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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

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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Page 1: 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

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

Page 2: 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
Page 3: 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

1. History of Modern AstronomyAstronomy circa 1600, the Copernican Revolution

Copernicus 1514Tycho Brahe 1573 Galileo 1609Kepler 1605, 1609Newton 1684

Page 4: 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

Geocentric UniverseThe Problem: The Retrograde Motion of Mars

Page 5: 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

..add epicycles to the Geocentric Model, but still doesn't work

Page 6: 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

A Heliocentric Model of the Universesolves the problem

Page 7: 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

Galileo invents the telescope 400 years ago.

Page 8: 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

All of Galileo's observations can be explained by a heliocentric model.

Page 9: 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

Heliocentric Model and everyday observations:Phases of the Moon, Eclipses, Seasons

Page 10: 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

The constellations are patterns we perceive of stars in space. Those stars are generally not near each other.

Page 11: 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

Right ascension and Declination are the coordinates of the Celestial Sphere. They are analogous to longitude

and latitude on Earth.

Page 12: 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

The moon's phases appear due to the relative positions of the Sun, the Earth, and the Moon.

Page 13: 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

What are eclipses and why don't they happen every month?

Page 14: 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

The origin of the seasons:

Page 15: 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
Page 16: 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

Kepler Laws of planetary motion

Page 17: 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

"The orbit of every planet is an ellipse with the sun at a focus."

Page 18: 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

Kepler's First Law Applet

Page 19: 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

"The line joining a planet and the sun sweeps out equal areas during

equal intervals of time."

Page 20: 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

Kepler's Second Law Applet

Page 21: 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

"The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its

orbit."

Page 22: 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

Newton's Law of Gravitation

Page 23: 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

The forces are equal and opposite

Page 24: 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

Is there gravity in space?Is there gravity in space?

Page 25: 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

Einstein's Law of Gravity

Page 26: 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

Space curves due to the presence of matter.

Page 27: 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

The path of light in curved space, near a black hole

Page 28: 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

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.

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A view of the Milky Way with a black hole in front of it.

Page 30: 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

LISA : Laser Interferometer Space Antenna

Page 31: 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

Matter and Light

Page 32: 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

Light is an electromagnetic wave

Page 33: 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

The visible spectrum is a portion of the full electromagnetic spectrum

Page 34: 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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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.

Page 36: 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

Blackbody Spectra

Page 37: 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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Emission Lines, Absorption Lines

Page 39: 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

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.

Page 40: 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

Light dims as the inverse-square

Page 41: 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

Telescopes

Page 42: 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

A telescope captures and brings light to a focus

Page 43: 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

Modern telescopes are reflectors (mirrors) not refractors (lenses).

Page 44: 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

The light gathering power of a telescope varies by the square of its mirror's diameter.

Page 45: 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

Angular Resolution of a telescope

Page 46: 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

Seeing: the blurring of an image due to atmospheric turbulence

Page 47: 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

Different astronomies require different telescope designs

Page 48: 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

The Milky Way in each band of the electromagnetic spectrum.