Introduction to Stars
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Introduction to Stars
Star briefing
Stars are enormous spheres of hot plasma held together by gravity. Most are made mainly of hydrogen and helium. Deep in a star’s core, pressure and temperature are so high that nuclear fusion can occur. In the Sun and other stars like it, hydrogen nuclei combine through a series of reactions that ultimately produce helium. A small amount of mass is converted into energy, which travels outward and is emitted as light and other forms of radiation. A star’s luminosity is the total energy it emits each second. It is not the same as how bright the star appears from Earth: distance also affects apparent brightness. Stars change over time, and their paths depend strongly on their initial mass. Elements heavier than helium are formed through stellar processes and are spread into space by stellar winds and, for some stars, explosive events. Later generations of stars and planets can form from this enriched material.
Decode the star
Use the briefing to answer.
- A solid ball of rock that reflects nearby light
- A sphere of hot plasma held together by gravity that emits energy
- A planet that shines because it orbits a star
- A cloud of cold gas with no internal energy source
- Luminosity
- Fusion
- Plasma
- Gravity
- Process in which atomic nuclei combine
- Attractive force that helps hold a star together
- Hot matter made of charged particles
- Total energy emitted by a star each second
- The farther star appears dimmer
- The farther star appears brighter
- They must appear equally bright
- Distance cannot affect apparent brightness
Evidence and consequences
Apply the ideas to the star team's investigation.
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