dc.contributor.author |
Duxbury, N.S. |
en_US |
dc.contributor.author |
Brown, R.H. |
en_US |
dc.date.accessioned |
2004-10-01T17:26:37Z |
|
dc.date.available |
2004-10-01T17:26:37Z |
|
dc.date.issued |
1995-03 |
en_US |
dc.identifier.citation |
Houston, TX |
en_US |
dc.identifier.clearanceno |
95-0073 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/28034 |
|
dc.description.abstract |
A mechanism is suggested and modeled whereby there may be boiling geysers on Triton. The geysers would be of nitrogen considering that Voyager detected cryovolcanic activity, that solid nitrogen conducts heat much less than water ice, and that there is internal heat on Triton. |
en_US |
dc.format.extent |
70548 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
Triton planetary geology geysers |
en_US |
dc.title |
The Plausibility of Boiling Geysers on Triton |
en_US |