Unit 8.4 Solar System
... 3. Three spacecraft and the planets they visited: a. Mariner 1 (Mercury) b. Voyager 1 (Jupiter) c. Venus Express (Venus) 4. a. Pluto lost its status as a planet in 2006. b. Pluto is regarded as a dwarf planet because normal planets have enough gravity to sweep their orbits clear of debris, whereas t ...
... 3. Three spacecraft and the planets they visited: a. Mariner 1 (Mercury) b. Voyager 1 (Jupiter) c. Venus Express (Venus) 4. a. Pluto lost its status as a planet in 2006. b. Pluto is regarded as a dwarf planet because normal planets have enough gravity to sweep their orbits clear of debris, whereas t ...
Solar System-3
... 3. The cube of each planet's radius is proportional to the square of its period. You have observed this relationship in this activity. Isaac Newton was able to demonstrate that a gravitational force between the Sun and the planets would lead to these three laws. This was very strong evidence that th ...
... 3. The cube of each planet's radius is proportional to the square of its period. You have observed this relationship in this activity. Isaac Newton was able to demonstrate that a gravitational force between the Sun and the planets would lead to these three laws. This was very strong evidence that th ...
The Outer Planets - Spokane Public Schools
... The eight planets of our solar system are divided into two groups: inner planets and outer planets. The outer planets are furthest from the sun and receive less light and heat therefore they are the colder planets. They are Jupiter, Saturn, Uranus, Neptune and Pluto, which is called a dwarf planet b ...
... The eight planets of our solar system are divided into two groups: inner planets and outer planets. The outer planets are furthest from the sun and receive less light and heat therefore they are the colder planets. They are Jupiter, Saturn, Uranus, Neptune and Pluto, which is called a dwarf planet b ...
Sample exam 2
... 11. Venus, unlike Earth, has almost no planetary magnetic field; the reason that is given in the text is that Venus’s rotation is quite slow compared to Earth. As you are reading this, one of your classmates (the annoying one) says, “No way! Venus doesn’t have a magnetic field because it doesn’t hav ...
... 11. Venus, unlike Earth, has almost no planetary magnetic field; the reason that is given in the text is that Venus’s rotation is quite slow compared to Earth. As you are reading this, one of your classmates (the annoying one) says, “No way! Venus doesn’t have a magnetic field because it doesn’t hav ...
planetary comparisons
... location in the solar system? PART B Directions: Use the Planetary Data (Table 21.1 on p 577) to help answer these questions .For this assignment, include Pluto as a Planet! 10. P 567 – What is the average distance of the earth to the moon? Answer in miles. 11. What is the distance of the earth to t ...
... location in the solar system? PART B Directions: Use the Planetary Data (Table 21.1 on p 577) to help answer these questions .For this assignment, include Pluto as a Planet! 10. P 567 – What is the average distance of the earth to the moon? Answer in miles. 11. What is the distance of the earth to t ...
Integrative Studies 410 Our Place in the Universe
... meteoroid impacts • Lots of them; all sizes – Copernicus ~ 90 km across – Reinhold ~ 40 km across – Also craters as small as 0.01 mm! ...
... meteoroid impacts • Lots of them; all sizes – Copernicus ~ 90 km across – Reinhold ~ 40 km across – Also craters as small as 0.01 mm! ...
solar system
... In 2006 , Pluto was reclassified as a `dwarf planet’ . During its orbit, the far – flung Pluto approaches closer to the sun ...
... In 2006 , Pluto was reclassified as a `dwarf planet’ . During its orbit, the far – flung Pluto approaches closer to the sun ...
Earth in Space - bvsd.k12.pa.us
... 11. The inner planets have (thin/thick) atmospheres and solid (rocky/gaseous) bodies. 12. A belt of (asteroids/comets) separates the inner and outer planets. 13. The atmospheres of the gaseous planets are made up mostly of (hydrogen/oxygen) and helium. 14. (Pluto/Saturn) is completely different from ...
... 11. The inner planets have (thin/thick) atmospheres and solid (rocky/gaseous) bodies. 12. A belt of (asteroids/comets) separates the inner and outer planets. 13. The atmospheres of the gaseous planets are made up mostly of (hydrogen/oxygen) and helium. 14. (Pluto/Saturn) is completely different from ...
Space_Poems_970709278
... With port holes all along the sides, I'd gaze amazed at Mars. With mast made strong with spider webs, And sail of fluffy cloud, I'd watch the Earth go sweeping past, As out to space I ploughed. With stars in front and stars behind, And planets far and near, I'd sail my yacht around the rings, Of Sat ...
... With port holes all along the sides, I'd gaze amazed at Mars. With mast made strong with spider webs, And sail of fluffy cloud, I'd watch the Earth go sweeping past, As out to space I ploughed. With stars in front and stars behind, And planets far and near, I'd sail my yacht around the rings, Of Sat ...
Diapositiva 1
... brightest stars, grouped in the famous Big Dipper asterism, are visible throughout the year in the northern hemisphere. Ursa Minor is a constellation of the northern sky. It is especially known because within it lies the north celestial pole, although its position is subject to a continuous, slow mo ...
... brightest stars, grouped in the famous Big Dipper asterism, are visible throughout the year in the northern hemisphere. Ursa Minor is a constellation of the northern sky. It is especially known because within it lies the north celestial pole, although its position is subject to a continuous, slow mo ...
View PDF
... Write an essay to explain the reason for seasons based on evidence Create a model that explains the reason for seasons Create a story book for younger students that explains the seasons Draw a diagram of the solar system which includes the correct position of planets, dwarf planets, comets, and aste ...
... Write an essay to explain the reason for seasons based on evidence Create a model that explains the reason for seasons Create a story book for younger students that explains the seasons Draw a diagram of the solar system which includes the correct position of planets, dwarf planets, comets, and aste ...
