Numerical Models of the Early Stages of Planet Formation | A New Perspective on the Role of Turbulence

Anders Johansen

ISBN 10: 3836488922 / ISBN 13: 9783836488921

Published by VDM Verlag Dr. Müller, 2008

About this Item

Numerical Models of the Early Stages of Planet Formation | A New Perspective on the Role of Turbulence | Anders Johansen | Taschenbuch | Englisch | VDM Verlag Dr. Müller | EAN 9783836488921 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu.

Seller Inventory # 101838479

Bibliographic Details

• Title: Numerical Models of the Early Stages of Planet Formation | A New Perspective on the Role of Turbulence
• Publisher: VDM Verlag Dr. Müller
• Publication Date: 2008
• Language: English
• ISBN 10: 3836488922
• ISBN 13: 9783836488921
• Binding: Taschenbuch
• Condition: Neu
• Dimensions: 13W x 150H x 220D millimeters 13 millimeters width by 150 millimeters height by 220 millimeters depth
• Weight: 338 grams
• Seller catalogs:
  • Bücher

About this title

Synopsis

In the earliest stages of planet formation micrometer-sized dust grains collide and gradually build up kilometer-sized {em planetesimals}, bodies that are so large that they can attract each other directly by gravity. This is an important landmark on the way to real planets because of the change to gravity-dominated growth. The road from boulders to planetesimals is however poorly known. Boulders have poor sticking properties and spiral into the young star due to the head wind from the slower rotating gas. This work presents the first detailed computer simulations of the motion of dust and boulders in turbulent protoplanetary discs. The turbulent diffusion coefficient of small dust grains is measured to be surprisingly high, whereas larger boulders concentrate by up to two orders of magnitude in transient high pressure regions that arise spontaneously in magnetorotational turbulence. The coupled motion of boulders and gas is found to be linearly unstable to the so-called streaming instability, leading to a turbulent state that is characterised by dense clumps of boulders that shield each other against the head wind of the gas.

About the Author

Anders Johansen finished his master's thesis at Copenhagen University in 2004. From 2004 to 2007 he was a PhD student at the Max Planck Institute for Astronomy and Heidelberg University, supervised by Hubert Klahr and Thomas Henning. He currently holds a postdoctoral position at Leiden University where his research is focused on planet formation.