Astrophysics and Space Science

, Volume 313, Issue 1, pp 175–181

Planetary atmospheres with ALMA

Authors

Original Article

DOI: 10.1007/s10509-007-9637-y

Cite this article as:
Lellouch, E. Astrophys Space Sci (2008) 313: 175. doi:10.1007/s10509-007-9637-y
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Abstract

Thanks to its sensitivity, spatial resolution and instantaneous uv-coverage, ALMA will permit many new studies related to the general topic of the couplings between chemistry and dynamics in planetary atmospheres. It will include: (1) three-dimensional mapping of composition, temperatures and winds in the atmospheres of Mars, Venus and Titan; (2) several aspects of Giant Planet composition and dynamics, such as the origin of oxygen, the evolution of Shoemaker–Levy 9 products in Jupiter’s atmosphere, and the deep atmosphere structure and meteorology; (3) the study of tenuous and distant atmospheres (Io, Enceladus, Pluto, Triton and other Kuiper Belt objects).

Keywords

PlanetsSubmillimeterInterferometry
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© Springer Science+Business Media B.V. 2007