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Are These Stars? 1 2 3 4. Definition of a Star (1) Bound by self gravity (spherical) (1) Bound by self gravity (spherical) Is this strictly true? (2)

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Presentation on theme: "Are These Stars? 1 2 3 4. Definition of a Star (1) Bound by self gravity (spherical) (1) Bound by self gravity (spherical) Is this strictly true? (2)"— Presentation transcript:

1 Are These Stars? 1 2 3 4

2 Definition of a Star (1) Bound by self gravity (spherical) (1) Bound by self gravity (spherical) Is this strictly true? (2) Radiates energy largely supplied by an internal source (2) Radiates energy largely supplied by an internal source A star is a body that satisfies two conditions: Source of radiation is usually nuclear energy released by FUSION reactions in stellar interior but could be gravitational potential energy released in contraction

3 Are These Stars?

4 No, this is a collection of stars  Galaxy

5 Are These Stars?  Galaxy No, not bound by gravity, not spherical Nebula

6 Are These Stars?  No, shines by reflected light, mass too small for gravity to be important Galaxy Nebula Comet

7 Are These Stars?  Galaxy No, largely shines by reflected light Nebula Comet Planet

8 Consequences of Definition of a Star Stars must evolve (as they release energy) - changes in structure and/or chemical composition Death of a star can occur in 2 ways (a) Violation of first condition - self gravity (breakup of star scattering material into space) (b) Violation second condition - internally supplied radiation (exhaustion nuclear fuel)

9 Astrophysics (physics of stars) Is not an experimental science - we cannot devise and conduct experiments in order to test theories Theory is validated by observations Evidence often derived from past events Information we can gather is very restricted - apparent brightness (depends on distance), luminosity, temperature, chemical composition, mass, radius

10 The Constellation Orion The Constellation Orion

11 Spectrum Arcturus Spectrum Arcturus

12 Binary Stars Binary Stars

13 A Problem The Earth’s mean distance from the Sun is 1.496 x 10 11 m, and its orbital period is 3.156 x 10 7 sec. In these units G is 6.673 x 10 -11 m 3 kg -1 s -2 Use this to derive the mass of the Sun in kg.

14 Binary Stars and Radii Binary Stars and Radii

15 Why should I care about stellar astrophysics? We live next to a star. It controls most of what happens on Earth For example: HAS THE SUN CAUSED GLOBAL WARMING?

16 Sun and Earth


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