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The sun shines by acting as a colossal natural nuclear reactor, and its primary fuel is the simplest and most abundant element in the universe. This element makes up roughly 75% of the sun's mass. Stars are born from immense, collapsing clouds of interstellar (Review) gas and dust, and these clouds are overwhelmingly composed of this light gas, providing the raw material for star formation.
Inside the sun's incredibly hot and dense core, the force of gravity is so strong that it smashes these atoms together. This process, known as nuclear fusion, forces them to combine and form the next-lightest element, helium. This is why helium makes up nearly all of the remaining 25% of the sun's mass. This constant conversion process releases the tremendous amount of energy that radiates out into the solar system as light and heat, making life on Earth possible.
All of the heavier elements we are familiar with, such as oxygen, carbon, and iron, account for less than 2% of the sun’s total mass. For over 4.5 billion years, our star has been steadily burning through its massive fuel supply, and it has enough to continue shining for another five billion years before its life cycle begins to change.
More Science Trivia Questions
What colorful marine invertebrate is known for its ability to split light into rainbow patterns and is popular in reef tanks?
70What famous catalog of deep-sky objects, compiled by a French astronomer in the 1700s, contains 110 entries?
69What type of coral does not rely on photosynthetic algae and must be fed directly?
61What is the approximate diameter of the largest known star, UY Scuti, compared to our Sun?
59What phenomenon causes stars to appear to twinkle when viewed from Earth's surface?
56What type of filtration uses live rock and sand beds to naturally process waste in a marine aquarium?