Interstellar Gas
Interstellar gas refers to the gas and dust that exists in the space between stars in a galaxy. This gas is primarily composed of hydrogen and helium, with trace amounts of other elements. Interstellar gas is an important area of study in astronautical engineering as it plays a crucial role in the formation and evolution of stars and galaxies. The study of interstellar gas includes its distribution, composition, and physical properties such as temperature, density, and pressure. Astronautical engineers use various instruments and techniques such as telescopes, spectroscopy, and computer simulations to study interstellar gas and its effects on the surrounding environment. Understanding interstellar gas is also important for space exploration as it can affect spacecraft and their instruments.
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