Hydrogen with some helium. However, trance amounts of other materials are seldom found in the interstellar regions of space like water, ammonia, methane, etc. And we are talking in terms of parts per trillion if not more.
Mainly hydrogen - which is currently the most abundant element in the Universe.
The interstellar medium is all the matter that exists between the stars in a galaxy. It mainly consists of gas (99%), with about 75% of this gas being in the form of molecular or atomic hydrogen, and about 25% in the form of helium. The other 1% is in the form of dust. The density of the interstellar medium is also very small: about 1 atom per cubic centimetre.There are two main types of interstellar mediums:Cold clouds of neutral atomic or molecular hydrogen, which are the raw materials wherein stars can be formed if it becomes gravitationally unstable and collapses.Hot ionized hydrogen near hot young stars.
A protostar forms when gravity pulls the dust and gases in a nebula together.
Nebulas are interstellar clouds made of dust and gases and a pulsar is a kind of star. A pulsar is formed inside of a nebula, therefore a scientist could conclude that without a nebula a pulsar could not exist.
Scientists concluded that the atom consists of mostly empty space.
the gravitational force
An interstellar cloud.
An interstellar cloud made of gas, dust, and plasma in a galaxy.
Interstellar gas and dust.
A nebula is what it is. :)
These are generically referred to as, not surprisingly; 'interstellar clouds'
solar nebula
New stars form from the interstellar gas and dust; mainly hydrogen and helium.
Interstellar dust
Cosmic dust, asteroidal dust, intergalactic dust, interstellar dust, comet dust, circumplanetary dust ~ it really depends on its astronomical location.
It is from interstellar gas and dust that we all came. The stars, planets, asteroids, and comets all came from clouds of gas and dust. As far as OUR gas and dust NOW, nothing much is produced. Its mostly all used up in the making of us.
A galaxy is a massive, gravitationally boundsystem that consists of stars and stellar remnants, an interstellar medium of gas and dust, and an important but poorly understood component tentatively dubbed dark matter.
If you're referring to the space between solar systems: lots. Rocks and planetoids wander; radiation is absorbed and produced; space stretches; Von Neumann probes originating from long-extinct civilisations slowly make their way towards our solar system to convert it to rubble - you name it, it's bound to be out there somewhere.