
An annular solar eclipse rises over the skyline of Toronto on Thursday, June 10, 2021.
Early risers captured spectacular footage of the eclipse, which played out around 6 a.m. over much of Canada.



The planet's red-dwarf star, though small, is quite bright in the infrared part of the light spectrum, or light beyond the red end of the spectrum that can't be seen with the naked eye. It is, however, ideal for investigation by Hubble and Webb. Also helpful: From our perspective on Earth, TOI-1231 b crosses the face of its star, which allowed its detection in the first place by NASA's Transiting Exoplanet Survey Satellite (TESS). And that crossing, called a "transit," takes nearly 3 ½ hours - plenty of time to capture and analyze starlight shining through the planet's atmosphere.
Fun facts: We might see evidence of clouds (perhaps even made of water) in this planet's atmosphere. And because this star-and-planet system is moving at a high velocity away from Earth, hydrogen atoms escaping from the planet's atmosphere might be readily detected. In other words, the planet could turn out to have a tail.
In general, such atoms are almost impossible to detect even when using space-based facilities; their presence is masked both by the outer wisps of Earth's atmosphere and by interstellar gas. But the TOI-1231 system is moving so quickly that escaping hydrogen atoms are shifted out of phase with the blocking material, where they could be detected by telescopes like Hubble.
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