Eclipses September 12th, 2013

Similar documents
Dive into Saturn.

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc.

Observing the Universe for Yourself

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc.

Phases of the Moon. Two perspectives: On Earth, or outside the Moon s orbit. More Phases. What if we zoom out? Phases of the Moon Demo 2/3/17

The changing phases of the Moon originally inspired the concept of the month

The Cause of the Seasons

Explain how Earth's movement and the moon's orbit cause the phases of the moon. Explain the difference between a solar eclipse and a lunar eclipse.

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself

Day, Night & the Seasons. Lecture 2 1/21/2014

Introduction To Modern Astronomy II

Astr 1050 Mon. Jan. 31, 2017

The Earth-Moon-Sun System. I. Lunar Rotation and Revolution II. Phases of the Moon III. Lunar Eclipses IV. Solar Eclipses

Astronomy 115 Section 4 Week 2. Adam Fries SF State

How can we describe the motion of the sun in the sky? Where is the Sun at noon today? What about the path of the Sun?

Exam 1 is Feb. 1 (next Tuesday) This will cover everything we have done so far Earth motions The celestial sphere and observations from Earth Seasons

2.2 The Reason for Seasons

Welcome back. Scale. Week 2 Updates. PHYS 1302 Astronomy of the Solar System

Locating the Planets (Chapter 19) and the Moon and Sun (Chapter 21)

Locating the Planets (Chapter 20) and the Moon and Sun (Chapter 22)

The Celestial Sphere. Chapter 1. Constellations. Models and Science. Constellations. Diurnal vs. Annular Motion 9/16/2010

1. The pictures below show the Sun at midday. Write winter, spring or summer under the correct picture.

Motion of the Sun. motion relative to the horizon. rises in the east, sets in the west on a daily basis. Basis for the unit of time, the DAY

2.1 Patterns in the Night Sky

Chapter 3: Cycles of the Sky

Academic Year Second Term. Science Revision Sheet. Grade

Brock University. Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014

STANDARD. S6E1 d: Explain the motion of objects in the day/night sky in terms of relative position.

The Moon -Around the Earth and in the Sky

At Home Phases Demo. Astronomy 210. Section 1 MWF Astronomy Building. Geocentric vs. Heliocentric system. The Motion of the Planets

The celestial sphere, the coordinates system, seasons, phases of the moon and eclipses. Chapters 2 and S1

12.2. The Earth Moon System KNOW? The Phases of the Moon. Did You

PHYSICS 107. Lecture 4 Ancient Astronomy

Astronomy. Today: Eclipses and the Motion of the Moon. First homework on WebAssign is due Thursday at 11:00pm

REVIEW CH #0. 1) Right ascension in the sky is very similar to latitude on the Earth. 1)

Earth in Space. The Sun-Earth-Moon System

[04] Seasons, Phases, and Eclipses (9/7/17)

The Sun-Earth-Moon System

The. Astronomy is full of cycles. Like the day, the month, & the year In this section we will try to understand these cycles.

Name: Exam 1, 9/30/05

The ecliptic and the sidereal motion of the sun Moon and the planets on it.

Term Info Picture. A celestial body that orbits a bigger celestial body (a moon) Earth s only natural satellite. It causes all of the tides.

Patterns of Change on Earth

Directions: Read each slide then fill in the blanks.

Name: Earth and Space Assessment Study Guide. Assessment Date : Term Rotation Revolution

Today. Tropics & Arctics Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME

Earth is rotating on its own axis

Brock University. Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016

SPI Use data to draw conclusions about the major components of the universe.

Announcements. Astronomical perspective. The Greek Model of the Solar System Geocentric model (because the Earth is at the center)

Name(s): Date: yourself (representing the Earth, with your nose representing the location of Las Cruces) Work in Groups of Three People!

Today FIRST HOMEWORK DUE NEXT TIME. Phases of the Moon. Eclipses. Lunar, Solar. Ancient Astronomy

ASTR 1P01 Test 1, September 2018 Page 1 BROCK UNIVERSITY

Lecture 3 Angular Sizes, Moon Phases, and Ptolemy September 13, 2017

Homework 1 (from text) Latest Deep Impact Results: 2. Discovering the Universe for Yourself.

Intro to Astronomy. Looking at Our Space Neighborhood

3. Lunar Motions & Eclipses. Lunar Phases: Static & Dynamic. Static & Dynamic Lunar Phases. Earth & Moon: Both Show Phases!

