by randall cameron » Sun Apr 30, 2006 7:11 am
As I recall, in interstellar space they estimated something like a few hundred particles (atom/ions or molecules) of hydrogen and helium per cubic meter, and a few particles of dust, except in nebulae and other "cloud" structures. Intergalactic space is estimated to be even more of a void, with an average density for the known universe of around one atom per cubic meter.
Of course this changes dramatically in close proximity to stars or other bodies, thus the ability to use solar sails to drive interplanetary probes where energy economy is more important than acceleration.
Maybe not a strict vacuum, but close enough for most purposes, i.e., not a lot of drag or pressure below cosmic scales.
Randall
As I recall, in interstellar space they estimated something like a few hundred particles (atom/ions or molecules) of hydrogen and helium per cubic meter, and a few particles of dust, except in nebulae and other "cloud" structures. Intergalactic space is estimated to be even more of a void, with an average density for the known universe of around one atom per cubic meter.
Of course this changes dramatically in close proximity to stars or other bodies, thus the ability to use solar sails to drive interplanetary probes where energy economy is more important than acceleration.
Maybe not a strict vacuum, but close enough for most purposes, i.e., not a lot of drag or pressure below cosmic scales.
Randall