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Since the launch of Kepler and Hubble more than a decade ago, we have come along way in the quest to find a potentially habitable exoplanet. To date, wehave already discovered more than 4000 exoplanets most of which are notsuitable for sustaining life. Of all those that can potentially sustain life, Alarge number has been found rotating synchronously around their parent star,mostly Red dwarf star. Due to their synchronous rotation, these planets receivevery uneven stellar heating. Synchronous rotation of these planets causes oneside of the planet to permanently face the parent star while the other sideremains dark. This results in an extreme climatic condition that is notfeasible for sustaining life. Although these theories about exoplanets are wellknown, a systemic study of habitability of polar regions within an exoplanetusing different climate models has not been done yet. Here I review the currentliterature on tidal locking and its impact on habitability and introduce theconcept of habitability in the poles of these exoplanets. I focus on myunderstanding of the climatic condition in the polar region of the earth andbased on that I present the concept of habitability in the poles of theseexoplanets.

Habitability of polar regions in tidally locked extrasolar planet near the M-Dwarf stars