Loss of water from Venus. I. Hydrodynamic escape of hydrogen

James F. Kasting, James B. Pollack

Research output: Contribution to journalArticlepeer-review

189 Scopus citations

Abstract

A one-dimensional photochemical-dynamic model is used to study hydrodynamic loss of hydrogen from a primitive, water-rich atmosphere on Venus. The escape flux is calculated as a function of the H2O mixing ratio at the atmospheric cold trap. The cold-trap mixing ratio is then related in an approximate fashion to the H2O concentration in the lower atmosphere. Hydrodynamic escape should have been the dominant loss process for hydrogen when the H2O mass mixing ratio in the lower atmosphere exceeded ∼0.1. The escape rate would have depended upon the magnitude of the solar ultraviolet flux and the atmospheric euv heating efficiency and, to a lesser extent, on the O2 content of the atmosphere. The time required for Venus to have lost the bulk of a terrestrial ocean of water is on the order of a billion years. Deutrium would have been swept away along with hydrogen if the escape rate was high enough, but some D/H enrichment should have occurred as the escape rate slowed down.

Original languageEnglish (US)
Pages (from-to)479-508
Number of pages30
JournalIcarus
Volume53
Issue number3
DOIs
StatePublished - Mar 1983

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Loss of water from Venus. I. Hydrodynamic escape of hydrogen'. Together they form a unique fingerprint.

Cite this