My Assistant
Titan Porous Grain Simulation, Are hydrocarbon oceans hiding in the surface of Titan? |
Feb 28 2009, 08:21 PM
Post
#1
|
||
![]() Senior Member ![]() ![]() ![]() ![]() Group: Moderator Posts: 2785 Joined: 10-November 06 From: Pasadena, CA Member No.: 1345 |
Recent articles have invoked porous ice sands or other crustal grains as an additional potential reservoir for methane on Titan. (Selected examples: Sotin et al., 2009; Mitchell et al., 2009; Turtle et al, 2009,; Hayes et al 2008)
Last week, I set up a very simple laboratory experiment using an analogous system to try to answer the following questions: 1) How much methane could porous sands possibly hold per unit volume? 2) How will it affect the evaporation rate? 3) How could it affect the surface reflectivity? As a laboratory analog for Titan’s hydrocarbon liquid mix (methane/ethane/nitrogen), I used solvent-grade heptane. As an analog for Titan’s polar ice grains, I used either Flash-grade silica gel or analytical grade quartz beach sand. (The polar hydroxyl groups of the ice grains being analogous by the siloxy groups of silica) The set-up Three standard size 600 mL beakers were used: Beaker A was charged with 400 mL silica gel Beaker B was changed with 400 mL sand Beaker C (control) was left empty. Here are the initial images: To initiate the experiment, a volume of Heptane was added to each beaker. Then, images and and weights were taken at key timepoints over a several day period to determine evaporation rate and monitor changes in visual appearance. [Note: Although the temperature was held constant 298 K, the beakers were placed side-by-side in a fume hood with varying hoodflow (face velocity minimum was 100 cfm).] Initial References: Mitchell K.L., et al., LPSC 40 (2009) Abstract 1966. “A global sub-surface alkanifer system on Titan?”. Hayes, A., et al. Geophysical Research Letters 35 (2008) L09204. “Hydrocarbon lakes on Titan: Distribution and interaction with a porous regolith”. doi: 10.1029/2008GL033409. Sotin , C., et al. LPSC 40 (2009) Abstract 2088. “Ice-hydrocarbon interactions under Titan-like conditions: implications for the carbon cycle on Titan.” Turtle, E. P., et al., Geophysical Research Letters 36 (2009) L02204. “Cassini Imaging of Titan’s High-Latitude Lakes, Clouds, and South-Polar Surface Changes.” doi: 10.1029/2008GL036186. -------------------- Some higher resolution images available at my photostream: http://www.flickr.com/photos/31678681@N07/
|
|
|
|
||
![]() |
Mar 15 2009, 04:00 AM
Post
#2
|
|
![]() Senior Member ![]() ![]() ![]() ![]() Group: Moderator Posts: 2785 Joined: 10-November 06 From: Pasadena, CA Member No.: 1345 |
-------------------- Some higher resolution images available at my photostream: http://www.flickr.com/photos/31678681@N07/
|
|
|
|
Juramike Titan Porous Grain Simulation Feb 28 2009, 08:21 PM
Juramike 1) How much methane could porous sands hold?
Imag... Feb 28 2009, 08:27 PM
nprev Wow! Neat experiment, Mike, thanks for shar... Mar 1 2009, 01:19 AM
Juramike QUOTE (nprev @ Feb 28 2009, 08:19 PM) By ... Mar 1 2009, 01:29 AM
nprev QUOTE (Juramike @ Feb 28 2009, 05:29 PM) ... Mar 1 2009, 09:19 PM
Juramike 2) How will it affect the evaporation rate?
Beak... Mar 1 2009, 01:46 AM
Juramike Assuming a constant surface evaporation rate of th... Mar 1 2009, 06:22 PM
rlorenz Great experiment, Mike. Nice and transparent.... Mar 7 2009, 04:42 PM
rlorenz QUOTE (rlorenz @ Mar 7 2009, 11:42 AM) ht... Mar 7 2009, 04:50 PM
ngunn QUOTE (rlorenz @ Mar 7 2009, 04:42 PM) Wh... Mar 7 2009, 08:05 PM
Juramike Assuming the heaviest materials on Titan's sur... Mar 1 2009, 10:23 PM
AndyG QUOTE (Juramike @ Mar 1 2009, 10:23 PM) O... Mar 1 2009, 11:04 PM
Juramike (I stand corrected. Quartz density is ca. 2.65 g/... Mar 1 2009, 11:54 PM
Juramike 3) How could it affect surface reflectivity?
Her... Mar 9 2009, 03:34 AM
marsbug Mike, would it be possible to place an optical mic... Mar 9 2009, 12:12 PM
Juramike QUOTE (marsbug @ Mar 9 2009, 07:12 AM) cl... Mar 10 2009, 12:37 AM
Juramike Here are the images of the top surface of a second... Mar 10 2009, 02:15 AM
Juramike So silica/heptane changes appearance on wetting or... Mar 10 2009, 02:17 AM
ngunn Thinking about the optical properties of methane-w... Mar 10 2009, 10:24 AM
Juramike Here is recently released Cassini ISS graphic PIA1... Mar 12 2009, 02:13 AM
Juramike Extending this to the Equatorial Sand Sea basins (... Mar 14 2009, 01:32 AM
Juramike Volume capacity of porous sediments in the sand se... Mar 15 2009, 04:04 AM
Juramike Here is a diagram of Titan’s possible methane cycl... Mar 16 2009, 11:59 PM
ngunn There are some striking turns of phrase in that pa... Mar 17 2009, 08:38 AM![]() ![]() |
|
Lo-Fi Version | Time is now: 17th December 2024 - 01:35 AM |
|
RULES AND GUIDELINES Please read the Forum Rules and Guidelines before posting. IMAGE COPYRIGHT |
OPINIONS AND MODERATION Opinions expressed on UnmannedSpaceflight.com are those of the individual posters and do not necessarily reflect the opinions of UnmannedSpaceflight.com or The Planetary Society. The all-volunteer UnmannedSpaceflight.com moderation team is wholly independent of The Planetary Society. The Planetary Society has no influence over decisions made by the UnmannedSpaceflight.com moderators. |
SUPPORT THE FORUM Unmannedspaceflight.com is funded by the Planetary Society. Please consider supporting our work and many other projects by donating to the Society or becoming a member. |
|