Chapter 26 ASTRONOMY THE SCIENTIFIC STUDY OF SPACE

  • Slides: 27
Download presentation

Chapter 26 ASTRONOMY THE SCIENTIFIC STUDY OF SPACE / THE UNIVERSE.

Chapter 26 ASTRONOMY THE SCIENTIFIC STUDY OF SPACE / THE UNIVERSE.

Galactic address Planet Star The Sun Star System/Galaxy The Milky Way Galactic Group Local

Galactic address Planet Star The Sun Star System/Galaxy The Milky Way Galactic Group Local Group Galactic Supercluster Virgo Supercluster

GALACTIC ADDRESS

GALACTIC ADDRESS

Measuring distances in the Universe • Astronomical Unit (AU) = 150 million km (

Measuring distances in the Universe • Astronomical Unit (AU) = 150 million km ( = 149, 597, 870. 66 km ) – The average distance from the EARTH to the SUN. • Light year = 9, 460, 700, 000 km ( = 9. 4607 x 1012 km ) This is based on the speed of light = 186, 000 mi/s = 300, 000 m/s - The distance that light travels in one year. • Parsec = 3. 26 light years = 19 trillion miles.

Astronomical Distances and Scales http: //htwins. net/scale 2/

Astronomical Distances and Scales http: //htwins. net/scale 2/

Units of Distance • Astronomical Unit – The average distance from Earth to the

Units of Distance • Astronomical Unit – The average distance from Earth to the sun ~ 150, 000, 000 meters • Light Year – The distance light travels in 1 year ~ 9, 500, 000, 000 meters

Powers of 10 •

Powers of 10 •

Scientific Notation • Step 1: Find decimal point (3000 = 3000. 0) • Step

Scientific Notation • Step 1: Find decimal point (3000 = 3000. 0) • Step 2: Move decimal point to where it is directly to right of first non-zero digit. Count the number of spaces the decimal point moves • Step 3: Write down the new number with x 10 on the end, put the number of spaces the decimal point moved at the top right corner of the x 10 (it is a positive number if point moved left and it is a negative number if point moved right)

Examples •

Examples •

Looking at distant objects is like looking back in time.

Looking at distant objects is like looking back in time.

Observing space • The electromagnetic spectrum represents different types of energy, each having different

Observing space • The electromagnetic spectrum represents different types of energy, each having different wavelengths, traveling at the speed of light. Link

Telescopes REFRACTING REFLECTING Optical telescope Uses lenses to bend light (refraction) Optical telescope Uses

Telescopes REFRACTING REFLECTING Optical telescope Uses lenses to bend light (refraction) Optical telescope Uses a curved mirror (reflection) to gather and focus light Problems: *Focuses different colors of light at different distances. *Ability to see distant objects is based on the size of their objective lens. Advantages: *Can be made larger, can gather more light, can see more distant/fainter objects. *Less distortion *Eliminates color differences

National Radio Astronomy Observatory (NRAO) • Green Bank, West Virginia

National Radio Astronomy Observatory (NRAO) • Green Bank, West Virginia

Robert C. Byrd Green Bank Telesco (100 meters in diameter)

Robert C. Byrd Green Bank Telesco (100 meters in diameter)

Keck Telescopes – 10 m OWL (Overwhelmingly Large Telescope) – 100 m - optical

Keck Telescopes – 10 m OWL (Overwhelmingly Large Telescope) – 100 m - optical and near-infrared Only Proposed!

Gran Telescopio Canarias

Gran Telescopio Canarias

Human Space Exploration National Aeronautics and Space Administration (NASA)

Human Space Exploration National Aeronautics and Space Administration (NASA)

100, 000 Stars

100, 000 Stars

Supernova in Messier 82

Supernova in Messier 82

Ant Nebula Horsehead Nebula

Ant Nebula Horsehead Nebula

Comet ISON

Comet ISON

Solar Prominence

Solar Prominence

Uranus

Uranus

Jupiter’s triple solar eclipse event

Jupiter’s triple solar eclipse event