'Fusion begins' presentation slideshows

How Stars Evolve

How Stars Evolve. Pressure and temperature Normal gases Degenerate gases The fate of the Sun Red giant phase Horizontal branch Asymptotic branch Planetary nebula White dwarf. Normal gas. Pressure is the force exerted by atoms in a gas Temperature is how fast atoms in a gas move.

886 views • 73 slides

How Stars Evolve

How Stars Evolve. Pressure and temperature Normal gases Degenerate gases The fate of the Sun Red giant phase Horizontal branch Asymptotic branch Planetary nebula White dwarf. Normal gas. Pressure is the force exerted by atoms in a gas Temperature is how fast atoms in a gas move.

771 views • 61 slides

Stars form from condensing clouds of gas & dust

550 views • 47 slides

Warm up

423 views • 35 slides

CH 25.5 Solar System Formation

CH 25.5 Solar System Formation . Objectives: How did our solar system form? What evidence supports our ideas?. http://atropos.as.arizona.edu/aiz/teaching/nats102/mario/solar_system.html. Nebular Theory. The solar system formed from a cloud of dust and gas (nebula). 4.6 billion years ago

274 views • 9 slides