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Chapter 1 Astronomy Today 7th Edition Chaisson/McMillan Grab your text book

Chapter 1 Astronomy Today 7th Edition Chaisson/McMillan

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Chapter 1 Astronomy Today 7th Edition Chaisson/McMillan. Grab your text book. Charting the Heavens Day 2. Celestial Sphere. The celestial sphere : Stars seem to be on the inner surface of a sphere surrounding the Earth - PowerPoint PPT Presentation

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Page 1: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Chapter 1

Astronomy Today

7th Edition

Chaisson/McMillan

Grab your text book

Page 2: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Charting the Heavens

Day 2

Page 3: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Celestial Sphere

The celestial sphere:

Stars seem to be on the inner surface of a sphere surrounding the Earth

They aren’t, but they can use two-dimensional spherical coordinates (similar to latitude and longitude) to locate sky objects

Page 4: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Celestial Coordinates

Right Ascension• Like longitude• Use units of time-hours

instead of degrees• 0 hour is the vernal equinox

Declination• Like latitude except use +/-

instead of north and south

Page 5: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Terms related to the Celestial Sphere

Terrestrial System• South Pole• North pole• Equator• Latitude

– 0° at the Equator• Longitude

– 0° at the Prime Meridian

Celestial System• South Celestial Pole• North Celestial Pole• Celestial Equator• Declination

0° at celestial Equator

• Right Ascension– 0 Hours at Vernal Equinox

Page 6: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Angular Measure

• Full circle contains 360° (degrees)• Each degree contains 60′ (arc-minutes)• Each arc-minute contains 60′′ (arc-seconds)• Angular size of an object depends on its actual size and distance from viewer

Page 7: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Earth’s Orbital Motion

• Daily cycle, noon to noon, is diurnal—solar day• Stars aren’t in quite the same place 24 hours later, though, due to Earth’s rotation around Sun; when they are once again in the same place, one sidereal day has passed

Page 8: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Earth’s Orbital Motion

Seasonal changes to night sky are due to Earth’s motion around Sun

Page 9: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Earth’s Orbital MotionTwelve constellations (some say thirteen) Sun moves through during the year are called the zodiac; path is ecliptic

Page 10: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Sun signs

• Are based on which constellation the sun was in on the day of your birth

• Moon sign: which constellation is the moon is at the time of your birth

• Most astrological signs areIncorrectly shown based on your birth where the sun was During Greek times.

Page 11: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Ophiucus

• The thirteenth zodiac sign• Sun passes through Ophiucus’ foot• November 30-Dec. 18• He is the serpent bearer• also used as the medical symbol

Page 12: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Seasons

• Turn to your elbow partner and discuss why you think we have seasons>WHEN YOU THINK YOU HAVE AN ANSWER < DRAW OR DESCRIBE YOUR ANSWER ON YOUR WHITE BOARD> ALL TABLES WILL BE REPORTING WHAT THEY THINK SO BE PREPARED.

Page 13: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Ecliptic• If the sun's path is

observed from the Earth's reference frame, it appears to move around the Earth in a path which is tilted with respect to the spin axis at 23.5°.

• The angle of earth’s axis=the plane of the angle of the ecliptic to the celestial equator

Page 14: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Earth’s Orbital Motion• Ecliptic is plane of Earth’s path around Sun; at 23.5° to celestial equator• Northernmost point of path (above celestial equator) is summer solstice; southernmost is winter solstice; points where path crosses celestial equator are vernal and autumnal equinoxes

• Combination of day length and sunlight angle gives seasons• Time from one vernal equinox to next is tropical year

Page 15: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Seasons

• On the Equinox, the Earth experiences equal amounts of day and night

• Summer solstice- the sun is at it’s highest point

• Winter Solstice –the sun is at it’s lowest point

Page 16: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Local co-ordinate systems

• Based on the objects above the plane of the horizon– Altitude is the angle above the horizon

horizon

star

altitude

NORTH STAR HAS AN ALTITUDE OF 0° IF YOU ARE ON THE EQUATOR

THE ALTITUDE OF THE NORTH STAR=YOUR LATITUDE ON EARTH!!!

Page 17: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

A ROUGH WAY TO ESTIMATE ALTITUDE

• PINKY =1°• 3 FINGERS=3°• FIST = 10°

Page 18: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Local Co-ordinate System

• Azimuth – starts with north a 0° and south is 180°

• Zenith is 90°

zenith

Page 19: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

North Star

• Even though Polaris is currently the North star, it doesn’t lie due North –and eventually will move Vega will be our North Star, Why do you think this is happening? Discuss with your elbow partner, write down your thoughts on your white board, be ready to defend them.

Page 20: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

CIRCUMPOLAR STARS

• STARS THAT NEVER GO BELOW THE HORIZON – CAN ALWAYS BE SEEN AT NIGHT– http://upload.wikimedia.org/wikipedia/commons/

2/21/Zirkumpolar_ani.gif

Page 21: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

The North Star

• Polaris, our current North Star is the 49th brightest star in the night sky!!!!!

• To find it, locate the cup of the Big Dipper to the handle of the Little dipper.

• It doesn’t appear to move in the night sky but the other stars rotate around it

• North pole and Polaris are about 1° off from one another

Page 22: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Earth’s Orbital Motion

Precession: rotation of Earth’s axis itself; makes one complete circle in about 26,000 years

Page 23: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

Precession

• Wobbles in a 26,000 year cycle• Wobble is between Polaris, Vega and Thuban• Changes the position of the Vernal Equinox

which will also change the co-ordinates of the stars

Page 24: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

SEASONAL CHANGES IN OUR NIGHT SKY

• Summer triangle: Vega, Denab, Altair• Winter: Orion, Sirius (Dog Star)

• The change occurs about 1°/night

Page 25: Chapter 1 Astronomy Today  7th Edition Chaisson/McMillan

1.4 Earth’s Orbital Motion

Time for Earth to orbit once around Sun, relative to fixed stars, is sidereal year

Tropical year follows seasons; sidereal year follows constellations—in 13,000 years July and August will still be summer, but Orion will be a summer constellation