Unit 3 Bell Ringers 1. Early historical models of the solar system
... 5. Which statement describes the temperature of Jupiter? A. All of Jupiter is very cold. B. The center of the planet is extremely hot. C. Its temperature depends only on the energy it gets from the sun. D. The upper layers of the atmosphere are the hottest part of the planet. 6. In which of the fol ...
... 5. Which statement describes the temperature of Jupiter? A. All of Jupiter is very cold. B. The center of the planet is extremely hot. C. Its temperature depends only on the energy it gets from the sun. D. The upper layers of the atmosphere are the hottest part of the planet. 6. In which of the fol ...
Topics on the Sun and the Life
... • All life on Earth is based on carbonbased compounds, called organic molecules • These organic molecules occur naturally in the interstellar clouds of gas and dust, called nebula, throughout galaxies ...
... • All life on Earth is based on carbonbased compounds, called organic molecules • These organic molecules occur naturally in the interstellar clouds of gas and dust, called nebula, throughout galaxies ...
Solar System Scale
... visualize and scale models are usually distorted in textbooks so that they will fit on the page. Materials: meter sticks, 400 cm heavy string for each group, masking tape Procedures: Ask students to draw a picture of what they think the solar system looks like. This will help them get focused on the ...
... visualize and scale models are usually distorted in textbooks so that they will fit on the page. Materials: meter sticks, 400 cm heavy string for each group, masking tape Procedures: Ask students to draw a picture of what they think the solar system looks like. This will help them get focused on the ...
Link to Unit 9
... SC.8.E.5.4 Explore the Law of Universal Gravitation by explaining the role that gravity plays in the formation of planets, stars, and solar systems and in determining their motions. SC.8.E.5.7 (AA) Compare and contrast the properties of objects in the Solar System including the Sun, planets, and moo ...
... SC.8.E.5.4 Explore the Law of Universal Gravitation by explaining the role that gravity plays in the formation of planets, stars, and solar systems and in determining their motions. SC.8.E.5.7 (AA) Compare and contrast the properties of objects in the Solar System including the Sun, planets, and moo ...
Chapter 26 – The Sun and the Solar System
... a. Some are barely visible while others are 4 times larger than Earth b. Small one may last a few hour – large ones months c. Are very hot and bright – look dark because the photosphere is so much hotter and brighter than the sunspots d. Move from left to right across surface i This gave evidence th ...
... a. Some are barely visible while others are 4 times larger than Earth b. Small one may last a few hour – large ones months c. Are very hot and bright – look dark because the photosphere is so much hotter and brighter than the sunspots d. Move from left to right across surface i This gave evidence th ...
105 Chapter 8 Review Notes • The Nebular Hypothesis, which is the
... Neptune (took much longer) • Delayed formation of Uranus and Neptune until after powerful solar winds of TTauri phase of Sun (after about 1 million years) prevented them from gathering much H and He gas because most of the remainder of these gases got blown out of the solar system Planetary embryos ...
... Neptune (took much longer) • Delayed formation of Uranus and Neptune until after powerful solar winds of TTauri phase of Sun (after about 1 million years) prevented them from gathering much H and He gas because most of the remainder of these gases got blown out of the solar system Planetary embryos ...
Chapter 28 - Trimble County Schools
... • Consist mostly of hydrogen and helium gas with small amounts of other elements and dust – Dust makes clouds look dark by blocking light – Dust also reflect starlight and makes clouds look bright ...
... • Consist mostly of hydrogen and helium gas with small amounts of other elements and dust – Dust makes clouds look dark by blocking light – Dust also reflect starlight and makes clouds look bright ...
The Sun Song - MIT Haystack Observatory
... Hans Bethe long ago reached the conclusion It changes Hydrogen to Helium by nuclear ______________ When fusion takes place light is created And it makes its way out (although rather belated) Through the photosphere that's the part that we _____________ The light comes out and shines on you and me Ab ...
