Title: The Death of the Sun!
1The Death of the Sun!
2Type of Death
- What a star becomes when it dies depends on the
mass left when all possible nuclear fuels are
exhausted and the star has lost some of its
original mass by ejecting it - M lt 1.4 M -----gt white dwarf/planetary nebulae
- 1.4 M ltM lt 3 M --gt neutron stars/pulsars
- M gt 3 M ----gt supernovae/black holes
3Stars like the Sun
- After a star like the sun exhausts its nuclear
fuels, it loses its outer layers as a "planetary
nebula" and leaves behind the remnant "white
dwarf" core. The white dwarfs are extremely small
stars -- they are the bare remnant cores of stars
after they have gone through all of their
lifetimes.
4Watch our sun die!
5Planetary Nebula
- Planetary nebulae were misnamed because of their
round shapes and greenish colors (caused by an
oxygen emission line) -- as in the bright central
part of the one to the right. They actually have
nothing to do with planets. A planetary nebula is
a shell of hot gas expanding away from a small,
very hot star (a white dwarf - you can just see
it near the center).
6- Planetary nebulae take many wonderful and
beautiful forms. However, they all are created
through similar processes. One step is when tiny
dust grains form near the surface of the star and
the pressure of the light photons on them expels
them, carrying some of the gas along.
7Here is a simulation of how it would look - the
diameter of the field is about 10 times the size
of the orbit
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10A very young planetary nebula. The optical image
shows shadowing by a disk, waves from pulsed mass
loss, and "searchlights" of light. The infrared
image on the right shows molecular hydrogen (red)
and the denser material that shapes the visible
searchlights.
11This animation shows the overall collapse of the
red giant accompanied by the ejection of material
that expends into the "Helix", a planetary nebula
(From NASA, STScI).
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13The sun will end its life as a white dwarf.
http//ircamera.as.arizona.edu/NatSci102/lectures/
whitedwrf.htm