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Page 1: J anuary 6th, 2012

January 6th, 2012

WARM UP: When viewed from the northern hemisphere, describe the position of the sun, at sun rise and sunset, on the local horizon, on the following points on the calendar: Vernal Equinox, Summer Solstice, Autumnal Equinox and the Winter Solstice.

1) Warm up 2) Discussions: Phases of the Moon and Task Analysis

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

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January 6th, 2012 FORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Milankovitch Cycle seasons, phases, eclipses, penumbra, umbra, synodic, sidereal

.

NOTES: Quiz Friday, Phases of the Moon

PRACTICE:

ASSIGNMENTS: Seasons

Seasons, Path of the Sun, Phases of the Moon.

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January 5th, 2012

WARM UP: How do we define the magnitude of stars? What is the intensity ratio between a magnitude -1 star and a 0 magnitude star?`

1) Warm up 2) Discussions: Seasons (2 and 5) Task Analysis Phases of the Moon (1,3,inish 4, 6) and Task Analysis

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

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January 5th, 2012 FORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Milankovitch Cycle seasons, phases, eclipses, penumbra, umbra, synodic, sidereal

.

NOTES: Quiz Friday, Phases of the Moon

PRACTICE:

ASSIGNMENTS: Seasons

Seasons, Path of the Sun, Phases of the Moon.

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January 4th, 2012

WARM UP: Define the following: Astronomical Unit (AU), Light Year (ly) and Parsec (PC). How is each used?

1) Warm up 2) Discussions: Seasons (finish for periods 2) and Task Analysis3) Phases of the Moon (1,3,5, Finish 4, 6) and Task Analysis

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

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January 4th2012 FORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Milankovitch Cycle seasons, phases, eclipses, penumbra, umbra, synodic, sidereal

.

NOTES: Quiz Friday, Phases of the Moon

PRACTICE:

ASSIGNMENTS: Seasons

Seasons, Path of the Sun, Phases of the Moon.

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January 3rd, 2012

WARM UP: Over the break, you probably had a chance to look at the night sky. What things were you able to observe and understand (even casually). What things are you able to share. If you did not observe the sky over break…well then you have failed this course. Welcome back!

1) Warm up 2) Discussions: Seasons (finish for periods 2)3) Phases of the Moon (1,3,5, Finish 4, 6)

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

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January 3rd, 2012 FORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Milankovitch Cycle seasons, phases, eclipses, penumbra, umbra, synodic, sidereal

.

NOTES: Quiz Friday, Phases of the Moon

PRACTICE:

ASSIGNMENTS: Seasons

Seasons, Path of the Sun, Phases of the Moon.

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December 15th, 2011 Honors Astronomy

WARM UP: Next Slide

1) Warm up 2) Discussions: Seasons (finish for periods 1,3,5)3) Phases of the Moon (Finish 4, 6)4) QUIZ RETAKE If you were not here Monday.

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

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A dime is 1.8 cm in diameter. Earth's moon is 3.844 x 105 km from Earth and has a diameter of 3.76 x 103 km. At what distance from your eye would you have to hold a dime so that it has the same angular diameter as the full moon (that it would cover the moon.) HINT: Drawing a picture will help you if your math skills have left the room)

a. 200 cmb. 2 cmc. 0.2 cmd. 2 AUe. 2 LY

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December 15th, 2011 Honors AstronomyFORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Milankovitch Cycle seasons, phases, eclipses, penumbra, umbra, synodic, sidereal

.

NOTES:.

PRACTICE:

ASSIGNMENTS: Seasons

Seasons, Path of the Sun, Phases of the Moon.

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December 14th, 2011 Honors Astronomy

WARM UP: What are solstices and equinoxes? When do they occur and what is the position of the sun on the celestial sphere for each solstice and equinox?

1) Warm up 2) Discussions: Seasons3) Phases of the Moon4) QUIZ RETAKE If you were not here yesterday.

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

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December 14th, 2011 Honors AstronomyFORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Milankovitch Cycle seasons, phases, eclipses, penumbra, umbra,

.

NOTES:.

PRACTICE:

ASSIGNMENTS: Seasons

Seasons

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December 13th, 2011 Honors Astronomy

WARM UP: Next Slide – Please do not simply write the letter!

1) Warm up 2) Discussions: Seasons3) Phases of the Moon4) QUIZ RETAKE ON TUESDAY DEC 13th . STUDY SEC 2.2-2.4

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

ASSIGNMENTS: Video Questions. DO NOT LOSE VIDEO HANDOUTS! Last 20 minutes replayed 12/12, 12/15 after school – if there is interest I can set up a session before school or during lunch. Alternate Observation Assignment will be assigned when I get back tomorrow.

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A. Yes, precession will naturally circularize the Earth’s orbit.

B. Yes, precession will eventually reduce the Earth’s axis tilt.

C. No, precession only changes the direction in which the North Pole points, and has nothing to do with the seasons.

D. Yes, precession will make summers occur at the same time, but in what is now the northern spring and southern fall.

E. Yes, but it would take tens of thousands of years, longer than current human history, for this to occur.

Because of precession, someday it will be summer everywhere on Earth at the same time.

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December 13, 2011 Honors AstronomyFORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Malinkovitch Cycle seasons, phases, eclipses, penumbra, umbra,

.

NOTES:.

