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Chapter 23 Vocabulary
Chapter 23 Vocabulary

... 2. inner planets- the four solid, rocky planets closest to the sun; Mercury, Venus, Earth, and Mars 3. Mars- in our solar system, the fourth planet from the sun 4. Jupiter- in our solar system, the fifth planet from the sun; largest planet, mostly gas and liquid 5. comet- moss of frozen gasses and r ...
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SL2 IIIC Carter 280911 - Particle Solids Interactions group

Chapter15 notes[1]
Chapter15 notes[1]

Parent Activity - The School District of Palm Beach County
Parent Activity - The School District of Palm Beach County

... Our solar system includes the sun, eight planets and their moons, comets, large Information space rocks called asteroids, and small space rocks called meteoroids. Beyond our solar system are stars and groups of stars called galaxies. The Earth is the third planet from the sun creating the perfect en ...
What is a Star? - Yale Astronomy
What is a Star? - Yale Astronomy

•TODAY •Chapter 5/10: The Sun Required: Sec. 1
•TODAY •Chapter 5/10: The Sun Required: Sec. 1

... Chemical reactions (like fire, metabolism) involve an atom’s electrons. Eg. 2 H2 + O2 = 2 H2O Nuclear reactions involve an atom’s nucleus.... They are much more powerful. They create new elements! All of the Sun’s energy comes from nuclear reactions. (so the Sun is not “on fire”) Since the Sun is mo ...
The Death of Stars - Mounds Park Academy Blogs
The Death of Stars - Mounds Park Academy Blogs

... White Dwarfs • Stars less than 1.4 times the mass of the sun continue to shrink. • Our Sun will shrink until it becomes the size of the earth. ...
Stars PowerPoint Slides
Stars PowerPoint Slides

Inverse Square Law, Blackbody Radiation y
Inverse Square Law, Blackbody Radiation y

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The death of a star

... I will answer it by the following shortened version of the life of a star such as our Sun after it has reached the 'normal' star state. As far as expansion and contraction are concerned it all depends which part of the stellar cycle you are interested in. Both occur between the 'normal' state and th ...
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Lecture 18

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Star in a Box

... •Luminosity up the vertical axis (measured relative to the Sun) •Temperature along the horizontal axis (measured in Kelvin) The stars Vega and Sirius are brighter than the Sun, and also hotter. Where would you put them? Where would you mark the Sun on the plot? ...
Solar System (Ch. 7)
Solar System (Ch. 7)

... What is the source of the sun’s energy? ...
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Solar_System_handout

... *Uranus has an unusual rotation as well, and rotates 90 degrees on its side. This is also due, probably, to an impact early in the formation process. ...
The Formation of the Solar System
The Formation of the Solar System

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... around the sun, it will have actually rotated one degree too much in its 23 hr, 56 min sidereal day. Hence, the solar day would be 23 hrs, 52 min, or 4 minutes shorter (instead of 4 minutes longer, as it is currently). 2. Defend or oppose the claim that “a theory in science is really just a guess.” ...
2011-01-17 SNC1D Space Review
2011-01-17 SNC1D Space Review

... Describe at least 3 key differences between the inner planets and outer planets of our solar system. Determine the component of our solar system that is being discussed in each of the statements. more mass that all the other planets combined closest to the Sun its atmosphere contains oxygen It is no ...
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Which of the following statements is TRUE

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Milky Way Galaxy

... hydrogen atoms and one oxygen atom. • Each H atom weighs 1.7 x 10-24 g. & has a radius of 1.2 Å ...
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Science Centre Talk

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The Sun The Sun

... light travels incredibly fast. When we see the Sun, we’re really seeing what it looked like 8 minutes ago. How Hot Is the Sun? The temperature of the Sun can reach 5,500ºC (10,000ºF) on the surface and more than 15.5 million ºC (28 million ºF) at the core. What Is the Sun Made Of? Made of scorching ...
The Sun`s Energy Supply (PowerPoint version)
The Sun`s Energy Supply (PowerPoint version)

... Consider a dime, with a mass of 2.3 grams. (Or equivalently, simply pick up a pebble of that mass!) E = m c 2 tells us that this lump could (in principle) be converted to 2 x 10 14 Joules of energy. That would be enough to supply the complete energy needs of a city of a couple of million people -- f ...
The Sun`s Energy Supply (PDF version)
The Sun`s Energy Supply (PDF version)

Physics Earth and the Solar system revision
Physics Earth and the Solar system revision

... Note: Venus is the hottest planet due to extreme global warming. Neptune is the coldest as it is furthest away, it also has a very long year due to it taking the longest to orbit the Sun. Earth • The Earth spins on its own axis in 24 hours (1 day). This causes the Earth to have day and night. • The ...
Why the sun is important too!
Why the sun is important too!

... feeling happier and more energized. Sunlight also stimulates the pineal gland deep in the brain. This gland regulates our sleep/wake cycle and triggers our bodies for activity or restful sleep. 4. Warmth Life on this planet would not be possible without the warmth that the sun provides. Mercury and ...
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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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