The Sun: A Nuclear Powerhouse

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Vocabulary flashcards based on the lecture notes about the Sun and its energy production.

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18 Terms

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Hydrostatic Equilibrium

The balance between the outward pressure of gases in a star and the inward gravitational force acting on it.

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Proton-Proton Chain

A series of thermonuclear reactions by which hydrogen nuclei are fused to form helium, releasing energy in the process.

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Nuclear Fusion

The process of combining lighter atomic nuclei into heavier ones, releasing energy.

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Neutrinos

Fundamental particles with no charge and very little mass that interact weakly with matter; produced in nuclear fusion in the Sun.

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Mass-Energy Equivalence

The principle that mass can be converted into energy, described by the equation E=mc².

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CNO Cycle

A set of fusion processes in stars where carbon, nitrogen, and oxygen isotopes act as catalysts to fuse hydrogen into helium.

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Helioseismology

The study of the sun’s pulsations to infer the characteristics of its interior.

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Luminosity

The total amount of energy radiated by the Sun per second.

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Binding Energy

The energy released when particles come together to form a nucleus; related to mass defect.

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Conduction

The transfer of heat through a substance by direct contact.

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Convection

The movement within a fluid where hotter, less dense material rises and cooler, denser material sinks.

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Fission

The splitting of heavy atomic nuclei into lighter ones, releasing energy.

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Photons

Quantum particles of light that carry energy and are emitted during nuclear reactions.

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Gravitational Contraction

The process by which a star generates energy as its mass contracts under its own gravity.

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Electromagnetic Radiation

Energy emitted in the form of photons, including visible light, gamma rays, and X-rays.

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Positron

The antimatter counterpart of an electron, with the same mass but a positive charge.

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Solar Interior

The internal structure of the Sun, where nuclear fusion occurs and energy is generated.

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Joule

The unit of energy equal to the work done when a force of one newton is applied over a distance of one meter.