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.

Slides:



Advertisements
Similar presentations
Knowing the Heavens Chapter Two.
Advertisements

Prof. D.C. Richardson Sections
Chapter 2: Discovering the Universe for Yourself
The Earth’s Movement.
Chapter 2 Discovering the Universe for Yourself
Celestial Coordinates
Celestial Sphere Stars seem to be on the inner surface of a sphere surrounding the Earth.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
Chapter 0 Charting the Heavens
The Earth Rotates.
Constellations. Celestial Sphere Our Point of View.
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 Night Sky. Diurnal (daily) motion of the stars Like the Sun, the stars generally rise in the east and set in the west. This daily motion of the.
Question 1 Constellations appear to move across the sky at night because 1) the Earth orbits the Sun. 2) the Moon orbits the Earth. 3) stars are in constant.
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,
Chapter 2: Discovering the Universe for Yourself
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.
ASTR211 EXPLORING THE SKY Coordinates and time Prof. John Hearnshaw.
We will discuss this in class, these are the volunteers so far Richard Avis Jillian Capano Brendan Forte Samantha Hunt Christian Madonna Shaina Singer.
End of Ch. 1.
Copyright © 2009 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself.
Discovering the Universe for Yourself
Constellations A constellation is a region of the sky.
Our goals for learning:
Chapter 2 Discovering the Universe for Yourself
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.
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.
Motions of the Earth Our goals for learning: What are the main motions of the Earth in space? How do we see these motions on the ground? How does it affect.
Tegrity Tegrity has been having issues the past few days. Service may be intermittent. Tegrity has been having issues the past few days. Service may be.
Seasons. Position of Ecliptic on the Celestial Sphere Earth axis is tilted w.r.t. ecliptic by 23 ½ degrees Equivalent: ecliptic is tilted by 23 ½ degrees.
SUN & SEASONS UFO Size of Stuff in the Sky Earth  * Eye/brain gauges angular size soccer ball  alone doesn’t give you true size!
The Earth, Sun, and Moon.
Motions of the Earth and Sky I. Outline for Today History: flat vs. spherical earth Map of the sky Constellations Diurnal and Yearly Motion The seasons.
© 2010 Pearson Education, Inc. Discovering the Universe for Yourself.
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.
Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as.
© 2010 Pearson Education, Inc. The sky varies as Earth orbits the Sun As the Earth orbits the Sun, the Sun appears to move eastward along the ecliptic.
Astronomy Picture of the Day
Astronomy 105 ä Student Information Sheet ä Class Syllabus ä Lab Syllabus ä Course Supplies ä Text ä Lab Manual ä Scantron 882-ES ä Flashlight with red.
Mastering Astronomy.
How do they work together to help life survive? Seasons
What causes the Seasons?. The Earth’s orbit Seasons do NOT arise from the distance the Earth is from the Sun but rather as a result of the Earth’s annual.
Survey of the Universe Tom Burbine
2.2 The Reason for Seasons Our goals for learning:
1 The Sun and the Celestial Sphere As the Earth orbits the Sun we seen the Sun in different locations against the backdrop of stars. The Earth reaches.
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.
Seasonal Motion. Daily and yearly motion intertwined Solar vs Siderial Day –Earth rotates in 23 h 56 m –also rotates around sun  needs 4 min. to “catch.
Daily and yearly motion intertwined Solar vs Siderial Day –Earth rotates in 23 h 56 m –also rotates around sun  needs 4 min. to “catch up” Consequence:
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
PSCI 1414 GENERAL ASTRONOMY LECTURE 6: THE REASON FOR SEASONS ALEXANDER C. SPAHN.
© 2010 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself.
Chapter 4: Rising & Setting Stars © BRIEF
Astronomy Unit 1 The celestial sphere and the seasons.
Chapter 2 Discovering the Universe for Yourself. 2.1 Patterns in the Night Sky What does the universe look like from Earth? Why do stars rise and set?
Research Experiences for Undergraduates (REU)
Knowing the Heavens Chapter Two.
Homework #2 degrees is how many degrees, arcminutes, and arcseconds?
Sun’s annual motion and the Seasons
Rotation and Revolution
Winter Sky – Facing North
November 8,2010 Celestial Motions.
Motions in the sky: The celestial sphere
ASTRO UNIT 1 REVIEW.
Presentation transcript:

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 poles. If you are standing at the poles, nothing rises or sets. If you are standing at the equator, everything rises & sets 90 to the horizon.

The Daily Motion The altitude of the celestial pole = [your latitude]. All stars at an angle < [your latitude] away from: your celestial pole never set. (circumpolar) the other celestial pole are never seen by you. Other stars, (& Sun, Moon, planets) rise in East and set in West at an angle = [90  your latitude].

The Daily Motion daily circles --- CCW looking north, CW looking south Höküpaÿa Newa

Time Exposure Photograph: • Estimate the exposure time • Which direction did stars move?

Annual Motion As the Earth orbits the Sun, the Sun appears to move eastward with respect to the stars. The Sun circles the celestial sphere once every year.

Annual Motion ecliptic equinox solstice zodiac the apparent path of the Sun through the sky equinox where the ecliptic intersects the celestial equator solstice where the ecliptic is farthest from the celestial equator zodiac the constellations which lie along the ecliptic

Annual Motion The Earth’s axis is tilted 23.5° from being perpendicular to the ecliptic plane. Therefore, the celestial equator is tilted 23.5° to the ecliptic. As seen from Earth, the Sun spends 6 months north of the celestial equator and 6 months south of the celestial equator.

The Cause of the Seasons Summer Winter Seasons are caused by the Earth’s axis tilt, not the distance from the Earth to the Sun!

The Cause of the Seasons

Axis tilt changes directness of sunlight during the year. This tool is taken from the Seasons tutorial on the Astronomy Place web site. You can use it to reinforce the ideas from the previous slide. As usual, please encourage your students to try the tutorial for themselves. Why Does Flux Sunlight Vary

Seasonal Change in Sun’s Altitude The “Figure 8” shows Sun at same time each day over a year.

When is summer? The solstice which occurs around June 21 is considered the first day of summer. It takes time for the more direct sunlight to heat up the land and water. Therefore, July & August are typically hotter than June.

Why doesn’t orbital distance from the Sun matter? Small variation for Earth — about 3% (but orbit distance does matter for some other planets, notably Mars and Pluto). Surprisingly, seasons are more extreme in N. hemisphere, even though Earth is closer to Sun in S. hemisphere summer (and farther in S. hemisphere winter) — because of land/ocean distribution

What is 55.435 degrees in degrees-minutes-seconds notation? What is in decimal degrees?

Homework #2 45.635 degrees is how many degrees, arcminutes, and arcseconds? How many degrees, arcminutes, and arcseconds does the moon move across the sky in one hour? (the lunar day is 24 hours and 48 minutes long) The moons diameter is about 30 arcminutes, so find out how long it takes for the moon to travel its diameter.

Precession of the Equinoxes The Earth’s axis precesses (wobbles) like a top, once about every 26,000 years. Precession changes the positions in the sky of the celestial poles and the equinoxes. Polaris won't always be the north star. The spring equinox, seen by ancient Greeks in Aries, moves westward and is now in Pisces!