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Center of the Universe Card Sort
Center of the Universe Card Sort

... Early peoples knew that the stars, planets, Sun and Moon “moved.”  They were able to make calendars and predict cosmic events like comets.  They often thought the stars and planets were demons, gods, demigods, etc. ...
AY1 Homework for Quiz 2: Spring 2017
AY1 Homework for Quiz 2: Spring 2017

... A. How  much  energy  can  the  Sun  produce  via  this  mechanism  with  the  2  ×  1032   grams  of  hydrogen  in  the  core  where  the  temperature  is  hot  enough  for  fusion   to  occur?   ...
Photoelectric Effect Practice Problems
Photoelectric Effect Practice Problems

Photoelectric Effect Practice Problems
Photoelectric Effect Practice Problems

... explain this contradiction by assuming that light energy is quantized and that higher frequencies of light have a bigger quantum. Explain why light energy being quantized this way means that a blackbody will emit less energy at higher frequencies. ...
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01 - Ionia Public Schools

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50 Years of Quasars

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Arrangement of Electrons in Atoms

... Calculate the wavelength of a radio wave with a frequency of 102.7 x 106s-1 Determine the frequency of light whose wavelength is 5.267 nm. ...
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File - Earth Science With Mrs. Locke

... More planets, moons around most planets, the asteroid belt, comets are made of ice and rock, tectonic plates are shifting, there is water on the moon and Mars, their might have been life on Mars or the moon that is covered in giant oceans, Jupiter has a really large storm, we are not the only galaxy ...
protostars low mass stars intermediatemass stars red giant planetary
protostars low mass stars intermediatemass stars red giant planetary

... Stars form inside relatively dense concentrations of interstellar gas and dust known as ​ molecular clouds​ .  Very cold  temperatures bind molecules together & cause density to increase. When density is high enough, stars form!  ...
File - Mr. Goodyear Astronomy
File - Mr. Goodyear Astronomy

Ch. 14 Formation of Stars
Ch. 14 Formation of Stars

... expands. This results in a lower central temperature and density and slows nuclear fusion until the star regained stability. • The same process works in reverse: if less energy were generated, then the star would contract slightly and cause central temperature and density (and energy production) to ...
6/24/11 You in Outer Space Curriculum Map Clever Crazes for Kids
6/24/11 You in Outer Space Curriculum Map Clever Crazes for Kids

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GIZMO H-RDiagramSE

... Gizmo Warm-up In the early 1900s, astronomers were able to identify many star characteristics such as color, size, temperature, and luminosity—or how bright a star is. However, astronomers did not yet understand exactly how these characteristics were related. Using the H-R Diagram Gizmo™, you will d ...
4.5 Band Gap Energies and Spectrometry
4.5 Band Gap Energies and Spectrometry

... The wavelength λ of the light can be calculated using   dSin d is the line spacing on the diffraction grating. Check the number of lines per millimetre on the grating (600lines/mm) and work out the distance between the lines. Calculate λ and convert your answer to nanometres the usual units for ...
A Red Giant - Cloudfront.net
A Red Giant - Cloudfront.net

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Grade 9 Science – Unit 4 Space Quiz

... d. A large rotating collection of gas, dust and other objects e. None of the above 3. What is “…a celestial object that orbits the Sun and has a spherical shape but does not ...
Solar Nebula Theory
Solar Nebula Theory

... Large (106 km), hot (106 K) region of diffuse gas surrounding Sun • Heated to such high temperatures by the Sun’s magnetic field • Visible during a total solar eclipse or with use of coronagraph ...
Seyfert Galaxies - Otterbein University
Seyfert Galaxies - Otterbein University

... • measure distances to other galaxies using the periodluminosity relationship for Cepheid variables • Type I supernovae also used to measure distances – Predictable luminosity – a standard candle ...
Gravity/An invisible force that pulls a less massive object - Zoe-s-wiki
Gravity/An invisible force that pulls a less massive object - Zoe-s-wiki

... galaxy/a system that is made up of billions of stars, star clusters and glowing clouds of dust and gas universe/all of the galaxies and the space around them; everything in space nebula/a cloud of dust and gas within a galaxy Big Bang Theory/the theroy that the universe was created by a huge explosi ...
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main-sequence stars

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TED Connection: Far, far away galaxies and why they matter
TED Connection: Far, far away galaxies and why they matter

... enormous and describe a trait that its size gives it that something similar yet smaller does not have. _________________________________________________________________________________________ _________________________________________________________________________________________ 5. The second rea ...
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8.1 Touring the Night Sky Pg. 308 #1

... 1. Astronomers study what is beyond Earth like stars, planets, and moons, solar systems, even other galaxy’s. 2. Being “luminous” means to have, produce or give off light. For example, the nuclear fusion on the light gives off light that shines on the earth. 3. The Moon reflects light from the sun w ...
Variable Stars
Variable Stars

... trillion times brighter than the Sun! Quasars are believed to produce their energy from massive black holes in the center of the galaxies in which the quasars are located. Because quasars are so bright, they drown out the light from all the other stars in the same galaxy. ...
COSMOLOGY A FLAT EARTH GEOCENTRIC MODEL or the
COSMOLOGY A FLAT EARTH GEOCENTRIC MODEL or the

... THE PREDICTIVE POWER OF THE CMB The CMB is one of the strongest pieces of evidence for the Big Bang model. The Big Bang theory makes highly accurate predictions about the size and types of anisotropies in the CMB as well as its nearly perfect blackbody spectrum, all of which have been verified by ex ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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