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interstellar water
Spatial distribution and isotopic compositions of the different water reser...
Scheme of interstellar normal (H 2 O) and heavy water (HDO) formation on th...
The Quest For Water
APPENDIX: A RECIPE FOR THE ATMOSPHERE AND THE OCEANS
An evolutionary system of mineralogy. Part II: Interstellar and solar nebula primary condensation mineralogy (>4.565 Ga)
Recent Advances in our Understanding of Water and Aqueous Activity in Chondrites
Oxygen in the Interstellar Medium
The mineralogy of cosmic dust: astromineralogy
We Drink Good 4.5-Billion-Year-Old Water
Oxygen in Comets and Interplanetary Dust Particles
Mass-independent Oxygen Isotope Variation in the Solar Nebula
Sketch of the four major steps involved in the formation of a planetary sys...
Organic Molecules and Volatiles in Comets
Flyby Missions to Comets and Return Sample Analysis
Incubating Life: Prebiotic Sources of Organics for the Origin of Life
ORIGINS AND EARLY EVOLUTION OF THE ATMOSPHERE AND THE OCEANS
Comets: Where We Are, How We Got Here, and Where We Want To Go Next
The impact of a large body in the oceans would inject large quantities of water through the tropopause cold trap into the stratosphere and lower mesosophere. We consider the consequences of enhanced water vapor concentrations on the middle atmosphere (50–100 km) chemistry and heat budget. The increased mixing ratio of hydrogen dramatically decreases the ozone concentration above 60 km. Catalytic reactions with odd hydrogen are the main sink of ozone in this region. The ozone reduction causes a lowering of the average height of the mesopause, as well as a lowering of the average temperature. The lower colder mesopause and the creation of saturation conditions over much of the upper mesosphere would have resulted in a permanent layer of mesospheric ice clouds of nearly world-wide extent. (At present, these exist only at high latitudes and are observed in summer as “noctilucent clouds.”) The globally-averaged albedo resulting from these clouds is dependent on the particulate size and shape, and can be as high as several percent, preferentially covering the summer hemisphere. This could have important implications for the short-term climate following a large-body impact. Similar effects would also result from an encounter with a more extended object such as a swarm of cosmic debris or a dense interstellar cloud.