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An alternative expression for the escape velocity v e particularly useful at the surface on the body is: = where r is the distance between the center of the body and the point at which escape velocity is being calculated and g is the gravitational acceleration at that distance (i.e., the surface gravity). [11]
One classical thermal escape mechanism is Jeans escape, [1] named after British astronomer Sir James Jeans, who first described this process of atmospheric loss. [2] In a quantity of gas, the average velocity of any one molecule is measured by the gas's temperature, but the velocities of individual molecules change as they collide with one another, gaining and losing kinetic energy.
This is why atomic hydrogen escapes preferentially from an atmosphere. If there is a strong thermally driven atmospheric escape of light atoms, heavier atoms can achieve the escape velocity through viscous drag by those escaping lighter atoms. [2] This is another way of thermal escape, called hydrodynamic escape.
The escape of any atmospheric gas can be diffusion-limited, but only diffusion-limited escape of hydrogen has been observed in our solar system, on Earth, Mars, Venus and Titan. [1] Diffusion-limited hydrogen escape was likely important for the rise of oxygen in Earth's atmosphere ( the Great Oxidation Event ) and can be used to estimate the ...
The bacteria B. subtilis.. Recent experiments have found organisms that can survive both the acceleration and jerk involved in reaching escape velocity. A major impact event was simulated using an air cannon to propel both ice and agar projectiles covered with chosen microorganisms to extreme speeds and then crashing the projectiles into a solid surface. [2]
Like carbon, dissociative recombination of N 2 + is important for the nitrogen escape on Mars. [60] [61] In addition, other photochemical escape mechanism also play an important role: [60] [62] N 2 + hν N + + N + e − N 2 + e − N + + N + 2e −. Nitrogen escape rate is very sensitive to the mass of the atom and solar activity.
In physics and chemistry, effusion is the process in which a gas escapes from a container through a hole of diameter considerably smaller than the mean free path of the molecules. [1] Such a hole is often described as a pinhole and the escape of the gas is due to the pressure difference between the container and the exterior.
Research concerning the relationship between the thermodynamic quantity entropy and both the origin and evolution of life began around the turn of the 20th century. In 1910 American historian Henry Adams printed and distributed to university libraries and history professors the small volume A Letter to American Teachers of History proposing a theory of history based on the second law of ...