How Hospitable Are Space Weather Affected Habitable Zones? The Role of Ion Escape

By V. Airapetian, A. Glocer, G. Khazanov, R. Loyd, K. France, J. Sojka, W. Danchi, M. Liemohn. 2017

145 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/4ecbe1e28306199bf789ab8696d30cb9823cb693

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

Citations in the corpus

Habitable Moist Atmospheres on Terrestrial Planets near the Inner Edge of the Habitable Zone around M Dwarfs (2017, background): “The validity of this assumption can be debated, particularly for planets in the HZ of M dwarf stars, due to their high pre-main-sequence luminosity (Ramirez & Kaltengger 2014; Luger & Barnes 2015; Tian & Ida 2015), or atmospheric erosion due to high X-ray and UV fluxes (Airapetian et al. 2017).”
Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets (2017, background): “…may potentially all be airless today, as a result of the star extreme X/UV irradiation (Wheatley et al. 2017; Bourrier et al. 2017) and stellar wind through history that could have blown away their atmosphere (Airapetian et al. 2017; Dong et al. 2017b; Garcia-Sage et al. 2017; Dong et al. 2017a).”
Exoplanet Biosignatures: A Review of Remotely Detectable Signs of Life (2017, background): “ility. These include the deleterious impacts of the ultraviolet (UV) and particle (ﬂare) activity of these stars (Segura et al., 2003; Lammer et al., 2007; Davenport et al., 2016; Ribas et al., 2016; Airapetian et al., 2017), their premain sequence evolution (Ramirez and Kaltenegger, 2014; Luger and”
The Detectability and Characterization of the TRAPPIST-1 Exoplanet Atmospheres with JWST (2019, background): “Simulations suggest that the TRAPPIST-1 planets could have had their atmospheres completely stripped (e.g., Airapetian et al. 2017; Roettenbacher & Kane 2017; Dong et al. 2018), although some models of M dwarf planets suggest that atmospheric loss rates may be less than the replenishment rate via…”