any object in space outside of Earth's atmosphere

Slides:



Advertisements
Similar presentations
Motions of the Earth and Sky
Advertisements

Why do we have night and day? Why do daylength’s change?
Actual Earth Motions.
Unit III: The Earth in Space
Motions of the Earth, Moon and Sun
Phys. 102: Introduction to Astronomy
Earth’s Rotation and Revolution
Earth’s Rotation and Revolution
Topic 4 Motions of the Earth, Moon, and Sun
Apparent Motions of Celestial Objects
The Earth Rotates.
OBSERVING THE SKY Chapter 1 Chapter 3 Constellations and Navigation Constellations and Navigation ORIGINS OF ASTRONOMY.
Latitude & Longitude.
Locating Positions on Earth
Day and Night.
Motions of the Celestial Sphere. Constellations Sky looks like a dome with the star painted on the inside. 88 constellations such as Ursa Major, Orion,
Sky Motions Diurnal Motion Annual Motion.
Earth Motions and the Heavens
Models and Dimensions of Earth
EARTH’S ROTATION CHAPTER 4.2. Objectives Give evidence of Earth’s rotation. Give evidence of Earth’s rotation. Relate Earth’s rotation to the day- night.
Celestial Observations
Aim: What are the apparent motions of the stars and planets?
Do Not Write What is in Yellow APPARENT MOTIONS OF THE CELESTIAL OBJECTS.
The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The 88 official constellations cover the celestial sphere.
Groups of dark brown streaks have been photographed by the Mars Reconnaissance Orbiter on melting pinkish sand dunes covered with light frost. Dark sand.
Latitude and longitude
Trivia Question of the Day. Astronomy Picture of the Day Astronomy Picture of the Day.
Solar Motion. Label front flap MOTIONS OF THE EARTH -DAY & NIGHT.
Earth’s Rotation and Revolution
Space, Earth and Celestial Objects © Lisa Michalek.
Our Place in the Cosmos and Introduction to Astrophysics Lecture 3 Patterns in the Sky - The Earth’s Rotation.
A scientific model.  Why do we use the model of the celestial sphere when studying the night sky, even though it does not accurately represent three-dimensional.
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.
 Celestial Sphere: an imaginary sphere on which all the celestial objects would appear  Celestial object: any object in the sky that genuinely appears.
Mrs. Horn Science  Earth’s axis is an imaginary line that runs through Earth. - It passes through the North and South poles. - Earth rotates (spins)
At the scale of the Milky Way Galaxy, distances are described in terms of Light-years, which is the distance light travels in one year.
1 “First day, I’d tell the class all I knew,” he told The Saturday Evening Post, “and there was nothin’ left to say for the rest o’ the semester.” - Andy.
Aim: What is Earth’s daily motion? DO NOW: 1. How many hours are in one day? 2. How many degrees is a full circle? 3. How many degrees does Earth spin.
EARTH IN SPACE. A reminder about earth  The earth is almost a sphere  We locate points on the sphere with 3 coordinates – Longitude (180º W º.
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.
Astronomy: Apparent Motions Making sense of celestial observations.
Constellations pg. 65. Constellation section of the sky with a recognizable star pattern. 88 listed 48 from Ptolemy.
Coriolis Effect. 2. Evidence for Rotation Coriolis Effect – the tendency of objects moving over the earth (air, water, planes, projectiles) to be deflected.
Earth’s Rotation Earth rotates counterclockwise Earth is tilted on its axis 23.5 degrees.
MOTIONS OF SKY. Goals To identify the different parts of the celestial sphere model To understand how to express the location of objects in the sky To.
Chapter 4: Rising & Setting Stars © BRIEF
What is apparent motion? Important to understand what we see and what is actually happening. Apparent motion is what we see from Earth Actual motion is.
Earth Motions 1)Rotation – the spinning of an object on its axis. (Like a figure skater or a CD) 2)Direction of Rotation – Earth turns west to east or.
Astronomy vs. Astrology Astronomy: Astronomy: The scientific study of matter in outer space, especially the positions, dimensions, distribution, motion,
New observations lead to changes in scientific theory What’s wrong with the image on the right, which shows Ptolemy’s popular scientific theory 2000 years.
Question of the Day What is the Shape of Earth’s Orbit?
Locating Positions on Earth
Rotation and Revolution
Aim: What are the apparent motions of the stars and planets?
Astronomy Motions of the Earth and Sun
The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2-dimensional surface – the Celestial Sphere.
November 8,2010 Celestial Motions.
The Earth’s Rotation, Revolution Around the Sun, and the Seasons
Investigating Astronomy Timothy F. Slater, Roger A. Freeman
Good Morning!!! TEST DAY.
Celestial Motions Chapter 2.
Astronomy Vocabulary Mr. Ahearn 2013.
Motions of Earth, Moon and Sun
Precession and The Celestial Poles
Aim: The Sun’s path each Season
Investigating Astronomy Timothy F. Slater, Roger A. Freeman
ASTRO UNIT 1 REVIEW.
Celestial Motions Chapter 2.
Homework #1 has been posted
What is the Relationship Between Latitude and Polaris?
Presentation transcript:

any object in space outside of Earth's atmosphere stars, planets, Moon, Sun, comets model of the sky Z zenith Z - highest point in sky - directly above the observer's head horizon imaginary boundary between the sky and ground

