Debris Disks and the Formation of Planets: a Symposium in Memory of Fred Gillett
نویسنده
چکیده
An overview regarding planetary debris disks: First, more history to complement Low and Aumann’s summary appearing elsewhere in this volume. Then, commentary on the nature of debris disks and what we’ve learned from them: properties of the original “Fabulous Four” archetypes, results from surveys showing that a large fraction of ordinary stars may be hosts for debris disks, and relatively detailed discussion of β Pictoris, the most prominent disk. Finally, discussion of the connection between debris disks, our solar system’s Kuiper Belt, and the zodiacal dust cloud. Open questions about these objects will be highlighted which can lead on to the remainder of the proceedings.
منابع مشابه
On the Relationship Between Debris Disks and Planets
Dust in debris disks is generated by collisions among planetesimals. The existence of these planetesimals is a consequence of the planet formation process, but the relationship between debris disks and planets has not been clearly established. Here we analyze Spitzer/MIPS 24 and 70μm data for 150 planet-bearing stars, and compare the incidence of debris disks around these stars with a sample of...
متن کاملA Spitzer Study of Debris Disks in the Young Nearby Cluster Ngc 2232: Icy Planets Are Common around 1.5y3 M Stars
We describe Spitzer IRAC and MIPS observations of the nearby 25 Myr old open cluster NGC 2232. Combining these data with ROSATAll-Sky Survey observations, proper motions, and optical photometry/spectroscopy, we construct a list of highly probable cluster members. We identify one A-type star, HD 45435, that has definite excess emission at 4.5Y24 m indicative of debris from terrestrial planet for...
متن کاملThe Kuiper Belt and Other Debris Disks
We discuss the current knowledge of the Solar system, focusing on bodies in the outer regions, on the information they provide concerning Solar system formation, and on the possible relationships that may exist between our system and the debris disks of other stars. Beyond the domains of the Terrestrial and giant planets, the comets in the Kuiper belt and the Oort cloud preserve some of our mos...
متن کاملVariations on Debris Disks: Icy Planet Formation at 30–150 AU for 1–3 M⊙ Main Sequence Stars
We describe calculations for the formation of icy planets and debris disks at 30–150 AU around 1–3 M⊙ stars. Debris disk formation coincides with the formation of planetary systems. As protoplanets grow, they stir leftover planetesimals to large velocities. A cascade of collisions then grinds the leftovers to dust, forming an observable debris disk. Stellar lifetimes and the collisional cascade...
متن کاملDynamics of small bodies in planetary systems
The number of stars that are known to have debris disks is greater than that of stars known to harbour planets. These disks are detected because dust is created in the destruction of planetesimals in the disks much in the same way that dust is produced in the asteroid belt and Kuiper belt in the solar system. For the nearest stars the structure of their debris disks can be directly imaged, show...
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تاریخ انتشار 2004