We need a soil sample from Antarctica

High School students working at the Barboza Space Center are working on growing better plants for Mars.  www.BarbozaSpaceCenter.com

We need a test-tube size sample of soil from your country for experiments we will be conducting in July, 2018 in Los Angeles and Long Beach, California.  We want to collaborate with other high school students from around the world.   Our project is the Occupy Mars Learning Adventures.  

Contact: Bob Barboza at (562) 221-1780 Cell.

Soil Sample Mars Project.jpg

Martian soil

Curiosity‘s view of Martian soil and boulders after crossing the “Dingo Gap” sand dune (February 9, 2014; raw color).

Martian soil is the fine regolith found on the surface of Mars. Its properties can differ significantly from those of terrestrial soil. The term Martian soil typically refers to the finer fraction of regolith. On Earth, the term “soil” usually includes organic content.[1] In contrast, planetary scientists adopt a functional definition of soil to distinguish it from rocks.[2] Rocks generally refer to 10 cm scale and larger materials (e.g., fragments, breccia, and exposed outcrops) with high thermal inertia, with areal fractions consistent with the Viking Infrared Thermal Mapper (IRTM) data, and immobile under current aeolian conditions.[2] Consequently, rocks classify as grains exceeding the size of cobbles on the Wentworth scale.

This approach enables agreement across Martian remote sensing methods that span the electromagnetic spectrum from gamma to radio waves. ‘‘Soil’’ refers to all other, typically unconsolidated, material including those sufficiently fine-grained to be mobilized by wind.[2] Soil consequently encompasses a variety of regolith components identified at landing sites. Typical examples include: bedform armor, clasts, concretions, drift, dust, rocky fragments, and sand. The functional definition reinforces a recently proposed genetic definition of soil on terrestrial bodies (including asteroids and satellites) as an unconsolidated and chemically weathered surficial layer of fine-grained mineral or organic material exceeding centimeter scale thickness, with or without coarse elements and cemented portions.[1]

Martian dust generally connotes even finer materials than Martian soil, the fraction which is less than 30 micrometres in diameter. Disagreement over the significance of soil’s definition arises due to the lack of an integrated concept of soil in the literature. The pragmatic definition “medium for plant growth” has been commonly adopted in the planetary science community but a more complex definition describes soil as “(bio)geochemically/physically altered material at the surface of a planetary body that encompasses surficial extraterrestrial telluric deposits.” This definition emphasizes that soil is a body that retains information about its environmental history and that does not need the presence of life to form.

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