'Triple alpha process' presentation slideshows

Advances in contemporary physics and astronomy --- our current understanding of the Universe

Advances in contemporary physics and astronomy --- our current understanding of the Universe. Lecture 6: Evolution of Universe after the First Three Minutes. May 7 th , 2003. The Epoch of Recombination. At t=300,000 years, T=3000 K: Electrons & nuclei combine into neutral atoms:

522 views • 36 slides

Stellar Evolution: After the Main Sequence

Stellar Evolution: After the Main Sequence. Chapter Twenty-One. Guiding Questions. How will our Sun change over the next few billion years? Why are red giants larger than main-sequence stars? Do all stars evolve into red giants at the same rate?

684 views • 35 slides

Stellar Evolution (of sun-like stars)

Stellar Evolution (of sun-like stars). How do stars age & die?. The Main Factor. The evolution of any star is controlled by its mass . Mass controls gravity. Gravity controls density. Density controls how fast the star uses up its available fuel.

554 views • 35 slides

Stellar Evolution

486 views • 31 slides

Announcements: -Public Viewing THIS Friday Evergreen Valley College evc

Announcements: -Public Viewing THIS Friday Evergreen Valley College http://www.evc.edu 7PM-10:30 check website for weather information maps available online Pick up copy of handout: required for credit!! Homework #9 due today Exam #3: May 3 (Chp 12, 13). Chapter 13.

412 views • 28 slides