et al., Astron. and Astrophys. 644, id. A67 (2020).

  12. L. M. Weiss, G. W. Marcy, E. A. Petigura, et al., 155 (1), article id. 48 (2018).

Download references

ACKNOWLEDGMENTS

The present study has made use of the data from the SIMBAD astronomical database and the archive of the TESS space mission.

Funding

The work was carried out within the framework of the Study of Stars with Exoplanets project under a grant from the Government of the Russian Federation for the scientific research conducted under the guidance of the leading scientists (agreements No. 075-15-2019-1875, No. 075-15-2022-1109).

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to I. S. Savanov.

Ethics declarations

The author of this work declares that he has no conflicts of interest.

Additional information

Publisher’s Note.

Pleiades Publishing remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Savanov, I.S. Activity of M-dwarf L 98-59 and Atmospheric Escape of its Exoplanets. Astrophys. Bull. 78, 588–593 (2023). https://doi.org/10.1134/S1990341323700165

Download citation

  • Received:

  • Revised:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1134/S1990341323700165

Keywords:

Navigation