'Radiative zone' presentation slideshows

The Sun

The Sun. Discussion. What does it mean to say the Sun is in hydrostatic equilibrium?. Discussion. What does it mean to say the Sun is in thermal equilibrium?. Discussion. How does the Sun maintain hydrostatic and thermal equilibrium?. Discussion.

786 views • 68 slides

GE 150 Astronomy

519 views • 42 slides

Clicker Question:

602 views • 35 slides

The Sun Chapter 16

The Sun Chapter 16. Key concepts: Energy production Stability. Basic data. Diameter 1.4 x 10 6 km = 109 D earth Mass 2 x 10 30 kg = 333,000 M earth Density 1400 kg/m 3 (160,000 kg/m 3 in center)

423 views • 33 slides

The Sun

417 views • 25 slides

Our star sol

331 views • 22 slides

Annoucements

Annoucements. Next test is in one week Review session will be next Wednesday Please hand-in or e-mail questions Practice test will be available by Monday. How Stars Evolve. Pressure and temperature Normal gases Degenerate gases Evolution of the Sun after the main sequence Red giant phase

340 views • 21 slides

Annoucements

Annoucements. Next test is in one week Review session will be next Wednesday Please hand-in or e-mail questions Practice test will be available by Monday. How Stars Evolve. Pressure and temperature Normal gases Degenerate gases Evolution of the Sun after the main sequence Red giant phase

212 views • 21 slides

The Sun

975 views • 18 slides

The Sun

The Sun. Layers of the Sun. The Core. Cannot be directly observed Theoretical studies of the energy it radiates Extremely hot, dense gas Plasma Density of 160,000 Kg/m3 Temperature of 1.5 x 10 7 Density + Temperature Nuclear Fusion EMR = gamma rays & particles.

467 views • 17 slides

With help from joy

7 F. With help from joy.

148 views • 8 slides