Passing through a giant molecular cloud: ``Snowball'' glaciations produced by interstellar dust

Details Passing through a giant molecular cloud: ``Snowball'' glaciations produced by interstellar dust Passing through a giant molecular cloud: ``Snowball'' glaciations produced by interstellar dust

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005georl..3203705p&link_type=abstract

Geophysical Research Letters, Volume 32, Issue 3, CiteID L03705

Mathematics

Logic

10

Atmospheric Composition And Structure: Evolution Of The Atmosphere (1610, 8125), Atmospheric Composition And Structure: Aerosols And Particles (0345, 4801, 4906), Planetary Sciences: Solar System Objects: Dust, Information Related To Geologic Time: Proterozoic, Information Related To Geologic Time: Paleozoic

Scientific paper

In its motion through the Milky Way galaxy, the solar system encounters an average -density (>=330 H atoms cm-3) giant molecular cloud (GMC) approximately every 108 years, a dense (~2 × 103 H atoms cm-3) GMC every ~109 years and will inevitably encounter them in the future [Talbot and Newman, 1977]. However, there have been no studies linking such events with severe (snowball) glaciations in Earth history. Here we show that dramatic climate change can be caused by interstellar dust accumulating in Earth's atmosphere during the solar system's immersion into a dense (~2 × 103 H atoms cm-3) GMC. The stratospheric dust layer from such interstellar particles could provide enough radiative forcing to trigger the runaway ice-albedo feedback that results in global snowball glaciations. We also demonstrate that more frequent collisions with less dense GMCs could cause moderate ice ages.

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