PRACTICE:

ASSIGNMENTS: Seasons

Seasons

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December 12th, 2011 Honors Astronomy

WARM UP: What is a “light bucket” and why is it called a “light bucket” (Please continue on last week’s sheet)

1) Warm up 2) Discussions: Seasons3) Phases of the Moon4) QUIZ RETAKE ON TUESDAY DEC 13th . STUDY SEC 2.2-2.4

ESSENTIAL QUESTION:What causes the phases of the moon

AGENDA

LEARNING OBJECTIVE:Be able to describe the phases of the moon as it revolves around the Earth.

ASSIGNMENTS: Video Questions. DO NOT LOSE VIDEO HANDOUTS! Last 20 minutes replayed 12/12, 12/15 after school – if there is interest I can set up a session before school or during lunch. Alternate Observation Assignment will be assigned when I get back tomorrow.

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December 12, 2011 Honors AstronomyFORMATIVE ASSESSMENT: .

Teacher led Questions on student’s understanding of today’s lesson.VOCABULARY: Solstice, Equinox, Malinkovitch Cycle seasons, phases, eclipses, penumbra, umbra,

.

NOTES:.

PRACTICE:

ASSIGNMENTS: Seasons

Seasons

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Per. 1 , 3 , 5What the differences between diurnal and annual motion?Period 6How do the shadows of a stick vary from hour to hour and season to season?

What are solstices and equinoxes? When do they occur and what is the position of the sun on the celestial sphere for each solstice and equinox?

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Conjunction

OppositionSuperior Conjunction

Inferior Conjunction AphelionPe

rihelion

EARTH

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For your concept maps – please draw!

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

Objects are located on the celestial sphere in units of:

A. MilesB. KilometersC. Light yearsD. ParsecsE. Degrees

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

The angular size of your fist, held at arms length, is about:

A. 1 degreeB. 10 degrees C. 5 inchesD. 10 inches

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

The apparent size of the moon in the sky is:

A. About ½ degreeB. About 5 degreesC. About 10 degreesD. About a mileE. About 2000 miles (1/4 the earth’s diameter)

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

What makes Polaris a special star?

A. It is the brightest star in the skyB. It is always directly overhead, no matter where you areC. It is near the axis about which the sky turnsD. Its azimuth (direction) is always due northE. C and D

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

When an astronomer describes the altitude of something in the local sky, he or she means:

A. How high something is in the sky, in units of miles or kilometers

B. How high something is in the sky, in units of degreesC. The direction toward something– north, south, east, or

west

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

During the year the Sun appears in front of different groups of stars. What are these called?

A. Circumpolar starsB. Circumsolar starsC. The constellations of the zodiacD. The tropical constellationsE. Solstice stars

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

When an astronomer describes the azimuth of something in the local sky, he or she means:

A. How high something is in the sky, in units of miles or kilometers

B. How high something is in the sky, in units of degreesC. The direction toward something– north, south, east, or

west

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

Why are different stars seen in different seasons?

A. The tilt of the Earth’s axisB. Stars move during the yearC. As the Earth orbits the Sun we see the Sun in front of

different constellations D. Because that’s how horoscopes workE. Precession

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

Why are the Moon and planets seen only in the constellations of the zodiac?

A. The planets all revolve in the same direction around the Sun

B. The planets all orbit in nearly the same plane, and the zodiacal constellations are in that plane.

C. The constellations in the zodiac are the oldest, and the planets have been known from ancient times

D. None of the above reasons

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

When it is summer in the United States, in Australia it is:

A. WinterB. SummerC. It is always summer in Australia

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

What causes the seasons?

A. In summer the (whole) Earth is closer to the SunB. In summer the tilt of the Earth’s axis makes the part of the

Earth we are on closer to the SunC. In summer the Sun is up for more hoursD. In summer the Sun climbs higher in the sky so its rays hit

the ground more directlyE. C and D

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

If the tilt of the Earth’s axis to its orbital plane was 40 degrees, instead of 23 ½, but its distance from

the Sun remained the same, what would happen to the seasons?

A. They wouldn’t change muchB. They would become less extreme–winter and summer

would be more alikeC. They would become more extreme–winter colder and

summer warmerD. The whole Earth would get colderE. The whole Earth would get warmer

Page 34: J anuary 6th, 2012

Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

A. It was the first star to be cataloged by ancient astronomers.

B. It lies close to the north celestial pole and is therefore very useful for navigation.

C. It is the brightest star in the entire sky.D. It is the brightest star in the northern sky.E. It is visible from both the northern and southern

hemispheres.

What makes the North Star special?

Page 35: J anuary 6th, 2012

Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

A. Yes, precession will naturally circularize the Earth’s orbit.B. Yes, precession will eventually reduce the Earth’s axis tilt.C. Yes, precession will make summers occur at the same time,

but in what is now the northern spring and southern fall.D. Yes, but it would take tens of thousands of years, longer than

current human history, for this to occur.E. No, precession only changes the direction in which the North

Pole points, and has nothing to do with the seasons.

Because of precession, someday it will be summer everywhere on Earth at the same time.

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Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

In the northern hemisphere When is the Sun directly overhead at noon?

A. March 21B. June 21C. July 21D. Never

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Reality Check for Mr. HellmundBecause I have too many scattered notes: I need to get a feel where we are. Have you done:1) Slides:

1) Per 1 - Seasons Slide #82) Per 2 – Start Seasons3) Per 3 – Seasons Slide #84) Per 4 – Phases Slide?5) Per 5 – Seasons Slide ?6) Per 6 – Phases slide 8

2) Thinking Map – Rotation/Revolution/Precession3) Thinking Map – Celestial Sphere4) Task Analysis: Seasons5) Practice: Seasons

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