Measuring Jupiter's water abundance by Juno: the link between interior and formation models

被引：37

作者：

Helled, Ravit ^{[1
]}

Lunine, Jonathan ^{[2
]}

机构：

[1] Tel Aviv Univ, Dept Geophys & Planetary Sci, IL-69978 Tel Aviv, Israel

[2] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2014年 / 441卷 / 03期

关键词：

planets and satellites: composition; planets and satellites: formation; planets and satellites: individual: Jupiter; planets and satellites: interiors; GIANT PLANETS; ORIGIN; MASS; ATMOSPHERE; PROBE;

D O I：

10.1093/mnras/stu516

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Juno mission to Jupiter is planned to measure the water abundance in Jupiter's atmosphere below the cloud layer. This measurement is important because it can be used to reveal valuable information on Jupiter's origin and its composition. In this paper, we discuss the importance of this measurement, the challenges in its interpretation, and address how it can be connected to interior and formation models of Jupiter.

引用

页码：2273 / 2279

页数：7

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