In Project 2.3 A we will probe poorly
constrained planet formation and disk transport processes, i.e., solid migration and planetesimal formation.
Not exact matches
I will discuss how these findings can be used to
constrain models of
planet formation and how they may be used to optimize
planet searches with future direct imaging missions, such as HabEx and LUVOIR.
«What's interesting is that just this one object flying by so quickly can help us
constrain some of our
planet formation models.»
We present a study of the planetary systems WASP - 45 and WASP - 46, both composed of a main - sequence star and a close - in ho... ▽ More Accurate measurements of the physical characteristics of a large number of exoplanets are useful to strongly
constrain theoretical models of
planet formation and evolution, which lead to the large variety of exoplanets and planetary - system configurations that have been observed.