In doing so, we will test
our models for planet formation and evaluate the probability that habitable planets are present around stars of various types.
Not exact matches
We were very surprised based on the fact that previous
models people used
for planet formation suggested a much higher critical shock pressure,» says Richard Kraus, now a scientist at Lawrence Livermore National Laboratory and lead author on the paper published in March in Nature Geoscience.
Scott Kenyon, a theorist at the Harvard — Smithsonian Center
for Astrophysics who builds numerical
models of
planet formation, echoes that assessment.
One of the reigning theories of planetary
formation, the Grand Tack
model, blames Jupiter
for the Red
Planet's paltry size.
If confirmed by further research, the new study would challenge a theoretical
model for atmosphere
formation in which Earth began with two reservoirs of solar gas captured during the
planet's
formation and youth — one surrounding the
planet, the other buried beneath the surface.
«Jupiter is the oldest
planet of the solar system, and its solid core formed well before the solar nebula gas dissipated, consistent with the core accretion
model for giant
planet formation.»
At this school, we will review physical
models for cloud
formation in Solar System
planets, exoplanet observations, and laboratory studies.
We are excited to connect and compare
planet formation models and their predictions to exoplanet populations; we are looking
for a postdoctoral researcher with expertise in
planet formation, exoplanet population studies, and / or statistical assessment of exoplanet surveys,
So, if there is a
planet in the gap and there is no dust larger than a grain of sand farther out, we have provided a challenge
for traditional
planet formation models.»
Numerous teams in the world are developing
models and simulations,
for example to reproduce the physical processes driving the
formation of
planets in circumstellar discs, the evolution of their orbits through migration or mutual interaction, or the properties of their atmospheres.
The well - determined planetary properties and unusually large mass also make this
planet an important benchmark
for theoretical
models of super-Jupiter
formation.
Assuming the rocky world has the smallest physical size allowed
for its mass (94 % Earth's diameter), according to planetary
formation models this would consist of a metal core, making up
for 65 % of the mass of the entire
planet.
Modeling long - term climate change
for the entire
planet, however, was held back by lack of computer power, ignorance of key processes such as cloud
formation, inability to calculate the crucial ocean circulation, and insufficient data on the world's actual climate.