stars, galaxies, and the universe chapter 21.1 & 21.2

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Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

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Page 1: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Stars, Galaxies, and the

UniverseChapter 21.1 & 21.2

Page 2: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Telescopes• Electromagnetic Radiation

- energy that can travel through space

in the form of waves

• Electromagnetic Spectrum

- the entire range of radiation

Page 3: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Telescopes

• Telescopes are instruments that collect and focus light and other forms of electromagnetic radiation.

• Telescopes make distant objects appear larger and brighter

Page 4: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Telescopes

• 3 kinds of telescopes

- Optical telescopes

1) Refracting telescopes

– use convex lenses

The larger the lens, the stronger the telescope

Page 5: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Largest Refracting Telescope

The Great Paris Exhibition Telescope of 1900

1.25 m diameter

Page 6: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Telescopes

2) Reflecting Telescopes

- use concave mirrors

The larger the mirror, the stronger the telescope

Page 7: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Largest Reflecting Telescope

Large Binocular Telescope

Mount Graham International Observatory, Arizona

Two 8.4 m diameter

Subaru Telescope

Hawaii

8.2 m diameter

Page 8: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Telescopes

- Radio Telescopes – devices used to detect radio waves from objects in space

The larger the dish, the stronger the telescope

Page 9: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Telescopes

Largest radio telescopes

Arecibo, Puerto Rico

1,001 ft

Page 10: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Telescopes

• Observatory – a building that contains one or more telescopes

• Usually located on mountain tops or in space

Hubble space telescope is a reflecting(optical) telescope

Page 11: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

• why do we study the stars?

Page 12: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Characteristics of Stars

• Constellations –

imaginary patterns

of stars in the sky

Page 13: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Classifying Stars

• Stars are classified using color and temperature

Hottest

Coldest

Page 14: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Classifying Stars

Stars are classified using size

Page 15: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Classifying Stars

Stars are classified according to composition

Page 16: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Brightness of Stars

• The brightness of a star depends on both its size and temperature

• A large star may look bright, even though it is relatively cool, because of its size

• A small star may look bright because it is hot

Page 17: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Brightness of Stars

Apparent Brightness- how bright a star appears from Earth

Page 18: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Brightness of Stars

Absolute Brightness- how bright a star would be at a standard distance

Page 19: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Measuring Distances to Stars

Light-year – distance light travels in a year

- used to express distance

between stars

-speed of light = 300,000 km/s

1 light-year is about 9.5 million million kilometers

Page 20: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

• how to measure extreme distances

Page 21: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Measuring Distances to Stars

Parallax – the apparent change in position of an object when you look at it from different places

Parallax can be used to measure stars that are only a few hundred light-years away

Page 22: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

• What is Parallax? - YouTube

Page 23: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2

Hertzsprung-Russell Diagram

Plotting of stars on a graph based on temperature and absolute brightness

Used to understand how stars change over time

Page 24: Stars, Galaxies, and the Universe Chapter 21.1 & 21.2