<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>Randolph L. Kirk</dc:contributor>
  <dc:contributor>T. V. Johnson</dc:contributor>
  <dc:contributor>Laurence A. Soderblom</dc:contributor>
  <dc:creator>R. H. Brown</dc:creator>
  <dc:date>1990</dc:date>
  <dc:description>Four geyser-like plumes were discovered near Triton's south pole in areas now in permanent sunlight. Because Triton's southern hemisphere is nearing a maximum summer solstice, insolation as a driver or a trigger for Triton's geyser-like plumes is an attractive hypothesis. Trapping of solar radiation in a translucent, low-conductivity surface layer (in a solid-state greenhouse), which is subsequently released in the form of latent heat of sublimation, could provide the required energy. Both the classical solid-state greenhouse consisting of exponentially absorbed insolation in a gray, translucent layer of solid nitrogen, and the "super" greenhouse consisting of a relatively transparent solid-nitrogen layer over an opaque, absorbing layer are plausible candidates. Geothermal heat may also play a part if assisted by the added energy input of seasonal cycles of insolation.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1126/science.250.4979.431</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Association for the Advancement of Science (AAAS)</dc:publisher>
  <dc:title>Energy sources for triton's geyser-like plumes</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>