SIMBAD references

2019MNRAS.485.3999M - Mon. Not. R. Astron. Soc., 485, 3999-4012 (2019/May-3)

Planetary magnetism as a parameter in exoplanet habitability.

McINTYRE S.R.N., LINEWEAVER C.H. and IRELAND M.J.

Abstract (from CDS):

Evidence from the Solar system suggests that, unlike Venus and Mars, the presence of a strong magnetic dipole moment on Earth has helped maintain liquid water on its surface. Therefore, planetary magnetism could have a significant effect on the long-term maintenance of atmosphere and liquid water on rocky exoplanets. We use Olson & Christensen's (2006) model to estimate magnetic dipole moments of rocky exoplanets with radii Rp <= 1.23 R. Even when modelling maximum magnetic dipole moments, only Kepler-186 f has a magnetic dipole moment larger than the Earth's, while approximately half of rocky exoplanets detected in the circumstellar habitable zone have a negligible magnetic dipole moment. This suggests that planetary magnetism is an important factor when prioritizing observations of potentially habitable planets.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): planets and satellites: general - planets and satellites: magnetic fields - planets and satellites: terrestrial planets

VizieR on-line data: <Available at CDS (J/MNRAS/485/3999): tablea1.dat>

Status at CDS : Tables of objects will be appraised for possible ingestion in SIMBAD.

Simbad objects: 474

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2019MNRAS.485.3999M and select 'bookmark this link' or equivalent in the popup menu


2022.12.08-11:54:10

© Université de Strasbourg/CNRS

    • Contact