Position 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.

3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.

1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.

AST 301 Introduction to Astronomy

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky.

Today. Solstices & Equinoxes Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME

Astronomy 101 Lab: Lunar Phases and Eclipses

TEK 8.7B Demonstrate and predict the sequence of events in the lunar cycle. Moon Phases or the Lunar Cycle

BROCK UNIVERSITY. Test 1: October 2014 Number of pages: 9 Course: ASTR 1P01, Section 2 Number of students: 950

Using Angles. Looking at the Night Sky. Rising and Setting Stars. Nightly Motion of the Stars. Nightly Motion of the Stars

Happy Tuesday! Pull out a half sheet of paper or share a whole with a friend!

Remember that for one of your observing projects you can go to a star party (stargazing). This is available at the Lawrence Hall of Science every 1st

ASTR 1P01 Test 1, May 2018 Page 1 BROCK UNIVERSITY. Test 1: Spring 2018 Number of pages: 10 Course: ASTR 1P01, Section 1 Number of students: 598

b. So at 12:00 p.m., are the shadows pointing in the direction you predicted? If they are not, you must explain this observation.

The sun then falls below the horizon, and it is nighttime for our little person:

2007 TU24. Astronomy 122. Compass Grading 2007 TU24. An asteroid cometh..

a. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU

3. a. In the figure below, indicate the direction of the Sun with an arrow.

What is in outer space?

The reason is that the Moon s rotation takes 27.3 days the same amount of time it takes to revolve once around Earth. Because these two motions take

Lunar Phases. (Ping Pong and Globe demo of phases).

Brock University. Test 1, October 2017 Number of pages: 9 Course: ASTR 1P01, Section 1 Number of Students: 470 Date of Examination: October 3, 2017

THE SUN-EARTH-MOON SYSTEM

ASTR 1P01 Test 1, September 2017 Page 1 BROCK UNIVERSITY

Chapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM)

Lecture 2: Motions of the Earth and Moon. Astronomy 111 Wednesday August 30, 2017

Astronomy 122 Section 1 TR Digital Computer Laboratory. Outline. Celestial Sphere. Motions in the Sky

Chapter 3 Cycles of the Moon

A. The moon B. The sun C. Jupiter D. Earth A. 1 B. 2 C. 3 D. 4. Sky Science Unit Review Konrad. Here is a selection of PAT style questions.

Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest).

Exploration Series. PHASES OF THE MOON Interactive Physics Simulation Page 01

Astronomy Club of Asheville January 2016 Sky Events

Copy the red text for your notes. Space Unit. Lesson 1. P , ScienceLinks 9 Chapter 13, SciencePower 9

1st Grade. Slide 1 / 90. Slide 2 / 90. Slide 3 / 90. The Sun, Moon, Earth and Stars. Table of Contents The Sun.

8 th Grade Earth, Moon and Sun Systems Review

The full, blue supermoon is coming to the night sky near you

Lecture 19: The Moon & Mercury. The Moon & Mercury. The Moon & Mercury

A) M D) The Moon s distance from Earth varies in a cyclic manner.

Chapter Introduction Lesson 1 Earth s Motion Lesson 2 Earth s Moon Lesson 3 Eclipses and Tides Chapter Wrap-Up. Jason Reed/Photodisc/Getty Images

Name: Date: 5. The bright stars Vega, Deneb, and Altair form A) the summer triangle. B) the winter triangle. C) the Big Dipper. D) Orion, the Hunter.

Transcription:

Eclipses September 12th, 2013

Who was the favorite Star Wars character of the class? A) Obi-Wan B) Jar Jar C) Luke Skywalker D) Yoda

News! Dark matter http://mcdonaldobservatory.org/news/releases/2013/09/10 New black holes http://www.space.com/22736-monster-black-holes-nasadiscovery.html

Review - Seasons Question 22: What are the two things most directly responsible for making summer warm and winter cold? Which of these has the strongest impact on the seasons? The least? A) Varying distance between Earth and Sun B) One hemisphere being slightly closer to the Sun than the other C) The Earth s axial tilt What axial tilt would cause the most extreme seasons? The least extreme?

