This international conference was held to give an overview of this rapidly developing field and promote discussion on future studies among observers, theorists, and instruments.
Includes bibliographical references and index.
|Statement||editors, Tomonori Usuda, Miki Ishii, Motohide Tamura.|
|Series||AIP conference proceedings -- v. 1158, AIP conference proceedings -- no. 1158.|
|Contributions||Usuda, Tomonori., Ishii, Miki., Tamura, Motohide.|
|LC Classifications||QB820 .E95 2009|
|The Physical Object|
|Pagination||xxii, 409 p. :|
|Number of Pages||409|
|LC Control Number||2009288697|
EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY Proceedings of the International Conference Kailua-Kona,Hawaii March r . The authors write in an almost breezy, accessible style, telling us, first the basics of exoplanets, how they are detected, what the current state is, and then they go into a kind of tour guide to some example types of exoplanets. The book concludes with short chapters on the Drake Equation, the search for intelligence, and the Fermi Paradox/5(49). The convention for designating exoplanets is an extension of the system used for designating multiple-star systems as adopted by the International Astronomical Union (IAU). For exoplanets orbiting a single star, the IAU designation is formed by taking the designated or proper name of its parent star, and adding a lower case letter. Letters are given in order of each planet's . Exoplanets and Disks: Their Formation and Diversity by Tomonori Usuda,Motohide Tamura,Miki Ishii Book Resume: Protoplanetary disks around young stars are the sites of planetary formation. Recent high spatial resolution observations from both ground and space have revealed wide varieties of disk morphology and composition.
Protoplanetary disks around young stars are the sites of planetary formation. Their detailed information has been obtained by recent high spatial resolution infrared and optical observations from both ground and space, and wide varieties of disk morphology and disk composition are uncovered. At longer wavelengths, ALMA has started its early science operation and will . Get this from a library! Exoplanets and disks their formation and diversity: proceedings of the international conference, Kailua-Kona, Hawaii, March [Tomonori Usuda; Miki Ishii; Motohide Tamura;] -- This international conference was held to give an overview of this rapidly developing field and promote discussion on future studies among observers, theorists, and . Exoplanet formation and evolution The way exoplanets form and evolve has a direct impact on the composition and dynamics of their atmospheres. The local conditions at their birth, the accretion mechanism and how they interact with their parent star, disk and potentially other planets, govern the diversity of compositions and atmospheric. A 'read' is counted each time someone views a publication summary (such as the title, abstract, and list of authors), clicks on a figure, or views or downloads the full-text.
Book. Full-text available We now enter a new era as we begin to investigate the chemical diversity of exoplanets, their atmospheric and interior processes, and their formation conditions. Understanding how planets form and evolve and how life emerged on Earth are among the most fundamental questions in planetary science and astronomy. We are living in an exciting era where, in addition to the planets in our Solar System, we can study and characterize over thousand exoplanets orbiting other stars. The statistical characterization of exoplanets through their mass-radius and mass-luminosity diagram is becoming possible. This is for planet formation and evolution theory of similar importance as the mass-distance diagram. Aims. Our aim is to extend our planet formation model into a coupled formation and evolution model. We want to calculate from. The work involves collaborations with many groups worldwide using related techniques. JPL researchers aim to answer numerous questions on the following topics: the kinds of exoplanets that exist, the factors that determine the properties of exoplanet atmospheres, and what the disks around young stars reveal about the formation of exoplanets.