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

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

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

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

Today FIRST HOMEWORK DUE. Ancient Astronomy. Competing Cosmologies. Geocentric vs. Heliocentric. Ptolemy vs. copernicus.

Observing the Universe for Yourself

Chapter 3 The Science of Astronomy

Chapter 2 Discovering the Universe for Yourself

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

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

2.2 The Reason for Seasons

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

2.1 Patterns in the Night Sky

The Cause of the Seasons

Dive into Saturn.

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

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

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

The Moon -Around the Earth and in the Sky

Introduction To Modern Astronomy II

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

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

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

Discovering the Night Sky

Discovering the Night Sky

Astronomy 110 Lecture Fall, 2005 Astronomy 110 1

The Ecliptic on the Celestial. Sphere. The Celestial Sphere. Astronomy 210. Section 1 MWF Astronomy Building. celestial equator are not

Chapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods?

Knowing the Heavens. Chapter Two. Guiding Questions. Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations

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.

1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d.) Ecliptic

Astronomy 11. No, this course isn t all about Star Wars

Eclipses September 12th, 2013

Chapter 0 2/19/2014. Lecture Outline. 0.1 The Obvious View. Charting the Heavens. 0.1 The Obvious View. 0.1 The Obvious View. Units of Chapter 0

Last time we finished Ch. 2

Astronomy 103: First Exam

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

Astronomy. Unit 2. The Moon

Chapter 3 Cycles of the Moon

Astr 1050 Mon. Jan. 31, 2017

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

Astronomy is the oldest science! Eclipses. In ancient times the sky was not well understood! Bad Omens? Comets

Dr. Tariq Al-Abdullah

Discovering the Universe for Yourself

Orbital Mechanics. CTLA Earth & Environmental Science

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

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.

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

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations.

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

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.

Lunar Motion. V. Lunar Motion. A. The Lunar Calendar. B. Motion of Moon. C. Eclipses. A. The Lunar Calendar. 1) Phases of the Moon. 2) The Lunar Month

Summary Sheet #1 for Astronomy Main Lesson

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

Unit 2. Cycles of the Sky

from The Walrus and the Carpenter Through the Looking-Glass -- Lewis Carroll

2. Modern: A constellation is a region in the sky. Every object in the sky, whether we can see it or not, is part of a constellation.

The Sun-Earth-Moon System

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

A100 Exploring the Universe: The Invention of Science. Martin D. Weinberg UMass Astronomy

Eclipses - Understanding Shadows

A User s Guide to the Sky

HNRS 227 Fall 2007 Chapter 14. Earth in Space presented by Prof. Geller 25 October 2007

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

Lecture 4. Dealing with multiple motions

Chapter S1 Lecture. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc.

Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION

18.2 Earth Cycles Days and years Calendars Years and days Leap years Calendars throughout human history 20,000 years ago. 7,000 BC. 4,000 BC.

Announcements. Homework 1 posted on Compass

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

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.

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

Chapter 3 The Science of Astronomy

b. Assuming that the sundial is set up correctly, explain this observation.

The Earth and the Moon. The Moon is our nearest neighbour. It crosses the sky at ~12º per day, or its own diameter (~30 arc minutes) in ~ 1 hour

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1

Chapter 22.2 The Earth- Moon-Sun System. Chapter 22.3: Earth s Moon

Introduction To Modern Astronomy I: Solar System

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

Appearance of the Sky Orientation Motion of sky Seasons Precession (?)

Chapter 1 Image Slides. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

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

Daily & Annual Motions

Chapter 3: Cycles of the Sky

The position of the Sun on the celestial sphere at the solstices and the equinoxes.

Ancient Astronomy. Lecture 3 February 14, Course website:

Solar System Glossary. The point in an object s elliptical orbit farthest from the body it is orbiting

What did ancient civilizations achieve in astronomy?

Academic Year Second Term. Science Revision Sheet. Grade

Guiding Questions. Discovering the Night Sky. iclicker Qustion

Benefit of astronomy to ancient cultures

PHYSICS 107. Lecture 4 Ancient Astronomy

A Warm Up Exercise. The Motion of the Sun. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise

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

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.

Today in Space News: Earth s oldest rock found on the Moon.

