Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.

Slides:



Advertisements
Similar presentations
Earth in Space 19-1 Astronomy is the study of objects beyond the Earth’s atmosphere. It is one of the oldest sciences, as ancient people studied the heavens.
Advertisements

Chapter S1 Celestial Timekeeping and Navigation
Earth’s Motions, Solar Radiation, and the Seasons
Unit III: The Earth in Space
PHYS 1025 – Introductory Astronomy Lecture 2, Either Semester
Celestial Coordinates
Apparent/Actual Motions Summary
Seasons and Calendar Lecture 4.
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
Prologue Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2003.
The Earth Rotates.
Constellations. Celestial Sphere Our Point of View.
Seasons Earth’s Tilt –Tilt of rotational axis with respect to its orbit around sun Solar Insolation –More Direct Sun Light –Longer Duration of Day Light.
Review Questions How do you write Scientific Notation? How do you write Scientific Notation? What is the difference between Angular Measurements and Linear.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
The Celestial Sphere The 88 official constellations cover the celestial sphere. If you do not have a model of the celestial sphere to bring to class, you.
Grab your text book Chapter 1 Astronomy Today 7th Edition
Grab your text book Chapter 1 Astronomy Today 7th Edition
Sky Motions Diurnal Motion Annual Motion.
Constellations A constellation is a region of the sky.
Introduction to Astronomy.  Observations lead to theories and laws  Laws are concise statements that summaries a large number of observations.  Theories.
The Seasons There would be no seasons if the Earth were not tilted on it’s axis!  Nick Devereux 2006.
Astronomical Coordinates Summary
NATS From the Cosmos to Earth A model of the celestial sphere shows the patterns of the stars, the borders of the 88 official constellations, the.
Terrestrial Coordinates (useful for specifying locations on the surface of the Earth) Longitude - Longitude -- East/West Coordinate -- 0  at the Prime.
SUN & SEASONS UFO Size of Stuff in the Sky Earth  * Eye/brain gauges angular size soccer ball  alone doesn’t give you true size!
Last time: 2.1. Patterns in The Sky: Stars and constellations, TODAY: celestial coordinates 2.2 Seasons,…Precession 2.2 (cont.) The Moon and Eclipses.
Where is it? On the Celestial Sphere. Longitude and Latitude On Earth: Longitude is how far you are, in degrees, East or West of the “Prime Meridian”
Coordinate Systems.
Celestial Sphere. Earthly Sphere Latitude measures the number of degrees north or south of the equator. –DeKalb at 41° 55’ N Longitude measures degrees.
Announcements Clear sky patrol has not yet started We will start using PRS units this week, make sure that you have one.
Mastering Astronomy.
1 Lines in the Sky In order to use the sky to measure time you need to measure the location of objects in the sky. We will look at two methods of measuring.
How do they work together to help life survive? Seasons
Earth in Space Mr. Woodham’s 6 th Grade Earth Science Class.
The Reason for the Seasons
Survey of the Universe Tom Burbine
The Daily Motion As the Earth rotates, the sky appears to us to rotate in the opposite direction. The sky appears to rotate around the N (or S) celestial.
1.Stars move from east to west over the course of the night 2.Change slightly from one night to the next 3.However, their relative positions remain.
Sky Motions  Diurnal Motion Annual Motion. DIURNAL MOTION o Daily East / West motion of the sky Due to the Earth’s rotation (15°/hour) [360°/24 hours.
Constellations come, and climb the heavens, and go, And thou dost see them rise, Star of the Pole! and thou dost see them set, Alone,
Aim: What are some of the results of Earth’s Motions? I. Earth’s Motions A. Rotation (Spinning) 1. Day and Night Why does the sun rise in the east and.
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
Warmup  How many stars are in our solar system?  What shape is our orbit around the sun?
Local and Sky Coordinates
PSCI 1414 GENERAL ASTRONOMY LECTURE 6: THE REASON FOR SEASONS ALEXANDER C. SPAHN.
Our Location on the Earth North South EastWest North South East you are here West.
Chapter 4: Rising & Setting Stars © BRIEF
Observational Astronomy Mapping the Heavens Coordinate Systems We have two different ways to locate objects in the sky: Celestial equatorial system -Right.
Research Experiences for Undergraduates (REU)
Knowing the Heavens Chapter Two.
Chapter S1 Celestial Timekeeping and Navigation
Ancient astronomers believed that the stars were attached to a celestial sphere surrounding the Earth.
Sun’s annual motion and the Seasons
Rotation and Revolution
Winter Sky – Facing North
The Sun’s Motion and The Four Seasons
November 8,2010 Celestial Motions.
Unit 1 Physics Detailed Study 3.1
LINES OF LATITUDE AND LONGITUDE
Finding Your Way Around the Night Sky
RELATIVE MOTION OF EARTH IN SOLAR SYSTEM
Sun-Earth System.
Tilt of the Earth’s Rotational Axis
Earth Motions and Tilt.
Relative Motion of Earth in Solar System
Relative Motion of Earth in Solar System
ASTRO UNIT 1 REVIEW.
The Reasons for Seasons
INTRODUCTION TO ASTRONOMY
Presentation transcript:

Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3

Our Point of View  We are all standing on different parts of a large spinning ball moving through space   Remember that everything is moving at once

The Changing Sky  North Pole of the Earth is pointed at Polaris (the North or Pole star), which stays stationary as the other stars move around it  Sky makes one complete rotation per 24 hours (Diurnal motion)   Sky also makes one complete rotation per year (Annual motion) 

Diurnal Motion

Annual Motion

The Observer’s View

Observing  Can measure distance on the sky in degrees (360 degrees = complete circle)  Horizon --  Zenith --  Meridian --

The Solar Year

The Seasons  Tilt of Earth’s axis causes seasons   Sunlight is more direct in the summer 

Direct and Indirect Sunlight

Solstice and Equinox  Solstice   When the Sun is highest or lowest in the sky  Equinox   When the Sun is overhead at the equator

Times of year  Vernal Equinox -- March  First day of spring   Summer Solstice -- June  First day of summer   Autumnal Equinox - -September  First day of autumn   Winter Solstice - December  First day of winter 

Changing Day Length

Lines on a Globe  Equator -- Sun is overhead at equinox  Tropic of Capricorn --  Tropic of Cancer --  Arctic and Antarctic Circles /2 degrees south or north of the pole, Sun never sets or rises at solstice time

Navigation  Latitude (degrees North of the Equator)   Only works in Northern hemisphere  Longitude (degrees East or West of the Prime Meridian running through Greenwich England) 

The Celestial Sphere  Project the lines on a globe into space to form a coordinate system  North Celestial Pole –  Celestial Equator --

Celestial Coordinates  Right Ascension --  Declination --  The coordinates do not move or vary with location on the Earth, they are fixed to the stars

The Ecliptic  Most of the objects in the solar system have their orbits in the same plane, called the ecliptic   The ecliptic passes through 12 constellations known as the zodiac

Constellations of the Zodiac

Precession  The Earth “wobbles” as it spins, causing the Earth’s axis to point at different parts of the sky   This changes where the equinoxes are in the sky

Astrology  The belief that the positions of heavenly bodies at the time of your birth foretells your future  Your sign is where the Sun was on the zodiac when you were born   For example: Sept 13th = Virgo, but Sun is in Leo. All star signs are about 1 month off

Science and Pseudoscience  Astronomy is a science, it tries to form a picture of the universe based on observation and reason. It is subject to proof 

Next Time  Meet back in Science 102  Read Chapter 1.6