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STARS AND THE HR DIAGRAM
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STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

Dec 20, 2015

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Page 1: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

STARS AND THE HR DIAGRAM

Page 2: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM

STELLAR STRUCTURE CONTROLLED BY1. HYDROSTATIC EQUILIBRIUM – PRESSURE BALANCES GRAVITY AT EVERY LEVEL –P=nkBT – IDEAL GAS LAW2. ENERGY TRANSFER – HEAT GENERATED INSIDE ISTRANSPORTED AT THE SAME RATE OUTSIDE

a. Radiative transportb. Convective transportc. Heat conduction

3. ENERGY GENERATION – FUSION a. Efficiency 7x10-3 mc2

b. p-p cycle – ignition 5x106Kc. CNO cycle – ignition 2x107 K

Page 3: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 4: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 5: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 6: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 7: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 8: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

Stability of Stars• Reaction rate ~ T4 for proton-proton chain and T15 for CNO

chain

• If fusion rate speeds up for some reason would the star explode ?

• Thermal pressure increases Star expands till gravity balances thermal pressure ; Expansion lowers temperature reduces fusion rate pressure decreases Stars shrinkstemperature increases….

• Stability is always established between nuclear reaction rates and gravity compression.

• Similar if fusion rate slows down

• Cepheid variables

Page 9: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 10: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

HR DIAGRAM

Effective Temperature

Page 11: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

NEARBY STARS OR STARS IN A

CLUSTER

Page 12: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

Temperature, Size, Luminosity

L=4R2T4

AssumeR=constantAll stars have the size of the Sunbut some are hotterand some colder

Page 13: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

Test R=constant Hypothesis

If hypothesis OKall data onblue line

Hypothesis wrongBut..

We learned thatHotter are bigColder are small

Page 14: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

Mass-Luminosity Diagram

TheoryL~M3

Use this tolabel HRdiagram

Measure Mass of Star independently – How?

Page 15: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 16: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

• Stars have different masses• Stars with same mass have similar properties• The more massive a star the more luminous

Most important property in Star is Mass – composition a smaller factor

Page 17: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.

Conclusions• Stars spend most of their lifetime in main sequence• During their lifetime T and L almost constant

• Something else for birth and death

• More Mass• Hotter• More luminous• Bigger

t~M/L L~Mp p=3-4t~1/Mp-1 1/M2-3

Star with 5 solar masses has a lifetime 625 times smaller than Sun

Page 18: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.
Page 19: STARS AND THE HR DIAGRAM. STAR IS A LARGE SELF-LUMINOUS, GASEOUS SPHERE IN STEADY STATE EQULIBRIUM STELLAR STRUCTURE CONTROLLED BY 1.HYDROSTATIC EQUILIBRIUM.