... Hans Bethe long ago reached the conclusion It changes Hydrogen to Helium by nuclear ______________ When fusion takes place light is created And it makes its way out (although rather belated) Through the photosphere that's the part that we _____________ The light comes out and shines on you and me Ab ...
Chapter 20: The Solar System
... 26. __________________ are areas of gas on the sun that are cooler than the surrounding area. 27. Reddish loops of gas on the sun that connect different parts of the sunspot regions are called ________________________________. 28. Explosions of hydrogen gas that go out into space away from the sun a ...
... 26. __________________ are areas of gas on the sun that are cooler than the surrounding area. 27. Reddish loops of gas on the sun that connect different parts of the sunspot regions are called ________________________________. 28. Explosions of hydrogen gas that go out into space away from the sun a ...
THE SOLAR SYSTEM - Mercer Island School District
... THE SOLAR SYSTEM • The solar system consists of the Sun and everything that is orbiting around it. • 8 Planets • Dwarf Planets • Moons • Comets • Meteoroids • Asteroids Images and information used in this presentation were taken from Microsoft Encarta Reference Suite. ...
... THE SOLAR SYSTEM • The solar system consists of the Sun and everything that is orbiting around it. • 8 Planets • Dwarf Planets • Moons • Comets • Meteoroids • Asteroids Images and information used in this presentation were taken from Microsoft Encarta Reference Suite. ...
SNC1P - MsKhan
... -Stars are luminous. What does that mean? -How large is our Sun compared to other stars? ...
... -Stars are luminous. What does that mean? -How large is our Sun compared to other stars? ...
Life in the Universe
... What about other solar systems? • Planets seem to be common around other stars • Hot, massive stars probably don’t live long enough for life (as we know it) to develop • Cool, low-mass stars are unlikely to have earth-like planets with liquid water • Best bet: sun-like stars, which are still fairly ...
... What about other solar systems? • Planets seem to be common around other stars • Hot, massive stars probably don’t live long enough for life (as we know it) to develop • Cool, low-mass stars are unlikely to have earth-like planets with liquid water • Best bet: sun-like stars, which are still fairly ...
The Sun - Tvining.us
... Recent data from the spacecraft Ulysses show that the solar wind emanating from the polar regions flows at nearly double the rate, 750 kilometers per second, that it does at lower latitudes. ...
... Recent data from the spacecraft Ulysses show that the solar wind emanating from the polar regions flows at nearly double the rate, 750 kilometers per second, that it does at lower latitudes. ...
Introduction to Astronomy
... to appear to rise and set each time; • The moon has orbited the earth 3.5 times, going through its phases; • Earth has completed more than 1/4 of its orbit around the sun, allowing us to see different stars and planets at night and causing changes in the sun’s position in our sky and the seasons; • ...
... to appear to rise and set each time; • The moon has orbited the earth 3.5 times, going through its phases; • Earth has completed more than 1/4 of its orbit around the sun, allowing us to see different stars and planets at night and causing changes in the sun’s position in our sky and the seasons; • ...
Astronomy Jeopardy / Microsoft PowerPoint
... Temperature, thin atmosphere=liquid H2O would turn into gas, Co2 atmosphere, ...
... Temperature, thin atmosphere=liquid H2O would turn into gas, Co2 atmosphere, ...
Solar System Brochure.notebook
... • Carefully fold paper into 8 equal segments. (Fold in half the "hamburger way" and in half again). Make sure the folds are like an accordion. • Title Page: Page 1 > Solar System > Your name > Color and decorate ...
... • Carefully fold paper into 8 equal segments. (Fold in half the "hamburger way" and in half again). Make sure the folds are like an accordion. • Title Page: Page 1 > Solar System > Your name > Color and decorate ...
AST 1A INTRODUCTION TO THE SOLAR SYSTEM Spring 2017 CH
... 2. What is the difference between our solar system, our galaxy, and the universe? 3. Why are light-years more convenient than miles, kilometers, or astronomical units for measuring certain distances? 4. Why is it difficult to detect planets orbiting other stars? 5. What does the size of the star ima ...
