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| Anything that can be detected with a telescope |
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| Simple time exposure reveals earth's rotation about the northern celestial pole |
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| Distance between the earth and the sun: |
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| A light year is defined as: |
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| The distance light travels in one year |
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| A light year equals ? miles |
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| Classes of Objects in Universe: |
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| Planets→Brown Dwarfs→Stars→Star Clusters→ Galaxies→Clusters of Galaxies |
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| The overhead point is called... |
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| The imaginary line from due south to due north is the... |
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- Measures Brightness
- 1st mag=brightest, 6th mag=dimmest
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| The way we see stars from earth |
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| The way a star would look if it were at 10 parsecs (3 light yrs) |
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| What factors is brightness determined by? |
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| Size, Distance, and Temperature |
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| What property of earth gives us the seasons? |
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| T/F: The Sun is lower in the sky during winter |
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| T/F: The Sun is lower in the sky during Summer |
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| False, the Sun is higher in the sky during Summer |
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(Diurnal)
Rising and setting of the Sun and Moon.
Earth spinning on its axis |
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(Annual)
365.25 days
Earth's motion around the sun |
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Planet wobbles on its axis
NCP points to different spots |
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We are not unique or at any special advantage with our position in the universe.
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| As Earth passes Mars faster, it looks like Mars is going backward |
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- Surface topography of the moon
- Phases of Venus
- Satellites of Jupiter
- Composition of the Milky Way
- "Ears" on Saturn
- Sunspots
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- Established government funded observatory
- Collected extensive data on positions of planets
- Invented the Tychonic System
- Discovered comets are extraterrestrial
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- 1st: Planets orbits ellipses with the sun at one focus
- 2nd: Planet-Sun line sweeps out equal areas in equal time.
- 3rd Law: There is a relationship between a planets orbital period(P) and its average distance from the sun (a), P2=a3
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A measure of the ellipse
Greater the ellipse=more eccentric |
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- An object in motion will stay in motion unless acted upon by an external force
- F=ma
- For every force there is an equal and oppositely directed reactionary force
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| Newton's Law of Gravitation |
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| Wavelength+Frequency Definitions: |
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λ=the distance between crests of a wave
f= the # of crests/troughs that pass by each second
v=fλ |
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| Order of Electromagnetic Spectrum |
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| Gamma→X-Ray→UV→Visible Light→Infrared→Microwaves→Radiowaves |
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| What is Brightness directly proportional to? |
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Definition
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| Learn: Temperature, Composition, Magnetic Field, or whether stars are coming or going |
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- Redshift: Wavelengths stretched
- Blue Shift: Wavelengths compressed(coming towards)
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| What is the advantage of having a telescope in space? |
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Definition
| Avoid Atmospheric Disruption |
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| Take a bunch of telescopes to produce one image |
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| Major types of telescopes: |
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| Ancient astronomers divided the sky into regions containing distinct groups of stars called |
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| The Earth’s atmosphere shields us from most kinds of electromagnetic radiation. The exceptions are |
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| Infrared Radiation+Visible Light |
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| The type of electromagnetic radiation with a wavelength just longer than that of red light is |
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| A curved lens or mirror can form an image by bringing light to a |
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| The annual path of the Sun through the sky, with respect to the stars is the |
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| When the Moon is lying on a line directly between the Earth and the Sun, close enough to cast a full shadow on the Earth, we have a |
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| A star that appears brighter to an observer on Earth has a low |
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? is given credit for the idea that the Earth is not the center of the solar system
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| Kepler was the first to show that planets move |
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| In eliptical orbits around the sun |
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| A discovery Galileo made with his telescope that contradicted Polemy’s ideas was |
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| An object is moving through space. If all forces are removed from the object, then it will |
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Definition
Continue in a straight line at constant speed
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| The standard means of methodically investigating nature is the |
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| To explain a set of facts we start with an educated guess called a |
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| All kinds of electromagnetic radiation taken together make up the |
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| It is often useful to think of light as particles of energy called |
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| Photons instead of as waves |
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| The annual path of the Sun through the sky with respect to the stars |
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| What is the North Celestial Pole? |
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Definition
Looking at the celestial sphere, it is the northern most axis, straight up from Earth, and is encapsulated by the northern meridian
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Why did Ptolemy include epicycles in his geocentric theory of the Universe?
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| He included epicycles because each planet orbited the circumference of their own epicycle, while still orbiting earth. |
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| List and explain three uses of spectroscopy in astronomy. |
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Three uses of spectroscopy are being able to look at the moon and learn more about its phases and topography, to try and get a greater understanding of our galaxy and universe, and to examine different planets such as Venus
- Temperature, Spectroscopy, Stars coming or going
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| Describe the characteristics of science, and give an example of a scientific theory. |
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| Science is something you have to research, spend time on, and most importantly be able to test and perform experiments on what you’re trying to prove. An example of a scientific theory is the Big Bang Theory. Scientists are still performing tests and experiments to try and understand more about the Big Bang Theory |
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| List Earth’s three primary motions through space. |
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| Rotational, Orbital, Precession |
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| Draw the Heliocentric and Geocentric models of the universe. |
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| Heliocentric: “My very easy method just set up nine planets” (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Plato) |
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