Conceptual Physics - Southwest High School
... letter F on the diagrams below. Note that each lens has two focal points - one on each side of the lens. Unlike mirrors, lenses can allow light to pass through either face, depending on where the incident rays are coming from. Subsequently, every lens has two possible focal points. The distance fro ...
... letter F on the diagrams below. Note that each lens has two focal points - one on each side of the lens. Unlike mirrors, lenses can allow light to pass through either face, depending on where the incident rays are coming from. Subsequently, every lens has two possible focal points. The distance fro ...
MT 1 Answers Version C - The University of Oklahoma Department
... The color is determined by the wavelength region where the object is brightest ...
... The color is determined by the wavelength region where the object is brightest ...
1. a. Collisionless Boltzmann—particles moving in smooth potential
... Note that the errors in Oort’s A and B combine with errors in the distance to make V0 depressingly uncertain so you will see a variety of values used in the literature. b. We can derive V(R) for R
... Note that the errors in Oort’s A and B combine with errors in the distance to make V0 depressingly uncertain so you will see a variety of values used in the literature. b. We can derive V(R) for R
Red-shift - Clark Planetarium
... Note that the position of the Ha line is no longer where it was in the laboratory spectrum of hydrogen. Instead, the peak has been shifted towards the longer wavelength part of the spectrum, which is the redder end of the spectrum. This phenomenon is called a “red-shift.” It turns out that the amoun ...
... Note that the position of the Ha line is no longer where it was in the laboratory spectrum of hydrogen. Instead, the peak has been shifted towards the longer wavelength part of the spectrum, which is the redder end of the spectrum. This phenomenon is called a “red-shift.” It turns out that the amoun ...
Slide 1
... Things are seen as they are since this is the best understood of all possible worlds Modulo variance. And physics. Of course galaxy formation models are correct. They have always been correct. Just different than they used to be. Models should be used to isolate and investigate what we do not unders ...
... Things are seen as they are since this is the best understood of all possible worlds Modulo variance. And physics. Of course galaxy formation models are correct. They have always been correct. Just different than they used to be. Models should be used to isolate and investigate what we do not unders ...
Expanding Universe
... A galaxy happens about every 100 years in an average galaxy. So every year is you look in 100 galaxies, Or 10 per year if you look in 1,000 galaxies. ...
... A galaxy happens about every 100 years in an average galaxy. So every year is you look in 100 galaxies, Or 10 per year if you look in 1,000 galaxies. ...
The Orbital Method and Galaxies
... The answer is not due to the strange properties of dark matter. The problem arises any time we use Newton’s law of universal gravitation, F = GM1 M2/r2, and the masses are not point masses. Now, there are no point masses - except possibly black holes - but many masses have negligible radii. For exam ...
... The answer is not due to the strange properties of dark matter. The problem arises any time we use Newton’s law of universal gravitation, F = GM1 M2/r2, and the masses are not point masses. Now, there are no point masses - except possibly black holes - but many masses have negligible radii. For exam ...
Teacher`s Show Guide
... home galaxy. Put a yellow dot roughly 2/3 of the way from the center to the edge and label it "Sun." Discuss how we see the band of faint starlight in our sky that we call the Milky Way given our Sun's position in the galaxy. Explain how all the stars we can see in the night sky are members of this ...
... home galaxy. Put a yellow dot roughly 2/3 of the way from the center to the edge and label it "Sun." Discuss how we see the band of faint starlight in our sky that we call the Milky Way given our Sun's position in the galaxy. Explain how all the stars we can see in the night sky are members of this ...
From Spyglasses to Space Telescopes
... As the 20th century began, Albert Einstein advanced his General Theory of Relativity, which fundamentally changed our understanding of gravity, and the Universe. One of the predictions of his theory was that the light should bend as it passed by a massive body like a star. In 1919, a team of astron ...
... As the 20th century began, Albert Einstein advanced his General Theory of Relativity, which fundamentally changed our understanding of gravity, and the Universe. One of the predictions of his theory was that the light should bend as it passed by a massive body like a star. In 1919, a team of astron ...
Seating Chart for Final Exam PHOTO ID REQUIRED! SIT IN YOUR ASSIGNED ROW!
... Slide 3: You must work your way out rung by rung, starting with the parallax method. How does the parallax method work? Pulsating variables used to get position of center of our galaxy + distance to M31, etc. What are pulsating variables and how are they used? Hubble’s law: v is measured from Dopple ...
... Slide 3: You must work your way out rung by rung, starting with the parallax method. How does the parallax method work? Pulsating variables used to get position of center of our galaxy + distance to M31, etc. What are pulsating variables and how are they used? Hubble’s law: v is measured from Dopple ...
