That is why the timing and
the scale of planet formation — fast or slow, big or small — is a critical issue.
Not exact matches
Canup is one
of the leading scientists using large -
scale hydrodynamical simulations to model
planet -
scale collisions, including the prevailing Earth - Moon
formation model.
The research activity
of our group «Interstellar Medium: star and
planet formation» is focused in the early stages
of the star and
planet formation process, with special emphasis on the role
of magnetic field at different
scales.
Observing in wavelengths ranging from the ultraviolet to the mid-infrared, this unique instrument will allow astronomers to address fundamental questions in astronomy ranging from understanding star and
planet formation to unraveling the history
of galaxies and the development
of large -
scale structure in the universe.