PROJECT 1: ORBIT OF MERCURY

• You may collaborate with your classmates but your submission should be your own work.

• Please answer questions in complete sentences and/or equations. Type or write legibly.

• The project is due in hard copy by 6 p.m. on Tuesday, September 25. You may hand it in in

class or in my drop box outside B-233. Late projects will

Name: Astronomy 1301

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• Go to the above website and find Mercury’s maximum elongations for 2016, 2017 and 2018.

Enter the data in the table below.

# date elongation

1

2

3

4

5

6

7

8

9

10

11

12

13

14

15

16

17

18

19

20

Name: Astronomy 1301

Fall 2018

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Drawing the orbit

Figure 21-1 shows Earth’s orbit, with the dates indicating Earth’s position throughout the year.

The scale is marked in astronomical units to allow you to convert measurements made on the

diagram into those units. The position of the Sun is indicated near the centre of Earth’s orbit.

To draw the orbit you will need a sharp pencil (the width of even a sharp pencil line on the

diagram is about 100,000 km), a millimetre ruler and a protractor. Now plot each elongation of

Mercury on the diagram as follows:

• Locate the date of the maximum elongation on Earth’s orbit. Draw a light pencil line from

Earth’s position to the Sun.

• Centre the protractor on Earth’s position and construct a line, so that the angle from this

constructed line to the Earth-Sun line is equal to the maximum elongation. Extend this line

well past the Sun. It represents the direction toward Mercury. Remember that, facing the Sun

from Earth, eastern elongations are to the left and western ones to the right, as shown in

Figure 21-2. On the date in question Mercury was somewhere along the sight line you have

drawn.

• Number the lines in chronological order.

• After you have plotted all the data, sketch in the orbit of Mercury. The orbit must be a

smooth, closed curve that just touches each of the sight

Name: Astronomy 1301

Fall 2018

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Name: Astronomy 1301

Fall 2018

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Questions

• Does it appear that the curve you have drawn is a circle? How can you tell? Be specific.

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Kepler had the same problem: his orbit was not a circle either. Eventually he hit on the idea of

using ellipses for orbits.

• On Figure 21-1 draw the longest diameter possible of the orbit of Mercury. Note that this

diameter must pass through the Sun. This is the major axis of the ellipse.

• Measure the major axis and bisect it to find the centre of the ellipse. Draw the minor axis

through the centre of the ellipse and perpendicular to the major axis.

• What is your “observed” value of the semimajor axis of Mercury’s orbit in cm as measured

on Figure 21-1?

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• What is your “observed” value of the semimajor axis of Mercury’s orbit in AU? Show the

conversion from cm to AU obtained using the scale at the bottom of Figure 21-1.

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• What is the accepted value of the semimajor axis of Mercury’s orbit in AU?

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Combining the information from the orbit you drew with the chronologically numbered sight

lines, you now know where Mercury was in its orbit on those dates.

• Find two orbital positions on different dates that are as close to one another along Mercury’s

orbit as possible. Mark these two positions on Figure 21-1 and write the corresponding dates

on the line below.

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Name: Astronomy 1301

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• How many days elapsed between those two dates?

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• How many orbits did Mercury complete between those two dates? (Hint: To determine the

number of orbits completed, you may find it helpful to number the positions where the sight

lines are tangent to Mercury’s orbit in chronological order.)

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• From the time elapsed and the number of orbits completed between the two dates, calculate

the orbital (i.e. sidereal) period of Mercury in days. This is your “observed” value of the

period. Show your calculation.

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• What is the accepted value of the orbital period of Mercury in days?

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• Kepler’s Third Law states that the orbital period squared equals the semimajor axis cubed,

2 = 3. Use your “observed” value of and Kepler’s Third Law to calculate in days. Show

your calculation. (Hint: In the above formula is in years.)

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• Compare the calculated and “observed” values of . Are the orbital parameters you found

for Mercury consistent with Kepler’s Third Law? Explain.

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Name: Astronomy 1301

Fall 2018

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The Sun lies at one of the foci of the elliptical orbit. Measure the distance from the Sun to the

centre of the ellipse and call it . The ratio =

is the eccentricity of the ellipse.

• What is your “observed” value of the eccentricity of Mercury’s orbit? Show your calculation.

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• What is the accepted value?

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• Use http://www.fourmilab.ch/images/3planets/elongation.html to find the first maximum

elongation for Mercury in 2020. Write down the date and the maximum elongation below

and plot it on Figure 21-1. Mark the line from Earth to Mercury in red. Is it tangent to

Mercury’s orbit?

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