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Lecture 4 ASTR 111 – Section 002
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Lecture 4

Jan 03, 2016

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Lecture 4. ASTR 111 – Section 002. Terms. While you are waiting for class to start, try to define these terms. Apogee/Perigee Subtend Parsec, light-year, AU Parallax Solar and Sidereal time Small angle formula Ecliptic Zenith Tropic of Cancer, Capricorn, Artic and Antarctic Circle - PowerPoint PPT Presentation
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Page 1: Lecture 4

Lecture 4

ASTR 111 – Section 002

Page 2: Lecture 4

Terms

• Apogee/Perigee• Subtend• Parsec, light-year, AU• Parallax• Solar and Sidereal time• Small angle formula• Ecliptic• Zenith• Tropic of Cancer, Capricorn, Artic and Antarctic Circle• Equinox, Solstice• Zodiac• Accuracy, Precision, and Bias

While you are waiting for class to start, try to define these terms

Page 3: Lecture 4

First Exam

• Slated for 9/29

• Based on lecture notes, problems worked in lecture, and quizzes.

• Approximately 50 questions

• In the Testing and Tutoring Center (using Blackboard system).

Page 4: Lecture 4

Tuesday September 15th• Class is canceled.

• Quiz is still due at 9 am on the 15th.

• I will be available via email.

Page 5: Lecture 4

Outline

1. Quiz Discussion

2. Rotation – review generally

3. The Seasons – review generally

4. The Moon in its orbit

5. Math review

Page 6: Lecture 4

Quiz Discussion

Page 7: Lecture 4
Page 8: Lecture 4

Outline

1. Quiz Discussion

2. Rotation – review generally

3. The Seasons – review generally

4. The Moon in its orbit

5. Math review

Page 9: Lecture 4

Rotation

Page 10: Lecture 4

Outline

1. Quiz Discussion

2. Rotation – review generally

3. The Seasons – review generally

4. The Moon in its orbit

5. Math review

Page 11: Lecture 4

The Seasons

Page 12: Lecture 4

Outline

1. Quiz Discussion

2. Rotation – review generally

3. The Seasons – review generally

4. The Moon in its orbit

5. Math review

Page 13: Lecture 4

• From http://www.dslreports.com/forum/remark,16822681• Uses color saturation http://

en.wikipedia.org/wiki/Saturation_(color_theory)

The Moon in its orbit

Page 14: Lecture 4

Eventually we want to be able to explain …

Page 15: Lecture 4

A simple model• Moon executes circular orbit

• Moon orbit is in Earth’s ecliptic plane

Page 16: Lecture 4
Page 17: Lecture 4

Looking down on North Pole

Can you “see” white ball if you are at Equator?

NO! You would need to see through Earth!

Page 18: Lecture 4

What is wrong with this picture?

Page 19: Lecture 4

Looking down on North Pole

Can you “see” white ball if you are at Equator?

Page 20: Lecture 4

Looking down on North Pole

If you walk around along the equator, where will you be able to see the white ball?

Page 21: Lecture 4

Looking down on North Pole

Can you “see” white ball if you are at Equator? NO! You would need to see through Earth!

NO!

Page 22: Lecture 4

Looking down on North Pole

Can you “see” white ball if you are at Equator? NO! You would need to see through Earth!

NO!

Page 23: Lecture 4

Looking down on North Pole

Closer to scale

Page 24: Lecture 4

• Draw a diagram that explains when you will first be able to see the first quarter moon if you live on the equator.

• Stated another way, at what time will you see the 1st quarter moon rise from Earth?

Page 25: Lecture 4
Page 26: Lecture 4

A

B

C

D

E

1. Fill in the dark and light parts of the Moon for A-D (from this perspective)

2. From the perspective of someone on Earth what position of A-E best fits the Moon view in the lower-left-hand corner?

3. In the blank boxes below, sketch how the Moon would appear from Earth from the four Moon positions that you did not choose for Question 2. Label each box with a letter.

Earth

View of Moon from Earth at one of thepositions (A-E) above.

Sun

’s r

ays

Page 27: Lecture 4

G

H

I

F

4. Shade in the part of the Moon that is not illuminated by the sun when it is at positions F-I.

5. Which Moon position (F-I) best corresponds with the Moon phase shown in the lower-left corner?

6. How much of the Moon’s surface is illuminated by the sun during this phase?

7. How much of the Moon’s illuminated surface is visible from Earth for this phase of the Moon?

Earth

View of Moon from Earth from one of the positions (F-I) above.

Sun

’s r

ays

Page 28: Lecture 4

A simple model• Moon executes circular orbit

• Moon orbit is in Earth’s ecliptic plane

Page 29: Lecture 4

Model can explain the phases of the Moon

• The phases of the Moon occur because light from the Moon is actually reflected sunlight

• As the relative positions of the Earth, the Moon, and the Sun change, we see more or less of the illuminated half of the Moon.

Page 30: Lecture 4

What does the Earth look like from the Moon at

• Full Moon

• New Moon

• First Quarter

• Third Quarter

Page 31: Lecture 4
Page 32: Lecture 4

What are 2 observations simple model does not predict?

1.

2.

Page 33: Lecture 4

What are 2 observations simple model does not predict?

1. Why there are not eclipses every month

2. Why there are “annular” and “total” eclipses

Page 34: Lecture 4

Eclipses occur only when the Sun and Moonare both on the line of nodes

Page 35: Lecture 4
Page 36: Lecture 4

What are 2 observations simple model does not predict?

1. Why there are not eclipses every month

2. Why there are “annular” and “total” eclipses of the sun

Page 37: Lecture 4

Solar eclipses can be either total, partial, orannular, depending on the alignment of

the Sun,Earth, and Moon

Page 38: Lecture 4
Page 39: Lecture 4
Page 40: Lecture 4

Eventually we want to be able to explain …

Page 41: Lecture 4

Lunar eclipses can be either total, partial, orpenumbral, depending on the alignment of

the Sun, Earth, and Moon

Page 42: Lecture 4

Question• If you were looking at Earth from the side

of the Moon that faces Earth, what would you see during– A total lunar eclipse?– A total solar eclipse?

Page 43: Lecture 4

The Moon’s rotation always keeps the same face toward the Earth due to synchronous rotation

Page 44: Lecture 4

• Two types of months are used in describing the motion of the Moon.

• With respect to the stars, the Moon completes one orbit around the Earth in a sidereal month, averaging 27.32 days.

• The Moon completes one cycle of phases (one orbit around the Earth with respect to the Sun) in a synodic month, averaging 29.53 days.

Time and the Moon

Page 45: Lecture 4
Page 46: Lecture 4

• sidereal month, averaging 27.32 days.

• sidereal day – 23 hr 56 min

• synodic (lunar) month, averaging 29.53 days.

• solar day – 24 hr

Page 47: Lecture 4

Question• On a certain date the Moon is in the

direction of the constellation Gemini as seen from Earth. When will the Moon next be in the direction of Gemini?

1. One year later?

2. 366.2425 days later?

3. One sidereal month later?

4. One synodic month later?

Page 48: Lecture 4

Outline

1. Quiz Discussion

2. Rotation – review generally

3. The Seasons – review generally

4. The Moon in its orbit

5. Math review

Page 49: Lecture 4
Page 50: Lecture 4