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Stellar Evolution. NGC 3603 Bok globules and giant gaseous pillars (evidence of embryonic stars), circumstellar disks around young stars progressing to.

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Presentation on theme: "Stellar Evolution. NGC 3603 Bok globules and giant gaseous pillars (evidence of embryonic stars), circumstellar disks around young stars progressing to."— Presentation transcript:

1 Stellar Evolution

2 NGC 3603 Bok globules and giant gaseous pillars (evidence of embryonic stars), circumstellar disks around young stars progressing to aging, massive stars in a young starburst cluster blue super-giant with its ring and bipolar outflow marks the end of the life cycle.

3 STAGE ONE u Stars begin as a NEBULA - a dark cloud of gas and dust u Made mostly of hydrogen and helium with small amounts of heavier elements Eagle Nebula M16

4 Horse Head Nebula

5 Veil NebulaTrifid Nebula

6 Thackeray's Globules in IC 2944

7 Omega or Swan Nebula

8 Ghost Head Nebula

9 u The nebula begins to contract and gravitational attraction increases u It continues shrinking and starts to spin. u Eventually it forms a flat disk with a PROTOSTAR in the middle

10 Planetary Disks Forming

11 STAGE TWO - Main Sequence u Longest part u Energy is produced as fusion take place in the core of the star u The energy from fusion balances the force of gravity and makes it a very stable stage

12 Stage Three u Happens when almost all of the hydrogen atoms have fused into helium atoms u The core contracts due to the force of gravity u This increases the temp and causes the helium to fuse into carbon u This gives off a lot of energy and the star swells up to a giant or supergiant star

13 Stage Four u Helium fusion ends u The star loses its outer gases and reveals a core u An expanding shell of gases shed by this dying star forms a PLANETARY NEBULA

14 Ant Nebula

15 Helix Nebula

16 Stingray nebula (Hen-1357), the youngest known planetary nebula.

17 The "Spirograph" Nebula

18 Cat’s Eye Nebula

19 u The star collapses inward and forms a hot dense core of matter called a WHITE DWARF u Some white dwarfs may explode into a NOVA while they are cooling

20 What about really BIG stars?? u Stars with masses 10 - 100 times greater than the sun can produce a huge explosion called a SUPERNOVA SN1987A

21 What happens after the explosion? u The core may contract into a very small, dense ball of neutrons called a NEUTRON STAR – u If it rotates it is called a PULSAR

22 u Really large stars contract with greater force and become a BLACK HOLE

23 Centaurus A (Hidden Black Hole)

24 Classifying Stars Hertzsprung-Russell (HR) Diagram Plots temp. v. luminosity Most stars are main sequence

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