The inner edge of the habitable zone for synchronously rotating planets around low-mass stars using general circulation models
R kumar Kopparapu, ET Wolf… - The Astrophysical …, 2016 - iopscience.iop.org
Terrestrial planets at the inner edge of the habitable zone (HZ) of late-K and M-dwarf stars
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
The Inner Edge of the Habitable Zone for Synchronously Rotating Planets around Low-mass Stars Using General Circulation Models
ET Wolf, J Haqq-Misra, J Yang… - The Astrophysical …, 2016 - ui.adsabs.harvard.edu
Terrestrial planets at the inner edge of the habitable zone (HZ) of late-K and M-dwarf stars
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
The Inner Edge of the Habitable Zone for Synchronously Rotating Planets Around Low-Mass Stars Using General Circulation Models
RK Kopparapu, ET Wolf, J Haqq-Misra, J Yang… - Astrophysical …, 2016 - ntrs.nasa.gov
Terrestrial planets at the inner edge of the habitable zone (HZ) of late-K and M-dwarf stars
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
The inner edge of the habitable zone for synchronously rotating planets around low-mass stars using general circulation models
ET Wolf, J Haqq-Misra, J Yang, JF Kasting… - arXiv preprint arXiv …, 2016 - arxiv.org
Terrestrial planets at the inner edge of the habitable zone of late-K and M-dwarf stars are
expected to be in synchronous rotation, as a consequence of strong tidal interactions with …
expected to be in synchronous rotation, as a consequence of strong tidal interactions with …
[PDF][PDF] THE INNER EDGE OF THE HABITABLE ZONE FOR SYNCHRONOUSLY ROTATING PLANETS AROUND LOW-MASS STARS USING GENERAL …
R kumar Kopparapu, ET Wolf, J Haqq-Misra, J Yang… - Victoria, 2016 - scholar.archive.org
Terrestrial planets at the inner edge of the habitable zone (HZ) of late-K and M-dwarf stars
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
THE INNER EDGE OF THE HABITABLE ZONE FOR SYNCHRONOUSLY ROTATING PLANETS AROUND LOW-MASS STARS USING GENERAL CIRCULATION …
R kumar Kopparapu, ET Wolf, J Haqq-Misra… - The Astrophysical …, 2016 - cir.nii.ac.jp
抄録< jats: title> ABSTRACT</jats: title>< jats: p> Terrestrial planets at the inner edge of the
habitable zone (HZ) of late-K and M-dwarf stars are expected to be in synchronous rotation …
habitable zone (HZ) of late-K and M-dwarf stars are expected to be in synchronous rotation …
THE INNER EDGE of the HABITABLE ZONE for SYNCHRONOUSLY ROTATING PLANETS AROUND LOW-MASS STARS USING GENERAL CIRCULATION …
RK Kopparapu, ET Wolf, J Haqq-Misra, J Yang… - Astrophysical …, 2016 - pure.psu.edu
Terrestrial planets at the inner edge of the habitable zone (HZ) of late-K and M-dwarf stars
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
The Inner Edge of the Habitable Zone for Synchronously Rotating Planets around Low-mass Stars Using General Circulation Models
ET Wolf, J Haqq-Misra, J Yang… - The Astrophysical …, 2016 - ui.adsabs.harvard.edu
Terrestrial planets at the inner edge of the habitable zone (HZ) of late-K and M-dwarf stars
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …
are expected to be in synchronous rotation, as a consequence of strong tidal interactions …