NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Recognizing the TrendsSolar system planetary science has traditionally focused on understanding in depth individual planets. While there have been some efforts at synergy, most studies have focused on understanding the details of individual planets. Now that we are in the era of exoplanet science, with thousands of known planets and hundreds that have been characterized to varying degrees, the systematics of planetary science are becoming apparent. This also means that, for the first time, what had previously been seen as individual quirks of solar system planets are instead being recognized as part of the normal range of planetary behavior. In my talk I will consider a number of such characteristics and explain how we are now starting to understand their true context. In particular I will discuss the atmospheric composition, clouds, hazes, and winds of giant planets, trace gasses in the atmosphere of Venus, and the presence and absence of atmospheres on various terrestrial worlds.
Document ID
20160004667
Acquisition Source
Ames Research Center
Document Type
Abstract
Authors
Marley, Mark Scott
(NASA Ames Research Center Moffett Field, CA United States)
Date Acquired
April 6, 2016
Publication Date
March 30, 2016
Subject Category
Astronomy
Report/Patent Number
ARC-E-DAA-TN28827
Report Number: ARC-E-DAA-TN28827
Meeting Information
Meeting: UK Exoplanet Community Meeting 2016 (UKEXOM 2016)
Location: Exeter
Country: United Kingdom
Start Date: March 30, 2016
End Date: April 1, 2016
Sponsors: Science and Technology Facilities Council (STFC), Exeter Univ.
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Keywords
atmosphere of Venus
exoplanet science
clouds
and winds of giant planets
hazes
No Preview Available