Review from last time Every 27.3 days, the Moon completes one orbit around the Earth. Every 29.5 days, the Moon returns to its same position relative to the Sun in the sky. The 29.5 day cycle of illumination patterns are called the phases of the Moon. The rotation period of the Moon (its day ) is also 27.3 days. This is because the Moon is tidally locked, so we always see the same side. During a crescent Moon, we can see the rest of the Moon illuminated faintly due to Earth-shine.

Do you know your phases?!? First quarter Waxing crescent New Waxing gibbous Full Waning gibbous Third quarter Waning crescent

Question What phase is this? A) Waxing crescent Lets check out an animation. B) Waning Crescent C) New D) Waxing gibbous

Description: The figure below shows a top view of the Sun, Earth and six different positions (A - F) of the Moon during one orbit of Earth. Note that the distances shown for the Sun to Earth and for Earth to the Moon are not drawn to scale. Ranking Instructions: Rank (from greatest to least) the amount of the Moon s illuminated surface that is visible from Earth at each of the six positions (A F) shown. Ranking Order: Greatest 1 2 3 4 5 6 Least Or, the amount of the Moon s illuminated surface visible from Earth is the same in all positions. (indicate with check mark). Carefully explain your reasoning for ranking this way:

Which position of the Moon best corresponds with the moon phase that shown at the upper right?

Tutorial: Cause of Moon Phases - p. 81 Work with a group of 2-3 people. Read the instructions and questions carefully Talk to each other and discuss your answers with each 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 as one of us for help. We will discuss as a class when done.

What causes eclipses? The Earth and Moon cast shadows. When either passes through the other's shadow, we have an eclipse.

Types of eclipses A lunar eclipse occurs when the Earth is directly between the Sun and the Moon. The Earth s shadow falls on the Moon. A solar eclipse occurs when the Moon lies directly between the Sun and the Earth. The Moon s shadow falls on the Earth.

Question At which position is a Solar eclipse possible? At which position is a Lunar eclipse possible? B A C D

Question Which of these statements is correct: a) Both solar and lunar eclipses occur during new moon. b) Both solar and lunar eclipses occur during full moon. c) Solar eclipses occur during new moon, and lunar eclipses occur during full moon. d) Lunar eclipses occur during new moon, and solar eclipses occur during full moon.

Why don t we have an eclipse every month? If the Moon s orbital plane was exactly aligned with the ecliptic, we should have a solar eclipse every new moon, and a lunar eclipse every full moon. However, the Moon s orbital plane is off the ecliptic by 5 degrees. To have an eclipse, the new or full moon has to occur at one of the nodes of the Moon s orbit - the point where the orbit crosses the ecliptic.

Lunar eclipse When the Earth blocks the sunlight from hitting the Moon for several hours, occurs when the Moon is in the full phase. The Moon does not go completely dark - rather, it turns a reddish color, due to sunlight hitting the moon after going through the Earth s atmosphere. Its reflecting the light from all of the sunrises and sunsets going on at that time.

There are a few types of solar eclipses. The Moon s orbit isn t perfectly circular, so we only see a total eclipse when the new moon occurs at a node at the closest point it its orbit. An annular eclipse occurs when the Moon is at a farther point in its orbit, so its angular size is not large enough to block out the entire Sun. A partial eclipse occurs if you are at a spot on the Earth that does not get completely covered by the Moon s shadow.

Solar Eclipse Annular Eclipse Partial Eclipse Total Eclipse

Image of eclipse I took from Kyoto, Japan in May 2012. What kind of eclipse is this? A) Lunar B) Annular Solar C) Partial Solar D) Total Solar

Motions of the Planets Planets known in ancient times: Mercury difficult to see; always close to Sun in sky Venus very bright when visible; morning or evening "star" Mars noticeably red Jupiter very bright Saturn moderately bright

What was once so mysterious about planetary motion in our sky? Planets usually move slightly eastward from night to night relative to the stars. But sometimes they go westward relative to the stars for a few weeks: apparent retrograde motion.

We see apparent retrograde motion when we pass by a planet in its orbit. Animation

Explaining Apparent Retrograde Motion Easy for us to explain: occurs when we "lap" another planet (or when Mercury or Venus laps us). But very difficult to explain if you think that Earth is the center of the universe! In fact, ancients considered but rejected the correct explanation. More about this next time.

Homework Don t forget to turn in your sheet of paper! Read text: Section 3.1, 3.2, 3.3 Mastering Astronomy Homework #4 Due by 7:00am Tuesday 9/17/13.