Self-assembly of tholins in environments simulating Titan liquidospheres: Implications for formation of primitive coacervates on Titan

Access this Article

Search this Article

Abstract

Titan, the largest satellite of Saturn, has a thick atmosphere containing nitrogen and methane. A variety of organic compounds have been detected in the atmosphere, most likely produced when atmospheric gases are exposed to ultraviolet light, electrons captured by the magnetosphere of Saturn, and cosmic rays. The Cassini / Huygens probe showed that the average temperature on the surface of Titan is 93.7 K, with lakes of liquid ethane and methane. Sub-surface mixtures of liquid ammonia and water may also be present. We have synthesized complex organic compounds (tholins) by exposing a mixture of nitrogen and methane to plasma discharges, and investigated their interactions with several different liquids that simulate Titan's liquidosphere. We found that coacervates formed when tholins were extracted in non-polar solvents followed by exposure to aqueous ammonia solutions. The results suggest that coacervates can self-assemble in Titan's liquidosphere which have the potential to undergo further chemical evolution. Similar processes are likely to occur in the early evolution of habitable planets when tholin-like compounds undergo phase separation into microscopic structures dispersed in a suitable aqueous environment.

Journal

  • International journal of astrobiology

    International journal of astrobiology 12(4), 282-291, 2013

    Cambridge University Press

Codes

  • NII Article ID (NAID)
    120005350123
  • NII NACSIS-CAT ID (NCID)
    AA11828626
  • Text Lang
    ENG
  • Article Type
    journal article
  • ISSN
    1473-5504
  • Data Source
    IR 
Page Top