1 / 10

Recap: Death of Stars: Low and Medium Mass

Life Cycle of Stars. Recap: Death of Stars: Low and Medium Mass. Low Mass. Main Sequence Star. Red Dwarf. Medium Mass. Red Giant. Planetary Nebula. White Dwarf. Black Dwarf ??. Life Cycle of Stars. Death of Stars: High Mass. Main Sequence Star. Red Super Giant. Supernova.

Télécharger la présentation

Recap: Death of Stars: Low and Medium Mass

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Life Cycle of Stars • Recap: Death of Stars: Low and Medium Mass Low Mass Main Sequence Star Red Dwarf Medium Mass Red Giant Planetary Nebula White Dwarf Black Dwarf ??

  2. Life Cycle of Stars • Death of Stars: High Mass Main Sequence Star Red Super Giant Supernova Neutron Star Black Hole

  3. Life Cycle of Stars • Recap: High Mass Stars: • Core size greater than 1.4x our sun • Create high mass elements such as iron • Neutron Star • Formed if remaining star is 1.4-3x sun’s mass. • Black Holes • Formed if remaining star > 3x sun’s mass Recap Video

  4. Death of Stars: • What stars end up as depend on mass • Low and Medium mass stars • Planetary nebula --------- white dwarf • High mass stars • Supernova --------- neutron star or black hole

  5. What about our Sun? • As fusion begins to slow down, the core of the sun will contract • Temperature in the core will rise • The outer layers of the sun will expand, consuming the inner planets • Sun will become a Red Giant

  6. Click ME! Video Link

  7. Core of the sun will begin to fuse helium into larger elements such as carbon and oxygen • Continuing over the next 100 million years… • Core will become entirely carbon and oxygen • Core will contract • Outer layers will expand • Outer layers will form a planetary nebula • Core of sun will become a white dwarf

  8. What about our solar system? How did it start?

  9. Gravity, gas pressure, magnetic fields, and rotation cause disk to form around protostar. Conservation of angular momentum! 

More Related