astronomy 1010-h planetary astronomy fall_2015 day-9

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Astronomy 1010-H Fall_2015 Day-9 Planetary Astronomy

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Page 1: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Astronomy 1010-HFall_2015

Day-9Planetary Astronomy

Page 2: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9
Page 3: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Course Announcements• Read Chapter 2• How is the lunar observing going?• How is the sunset/sunrise observing going?• 1st Quarter night – Mon. 9/21 -7:30pm – on campus• Exam 1: Fri. Sept. 18 or Mon. Sept. 21• This Week: APSU-OUR: Research & Creative Activity

Week. Events in the library 2:30-3:30 every day.

Page 4: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Spacecraft Reports• Chantal H. – New Horizons• Ashley G. – Dawn• Mahalia S. – NuStar• Tristan C. – Mangalyaan• Spencer B. – Voyager• Arielle P. – Curiosity Rover• Lars A. – Cassini• Sarah E. – Rosetta• John M. – Mars Phoenix• Jordan T. – Galileo• Rashun B. – Apollo Missions

Page 5: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Definitions & Terms -1• Season: A time

Page 6: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Stuff in Chapter 2• Coordinates• Position• Daily Motion (spin of Earth on its

axis)• Visibility of the sky• Year Motion (Earth orbits the Sun)• Seasons (tilt of the Earth’s axis)• Precession of the equinoxes• Motion and phases of the Moon• Eclipses

Page 7: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Earth’s Axis

Earth’s axis is not perpendicular to the ecliptic plane.

Instead, it is at an angle of 23.5 degrees. This is why there are seasons.

Page 8: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Earth’s Axis

The angle of sunlight is closer to perpendicular in summer.

Energy is more concentrated. The southern hemisphere is opposite the

northern hemisphere.

Page 9: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Special Days of the Year

Summer solstice: Sun farthest north.

Autumnal equinox: Sun on the equator, moving southward.

Winter solstice: Sun farthest south.

Vernal equinox: Sun on the equator, moving northward.

Page 10: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Lecture – TutorialPath of the Sun: pg 89

Work with a partner!Read the instructions and questions carefully.Discuss the concepts and your answers with

each other.Come to a consensus answer you both agree

on.If you get stuck or are not sure of your answer,

ask another group.If you get really stuck or don’t understand what

the Lecture Tutorial is asking, ask one of us for help.

Page 11: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9
Page 12: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Lecture – TutorialSeasons: pg. 93

Work with a partner!Yada Yada Yada …This one is homework

Page 13: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Stuff in Chapter 2• Coordinates• Position• Daily Motion (spin of Earth on its

axis)• Visibility of the sky• Year Motion (Earth orbits the Sun)• Seasons (tilt of the Earth’s axis)• Precession of the equinoxes• Motion and phases of the Moon• Eclipses

Page 14: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Precession

Currently, the north celestial pole is near the bright star Polaris.

Earth’s axis wobbles with a period of 26,000 years.

Location of the poles slowly shifts.

Page 15: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Earth wobbles like a top, slowly. Since the axis shifts, the equator shifts. Positions of the equinoxes precess as well.

Page 16: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Stuff in Chapter 2• Coordinates• Position• Daily Motion (spin of Earth on its

axis)• Visibility of the sky• Year Motion (Earth orbits the Sun)• Seasons (tilt of the Earth’s axis)• Precession of the equinoxes• Motion and phases of the Moon• Eclipses

Page 17: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

The Moon’s Motions

Because the orbit is elliptical and not circular, the rotation speed doesn’t always match the orbital speed.

Page 18: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Full Moon to Full Moon takes 29.53 days

Page 19: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9
Page 20: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9
Page 21: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

The moon takes the same amount of time to complete one rotation as it does to complete one orbit

Page 22: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Cycle of phases:The synodic month 29.53 days

The Orbital Period is the Sidereal Month: 27.32 days

Page 23: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Lecture – TutorialCause of Moon Phases: pg 81

Work with a partner!Read the instructions and questions carefully.Discuss the concepts and your answers with

one another.Come to a consensus answer you both agree on.If you get stuck or are not sure of your answer,

ask another group.If you get really stuck or don’t understand what

the Lecture Tutorial is asking, ask one of us for help.

