ACCEL: PATTERNS OF MASS AND DENSITY IN THE SOLAR SYSTEM

Similar documents
Patterns in the Solar System (Chapter 18)

Patterns in the Solar System (Chapter 18)

Name Class Date. For each pair of terms, explain how the meanings of the terms differ.

The Outer Planets (pages )

Phys 214. Planets and Life

Chapter 23: Touring Our Solar System

Lesson 2 The Inner Planets

Celestial Objects. Background Questions. 1. What was invented in the 17 th century? How did this help the study of our universe? 2. What is a probe?

Lesson 3 The Outer Planets

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)

4. THE SOLAR SYSTEM 1.1. THE SUN. Exercises

1/13/16. Solar System Formation

Which of the following planets are all made up of gas? When a planets orbit around the Sun looks like an oval, it s called a(n)

Unit 12 Lesson 1 What Objects Are Part of the Solar System?

After you read this section, you should be able to answer these questions:

Astronomy Test Review. 3 rd Grade

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury.

Inner and Outer Planets

Our Solar System. Lesson 5. Distances Between the Sun and the Planets

Which of the following statements best describes the general pattern of composition among the four jovian

Astro 1: Introductory Astronomy

Inner and Outer Planets

Lesson 1 The Structure of the Solar System

2. Which of the following planets has exactly two moons? A) Venus B) Mercury C) Uranus D) Mars E) Neptune

The Solar System 6/23

3. The name of a particularly large member of the asteroid belt is A) Halley B) Charon C) Eris D) Ceres E) Triton

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits

Astronomy Section 2 Solar System Test

Formation of the Solar System. What We Know. What We Know

The sun is the hub of a huge rotating system of nine planets, their

Outline. Question of Scale. Planets Dance. Homework #2 was due today at 11:50am! It s too late now.

Planetarium observing is over. Nighttime observing starts next week.

Cosmology Vocabulary

Our Planetary System. Chapter 7

The Gas Giants Astronomy Lesson 13

9.2 - Our Solar System

Name Topic 3 Free Response 2017

Label next 2 pages in ISN Gas Giants. Make sure the following assignments are turned in:

Dwarf Planets and Other Objects

The Solar System. Sun. Rotates and revolves around the Milky Way galaxy at such a slow pace that we do not notice any effects.

CVtpf 2-1. Section 1 Review. 3. Describe How did the process of outgassing help shape Earth's atmosphere?

UNIT 3: Chapter 8: The Solar System (pages )

The Solar System LEARNING TARGETS. Scientific Language. Name Test Date Hour

Yes, inner planets tend to be and outer planets tend to be.

OUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC

CHAPTER 2 Strand 1: Structure and Motion within the Solar System

5. How did Copernicus s model solve the problem of some planets moving backwards?

Human Understanding of both Earth and Space has Changed Over Time. Unit E: Topic One

Moon Obs #1 Due! Moon visible: early morning through afternoon. 6 more due June 13 th. 15 total due June 25 th. Final Report Due June 28th

The Planets and Scale

Prentice Hall EARTH SCIENCE

Name Period Date Earth and Space Science. Solar System Review

Comparative Planetology I: Our Solar System. Chapter Seven

Overview of Solar System

Space Notes 2. Covers Objectives 3, 4, and 8

Prentice Hall EARTH SCIENCE

Our Solar System and Its Place in the Universe

The Solar System. Name Test Date Hour

Starting from closest to the Sun, name the orbiting planets in order.

When you have completed this workbook, you should know and understand the following:

PTYS/ASTR 206 Section 2 Spring 2007 Homework #5 (Page 1/4) NAME: KEY

Activity 12: Solar System

Your task for each planet...

Planets. Chapter 5 5-1

Chapter Outline. Earth and Other Planets. The Formation of the Solar System. Clue #1: Planetary Orbits. Clues to the Origin of the Solar System

Today. Solar System Formation. a few more bits and pieces. Homework due

9/22/ A Brief Tour of the Solar System. Chapter 6: Formation of the Solar System. What does the solar system look like?

Object Type Moons Rings Planet Terrestrial none none. Max Distance from Sun. Min Distance from Sun. Avg. Distance from Sun 57,910,000 km 0.

