Skip to content
Lord Sterling
Space

The Sun balances inward gravity and outward pressure

Archive 01431

Slide 1

Pressure supports the Sun against inward gravity

The Sun is made mainly of hot plasma, gas containing charged particles. Gravity pulls inward. Pressure increasing toward the centre provides outward support.

More to Read

Plasma contains freely moving charged particles. The Sun’s visible surface is therefore not a solid crust: it is the layer from which much of the light we observe escapes.

Slide 2

Deeper pressure supports the material above

Pressure increases toward the solar interior. Each layer must support the weight of material farther out while responding to the gravity acting on it.

More to Read

The balance is called hydrostatic equilibrium. It describes opposing influences within the star, not an absence of motion in the material or an assertion that the Sun never changes.

Slide 3

Core fusion supplies energy to maintain the hot interior

Nuclear fusion in the core releases energy that eventually escapes from the surface. This energy source helps maintain the hot interior.

More to Read

Fusion is concentrated where temperature and density make reactions sufficiently likely. The visible surface is far cooler than the core, so observing sunlight does not mean looking directly at the reaction region.

Slide 4

Radiation and moving plasma carry energy outward

Radiation carries energy through much of the interior. In the outer convection zone, moving plasma also transports energy toward the surface.

More to Read

Convection involves warmer material rising and cooler material sinking. The pattern of granules visible on the Sun reflects this churning near the surface rather than a fixed arrangement of solid features.

Slide 5

Changing core conditions eventually change the star

The Sun’s present structure depends on its composition and energy production. Changes in the core eventually alter the balance and the star’s size.

More to Read

A stable star is not an object with an unlimited fuel supply. Stellar evolution studies how gradual internal changes lead to new structures even when the star appears nearly constant over a human lifetime.

Sources

Join Lord Sterling to explore your personal Discover feed and preserve what interests you.