The Lives of Stars

Written by Studio AM.

A star is not eternal; it is born, lives, and dies over spans that dwarf human history. Stars begin within vast clouds of gas and dust drifting through space. Gravity slowly pulls a clump of this material inward, and as the clump shrinks it grows denser and hotter. When the core becomes hot enough, hydrogen nuclei begin fusing to form helium, releasing enormous energy and igniting the star.

For most of its life a star maintains a steady balance: the outward push of this fusion energy resists the inward crush of gravity. When hydrogen fuel in the core runs low, that balance breaks, and the star's fate depends on its mass.

A modest star like the Sun swells into a red giant, sheds its outer layers, and leaves a hot core called a white dwarf, which gradually cools. A far more massive star can collapse and explode as a supernova, sometimes briefly shining as brightly as a galaxy. Other massive stars may collapse with little visible explosion. The debris of such explosions scatters heavy elements across space. Gathered by gravity over billions of years, that scattered debris becomes the raw material for new clouds, new stars, and the planets that circle them.

Remarkably, the carbon in living bodies and the iron in blood were forged inside ancient stars, and later spread into the material from which our solar system formed. Many elements in living cells therefore connect the history of life on Earth with earlier generations of stars.

Questions

Choose an answer. The explanation appears after you answer.

  1. Question 1 of 4

    Which factor does the passage emphasize in explaining a star’s eventual fate?

  2. Question 2 of 4

    What keeps a star in a steady balance for most of its life?

  3. Question 3 of 4

    As used in the passage, 'forged' most nearly means

  4. Question 4 of 4

    Which statement best expresses the central idea of the passage?

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