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Eyeball Earths

Posted

April 13, 2017

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Earth-sized planets found in the habitable-zones of low-mass stars are likely to become tidally locked to the star, with one side baked in perpetual sunlight and other trapped in an eternal night. These so-called "Eyeball Earths" turn out to be extremely common and some famous examples include Proxima b and the planets around TRAPPIST-1. Here, we explain why this tidal locking happens and what it means for the potential habitability of these alien worlds.

::More about this Video::

► "Discovery of a Planet around our Nearest StarProxima b" Cool Worlds video by Dr Guillem Anglada

► "Proxima bTransits, Habitability & How to Get There!" Cool Worlds video by Prof Kipping

► Gillon et al. (2017), "Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST1"

► Video of zonal winds on a tidally locked planet taken from Merlis & Schneider (2010), "Atmospheric dynamics of Earthlike tidally locked aquaplanets"

► Leconte et al. (2015), "Asynchronous rotation of Earthmass planets in the habitable zone of lowermass stars"

► Cool Worlds Lab website

► Columbia University Department of Astronomy

► Outro music by Daft Punk "Harder, Better, Stronger, Faster"and

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Guests & Subjects Covered

Eyeball EarthsTRAPPIST- HereNearest Star ProximaDr Guillem AngladaTransits HabitabilityGet There Cool WorldsProf KippingCool Worlds Lab

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