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Stellar Evolution
Stellar Evolution

How Big Is the Solar System
How Big Is the Solar System

Sun, Earth, Moon
Sun, Earth, Moon

... Solar System memory game 15 min The children are going to play the memory game. This will teach them the differences between the Sun, Earth, and Moon. They will need this knowledge for the activity The Sun mobile. Before starting the game, encourage the children to look at all the cards from the mem ...
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0802c - Thephysicsteacher

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space-rocks - WLWV Staff Blogs

... • Comets are relatively small, fragile, irregularly shaped rocks, and often resemble asteroids in the sense that they are made from left over break offs from the solar system formation. Comets however are icy dirtballs that form in the outer solar system. The icy surface is embedded with dust, grit, ...
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... Our  journey  will  begin  by  observing  the  local  environment  around  the  University  of  Louisville  and  Kentucky   before  taking  a  virtual  spaceship  back  in  time.    We  will  fly  to  the  outermost  distances  of  sp ...
Astr604-Ch4
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The center of the Solar System: Heliocentric Model vs
The center of the Solar System: Heliocentric Model vs

... – States that the Earth is the center of all things and the Sun, moon and planets revolve around it – Works for the Sun and moon, – Sucks for the planets • Can’t explain: – Their changing brightness and – Retrograde motion: » Appear to stop and move backwards in the sky during the year ...
Research Essay “On the Origin of the Solar System”
Research Essay “On the Origin of the Solar System”

The Hidden Lives of Galaxies NSTA 2001
The Hidden Lives of Galaxies NSTA 2001

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... Wien's law is very useful for determining the surface temperatures of stars. It is not necessary to know how far away the star is, how large it is, or how much energy it radiates into space. All we need to know is the dominant wavelength of the star's electromagnetic radiation. The other useful form ...
Lesson 1 The Sun and Other Stars
Lesson 1 The Sun and Other Stars

... of the Sun? The Sun is a huge sphere made up mostly of two very light gases, hydrogen and helium. Hydrogen makes up about 71 percent of the Sun’s mass. Another 27 percent is made up of helium. Oxygen, carbon, and other gases make up the remaining 2 percent of the Sun’s mass. Most of the energy that ...
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An Introduction  - Solar Physics and Space Weather
An Introduction - Solar Physics and Space Weather

... •At t=10-6 second, the temperature in the universe dropped to the threshold temperature of 1013 K, at which the photons can not produce proton and anti-proton pairs (and neutron and antineutron pairs) •At about t = 1 second, temperature fell below 6 X 109 K, electrons and positions annihilated to fo ...
Astronomy 100  Name(s):
Astronomy 100 Name(s):

... In this exercise, you will construct (with welding rods and Styrofoam balls) a model of nearby space including 50 or so of the nearest stars. Of course, you will need information on where to place the stars accurately; you will need a coordinate system to specify the position of an object in space. ...
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The Masses and Lifetimes of Stars

... 1010 years. According to the mass-lifetime relation, a star with a mass of 10 Msun has a lifetime of: 1. 107 years 2. 3x107 years 3. 108 years 4. 3x108 years 5. 109 years 6. 1011 years 7. 3x1011 years ...
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... The only free parameter is number density of n and p. • Measured and calculated abundances are consistent. – 7Li is slightly off ...
EGU2017-12309 - CO Meeting Organizer
EGU2017-12309 - CO Meeting Organizer

... A weighting lysimeter has been constructed in the Hydraulic Laboratory of Politecnico di Milano. It consists of a steel box of 1.5 x 1.5 x 1 m containing reconstructed soil. The box is mounted on a scale with four load cells with a nominal weight of 6000 kg and a precision of 0,5 kg. The lysimeter i ...
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Standard solar model

The standard solar model (SSM) is a mathematical treatment of the Sun as a spherical ball of gas (in varying states of ionisation, with the hydrogen in the deep interior being a completely ionised plasma). This model, technically the spherically symmetric quasi-static model of a star, has stellar structure described by several differential equations derived from basic physical principles. The model is constrained by boundary conditions, namely the luminosity, radius, age and composition of the Sun, which are well determined. The age of the Sun cannot be measured directly; one way to estimate it is from the age of the oldest meteorites, and models of the evolution of the Solar System. The composition in the photosphere of the modern-day Sun, by mass, is 74.9% hydrogen and 23.8% helium. All heavier elements, called metals in astronomy, account for less than 2 percent of the mass. The SSM is used to test the validity of stellar evolution theory. In fact, the only way to determine the two free parameters of the stellar evolution model, the helium abundance and the mixing length parameter (used to model convection in the Sun), are to adjust the SSM to ""fit"" the observed Sun.
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