James T. Shipman Jerry D. Wilson Charles A. Higgins, Jr. Chapter 15 Place and Time

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

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

Transcription:

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

Tropic: Latitude where the sun [just] reaches the zenith at noon on the summer solstice Arctic/Antarctic Circle: Latitude where the sun does not set [just barely] on the summer solstice (like a circumpolar star) nor does it rise on the winter solstice arctic Ecliptic plane Equator 23.5 o Tropic of Cancer 66.5 o Tropic of Capricorn antarctic

Precession: the orientation of Earth s axis slowly changes with time: The tilt remains about 23.5 degrees (so the season pattern is not affected), but Earth has a 26,000 year precession cycle that slowly and subtly changes the orientation of the Earth s axis. The discovery of precession is attributed to the Ancient Greek astronomer Hipparchus (c. 280 BC)

Lunar phases Lunar phases are a consequence of the Moon s 27.3-day orbit around Earth. This is the sidereal period - how long it takes to complete one orbit. The synodic period - full moon to full moon - is 29.5 days

Phases of Moon Half of the Moon is illuminated by the Sun and half is dark. We see a changing combination of the bright and dark faces as the Moon orbits Earth. Phases of the Moon

Phases of the Moon: 29.5-day cycle new crescent first quarter gibbous full } Synodic (observed) period waxing Moon visible in afternoon/evening Gets fuller and rises later each day gibbous last quarter crescent } waning Moon visible in late night/morning Gets less and sets later each day

We see only one side of the Moon Synchronous rotation: The Moon rotates exactly once with each orbit. This is why only one side is visible from Earth. This is an example of tidal locking in which the spin rate of a smaller moon is coupled to its orbital period around a larger planet.

Eclipses The Earth and Moon cast shadows. When either passes through the other s shadow, we have an eclipse. A lunar eclipse is when the Earth shades the Moon. A solar eclipse is when the Moon shades the Earth.

Lunar Eclipse Lunar Eclipse

When can eclipses occur? Lunar eclipses can occur only at full moon when the earth is between the sun and moon. Lunar eclipses can be penumbral, partial, or total.

much longer exposure

12

Solar Eclipse Evolution of a Total Solar Eclipse

When can eclipses occur? Solar eclipses can occur only at new moon when the moon is between the earth and the sun. Solar eclipses can be partial, total, or annular. It is a coincidence that the angular size of the sun and moon are approximately equal.

Why don t we have an eclipse at every new and full moon? The Moon s orbit is tilted 5 to ecliptic plane. So we have about two eclipse seasons each year, with a lunar eclipse at new moon and solar eclipse at full moon. Play Moon s orbit & ecliptic

Summary: Two conditions must be met to have an eclipse: 1. It must be a full moon (for a lunar eclipse) or a new moon (for a solar eclipse). AND 2. The Moon must be at or near one of the two points in its orbit where it crosses the ecliptic plane (its nodes).

Predicting Eclipses Eclipses recur with the 18 year, 11 1/3 day saros cycle, but type (e.g., partial, total) and location may vary. Next up: Aug 21, 2017 a few hundred miles south of Cleveland

Astronomical observations were important to ancient societies In keeping track of time and seasons for practical purposes, including agriculture for religious and ceremonial purposes In aiding navigation

Ancient people of central Africa (6500 B.C.) could predict seasons from the orientation of the crescent moon.

Ancient achievements Daily timekeeping Tracking the seasons and calendar Monitoring lunar cycles Monitoring planets and stars Predicting eclipses Discovered precession And more Aztec calendar

Egyptian obelisk: Shadows tell time of day.

England: Stonehenge (completed around 1550 B.C.)

Stonehenge 23

Scotland: 4,000-year-old stone circle; Moon rises as shown here every 18.6 years.

Antikythera mechanism (c. 90 BC)

Antikythera mechanism (c. 90 BC) The Ancients had developed a sophisticated and detailed empirical knowledge of the motions of the sky (improved lunar cycle) (months/year) (improved eclipse with location info)

SW United States: Sun Dagger marks summer solstice

South Pacific: Polynesians were very skilled in the art of celestial navigation.

"On the Jisi day, the 7th day of the month, a big new star appeared in the company of the Ho star." SN 1987A "On the Xinwei day the new star dwindled." Bone or tortoiseshell inscription from the 14th century B.C. China: earliest known records of supernova explosions (1400 B.C.)