Page 24: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Lecture – TutorialPredicting Moon Phases: pg 85

Work with a partner!Read the instructions and questions carefully.Discuss the concepts and your answers with

one another.Come to a consensus answer you both agree on.If you get stuck or are not sure of your answer,

ask another group.If you get really stuck or don’t understand what

the Lecture Tutorial is asking, ask one of us for help.

Page 25: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Course Announcements• Smartworks Chapter 2: Fri. 9/19

• Read Chapter 2, 3

• Dark Night Observing – • Tues. 9/16 & Wed. 9/24 – 7:30pm at the

Observatory

• Exam-1 – Friday Sept. 19• Bring L-T book to the Exam on Friday

Page 26: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Lecture – TutorialPredicting Moon Phases: pg 85

Work with a partner!Read the instructions and questions carefully.Discuss the concepts and your answers with

one another.Come to a consensus answer you both agree on.If you get stuck or are not sure of your answer,

ask another group.If you get really stuck or don’t understand what

the Lecture Tutorial is asking, ask one of us for help.

Page 27: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Stuff in Chapter 2• Coordinates• Position• Daily Motion (spin of Earth on its

axis)• Visibility of the sky• Year Motion (Earth orbits the Sun)• Seasons (tilt of the Earth’s axis)• Precession of the equinoxes• Motion and phases of the Moon• Eclipses

Page 28: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9
Page 29: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Three types of solar eclipses:• Total: The Moon

completely blocks the Sun’s light.

• Partial: Only part is blocked.

• Annular: The Sun appears as a bright ring surrounding the Moon.

Page 30: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Solar Eclipses

Solar eclipses happen at new Moon. Moon passes between Earth and the Sun. Only a small portion of Earth can witness

each one.

Page 31: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

The part of the Moon’s shadow you are in determines which type of solar eclipse you see.

Umbra: Total or annular. Penumbra: Partial.

Page 32: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Lunar eclipses happen at full Moon. Earth is between the Sun and the

Moon. Visible over a wider area of Earth. Last a lot longer than solar eclipses.

Page 33: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Eclipses do not occur every month because the Moon’s orbit is tilted 5.2° with respect to Earth’s orbit around the Sun.

Intersection: line of nodes.

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Page 35: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Next one is April 15, 2014 for

North America

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The Saros Cycle…18 years 11.3 days

Page 43: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

What Would You See on Mars?

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Page 45: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Projected Eclipse Times Eclipse Path Point of Greatest Eclipse

Lat.: 36.9664° NLong.: 87.6639° W Total Solar Eclipse Duration of Totality: 2m40.1s

APSU Observatory Lat.: 36.5631° N

Long.: 87.3433° W Total Solar EclipseDuration of Totality: 2m23.4s

Page 46: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Projected Eclipse Times APSU Observatory

Lat.: 36.5631° NLong.: 87.3433° W Total Solar EclipseDuration of Totality: 2m23.4sMagnitude: 1.008

Event Date Time (UT) Alt Azi (C1) : 2017/08/21 16:56:59.80 62.3° 149.7° (C2) : 2017/08/21 18:25:28.70 64.2° 198.9°

Max : 2017/08/21 18:26:40.50 64.1° 199.5° (C3) : 2017/08/21 18:27:52.10 64° 200.2° (C4) : 2017/08/21 19:52:25.50 53.4° 235.2°

Page 47: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Projected Eclipse Weather

Page 48: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Clarksville, TN

Page 49: Astronomy 1010-H Planetary Astronomy Fall_2015 Day-9

Two-Minute Essay My name is…

The scientist (living or dead, but real) I would most like to meet is: