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Interstellar Exploration Stars beyond our imagination are fascinating with the information that they can provide. Experiments such as Voyager 1 and Voyager 2 are exploring outer space at this very moment, signaling information about interstellar exploration and the science behind it. Interstellar exploration is made up of many factors such as interstellar dust and the interstellar medium. Not many people are aware of the events that occur in outer space. The existing space between stars is composed of gases and dust. The formation of new stars cause excitement in emission lines that are in the gas of the clouds. These new stars emit light to surrounding clouds. Gases that exist in interstellar space are hydrogen and helium. …show more content…
Estimately 99% of the gas is composed of interstellar gas. Twenty five percent of interstellar medium is composed of interstellar gas, seventy five is the mass of the gas in the form of a new language. and twenty five percent is the formation of hydrogen. Neutral atoms, molecules, charged ions and charged electrons compose interstellar gas. Interstellar dust particles at small and are approximately the length of blue wavelengths, which are 450-495 nm (nanometer). These participles have no strict shape and are composed of ice, silicates, carbon and may contain iron compounds. Interstellar dust clouds have clumped together over a span of millions of years and this cloud is composed of many different elements and mixtures. Some of these clouds contain organic molecules. Clouds that are denser become stellar nuances and these stars will die. When these stars die, some will die more spontaneously than others and the stars will repeat the cycle of a star's life. At times, matter will become too sparse to pull together and the cycle will not be repeated during the expansion of the …show more content…
The more intense sunlight becomes; the closer the proximity to the sun the more pressure, the more a change in the atoms is visible. These positive charged atoms are not able to cross the magnetic field. Light is separated into wavelengths and black lines that continuously appear represent some of the light that is absorbed on its journey to us. This black line is able to express what is being exposed to scientists. Interstellar medium and solar wind have a relationship in which one is consistently trying to shove the other to the side. Depending on the proximity of the solar wind, if it is closer to the sun than its pressure is large and it is able to push away the interstellar medium. As its proximity decreases, interstellar medium is powerful enough to slow down the flow of solar wind from entering and being able to travel its surroundings. The increased pressure of interstellar space was first exposed in 2004 during the trip of Voyager 1. Plasma wave instruments are created to detect sounds in interstellar space. The instrument is able to sense waves of electrons in the

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