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For centuries, Betelgeuse, the iconic red supergiant in Orion, has fascinated astronomers with its changing brightness.
Why does its light vary over a ~6-year cycle?
Thanks to the Gemini North telescope, we now have an answer: Betelgeuse has a companion star!
🔭 🧪 #stellarastro #galactic
For centuries, Betelgeuse, the iconic red supergiant in Orion, has fascinated astronomers with its changing brightness.
Why does its light vary over a ~6-year cycle?
Thanks to the Gemini North telescope, we now have an answer: Betelgeuse has a companion star!
🔭 🧪 #stellarastro #galactic
These tremendous explosions are blasting away the planet’s wispy atmosphere, causing it to shrink every year.
Find out more 👉 www.esa.int/Science_Expl...
🔭 🧪
These tremendous explosions are blasting away the planet’s wispy atmosphere, causing it to shrink every year.
Find out more 👉 www.esa.int/Science_Expl...
🔭 🧪
Two NEW papers on HIP 67522, a young star with two close-in giants and clear signs of magnetic star–planet interaction. The inner planet triggers flares on its host star, exposing itself to a 6 times higher flaring rate than without interaction. #astronomy #exoplanets
Two NEW papers on HIP 67522, a young star with two close-in giants and clear signs of magnetic star–planet interaction. The inner planet triggers flares on its host star, exposing itself to a 6 times higher flaring rate than without interaction. #astronomy #exoplanets
www.newscientist.com/article/2485...
www.newscientist.com/article/2485...