Ram pressure

Ram pressure stripping in NGC 4402 as it falls towards the Virgo Supercluster (off image, toward bottom left). Note the dust (brown) trailing behind (toward upper right) the galaxy, versus the dust-free (blue-white) leading edge.

Ram pressure is a pressure exerted on a body moving through a fluid medium, caused by relative bulk motion of the fluid rather than random thermal motion.[1] It causes a drag force to be exerted on the body. Ram pressure is given in tensor form as

([2],

where is the density of the fluid; is the momentum flux per second in the direction through a surface with normal in the direction. are the components of the fluid velocity in these directions. The total Cauchy stress tensor is the sum of this ram pressure and the isotropic thermal pressure (in the absence of viscosity).

In the simple case when the relative velocity is normal to the surface, and momentum is fully transferred to the object, the ram pressure becomes

.
  1. ^ Clarke, Cathie; Carswell, Bob (2007). Principles of astrophysical fluid dynamics. Cambridge University Press. p. 18. ISBN 978-0521853316.
  2. ^ Dowling, Timothy E.; Bradley, Mary E. (2023). "Ram pressure in astronomy and engineering". Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences. 479 (2270). Bibcode:2023RSPSA.47920504D. doi:10.1098/rspa.2022.0504.