Outer space
Main article: Outer space
Outer
space is not a perfect vacuum, but a tenuous plasma awash with charged
particles, electromagnetic fields, and the occasional star.
Outer space has very low density and pressure, and is the closest physical
approximation of a perfect vacuum. It has effectively no friction, allowing
stars, planets and moons to move freely along ideal gravitational trajectories.
But no vacuum is truly perfect, not even in interstellar space, where there are
still a few hydrogen atoms per cubic centimetre.[citation needed]
Stars, planets and moons keep their atmospheres by gravitational attraction,
and as such, atmospheres have no clearly delineated boundary: the density of
atmospheric gas simply decreases with distance from the object. The Earth's
atmospheric pressure drops to about 1 Pa (10−3 Torr) at 100 km of
altitude, the Kármán line which is a common definition of the boundary with
outer space. Beyond this line, isotropic gas pressure rapidly becomes
insignificant when compared to radiation pressure from the sun and the dynamic
pressure of the solar wind, so the definition of pressure becomes difficult to
interpret. The thermosphere in this range has large gradients of pressure,
temperature and composition, and varies greatly due to space weather.
Astrophysicists prefer to use number density to describe these environments, in
units of particles per cubic centimetre.
But although it meets the definition of outer space, the atmospheric density
within the first few hundred kilometers above the Kármán line is still
sufficient to produce significant drag on satellites. Most artificial satellites
operate in this region called low earth orbit and must fire their engines every
few days to maintain orbit. The drag here is low enough that it could
theoretically be overcome by radiation pressure on solar sails, a proposed
propulsion system for interplanetary travel. Planets are too massive for their
trajectories to be affected by these forces, although their atmospheres are
eroded by the solar winds.
All of the observable universe is filled with large numbers of photons, the
so-called cosmic background radiation, and quite likely a correspondingly large
number of neutrinos. The current temperature of this radiation is about 3 K, or
-270 degrees Celsius or -454 degrees Fahrenheit.