Class 1 Introduction, Background Class 2 Solar System Class 3 Stars Class 4 Galaxies Class 5 Cosmology Class 6 Special Topics Class 1 Introduction, Background ● History of Modern Astronomy ● The Night Sky, Eclipses and the Seasons ● Kepler's Laws ● Newtonian Gravity ● General Relativity ● Matter and Light ● Telescopes
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Class 1 Introduction, Background Class 2 Solar SystemClass 1 Introduction, Background Class 2 Solar System Class 3 Stars Class 4 Galaxies Class 5 Cosmology Class 6 Special Topics Class
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Class 1 Introduction, Background Class 2 Solar System Class 3 Stars Class 4 Galaxies Class 5 Cosmology Class 6 Special Topics
Class 1 Introduction, Background
●History of Modern Astronomy●The Night Sky, Eclipses
and the Seasons●Kepler's Laws●Newtonian Gravity●General Relativity●Matter and Light●Telescopes
1. History of Modern AstronomyAstronomy circa 1600, the Copernican Revolution
"The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its
orbit."
Newton's Law of Gravitation
The forces are equal and opposite
Is there gravity in space?Is there gravity in space?
Einstein's Law of Gravity
Space curves due to the presence of matter.
The path of light in curved space, near a black hole
Hubble Space Telescope: Gravitational lens G2237 + 0305, sometimes referred to as the "Einstein Cross".
The photograph shows four images of a very distant quasar which has been multiple-imaged by a relatively nearby galaxy acting as a gravitational lens.
The quasar seen here is at a distance of approximately 8 billion light years, whereas the galaxy at a distance of 400 million light years is 20 times closer. The light from the
quasar is bent in its path by the gravitational field of the galaxy. The bright central region of the galaxy is seen as the diffuse central object.
A view of the Milky Way with a black hole in front of it.
LISA : Laser Interferometer Space Antenna
Matter and Light
Light is an electromagnetic wave
The visible spectrum is a portion of the full electromagnetic spectrum
Kirchoff's LawsBlackbody Spectrum 1. A luminous solid or liquid, or a sufficiently dense gas, emits light of all wavelengths and so produces a continuous spectrum of radiation.Emission Line Spectrum 2. A low-density, hot gas emits light whose spectrum consists of a series of bright emission lines. These lines are characteristic of the chemical composition of the gas.Absorption Spectrum 3. A cool, thin gas absorbs certain wavelengths from a continuous spectrum, leaving dark absorption lines in their place, superimposed on the continuous spectrum. Once again, these lines are characteristic of the composition of the intervening gas--they occur at precisely the same wavelengths as the emission lines produced by that gas at higher temperatures.
Blackbody Spectra
Emission Lines, Absorption Lines
Photon is another word for light
When an electron changes its position in an atoma photon is produced or absorbed.
Like doesn't always just act like a wave. Sometimes it acts like a particle, like a billiard ball on a pool table.
When light acts like a particle, it's generally referred to as a photon.
Light dims as the inverse-square
Telescopes
A telescope captures and brings light to a focus
Modern telescopes are reflectors (mirrors) not refractors (lenses).
The light gathering power of a telescope varies by the square of its mirror's diameter.
Angular Resolution of a telescope
Seeing: the blurring of an image due to atmospheric turbulence
Different astronomies require different telescope designs
The Milky Way in each band of the electromagnetic spectrum.