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Showing posts with the label Tidally Locked Planet

The Thermal Radiation and Airless Basalt Crust of Exoplanet TRAPPIST-1b

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Located approximately 39.5 light-years from Earth in the constellation Aquarius, TRAPPIST-1b represents one of the most rigorously measured terrestrial exoplanets discovered to date. As the innermost world orbiting the ultra-cool M-dwarf star TRAPPIST-1 , this rocky world exists in a state of extreme gravitational lock . Completing a full revolution around its parent star in a mere 1.51 Earth days, the planet’s rotational period is perfectly synchronized with its orbital period. This tidal configuration forces one hemisphere into eternal stellar bombardment while the opposite hemisphere faces permanent, frigid shadow. With a radius roughly 1.11 times that of Earth and a mass measured at 1.37 Earth masses, TRAPPIST-1b possesses a bulk density of approximately 5.4 grams per cubic centimeter. This density profile is strikingly similar to Earth’s uncompressed density, pointing toward a rocky composition dominated by iron, magnesium, and silicate minerals. However, its proximity to its h...

The Extreme Day-Night Thermal Divide and Winds of Exoplanet WASP-43b

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Located approximately 280 light-years from Earth in the constellation Sextans, WASP-43b represents one of the most extreme thermodynamic laboratories known to observational astronomy. Discovered in 2011 by the Wide Angle Search for Planets (WASP) survey via the transit method, this short-period gas giant orbits an active K-type main-sequence star, WASP-43, at an exceptionally tight semi-major axis of approximately 0.015 astronomical units (roughly 2.2 million kilometers). Because of its ultra-short orbital distance, the planet completes a full revolution in just 19.5 hours. At this proximity, gravitational tidal forces have irrevocably locked the planet’s rotational period to its orbital period, forcing WASP-43b into a permanent synchronous lock where one hemisphere faces perpetual stellar radiation while the other is consigned to endless shadow. With a mass approximately 2.05 times that of Jupiter and a radius nearly identical to Jupiter’s (1.03 Jovian radii), WASP-43b posses...

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