Cosmic Perspective Fundamentals
3rd Edition
ISBN: 9780134988504
Author: Bennett, Jeffrey O., Donahue, M. (megan), SCHNEIDER, Nicholas, Voit, Mark
Publisher: Pearson,
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Chapter 2, Problem 2QQ
To determine
Whether the Axis of the Earth points towards Polaris or Vega or Sun in spring time.
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Chapter 2 Solutions
Cosmic Perspective Fundamentals
Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Prob. 2QQCh. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....
Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Choose the best answer to each of the following....Ch. 2 - Prob. 13SEQCh. 2 - Explain all answers clearly, using complete...Ch. 2 - Explain all answers clearly, using complete...Ch. 2 - Explain all answers clearly, using complete...Ch. 2 - Prob. 17SEQCh. 2 - Prob. 18SEQCh. 2 - Explain all answers clearly, using complete...Ch. 2 - Explain all answers clearly, using complete...Ch. 2 - Explain all answers clearly, using complete...Ch. 2 - Explain all answers clearly, using complete...
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- As discussed in class, the moon is receding from the Earth due to tides at a rate of ~4 cm/year. Let’s assume that rate has been constant throughout time (it wasn’t, but we can use it to illustrate some key points). Its current semi-major axis is 384,400 km.a) If the moon formed 4.5 billion years ago and has been receding from the Earth ever since, what was its original semi-major axis? What was its original orbital period?b) What would the apparent size of the Moon have been in the sky as viewed from Earth? That is, in Hmwk 2, you were told the diameter of the Moon spans about 0.5o when viewed from Earth today. What would it have been when the Moon first formed? Reletive Numbers Relevant Numbers1 AU = 150,000,000 km = 1.5x108 kmEccentricity of Earth’s Orbit: 0.0167Radius of Earth: 6371 kmMass of Earth: 5.96x1024 kgRadius of the Moon: 1737 kmMass of Moon: 7.34x1022 kgRadius of Mars: 3390 kmMass of Mars: 6.4x1023 kgRadius of the Sun: R⦿=696,300 kmMass of the Sun: M⦿=2x1030…arrow_forwardThe table below presents the semi-major axis (a) and Actual orbital period for all of the major planets in the solar system. Cube for each planet the semi-major axis in Astronomical Units. Then take the square root of this number to get the Calculated orbital period of each planet. Fill in the final row of data for each planet. Table of Data for Kepler’s Third Law: Table of Data for Kepler’s Third Law: Planet aau = Semi-Major Axis (AU) Actual Planet Calculated Planet Period (Yr) Period (Yr) __________ ______________________ ___________ ________________ Mercury 0.39 0.24 Venus 0.72 0.62 Earth 1.00 1.00 Mars 1.52 1.88 Jupiter…arrow_forwardThis is Pre-Calc! Please help and Thank you! Please click the pics for the background info Directions: Answer questions 1-8 based on the information on Table 1. Round all answers to the nearest thousandth and label with the appropriate units. 1. According to Table 1, what is the closest distance between Earth and Mars? 2. According to Table 1, what is the farthest distance between Earth and Mars? 3. Based on your answers from #2 and #3, what is the average distance between the two planets? 4. Based on your answers from #2 and #3, what is the amplitude of the distances? 5. The distance has a period of 772 days. Write a sinusoidal equation relating the number of days and distance from Earth to Mars. 6. Based on the equation from #5, what is the distance between our planets on Mr. Schutt’s birthday (day 187)? 7. Write a sinusoidal equation relating the number of days and the one-waycommunication between Earth to Mars. 8. What is the one-way communication time delay between our planets on…arrow_forward
- Please use the info to answer the question. Please circle your answer.arrow_forwardbetween a planet and its moon. Procedure/Analysis: Go to: https://www.physicsclassroom.com/Physics-Interactives/Circular-and-Satellite- Motion/Gravitational-Fields/Gravitational-Fields-Interactive Use the program to answer the following questions. 1. A planet and its moon are shown in the simulation window. Click and drag the moon to various positions about the planet and observe the gravitational force vector. In the diagram below, draw a force vector (arrow with arrowhead) to depict the direction and relative magnitude of the force acting upon the moon at the designated locations. Note: the size of the arrow should be representative of the strength of the force.arrow_forwardI need help with this questionarrow_forward
- In the figure below, Planet X is moving in a perfectly circular orbit around its companion star.The time between each position shown is exactly one month: 1. Write down Kepler’s second Law of planetary motion.2. Does the planet obey Kepler’s second law? How do you know?3. If you carefully watched this planet during the entire orbit, would its speed be increasing, decreasing, orstaying the same? How do you know?arrow_forwardDelay time for communication between GEO satellites and Earth. Use the relationship between distance (d), time (t) and speed (v), d = vt to repeat the calculation we did in class, but this time using the English units. Use the fact that GEO satellites orbit at 22,236 miles above Earth's equator, and that the speed of light is 1.86 x 105 mi/s. (Note that both of these values are equivalent to those used in class.) You may want to write this calculation on paper and insert a photo here.arrow_forwardI need quick help pleasearrow_forward
- (If relevant) A clearly labeled diagram (or diagrams) clearly pertaining to your analysis with a coordinate system and relevant labels. Final answer with appropriate units and significant figures. A 2-3 sentence reflection on your answer. Does it make sense? Why or why not? What are some implications? Do not just summarize your solution procedure.arrow_forwardq4 1, 2, 3arrow_forwardWe need to create a scale model of the solar system (by shrinking the sun down to the size of a basketball or ~30cm). First, we will need to scale down actual solar system dimensions (planet diameters and average orbital radiuses) by converting our units. There are two blank spaces in the table below. We will effectively fill in the missing data in the next set of questions. Use the example below to help you. Example: What is the scaled diameter of Mercury if the Sun is scaled to the size of a basketball (30 cm)? The actual diameter of Mercury is 4879 km The Sun's diameter is 1392000 km If the Sun is to be reduced to the size of a basketball, then the conversion we need for this equation will be: 30cm1392000km Here is how we run the conversion: 4879km×30cm1392000km=0.105cm or 0.11cm if we were to round our answer. This means that if the sun in our model is the size of a basketball, Mercury is the size of a grain of sand. We can also see by looking at the table, that we would…arrow_forward
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