期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 328, 期 1-2, 页码 319-323出版社
SPRINGER
DOI: 10.1007/s10509-010-0299-9
关键词
Methods: photometry; Stars: oscillations; Extrasolar planets
The satellite PLATO represents a new challenge for future investigations of exoplanets and oscillations of stars. It is one of the proposed missions of ESA COSMIC VISION 2015-2025 and it is scheduled for launch in 2017. The goal of the mission is a full characterization of the planet star systems with an asteroseismic analysis of the host stars. The PLATO Payload Consortium (PPLC) includes several European countries which are employed in the assessment study of the mission. Thanks to the high precision photometry, PLATO is thought to be able to detect planets and oscillations within a large sample of targets.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据