Finding the Small Moons of the Outer Planets
... of the solar system. These asteroid and comet type objects would have likely had collisions or gravitational How to Capture a Satellite interactions with each other within the Hill spheres Only the four giant planets have known outer satellite of the planets. During these Hill sphere interactions, p ...
... of the solar system. These asteroid and comet type objects would have likely had collisions or gravitational How to Capture a Satellite interactions with each other within the Hill spheres Only the four giant planets have known outer satellite of the planets. During these Hill sphere interactions, p ...
Rocky The Rock Cycle
... are normally dumped first and then covered by finer material. Layers of sediment build up over time. These layers form a sedimentary sequence. ...
... are normally dumped first and then covered by finer material. Layers of sediment build up over time. These layers form a sedimentary sequence. ...
The Dimensions of the Solar System
... Next use the ruler (under the “Tool” menu in Google Earth) to help set the overlay to the scale you want. For our example, we want the Sun to be 1 meter in diameter, so we used the ruler tool to draw a horizontal bar on the figure that is 1 kilometer across (yellow bar in Figure 3). You can choose o ...
... Next use the ruler (under the “Tool” menu in Google Earth) to help set the overlay to the scale you want. For our example, we want the Sun to be 1 meter in diameter, so we used the ruler tool to draw a horizontal bar on the figure that is 1 kilometer across (yellow bar in Figure 3). You can choose o ...
Picture File - WordPress.com
... – 2nd from the sun – It takes 224.7 Earth days for Venus to orbit the sun. It has the longest rotation period of any planet in the Solar System. It unusually rotates in the opposite direction to most other ...
... – 2nd from the sun – It takes 224.7 Earth days for Venus to orbit the sun. It has the longest rotation period of any planet in the Solar System. It unusually rotates in the opposite direction to most other ...
Document
... the top of Mt. Everest in a direction tangent to the ground. If the initial speed were high enough to cause the ball to travel in a circular trajectory around Earth Earth, the ball’s ball s acceleration would – a) be much less than g (because the ball doesn’t fall to the ground). Note: someone in a ...
... the top of Mt. Everest in a direction tangent to the ground. If the initial speed were high enough to cause the ball to travel in a circular trajectory around Earth Earth, the ball’s ball s acceleration would – a) be much less than g (because the ball doesn’t fall to the ground). Note: someone in a ...
–1– AST104 Sp2006: EXAM 1 Multiple Choice Questions: Mark the
... e. 105 times brighter than what angle would you measure between the north13. The 26,000 year precession cycle of the Earth’s ern horizon and the Zenith? spin axis implies that a. 62 degrees a. Polaris will not always be the star currently nearest to the North Celestial Pole. b. 5 degrees c. 90 degre ...
... e. 105 times brighter than what angle would you measure between the north13. The 26,000 year precession cycle of the Earth’s ern horizon and the Zenith? spin axis implies that a. 62 degrees a. Polaris will not always be the star currently nearest to the North Celestial Pole. b. 5 degrees c. 90 degre ...
Astr 3020 Cosmology Samples for Exam 2 Foundations of Modern
... Newton’s form of Kepler’s third law showed that the ratio of the cube of a planets semimajor axis to the square of its orbital period is a) equal to the mass of the sun. b) equal to the sum of the suns mass and the planets mass. c) equal to the mass of the planet. d) equal to the product of the plan ...
... Newton’s form of Kepler’s third law showed that the ratio of the cube of a planets semimajor axis to the square of its orbital period is a) equal to the mass of the sun. b) equal to the sum of the suns mass and the planets mass. c) equal to the mass of the planet. d) equal to the product of the plan ...
Understanding the Solar System
... solar system. This will be done in your groups of 5. We will provide you with the materials to do this. Step 1: You will need to use the glitter paint to paint the black construction paper. This will symbolize the stars in our solar system. Step 2: You will need to get your box and paste the black c ...
... solar system. This will be done in your groups of 5. We will provide you with the materials to do this. Step 1: You will need to use the glitter paint to paint the black construction paper. This will symbolize the stars in our solar system. Step 2: You will need to get your box and paste the black c ...
Chapter 28
... the lowest layer of the Sun’s atmosphere, with an average temperature of about 5800K. • The chromosphere, which is above the photosphere and approximately 2500 km in thickness, has a temperature of nearly 30,000 K at the top. • The corona, which is the top layer of the Sun’s atmosphere, extends seve ...
... the lowest layer of the Sun’s atmosphere, with an average temperature of about 5800K. • The chromosphere, which is above the photosphere and approximately 2500 km in thickness, has a temperature of nearly 30,000 K at the top. • The corona, which is the top layer of the Sun’s atmosphere, extends seve ...
The Jovian Planets
... Introduction to Astronomy • Announcements – Midterm Exam on Thursday • Closed-book/notes/etc. ...
... Introduction to Astronomy • Announcements – Midterm Exam on Thursday • Closed-book/notes/etc. ...
Boonesborough Days - Tri
... revolution time. But with the last three planets, we have known their orbital periods shortly after their discovery. Here is where that guy Johannes Kepler can help us understand the planets once again with his Third Law. Law Three: The squares of the period of revolution of any two planets are prop ...
... revolution time. But with the last three planets, we have known their orbital periods shortly after their discovery. Here is where that guy Johannes Kepler can help us understand the planets once again with his Third Law. Law Three: The squares of the period of revolution of any two planets are prop ...
