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What distinguishes Jupiter from being classified as a star or a brown dwarf?

Although the most massive planet in our solar system, Jupiter does not contain enough material to ignite fusion.

Jupiter, despite being 318 times more massive than Earth, would require 80 times more mass for its core to reach the necessary temperature for sustaining thermonuclear fusion. This process involves the conversion of four hydrogen atoms into helium, accompanied by the release of energy. It is through fusion that stars are able to emit light and heat.

Similarly, brown dwarfs lack the necessary mass to sustain fusion. These objects, often referred to as “failed stars,” are formed solely from interstellar gas. In contrast, planets are formed from the remnants of a disk composed of dust and gas that accumulates around a star during the process of matter accretion. It is currently uncertain whether these two categories, brown dwarfs and planets, can overlap.

Brown dwarfs are considered “failed stars” whose masses span the range between the lowest-mass stars and the highest-mass planets. Credit: NASA’s Goddard Space Flight Center

James B. Kaler

University of Illinois at Urbana-Champaign

Furthermore, it should be noted that the International Astronomical Union currently designates the demarcation point between brown dwarfs and planets at 13 times the mass of Jupiter. This specific threshold represents the minimum mass necessary for the initiation of deuterium fusion, with deuterium being an isotope of hydrogen.

This article is republished from astronomy.com under a Creative Commons license. Read the original article.

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