The MIPS instrument team has documented the incidence, properties, and evolution of
planetary debris disks around nearby stars.
Not exact matches
These «
debris disks» are constantly fed by collisions among rocky bodies — the larger of which can survive and grow by continued accretion — because the tiny dust grains quickly fall onto the central star or get blown out of the
planetary system.
«Over the past decade, we have learned that remnants of
planetary systems around white dwarfs are ubiquitous, and over thirty
debris disks have been found by now.
This finding is counterintuitive because higher - mass stars flood their
planetary systems with energetic ultraviolet radiation that should destroy the carbon monoxide gas lingering in their
debris disks.
The astronomers narrowed their search to stars between five and ten million years old — old enough to host full - fledged
planetary systems and
debris disks — and used ALMA to examine the millimeter - wavelength «glow» from the carbon monoxide in the stars»
debris disks.
The discovery that the
debris disks around some larger stars retain carbon monoxide longer than their Sun - like counterparts may provide insights into the role this gas plays in the development of
planetary systems.
His calculations were the first to demonstrate that
debris disks around the nearby stars Vega and β Pictoris are newly - formed
planetary systems containing planets at least as large as Pluto and Mars.
Comparisons of the Kuiper belt with the
debris disks around other stars provide important indications about both the Kuiper belt itself and the
planetary environment around other stars.
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 particular, I will focus on planets on eccentric orbits, not only because typical exoplanetary systems have been found to contain these, but also because their interactions with
debris disks theoretically facilitates the transport of icy bodies within the habitable zone of
planetary systems.
There has been no shortage of proposed explanations that have been put forth in order to account for the unusual observations, from the more mundane ones which include the presence of cometary fragments and large
disk of
debris from
planetary collisions within the star system, to the more imaginative and fascinating ones which have invoked the presence of an extraterrestrial super-civilisation that is in the process of constructing gigantic megastructures around the star itself.
Kuchner has also led a citizen science project called
Disk Detective that allows users to scan WISE images for
debris disks that could provide clues to
planetary formation.
Once these
planetary bodies acquire enough mass, they dramatically reshape the structure of their natal
disk, fashioning rings and gaps as the planets sweep their orbits clear of
debris and shepherd dust and gas into tighter and more confined zones.