I'd be pretty interesting to be able to study the effects of a planetoid sized object hurtling through a nebula at a speed great enough to affect the super-low density gaseous body. Especially if it was capable of causing a shockwave in such a body. Of course, thinking realistically, it would probably have to be traveling at near c to be able to impart enough kinetic energy into the surronding low-density matter to create a shockwave.
The average density of an interstellar molecular cloud is about 1000 to 1000000 atoms every cubic centi-meter. Other Inter Stellar Mediums have much lower densitys, but most of these are charged plasmas and so are far hotter than the 10 - 20 k of an IMC. [very close to absolute zero]
It should be noted that very, very little is understood of the properties of the Interstellar medium in general, especially how things such as large organic molecules can be made in the quantities they are at the low tempertures exhbited by the clouds.
It should also be noted that these clouds are rather large, varying from a light year to several thousand light years. Very. Very. Big.
Anywho, it'd be pretty damn interesting.


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