Biology: Unit One Calendar
... Describe how the planets formed. (1b) Describe the formation of land, the atmosphere, and the oceans of Earth. (1a, 1c) Section 27.2 Models of the Solar System Compare the models of the universe developed by Ptolemy, and Copernicus. (IE, 1k, IE.1n) Summarize Kepler’s three laws of planetary ...
... Describe how the planets formed. (1b) Describe the formation of land, the atmosphere, and the oceans of Earth. (1a, 1c) Section 27.2 Models of the Solar System Compare the models of the universe developed by Ptolemy, and Copernicus. (IE, 1k, IE.1n) Summarize Kepler’s three laws of planetary ...
Across 2. a slightly cooler region on the surface of the sun, caused
... 125. hottest planet in the solar system 126. the name of the biggest volcano in the solar system 127. constellation we call "the scorpion" 129. the type of asteroids that are the most rocky ones 130. the "north star" 131. what happens to light when a star is moving away from us quickly 132. the caus ...
... 125. hottest planet in the solar system 126. the name of the biggest volcano in the solar system 127. constellation we call "the scorpion" 129. the type of asteroids that are the most rocky ones 130. the "north star" 131. what happens to light when a star is moving away from us quickly 132. the caus ...
For Chapter 16
... • If so, we would expect to find some of these systems in different stages of formation • In other words, we should be able to find clouds of gas and dust, primordial nebula, and protosuns, etc. ...
... • If so, we would expect to find some of these systems in different stages of formation • In other words, we should be able to find clouds of gas and dust, primordial nebula, and protosuns, etc. ...
6TH GRADE ACCURATE PLANET SIZES AND DISTANCE FROM
... column on the data table to check the sizes of objects. These objects are approximately correct for their size. Feel free to substitute other objects you may have that are also accurate to size. Softball - Jupiter Baseball - Saturn Two small seeds – Mercury and Mars (Mars is slightly larger) Two di ...
... column on the data table to check the sizes of objects. These objects are approximately correct for their size. Feel free to substitute other objects you may have that are also accurate to size. Softball - Jupiter Baseball - Saturn Two small seeds – Mercury and Mars (Mars is slightly larger) Two di ...
Summative Assessment 1
... 3. Which planet has the most satellites (moons)? 4. Which planet is coldest? 5. Which two planets are very much alike? (They are close to the same size. Their temperature is very close. Their rotation period is very similar.) 6. Which planet takes longest to rotate around the sun? 7. Name one of the ...
... 3. Which planet has the most satellites (moons)? 4. Which planet is coldest? 5. Which two planets are very much alike? (They are close to the same size. Their temperature is very close. Their rotation period is very similar.) 6. Which planet takes longest to rotate around the sun? 7. Name one of the ...
Astronomy - Educator Pages
... The phases of the moon are caused by relative positions of the moon, earth, and sun. In order for you to see the moon it must be facing the Earth (so you can see it) and the Sun (so there is light reflecting off of it). ...
... The phases of the moon are caused by relative positions of the moon, earth, and sun. In order for you to see the moon it must be facing the Earth (so you can see it) and the Sun (so there is light reflecting off of it). ...
Planet Locations for the - Warren Astronomical Society
... has since faded to light pink and deepened back to red periodically, has its own private rotation rate, slower than the air belt around it. And the rate changes erratically, the Red Spot will sometimes lag fifteen minutes behind the mean value, then move faster to partly catch up again. The Spot was ...
... has since faded to light pink and deepened back to red periodically, has its own private rotation rate, slower than the air belt around it. And the rate changes erratically, the Red Spot will sometimes lag fifteen minutes behind the mean value, then move faster to partly catch up again. The Spot was ...
Planets - burnsburdick11
... fire, and gas. You would die before you even got to the sun, since it is so hot. The sun is just at its medium stage. It will hurt your eyes if you look at the sun. The Sun was a god of many religions back in the day. The sun is half way through its lifetime. More than 1 million earths would fit ins ...
... fire, and gas. You would die before you even got to the sun, since it is so hot. The sun is just at its medium stage. It will hurt your eyes if you look at the sun. The Sun was a god of many religions back in the day. The sun is half way through its lifetime. More than 1 million earths would fit ins ...
History of Astronomy
... same speed? No. A planet’s speed depends on its average distance from the Sun. The closest planet moves fastest, the most ...
... same speed? No. A planet’s speed depends on its average distance from the Sun. The closest planet moves fastest, the most ...
Brock physics - Brock University
... 28. Observations during a total solar eclipse show that the angular sizes of the Sun and Moon are nearly equal. Therefore, if the Sun is about 400 times farther from us than the diameter of the Moon. the Moon, the diameter of the Sun must be about (a) 1/400th of (b) 1/20th of (c) the same as (d) 20 ...
... 28. Observations during a total solar eclipse show that the angular sizes of the Sun and Moon are nearly equal. Therefore, if the Sun is about 400 times farther from us than the diameter of the Moon. the Moon, the diameter of the Sun must be about (a) 1/400th of (b) 1/20th of (c) the same as (d) 20 ...
Chap. 4: Gravitation and the Waltz of the Planets
... Why did Copernicus (1473-1543) think that the Earth and the other planets go around the Sun? How did Tycho Brahe (1546-1601) attempt to test the ideas of Copernicus? What paths do the planets follow as they move around the Sun? Johannes Kepler (1571-1630) What did Galileo (1564-1642) see in his tele ...
... Why did Copernicus (1473-1543) think that the Earth and the other planets go around the Sun? How did Tycho Brahe (1546-1601) attempt to test the ideas of Copernicus? What paths do the planets follow as they move around the Sun? Johannes Kepler (1571-1630) What did Galileo (1564-1642) see in his tele ...
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.