Friday, September 19, 2025

TTS: Grade 9 Mini-Passages - Heavenly Bodies

Grade 9 Mini-Passages - Heavenly Bodies
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Grade 9 Mini-Passages — Heavenly Bodies

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🏠 Tchers' Den
Voice: selecting best available…

Lives of Stars

A star forms when gravity compresses a cold cloud of gas until the core grows hot enough for nuclear fusion. In the main sequence stage, hydrogen fuses into helium and the outward pressure of energy balances the inward pull of gravity. The star’s mass acts like a script: small stars burn fuel slowly and can shine for tens of billions of years, while massive stars live fast and die young. When the hydrogen thins, the core contracts and the outer layers swell into a red giant or supergiant. The ending depends on mass—some stars cast off their outer shells to reveal white dwarfs, and the most massive collapse and explode as supernovae, seeding space with heavy elements that future planets and life can use.

Comprehension Check

  1. What keeps a main sequence star in balance?
  2. Why do massive stars have shorter lifetimes than small stars?
Idle

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