These results will aid in our understanding of
both planetary system architectures as well as the frequency of exoplanets throughout our galaxy.
These studies are aimed at understanding the physical mechanisms that govern star formation and how the evolution of the gaseous component of disks impacts the resulting
planetary system architectures.
Not exact matches
The discovery shows for the first time that hot Jupiters can appear at a very early stage in the formation of
planetary systems, and therefore have a major impact on their
architecture.
«This star is a not a good candidate for direct imaging of planets, but it demonstrates what LBTI is good for: We are figuring out the
architecture of
planetary systems in a way that has not been done before.»
The current SDSS - III project is focussing on three areas: dark energy and cosmological parameters; the structure, dynamics, and chemical evolution of the Milky Way; and the
architecture of
planetary systems.
More generally, these two results demonstrate that the longterm habitability (and astronomical observables) of a terrestrial planet can depend on the detailed
architecture of the
planetary system in which it resides.
But to fully understand the
architecture of distant
planetary systems, astronomers must map the entire distribution of planets around a star.
My research is in celestial mechanics, including the
architecture of extra-solar
planetary systems, debris disks around stars, the Kuiper belt and asteroid belt, orbital resonances, and meteoritic bombardment on planets in the solar
system.
In combinations with other methods of planet detection, direct imaging and spectroscopy will allow us to eventually: 1) fully map out the
architecture of typical
planetary systems and 2) study the atmospheric properties of exoplanets in depth.
The discovery of thousands of extrasolar planets by ground - and space - based observatories has shown that
planetary systems exhibit an astonishing diversity of
architectures.
Abstract: The
planetary system discovered around the young A-type HR8799 provides a unique laboratory to: a) test planet formation theories, b) probe the diversity of
system architectures at these separations, and c) perform comparative (exo) planetology.
We present and exploit new near - infrared images and integral - field spectra of the four gas giants surrounding HR8799 obtained with SPHERE, the new planet f... ▽ More The
planetary system discovered around the young A-type HR8799 provides a unique laboratory to: a) test planet formation theories, b) probe the diversity of
system architectures at these separations, and c) perform comparative (exo) planetology.
Finding these planets tells us about the
architecture of
planetary systems.
Before the discovery of the first exoplanets, astronomers thought they understood the
architecture of
planetary systems.
The team performed numerical simulations of
planetary migration that generated the Kepler - 223
system's current
architecture, which is similar to the migration suspected for planets of our outer solar
system, Jupiter, Saturn, Uranus, and Neptune.