astronomy unit 3: big bang and electromagnetic radiation
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Astronomy Unit 3: Big Bang and Electromagnetic Radiation. Electromagnetic Radiation and the Big Bang Astronomy Unit 3. Electromagnetic Spectrum How we know what stars are made of. The Big Bang Inflation of the Universe 13.7 Billion Years ago. Vocabulary. - PowerPoint PPT PresentationTRANSCRIPT
Astronomy Unit 3:Big Bang and Electromagnetic Radiation
Electromagnetic Radiation and the Big Bang
Astronomy Unit 3
• Electromagnetic Spectrum– How we know what stars are made of.
• The Big Bang– Inflation of the Universe– 13.7 Billion Years ago
Voca
bula
ry• electromagnetic radiation: a form of energy that travels
through space as waves; called EM radiation for short
• electromagnetic spectrum: the variety of forms of EM
radiation, such as radio waves, microwaves, visible light, and X-
rays
• optical telescope: an instrument that uses light and lenses to
study distant objects
• radio telescope: an instrument that collects and analyzes radio
waves from stars and other objects in space
• observatory: a building or room that houses one or more
telescopes
Unit
3 Vo
cabu
lary
electromagnetic radiation: a form of energy that travels
through space as waves; called EM radiation for short
electromagnetic spectrum: the variety of forms of EM
radiation, such as radio waves, microwaves, visible light, and
X-rays
optical telescope: an instrument that uses light and lenses to
study distant objects
radio telescope: an instrument that collects and analyzes
radio waves from stars and other objects in space
observatory: a building or room that houses one or more
telescopes
electromagnetic radiation: a form of energy that travels
through space as waves; called EM radiation for short
electromagnetic spectrum: the variety of forms of EM
radiation, such as radio waves, microwaves, visible light, and X-
rays
optical telescope: an instrument that uses light and lenses to
study distant objects
radio telescope: an instrument that collects and analyzes radio
waves from stars and other objects in space
observatory: a building or room that houses one or more
telescopes
Unit
3 Vo
cabu
lary
Unit
3 Vo
cabu
lary
electromagnetic radiation: a form of energy that travels through
space as waves; called EM radiation for short
electromagnetic spectrum: the variety of forms of EM radiation,
such as radio waves, microwaves, visible light, and X-rays
optical telescope: an instrument that uses light and lenses to
study distant objects
radio telescope: an instrument that collects and analyzes radio
waves from stars and other objects in space
observatory: a building or room that houses one or more
telescopes
electromagnetic radiation: a form of energy that travels
through space as waves; called EM radiation for short
electromagnetic spectrum: the variety of forms of EM
radiation, such as radio waves, microwaves, visible light, and
X-rays
optical telescope: an instrument that uses light and lenses to
study distant objects
radio telescope: an instrument that collects and analyzes
radio waves from stars and other objects in space
observatory: a building or room that houses one or more
telescopes
Unit
3 Vo
cabu
lary
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Gam
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Ultra
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Visi
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Infra
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Mic
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Glue HereRemember only 8 dots of glue!
Electromagnetic SpectrumFold here
Electromagnetic Radiation• What are the 6 different
types of electromagnetic radiation?
• What makes them different from one another?
• What type of EM radiation is a rainbow?
• They Might Be Giants: Roy G. Biv
Electromagnetic Spectrum
• electromagnetic radiation: a form of energy that travels through space as waves; called EM radiation for
short
• electromagnetic spectrum: the variety of forms of EM radiation, such as radio waves, microwaves, visible
light, and X-rays
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WavestownWaves
Electromagnetic Spectrum
Radio Waves• Size: Radio waves range from the
size of a water bottle to the diameter of the Earth
• Source– Neutron Stars– Radio Tower
• Detection– Radio Satellite
Austin’s Radio Towers on Mount Larsen
Microwaves• Size millimeter
wavelengths• Sources
– Human Signals UHF TV– Big Bang – Cosmic
Background Radiation– Sun– Supermassive Black Holes
• Detection– Remote Sensing and
Weather
Simulated microwave release from supermassive blackhole
Cosmic Background Radiation from the Big Bang
Infrared Radiation (IR)
• Source– Heat From sun– Re-radiation of Heat– Warming effect on Earth
• Detection– Spitzer Space Telescope– Weather Radars– Pit Vipers
Infrared Cat
The image on the left shows an optical view of a star forming region. The same area is shown on the right in infrared radiation. Notice how the infrared observations penetrate the obscuring cloud to reveal many new details.