II. Star Motions. 1. Looking up, the sky appears to be a ________ dome Watch a _______ rise. It moves in a wide _______. But one point in the sky __________________________ star arc star does not move. That point appears fixed. Later the star ________. It is as if the stars move on a ____________________ that ____________________ Earth on a _____________ _______. Half of the sphere is ______________________. sets transparent sphere rotates around gigantic axis hidden beneath you.

4. The fixed point that does not move is directly above _________ _______________________. It is near the star _________________. Its altitude above the horizon equals the __________________ of the observer. Polaris north on the horizon Polaris latitude rise 5. Some stars _________ and _____. See A and B at right. Other stars _______________ ____________. They circle the ____________ , and are called _______________________ stars. See star C at right . A set never rise and B C never set pole/axis circumpolar

Star C 350 Notice: -Star A is _______________________ -Most stars do NOT rise directly in the _________ and do NOT set directly in the ___________ -The latitude of this observer is ____________ circumpolar east west 350 N

Which direction are you looking in this picture?

Which direction are you looking in this picture?

How long was the exposure? What latitude is this?

Stars appear to rotate around Earth from _______ the spinning of Earth on its own axis W east west E 3600 24 3600 150 / hour 24 h Stars appear to rotate around Earth from _______ to _________ at a rate of ________________ because of Earth's _________________________________ east west 150 / hour rotation in the opposite direction.

circumpolar = Polaris 4 2 3 N E W NY Notice: _____ x 150/h = _________ between each position above mid October 6 h 1 900 2 3 4

D. 1. The stars, Sun, moon and planets move ______/h 150 D. 1. The stars, Sun, moon and planets move ______/h across the ________________________. celestial sphere = celestial object etc 9 am 8 am 150 Sun's path S N

from to hours degrees 8 am 9 am 1 10 am 2 pm 12 pm 4 pm 150 2 300 4 600 5 750 3 450 6 900

the same 2. Because all stars move across the sky at ___________ ____________ , any star with a ______________ path will be above the horizon for ____________________________. rate longer a longer time B C E S A N W Star A: __________ path  above horizon for _____ h Star B: rises/sets in _______  above horizon for _____ h Star C: __________ path  above horizon for _______ h longest > 12 E/W___ 12 shortest < 12

IV. Effects of Earth's Rotation 1. ___________________. As Earth rotates on its axis, half of it faces the sun and has daylight. The other half is in darkness and has nighttime. Night and Day view from above North Pole: light from the Sun Day Night

Earth rotates, so points on its surface rotate into and out of _____________: sunlight 6 am View from North Pole: 8 am 4 am 10 am sunrise 2 am light from the Sun 12 pm noon midnight 12 am sunset 2 pm 10 pm 4 pm 8 pm 6 pm 300 2 Meridians shown are ______ apart  every ______ hours (All times are approximate.)

2. Time – is based on Earth's _________, which causes the Sun to _______ and _______ rotation set rise imaginary line from N to S passing through the zenith Z local meridian - _____________________________________ _____________________________________ Z 12:00 p.m. -Sun is directly S - Sun is highest - looking south: local noon- __________ _______________________ 12 pm S a.m. p.m. N E S W Sun's path looking south

3. Change in Shadow Length. shadow of a pole - ________________________________ _________________________________ -points directly opposite the Sun -shortens in the a.m. -shortest at local noon and points N -lengthens in the p.m. top view 12 pm S 9 am 3 pm pole pole S 3 pm 9 am noon N N

This is the basis of sundials.

- Earth rotates _____ degrees every hour Earth's Time Zones - Earth rotates _____ degrees every hour - The Sun reaches local noon ______ degrees further__________ every hour - Time zones are ______ apart from each other 15 15 west 150 11 am noon 1 pm 2 pm Pacific Mountain Eastern Central

V. Evidence of Earth's rotation: Foucault Pendulum: ________________________ A pendulum swung in one direction (A-A') appears to change to a new direction (B-B') because Earth rotates underneath it 6 ___ hours later, Earth has rotated ______ degrees: Top view of pendulum at the North Pole: 90 Notice the Pendulum keeps the same direction ___________ A A' B B'

2. Coriolis Effect: ________________________________ ___________________________________________________ the apparent curving or turning of winds, currents and projectiles caused by Earth's rotation. = original path = curved path Turns to the _______ in Northern Hemisphere right The equator moves _________, than the poles. So projectiles curve _________ of the _________ path. faster direction of rotation in front Turns to the _______ in Southern Hemisphere original left Earth