Astronomy: The Sun, Our Star Flashcards
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Questions and Answers

What is the surface temperature of the sun and its central temperature?

The surface temperature of the sun is 5800K and its central temperature is 15 million kelvin.

What class of star is the sun?

The sun is a G2V star.

What elements is the sun comprised of?

91.2% Hydrogen, 8.7% Helium, 0.1% other.

How many times bigger is the sun than the earth?

<p>The sun is 109 times bigger than the radius of the Earth.</p> Signup and view all the answers

What is hydrostatic equilibrium?

<p>The outward pressure force balances the inward gravitational force everywhere inside the sun.</p> Signup and view all the answers

What is the force that keeps stars together inward?

<p>Gravity.</p> Signup and view all the answers

What is the force that keeps the sun from collapsing on itself?

<p>Pressure force.</p> Signup and view all the answers

What is the job of a star?

<p>To make energy and move it to the surface and then out to space.</p> Signup and view all the answers

For the sun's interior, what are the three ways that the sun moves energy out of its core?

<p>Thermonuclear core, radiative zone, convective zone.</p> Signup and view all the answers

What is the job of the thermonuclear core?

<p>This is the central region of the sun where fusion takes place due to high temperatures and pressure.</p> Signup and view all the answers

What is the radiative zone?

<p>A region inside the star where energy is transported outward by the movement of photons.</p> Signup and view all the answers

Do all small stars have a radiative zone?

<p>False</p> Signup and view all the answers

What is the convection zone?

<p>A layer inside a star where energy is transported outward by means of heat flow through the gases of the star.</p> Signup and view all the answers

What is the order of really big stars to moving energy out of its core?

<p>Some big stars start with the thermonuclear core, then the convection, and then radiation.</p> Signup and view all the answers

What is helioseismology?

<p>It is the way we can see into the sun's inner core, like a seismic motion going through the sun.</p> Signup and view all the answers

How can we use the Doppler effect to look at a star?

<p>We can see the red and blue shift of gases on the star's surface.</p> Signup and view all the answers

What makes the sun shine?

<p>Thermonuclear fusion at the sun's core is the source of the sun's energy.</p> Signup and view all the answers

Do stars use fusion or fission?

<p>False</p> Signup and view all the answers

What is fission?

<p>Fission is taking one large atom and breaking it apart and it releases energy.</p> Signup and view all the answers

What is fusion?

<p>Fusion is taking two small molecules and smashing them together and that creates energy.</p> Signup and view all the answers

Why do stars use fusion and not fission?

<p>Stars are mostly made of hydrogen which is a small atom, so it uses fusion.</p> Signup and view all the answers

What is the output of all the energy stars make?

<p>The main part is 4 hydrogen atoms put together to make 1 helium atom.</p> Signup and view all the answers

What is a positron?

<p>An electron with a positive charge.</p> Signup and view all the answers

What type of chain do smaller stars use to make their energy?

<p>Proton-proton chain.</p> Signup and view all the answers

What type of chain or cycle do bigger stars use to make their energy?

<p>They use the 6 step cycle which is the CNO cycle.</p> Signup and view all the answers

Is the CNO part of the cycle ever actually used up or consumed?

<p>False</p> Signup and view all the answers

Can energy be created or destroyed?

<p>False</p> Signup and view all the answers

Study Notes

The Sun: Key Facts

  • Surface temperature of the Sun: 5800K; central temperature: 15 million K.
  • Classified as a G2V star, indicating it's an average star compared to others.
  • Composition: 91.2% Hydrogen, 8.7% Helium, and 0.1% other elements.

Size and Scale

  • Radius of the Sun: 109 times that of Earth, categorizing it as an average-sized star.
  • Hydrostatic equilibrium: Outward pressure balances inward gravitational force, maintaining stability.

Forces at Play

  • Gravity is the inward force that keeps stars together.
  • Pressure force counteracts gravitational collapse, preventing the Sun from collapsing.

Energy Production

  • The Sun’s primary function is to generate energy and radiate it into space.
  • Energy moves from the core through three regions:
    • Thermonuclear core (where fusion occurs).
    • Radiative zone (energy is transported by photon movement).
    • Convective zone (energy is transported via convection).

Energy Transport Mechanisms

  • In the thermonuclear core, fusion happens due to high temperatures and pressures.
  • The radiative zone allows photons to bounce around before reaching the surface.
  • Smaller stars might lack a radiative zone, relying solely on a thermonuclear core and convection.
  • Larger stars may utilize a combination of thermonuclear core, convection, and radiation for energy transport.

Helioseismology and Doppler Effect

  • Helioseismology analyzes seismic motions to study the Sun’s interior structure.
  • Doppler effect allows observation of red and blue shifts of gases to deduce star motion and energy output.

Fusion vs. Fission

  • Stars utilize nuclear fusion, combining small atoms (like hydrogen) to release energy.
  • Fission involves splitting large atoms and is not a process used by stars.
  • Output of energy from fusion: 4 hydrogen atoms fuse to create 1 helium atom, producing energy in various light forms, along with positrons and neutrinos.

Reaction Chains

  • Smaller stars use the proton-proton chain (4 H to 1 He) for energy production.
  • Larger stars utilize the CNO cycle, a six-step process reliant on catalysts that are not consumed in the reaction.

Conservation of Energy

  • Energy cannot be created or destroyed but can change forms.

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Test your knowledge about our celestial star, the Sun, with these flashcards. Learn about its surface temperature, classification as a G2V star, and its elemental composition. Ideal for astronomy enthusiasts looking to enhance their understanding of stellar properties.

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