A theoretical look at the direct detection of giant planets outside the Solar System
Adam Burrows ()
Additional contact information
Adam Burrows: The University of Arizona
Nature, 2005, vol. 433, issue 7023, 261-268
Abstract:
Abstract Astronomy is at times a science of unexpected discovery. When it is, and if we are lucky, new intellectual territories emerge to challenge our views of the cosmos. The recent indirect detections using high-precision Doppler spectroscopy of more than 100 giant planets orbiting more than 100 nearby stars is an example of such rare serendipity. What has been learned has shaken out preconceptions, for none of the planetary systems discovered so far is like our own. The key to unlocking a planet's chemical, structural, and evolutionary secrets, however, is the direct detection of the planet's light. Because there have been as yet no confirmed detections, a theoretical analysis of such a planet's atmosphere is necessary for guiding our search.
Date: 2005
References: Add references at CitEc
Citations:
Downloads: (external link)
https://www.nature.com/articles/nature03244 Abstract (text/html)
Access to the full text of the articles in this series is restricted.
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:433:y:2005:i:7023:d:10.1038_nature03244
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/nature03244
Access Statistics for this article
Nature is currently edited by Magdalena Skipper
More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().