Suppr超能文献

太阳系外行星仙女座Upsilon b的相位相关红外亮度。

The phase-dependent infrared brightness of the extrasolar planet upsilon Andromedae b.

作者信息

Harrington Joseph, Hansen Brad M, Luszcz Statia H, Seager Sara, Deming Drake, Menou Kristen, Cho James Y-K, Richardson L Jeremy

机构信息

Department of Physics, University of Central Florida, Orlando, FL 32816, USA.

出版信息

Science. 2006 Oct 27;314(5799):623-6. doi: 10.1126/science.1133904. Epub 2006 Oct 12.

Abstract

The star upsilon Andromedae is orbited by three known planets, the innermost of which has an orbital period of 4.617 days and a mass at least 0.69 that of Jupiter. This planet is close enough to its host star that the radiation it absorbs overwhelms its internal heat losses. Here, we present the 24-micrometer light curve of this system, obtained with the Spitzer Space Telescope. It shows a variation in phase with the orbital motion of the innermost planet, demonstrating that such planets possess distinct hot substellar (day) and cold antistellar (night) faces.

摘要

仙女座υ星有三颗已知行星环绕,其中最内侧的行星轨道周期为4.617天,质量至少是木星的0.69倍。这颗行星距离其主恒星足够近,以至于它吸收的辐射超过了其内部的热量损失。在此,我们展示了利用斯皮策空间望远镜获得的该系统的24微米波段光变曲线。它显示出与最内侧行星轨道运动的相位变化,表明这类行星具有明显的热的星下点(白昼)和冷的反星下点(夜晚)表面。

文献AI研究员

20分钟写一篇综述,助力文献阅读效率提升50倍。

立即体验

用中文搜PubMed

大模型驱动的PubMed中文搜索引擎

马上搜索

文档翻译

学术文献翻译模型,支持多种主流文档格式。

立即体验