Planets go “weeee!”
When planets form, where should they move? Towards their host star? In the other direction? The authors of today’s paper show that this is not obvious!
When planets form, where should they move? Towards their host star? In the other direction? The authors of today’s paper show that this is not obvious!
Some things are really hard to observe, but we still can study them using computer simulations! Today’s paper will show you how people study planets-driven spiral arms!
It’s nice to have the conclusion of a paper in its title – Super-Jupiters migrate outward. Today, let’s investigate what exactly this means!
The fractal dimension as a new way to explore the mysterious link between turbulence and star formation.
The spectacular disk around HD142527 is a carnival of spirals and gaps: is it all caused by a single massive companion?
While a planet is forming, its passage through the protoplanetary disk can prevent pebbles from migrating inwards and accreting onto the planet.