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Solar winds composed of free protons, electrons, and a particles bombard Earth constantly, knocking gas molecules out of the atmosphere. In this way, Earth loses about 3.0 kg of matter per second. It is estimated that the atmosphere will be gone in about 50 billion years. Use this estimate to calculate (b) the amount (mol) of nitrogen, which makes up 75.5 mass % of the atmosphere.

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Solar wind is composed of charged particles and the sun's magnetic field and is continually released from our star.

What is Solar wind?

The solar wind travels at speeds of 250–750 km/s and is supersonic, which means it travels faster than the fast magnetosonic wave, at a distance of more than a few solar radii from the Sun. At the termination shock, the solar wind's movement is no longer supersonic. The aurora, also known as the northern and southern lights, comet plasma tails, which are always pointed away from the Sun, and geomagnetic storms, which can shift the direction of magnetic field lines, are further occurrences in this category.

Over time and across solar latitude and longitude, the solar wind fluctuates in density, warmth, and speed.

To learn more about Solar wind from the given link:

brainly.com/question/10258008

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