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teachers version.
teachers version.

... 2) A hundred years ago Edwin Hubble and other scientists looked at galaxies and measured how far away they were and how fast they were moving. Some modern sample data is shown below. Name of galactic cluster ...
Study and Be Confident!! - Grade 5
Study and Be Confident!! - Grade 5

... d. All planets revolve around a star. 10. What is one of the reasons why the outer planets are referred to as gas giants? e. We can see the rings of particles orbiting them. f. The outer planets have solid crusts. g. The outer planets have liquid cores. h. We can only see their atmospheres. ...
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Properties of stars

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Chapter 36 Summary – Magnetism
Chapter 36 Summary – Magnetism

... Directions: #1-6, are true/false. Write the sentence and explain why it’s true, or how to make it true. #7-23 are multiple choice. Write the question and correct answer and explain why. 1) Diffuse reflection occurs when light is refracted in many directions from a rough surface. 2) Reflection occurs ...
Requiem for a Star
Requiem for a Star

... Stars Comparable to Sun • M up to about 3 or 4 solar masses • As a Main Sequence star can only use hydrogen as a fuel • When hydrogen is exhausted collapse of interior is inevitable • Increase in temperature caused by collapse suddenly ignites unprocessed hydrogen, causing star to expand to become ...
RELATIVITY
RELATIVITY

... MICHELSON 1878 Repeated Foucault’s experiment with rotating mirror, but passed the beam back and forth between two mirrors for a total distance of 22 miles. C= 186,295 mps in air (0.007% too high) When Michelson evacuated the tube, and set up a beam length of 10 miles. c= 186,271 mps (0.006% too low ...
What stars do Summary: Nuclear burning in stars •
What stars do Summary: Nuclear burning in stars •

... supernova ...
Astronomy and the Universe - Department of Physics and Astronomy
Astronomy and the Universe - Department of Physics and Astronomy

... What are the stars? Do they last forever? What are galaxies? What do astronomers learn by studying them? How does measuring angles help astronomers learn about objects in the sky? What is powers-of-ten notation, and why is it useful in ...
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... Field Observed ...
Investigation of the FIR-Radio correlation at small scales in the Galaxy
Investigation of the FIR-Radio correlation at small scales in the Galaxy

... In my PhD. Project I will study these correlations, most notably, the far-infrared and radio continuum correlation on scales corresponding to the size of small molecular clouds. I will also study the possibility that the correlation between CO and far-infrared luminosities is caused by strong select ...
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... The classical view begins with the observation that atoms and molecules are composed of charged particles, and these charges are the handle by which an electromagnetic field exerts a force on the atom or molecule. The force exerted on the molecules depends on the strength of the field, the magnitude ...
“solar system” model of the atom
“solar system” model of the atom

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Variable Stars: Pulsation, Evolution and applications to Cosmology
Variable Stars: Pulsation, Evolution and applications to Cosmology

Stellar Evolution Game (PDF: 112k)
Stellar Evolution Game (PDF: 112k)

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Chapter 4 Questions Perception of Color
Chapter 4 Questions Perception of Color

... • A red object absorbs all visible light except red light. • A blue object absorbs all visible light except blue light. • A black object absorbs all visible light and does not reflect light back. ...
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Star formation jeopardy

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Astronomy Assignment

... ‘We are all just Star Stuff”- Carl Sagan, truer words have never been spoken. Every atom of our bodies was formed in the core of some long dead star. But how and where and why? In order to answer these questions we must understand the stars themselves and the clouds from which they arise and often a ...
Introduction to Astronomy
Introduction to Astronomy

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"Seeing" Dark Matter

... These particular predictions are powerful, because they do not depend on assumptions about how gravity operates over cosmic distances. Since Zwicky’s original observations, astronomers have found many astronomical objects that demand far more gravity than the observed normal matter and the conventi ...
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56.Kirkpatrick_sci_hi

... I-band DSS image from 1989 (blue) and J-band 2MASS image from 1999 (red). Motion object is marked. ...
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Nature template

... Supplementary Figure 4. Results of Monte-Carlo simulation. The plot shows the probability distribution of systems with no stars having initial masses greater than 130 M versus the mass of the upper mass cutoff. The simulation uses 60,000 systems, each with test points having a mass distribution tha ...
TEKS PDF - Virtual Observatory
TEKS PDF - Virtual Observatory

... investigation. On the other hand, when conditions can be controlled in order to focus on a single  variable, experimental research design is used to determine causation. Students should experience both  types of investigations and understand that different scientific research questions require diffe ...
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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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