Physics
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007icar..188..154t&link_type=abstract
Icarus, Volume 188, Issue 1, p. 154-161.
Physics
31
Scientific paper
Monte Carlo simulations are used to model the July 14, 2005 UVIS stellar occultation observations of the water vapor plumes on Enceladus. These simulations indicate that the observations can be best fit if the water molecules ejected along the Tiger Stripes in the South Polar region of Enceladus have a vertical surface velocity of 300 500 m/s at the surface. The high surface velocity suggests that the plumes on Enceladus originate from some depth beneath the surface. The total escape rate of water molecules is 4 6×10 s, or 120 180 kg/s, consistent with previous works, and more than 100 times the estimated mass escape rate for ice particles. The average deposition rate in the South Polar region is on the order of 1011 cm-2 s-1, yielding a resurfacing rate as high as 3×10 cm/yr. The globally averaged deposition rate of water molecules is about one order of magnitude lower.
Esposito W. L. W. L.
Larsen Kristopher William
Stewart Ian F. A.
Tian Feng
Toon Brian O.
No associations
LandOfFree
Monte Carlo simulations of the water vapor plumes on Enceladus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Monte Carlo simulations of the water vapor plumes on Enceladus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Monte Carlo simulations of the water vapor plumes on Enceladus will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-770374