Extrasolar Planets: Constraints for Planet Formation Models-Reference-Cited by-同舟云学术

Extrasolar Planets: Constraints for Planet Formation Models

Published:2005-10-14 Issue:5746 Volume:310 Page:251-255
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Santos Nuno C.¹²³,Benz Willy¹²³,Mayor Michel¹²³

Affiliation:

1. Centro de Astronomia e Astrofísica da Universidade de Lisboa, Observatório Astronómico de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal.

2. Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.

3. Observatoire de Genève, 51 chemin des Maillettes, 1290 Sauverny, Switzerland.

Abstract

Since 1995, more than 150 extrasolar planets have been discovered, most of them in orbits quite different from those of the giant planets in our own solar system. The number of discovered extrasolar planets demonstrates that planetary systems are common but also that they may possess a large variety of properties. As the number of detections grows, statistical studies of the properties of exoplanets and their host stars can be conducted to unravel some of the key physical and chemical processes leading to the formation of planetary systems.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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