1. thought the earth was at the center of the solar system and the planets move on small circles that move on bigger circles

23.1 The Solar System. Orbits of the Planets. Planetary Data The Solar System. Scale of the Planets The Solar System

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

Did you know that ALL Jovian Planets have rings??

Stern/March 09. Century. Alan Stern

Lecture 23: Jupiter. Solar System. Jupiter s Orbit. The semi-major axis of Jupiter s orbit is a = 5.2 AU

It Might Be a Planet If...

Exam# 2 Review. Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280

ASTR 380 Possibilities for Life in the Outer Solar System

Name Date Class. Earth in Space

Chapter 8 2/19/2014. Lecture Outline. 8.1 The Galilean Moons of Jupiter. Moons, Rings, and Plutoids. 8.1 The Galilean Moons of Jupiter

Science Skills Station

Earth Science 11 Learning Guide Unit Complete the following table with information about the sun:

Grade 9 End semester exam Revision sheet Answer key. Kingdom of Bahrain Ministry of Education Ahlia School -ABCD

The escape speed for an object leaving the surface of any celestial body of mass M and radius d is

Ag Earth Science Chapter 23

The Jovian Planets. Huge worlds, heavily mantled in gas at the time of the formation of the Solar System.

Planetary Interiors. Earth s Interior Structure Hydrostatic Equilibrium Heating Constituent Relations Gravitational Fields Isostasy Magnetism

What is it like? When did it form? How did it form. The Solar System. Fall, 2005 Astronomy 110 1

Unit 2. Galaxies, Stars and the Solar System

Solar System Research Teacher Notes The Sun

The Solar System. Tour of the Solar System

Exploring The Planets: Jupiter

Chapter 16 Astronomy Study Guide. VOCABULARY WORDS TO KNOW geocentric system meteorite meteoroid

6 TH GRADE ACCURATE PLANET SIZES AND DISTANCE FROM THE SUN ACTIVITY

Comparative Planetology I: Our Solar System. Chapter Seven

What is the maximum mass, in grams, that could be measured by this balance?

Name: Pd Parent Signature of completion:

Joy of Science Experience the evolution of the Universe, Earth and Life

Astronomy 241: Foundations of Astrophysics I. The Solar System

1. Solar System Overview

GEOLOGY 12 CHAPTER 22 WORKSHEET COMPARATIVE PLANETOLOGY INTRODUCTION (VIDEO) Name

Transcription:

ACCEL: PATTERNS OF MASS AND DENSITY IN THE SOLAR SYSTEM Name: Date: Purpose: To investigate the patterns of mass, density, and size of planets in the solar system and compare the terrestrial and giant planets. Background: Mass is a measure of the amount of matter an object contains. The masses of the planets on the Planet Data Table are given in relation to Earth s mass. For example, mercury s mass is given as 0.056, which means that it contains only a small fraction of the matter that Earth contains. On the other hand, the giant planets contain several times more matter than Earth. Density is the amount of matter in a given amount of space, or the mass per unit volume of a substance. The average densities on the Planet Data Table are expressed in grams per cubic centimeter (g/cm 3 ). For density, the density of pure water is approximately 1 g/cm 3. Hypothesis: What relationship do you think you will observe between the mass, density, and size of planets. Procedure: Refer to the Planet Data Table handout to find the information needed to answer the following questions. Answer in complete sentences unless answer is a fill-in. 1. The planet is the most massive planet in the solar system. It is times more massive than Earth. 2. The least massive planet (excluding Pluto) is, which contains only as much mass as Earth. 3. How many times more massive than Mercury is Jupiter? times The gravitational attraction of a planet is directly related to its mass. In other words, as a planet s mass increases, its gravitational attraction increases. Your weight is a function of the gravitational attraction of an object acting on your mass. 4. Which planet exerts the greatest pull of gravity? Explain your answer. 5. On which planet would you weigh the least? Explain your answer. 6. Which of the two groups of planets: terrestrial or giant, would have the greatest ability to hold large quantities of gas as part of their composition? Explain your answer. 7. Write a general statement comparing the masses of the terrestrial planets to the masses of the giant planets.