Infrared Image of Boston Bomber
Visible Light
• Source– Sun and Lightbulbs
• Detection– Telescope on the roof of
RLM Building at UT– McDonald Observatory– Hubble Space Telescope
Photo of Saturn from telescope on top of RLM at UT
Hubble and Hubble photo of Jupiter
Ultraviolet (UV)
• Source– Stars – (Produces sunburns and makes
vitamin D)– Ozone blocks UV radiation
– Black Lights and Electric Arcs
• Detection– Insects– NASA's Extreme
Ultraviolet Explorer satellite
X-Rays
• Source– Stars– Neutron stars and from
object being pulled into a black hole
• Detection– Chandra X-Ray
Observatory
Auroras of Jupiter Picture used overlain images from Chandra and Hubble
Gamma Radiation
• Size– Wavelengths are smaller
than an atom• Source– Supernovas– Produced on Earth from
Radioactive Decay and Lightning
• Detection– Fermi Gamma Ray Space
Telescope
Fermi Gamma Ray Space Telescope
Concepts Regarding Electromagnetic Spectrum
• Electromagnetic (EM) radiation is a form of energy that can travel through space. The different forms of EM radiation make up the electromagnetic spectrum. Light, radio waves, microwaves, and X-rays are all forms of EM radiation.
• Each form of EM radiation has a certain range of wavelengths and frequencies. All forms travel through space at the same speed, which is 3.0 108 meters per second. This value is called the speed of light.
• Stars and other objects of the universe give off visible light and other forms of EM radiation. The eyes and optical telescopes can detect the light that they give off. Other telescopes have been built to detect radio waves, microwaves, and X-rays from space.
• To reach Earth’s surface, EM radiation from space must pass through Earth’s atmosphere. The atmosphere distorts or blocks some of the radiation. This limits the usefulness of Earth-bound telescopes.
• Other telescopes, such as the Hubble Space Telescope, are aboard satellites. These telescopes can detect EM radiation from space very clearly. They produce very detailed, highly magnified images of objects in space.
• Scientists study the data from telescopes. This lets them learn about the distances and physical properties of stars and other components of the universe.
Telescopes and their WavelengthsVideo: Wavelenths and Fermi
All EM Radiation Travels at the speed of light.
• Each form of EM radiation has a certain range of wavelengths and frequencies. All forms travel through space at the same speed, which is 3.0 108 meters per second. This value is called the speed of light.
Electromagnetic Radiation meets the Earth’s Atmosphere
• Which type of EM radiation reaches the earth’s surface?
UltravioletVisible
Infrared Radio
What types of Electromagnetic radiation reach the Earth’s Surface?1.2.3.4.
Electromagnetic Radiation
What types of Electromagnetic radiation reach the Earth’s Surface?1.2.3.4.
Electromagnetic Radiation
How do we know what we know about the Universe?
• We know what we know because these inventions.
• Collect this data.
• Which is interpreted by these scientist.
Importance of Electromagnetic Radiation
• Astronomical Images in Different Wavelengths
• Electromagnetic Radiation provides the data that scientist use to understand the distances and physical properties of stars and other components of the universe.
• Scientist use telescopes to detect electromagnetic radiation from space.
• To reach Earth’s surface, EM radiation from space must pass through Earth’s atmosphere. The atmosphere distorts or blocks some of the radiation. This limits the usefulness of Earth-bound telescopes.
Images using different wavelengthsAstronomical Images in Different Wavelengths