Tootfinder

Evolution of the Accretion Rate of Young Intermediate-mass Stars - Implications for Disk Evolution and Planet Formation: #planets to form after all: https://news.clemson.edu/late-growth-spurt-of-young-stars-allows-giant-planets-to-form-after-all/ - the finding sheds light on the origins of giant planets.

Observation of nonaxisymmetric standard magnetorotational instability induced by a free-shear layer: #Planets Might Form When Dust “Wobbles” in Just the Right Way: https://eos.org/articles/planets-might-form-when-dust-wobbles-in-just-the-right-way - a liquid metal experiment has shown how magnetic rotational instability might allow dust to pool together in disks around young stars to form new worlds.

Determining the impact of post-main-sequence stellar evolution on the transiting giant planet population: #planets: https://ras.ac.uk/news-and-press/research-highlights/ageing-stars-may-be-destroying-their-closest-planets

🪱 Bioinspired Drilling for Extraterrestrial Applications
#space #planets