Same and Different - Passport to Knowledge
... * Sun: our star, a giant ball of plasma, primarily composed of hydrogen and helium * Jovian planets: named after Jupiter, also includes Saturn, Uranus and Neptune: huge compared to Earth, but not the Sun; also balls of gas and primarily composed of hydrogen and helium, but not large enough to have c ...
... * Sun: our star, a giant ball of plasma, primarily composed of hydrogen and helium * Jovian planets: named after Jupiter, also includes Saturn, Uranus and Neptune: huge compared to Earth, but not the Sun; also balls of gas and primarily composed of hydrogen and helium, but not large enough to have c ...
Sample Final - Lawrence University
... 21. Which of the following is true about the asteroids in our solar system? (a) The average separation between asteroids in the main belt is about 1 million kilometers. (b) Most asteroids orbit beyond the orbit of Saturn (c) There are no asteroids larger than a few meters. (d) Asteroids are typicall ...
... 21. Which of the following is true about the asteroids in our solar system? (a) The average separation between asteroids in the main belt is about 1 million kilometers. (b) Most asteroids orbit beyond the orbit of Saturn (c) There are no asteroids larger than a few meters. (d) Asteroids are typicall ...
Physics 110 - Lawrence University
... 21. Which of the following is true about the asteroids in our solar system? (a) The average separation between asteroids in the main belt is about 1 million kilometers. (b) Most asteroids orbit beyond the orbit of Saturn (c) There are no asteroids larger than a few meters. (d) Asteroids are typicall ...
... 21. Which of the following is true about the asteroids in our solar system? (a) The average separation between asteroids in the main belt is about 1 million kilometers. (b) Most asteroids orbit beyond the orbit of Saturn (c) There are no asteroids larger than a few meters. (d) Asteroids are typicall ...
The Planets - WordPress.com
... in our solar system. Pluto has three moons. The mantle layer on Ceres could contain more fresh water than Earth’s surface! ...
... in our solar system. Pluto has three moons. The mantle layer on Ceres could contain more fresh water than Earth’s surface! ...
A B C`s of Space Aleks Slocum Second Grade SCI.2.2 2010
... A “day” is the time it takes the earth to spin around one complete time. It is also the time frame when the sun is in the sky. ...
... A “day” is the time it takes the earth to spin around one complete time. It is also the time frame when the sun is in the sky. ...
Solar System Notes
... Solar System Notes Solar System- A group of planets, moons and other satellites that orbit around a star. The Sun-the most important object in our solar system. Our sun provides light and heat for earth Our sun is a star When the sun rises and sets it looks like it is moving but it is not actually m ...
... Solar System Notes Solar System- A group of planets, moons and other satellites that orbit around a star. The Sun-the most important object in our solar system. Our sun provides light and heat for earth Our sun is a star When the sun rises and sets it looks like it is moving but it is not actually m ...
Inner and Outer Planets
... (primarily hydrogen & helium; smaller solid or liquid core). • They are very light for their size. • They move quickly in space. • They have rings and many moons. • They have a diameter of less than 48,000 km ...
... (primarily hydrogen & helium; smaller solid or liquid core). • They are very light for their size. • They move quickly in space. • They have rings and many moons. • They have a diameter of less than 48,000 km ...
Solar System Astronomy
... Ellipse: a closed curve around two fixed points; called foci. The orbits of all planets around the Sun are ellipses. Focus (foci): one of the two fixed points is an ellipse. Foucault pendulum: a freely swinging pendulum whose path appears to change over time in a predictable manner; provides evidenc ...
... Ellipse: a closed curve around two fixed points; called foci. The orbits of all planets around the Sun are ellipses. Focus (foci): one of the two fixed points is an ellipse. Foucault pendulum: a freely swinging pendulum whose path appears to change over time in a predictable manner; provides evidenc ...
Power Point
... elliptical in shape. • The nine known planets, in order of distance from the sun, are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Neptune, and Pluto. ...
... elliptical in shape. • The nine known planets, in order of distance from the sun, are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Neptune, and Pluto. ...
Solar System Project (revised 2014)
... What does a planet need to sustain complex life? What planets like Earth have been found? Where are they? What life sustaining features do they have? What features do they lack? Has proof of life been found and verified on any other planet so far? What’s the evidence? ...
... What does a planet need to sustain complex life? What planets like Earth have been found? Where are they? What life sustaining features do they have? What features do they lack? Has proof of life been found and verified on any other planet so far? What’s the evidence? ...
The Solar System
... The Solar System The Sun and all of the objects that travel around it •the Sun is a star •planets •natural satellites of the planets; rings •the asteroid belt (rocks between Mars and Jupiter: meteoroids) •comets (frozen masses of gas and dust) ...
... The Solar System The Sun and all of the objects that travel around it •the Sun is a star •planets •natural satellites of the planets; rings •the asteroid belt (rocks between Mars and Jupiter: meteoroids) •comets (frozen masses of gas and dust) ...
Solar System Webquest Go to http://www.kidsastronomy.com
... 3. The object pictured to the left can also be seen in the picture of the solar system. a. Identify this object _________________________ b. When is this object's "tail" visible? ____________ c. Which direction does its tail point (in reference to the sun)? ___________________ d. How does its orbit ...
... 3. The object pictured to the left can also be seen in the picture of the solar system. a. Identify this object _________________________ b. When is this object's "tail" visible? ____________ c. Which direction does its tail point (in reference to the sun)? ___________________ d. How does its orbit ...
Deep Dark Space
... It is the largest planet in our solar system. Jupiter is a giant ball of gases with a rocky ...
... It is the largest planet in our solar system. Jupiter is a giant ball of gases with a rocky ...
Late Heavy Bombardment
The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.