8. Plot a point on the graph below for each planet (excluding Pluto). The point should be plotted where the planet s diameter intersects its density. Use the diameter measurements in kilometers from the Planet Data Table. Label each point with the planet s name. Use a different color for the terrestrial planets and the giant planets. Give the graph a title and include a key. 150 DIAMETER (km X 0) 50 0 0 1.0 2.0 3.0 4.0 5.0 6.0 DENSITY (g/cm 3 ) 9. What general relationship exists between a planet s diameter and its density? Circle your answers for the next two questions. 10. The densities of the two rock types that form the majority of Earth s surface, the igneous rocks granite and basalt, are each about 3.0 g/cm 3. The average densities of the terrestrial planets are (greater than, less than) the density of Earth s surface rocks. The average densities of the giant planets are (greater than, less than) the density of Earth s surface rocks. 11. The term (rocky/gaseous) best describes the terrestrial planets. 12. The average density of Earth is about 5.5 g/cm 3. Considering that the densities of Earth s surface rocks are much less than Earth s average density, you could infer that the center of the Earth is made of (rock/gas) that is (more than /less than) 5.5g/cm 3. 13. Which of the planets has a density less than water and could therefore float (if you could find a large enough container!)?

14. Explain why it is possible for Jupiter to be such a massive object and yet have such a low density. 15. Write a general statement comparing the densities of the terrestrial planets to the densities of the giant planets. 16. Why are the densities of the terrestrial and giant planets so different? 17. Examine the estimated mass, diameter and density of Pluto. Complete the following statements by circling the correct response. The mass of Pluto is most like the masses of the (terrestrial, giant) planets, while the density is similar to that of the (terrestrial, giant) planets. This suggests that Pluto is a (small, large) body made of (rock, ice and frozen gas). 17. Pluto makes up the Kuiper belt. What do you think the other objects in the Kuiper belt would be like in terms of density and composition (use the data in the chart and the patterns seen to support your statement)? 18. If the material in the asteroid belt (2.8AU) had coalesced to form a planet, what do you think it would have been like in terms of density and compostion? Would it likely have become a terrestrial planet or a Jovian planet? Explain your reasoning OTHER PATTERNS IN THE SOLAR SYSTEM Use the information in the Planet Data Table to explore some of the other relationships between the planets. 19. Describe the relationship between: (a) distance from the sun and a planet s period of revolution (b) distance from the sun and a planet s orbital velocity. 20. Describe the relationship between the number of moons (satellites) a planet has and (a) its mass. (b) its general distance from the sun. 21. How do the patterns you see between inner and outer planets fit in with the Nebular Hypothesis?What accounts for their differences?

PART 2 Density of Moons We know that rocks have an average density of 3.5g/cm 3 and ice has a density of 0.9 g/cm 3. We can calculate the density of a moon by using the following formula: (3.5 x percentage of rock) + (0.9 x percentage of ice) = density Scientists can estimate the mass of something by its gravitational pull and they can estimate its size using techniques like angular size. From this we can determine a density of objects in space. If we wanted to know the percentage that was ice or rock we would need to use the formula above except the problem is that there are now two unknowns (both the % ice AND the % rock). However because the two together must equal %, we can assume that the percentage of 1ce is always equal to minus % rock. So we can rewrite the equation as follows: (3.5 x % rock) + (0.9 x ( - %rock) = density Now you can simply solve for the % rock to figure out the portion of the objects density that is ice versus that which is water. 1. Use this formula to determine the % of rock for Jupiter s moon Callisto, which has a density of 1.8g/cm 3 Show your calculations and circle your answer. 2. What would be the % ice for Callisto? When dealing with lots of moons its is easiest to make a graph since there is a relationship between the % of rock and % ice and the density. Use the formula to complete the chart: (3.5 x percentage of rock) + (0.9 x percentage of ice) = density Percent rock Percent Ice Density of moon g/cm3 0 3.5 80 20 60 40 40 60 20 80 0 Make a line graph on the next page of the density of moon vs. the percent Rock. Give it a title.

DENSITY OF MOON 3.0 2.0 1.0 % ROCK 1. Jupiter s moon Ganymede has a density of 1.9 g/cm3. Based on your graph what percentage of it is rock? 2. Neptune s moon Triton has a density of 2.1 g/cm3 and would therefore be % rock. 3. Jupiter s moon Europa has a density of 3.0g/cm3. What is its % of rock? 4. How do you think the rock and ice is distributed inside the moons? Give the reason for your answer.