... 2. What is the difference between our solar system, our galaxy, and the universe? 3. Why are light-years more convenient than miles, kilometers, or astronomical units for measuring certain distances? 4. Why is it difficult to detect planets orbiting other stars? 5. What does the size of the star ima ...
The Sun - www .alexandria .k12 .mn .us
... • Prominences (aka coronal loops) are large, bright loop-shaped features on the photosphere that extend out into the corona • A prominence takes ~1 day to form and may persist for several months. • A typical prominence extends over many 1000s of kms; the largest recorded was over 800000 kms long ...
... • Prominences (aka coronal loops) are large, bright loop-shaped features on the photosphere that extend out into the corona • A prominence takes ~1 day to form and may persist for several months. • A typical prominence extends over many 1000s of kms; the largest recorded was over 800000 kms long ...
Sailing on electricity - Space Propulsion Synergy Team
... NASA’s Voyager 1 took 35 years to reach the heliopause, the unexplored region where the solar wind stops and the interstellar plasma eventually takes over. There has to be a faster way to explore the outer planets and the heliopause than Voyager 1’s chemical-rocket propulsion. Two researchers at NAS ...
... NASA’s Voyager 1 took 35 years to reach the heliopause, the unexplored region where the solar wind stops and the interstellar plasma eventually takes over. There has to be a faster way to explore the outer planets and the heliopause than Voyager 1’s chemical-rocket propulsion. Two researchers at NAS ...
Final Exam Study Guide
... This guide is meant to assist with studying for the final exam on May 1, 2017. However this study guide will not cover every single topic that might show up on the final. Remember that everything on the final is in the slides in some form. You may NOT use this sheet when you are taking the exam. ...
... This guide is meant to assist with studying for the final exam on May 1, 2017. However this study guide will not cover every single topic that might show up on the final. Remember that everything on the final is in the slides in some form. You may NOT use this sheet when you are taking the exam. ...
GLOSSARY
... most stars with mass less than about 1.2M . In most of the solar interior, radiation is sufficient to transport energy from the interior, where energy is generated by nuclear fusion, to the surface, where energy is radiated into space. Near the surface, the opacity increases because of partial ioniz ...
... most stars with mass less than about 1.2M . In most of the solar interior, radiation is sufficient to transport energy from the interior, where energy is generated by nuclear fusion, to the surface, where energy is radiated into space. Near the surface, the opacity increases because of partial ioniz ...
A SOLAR SYSTEM IS BORN
... • Gravity causes the particles in a nebula to be attracted to each other. • As particles move closer together, collisions cause pressure to increase and particles are pushed apart. • If the inward force of gravity is balanced by outward pressure, the nebula becomes stable. ...
... • Gravity causes the particles in a nebula to be attracted to each other. • As particles move closer together, collisions cause pressure to increase and particles are pushed apart. • If the inward force of gravity is balanced by outward pressure, the nebula becomes stable. ...
Heliosphere
The heliosphere is the bubble-like region of space dominated by the Sun, which extends far beyond the orbit of Pluto. Plasma ""blown"" out from the Sun, known as the solar wind, creates and maintains this bubble against the outside pressure of the interstellar medium, the hydrogen and helium gas that permeates the Milky Way Galaxy. The solar wind flows outward from the Sun until encountering the termination shock, where motion slows abruptly. The Voyager spacecraft have actively explored the outer reaches of the heliosphere, passing through the shock and entering the heliosheath, a transitional region which is in turn bounded by the outermost edge of the heliosphere, called the heliopause. The overall shape of the heliosphere is controlled by the interstellar medium, through which it is traveling, as well as the Sun, and does not appear to be perfectly spherical. The limited data available and unexplored nature of these structures have resulted in many theories.On September 12, 2013, NASA announced that Voyager 1 had exited the heliosphere on August 25, 2012, when it measured a sudden increase in plasma density of about forty times. Because the heliopause marks one boundary between the Sun's solar wind and the rest of the galaxy, a spacecraft such as Voyager 1 which has departed the heliosphere can be said to have reached interstellar space.