Terms and Concepts for Jones et al. (2000)

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dust/gas ratio -   In the solar nebula, the amount of condensed matter ("dust") is relatively small compared to the amount of gas -- chiefly H and He.  The dust/gas ratio increases as temperature decreases and more condensed material becomes stable.  Researchers usually refer to an elevated dust/gas ratio to describe a system that has a non-cosmic composition which is depleted in gas compared to rocky or icy components.  An elevated dust/gas ratio implies that dust was locally concentrated by some mechanism.  Vaporization of such dust would enrich the gas in those components present in the dust, resulting in a gas of non-solar composition.

planetesimal  - This refers to a small planetary body in the early solar system.  Planetesimals are the smaller bodies that must have formed before larger objects such as planets, moons, asteroids, etc., accreted.

protoplanet - This refers to a larger planetary body that has not yet fully accreted into a planet.  Such objects can have atmospheres.

mach number - This is the speed of an object relative to the speed of sound in the medium traversed by the object.  Mach 1 is equivalent to the speed of sound, Mach 2 is twice the speed of sound, etc.  An object moving faster than the speed of sound will create a shock wave.  [For an ideal gas, the speed of sound v = sqrt(gamma * pressure / density), where gamma = a constant, and pressure and density refer to the gas.]
 
 
The X-wind model for chondrule and CAI formation.  The wedge-shaped
reddish and yellow areas represent the solar nebula disk, here seen along
the mid-plane.  The disk is wedge-shaped owing to a balance between
gravity and gas pressure.