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

Alexander A. Pavlov, Owen B. Toon, Anatoli K. Pavlov, John Bally, David Pollard

Research output: Contribution to journalArticle

36 Scopus citations

Abstract

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.

Original languageEnglish (US)
Pages (from-to)1-4
Number of pages4
JournalGeophysical Research Letters
Volume32
Issue number3
DOIs
StatePublished - Feb 16 2005

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Earth and Planetary Sciences(all)

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