Open Suzibianco opened 6 years ago
A regolith density equation adaptable to highland or mare soils, porosity from agglutinates a percentage, the other two terms are basic specific-gravity then depth: https://drive.google.com/file/d/1KobDfKSZukTNKKuHQcfWs6FwGzG8u7eN/view?usp=drivesdk
Tom, Do you have a reference for that? I'm struggling to parse it.
@jrcgarry I haven't fount the log function, yet, for surface you can use estimated values from just the average density for the type from the first integral, forget the term for depth and use porosity percent by type, doing that I came up with 2-1/3 g/cc two ways for our landing site. If anyone finds the log function we'll add it, keeping an eye open.
Tom, I meant, do you have a reference for where this equation came from? (textbook, paper, etc.)
@jrcgarry It's my equation as an estimation tool, I took the limits from Chapter 6, Table 6.8 on Mare vs Highland soils, still no dice on the log function. This gave me a 3-1/3 cc shot per coin of as-is regolith for Mare, it's more for Highland from that being more porous than Mare by quite a lot, 59% voids vs 26%.
This also implies less compaction for adobes from Mare soils, heat pressing will be faster.
?:) I'm no closer to understanding. Is the goal to identify the density of regolith at depth? (if so, the removal of said regolith will surely perturb it)
If not, then I'm puzzled by the integral over depth (presumably with respect to depth)
And I'm a little unsure about your dimensions. You have mass per unit volume on the left, and then on the right some function of specific density (referenced to something I suppose), multiplied by an integral of something (again, integrated over depth I guess), and then porosity (another scalar).
Can you explain what it is that you're trying to calculate and I can then propose a defensible model.
Mind, if the goal is to quantify a specimen's density, the simplest way is to measure it (!). Either gravimetrically (load cell, known cavity volume) or by some kind of densitometer (a la Venera 9/Philae).
This might help... https://sciences.ucf.edu/class/planetary-simulant-database/
Generate a reference database on sample properties from all surface sites (Apollo 12, 14, 15, 16 & 17; Luna).
Draft Example: