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... microscopic, multidimensional strings ...
PPT - University of Arizona
PPT - University of Arizona

... • 4.2 light years from the Sun • Alpha Centauri A and Alpha Centauri B are orbiting each other with period 80 years, separation 23 Astronomical Units. • Proxima Centauri is 13,000 AU from Alpha Centauri A and B. ...
Astronomy 201: Cosmology
Astronomy 201: Cosmology

... 1 light year = the distance light travels in one year = almost 10 trillion kilometers or 6 trillion miles (one trillion = 1012 = 1,000,000,000,000) Because light takes time to travel through space, when we look farther away in distance, we look farther back in TIME. The farthest we can see in space ...
stars
stars

... is good because we want to stay far away from the supermassive black hole at the center of our galaxy. ...
Newton
Newton

...  He figured out that you can calculate the pull of gravity between 2 objects by multiplying their mass by the square of the distance between them.  This calculation allows astronomers to predict precisely the movement of every planet, star, and galaxy in the Universe. ...
Galaxies
Galaxies

... • The first formation was about 13 billion years ago. • Gravity pulled small gas clouds together—with enough density, stars form. • These first galaxies were elliptical shapes. ...
Refraction Rules for a Converging Lens
Refraction Rules for a Converging Lens

... depends upon the total internal reflection of light rays traveling through tiny optical fibers. The fibers are so small that once the light is introduced into the fiber with an angle within the confines of the numerical aperture of the fiber, it will continue to reflect off the walls of the fiber an ...
Pre-Visit Classroom Activity
Pre-Visit Classroom Activity

... from the two elements _____________(Fe) and ___________(Ni) which make it so heavy and dense. It is 4.5 billion years old (the oldest thing you could ever touch!) and can help us answer questions about the origin of our planet and solar system. ...
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HST Observations of the

... because it did not become obstructed during orbit by the Earth or Moon and it is also relatively free of foreground stars and other galaxy clusters  images of the region were taken using ultraviolet, optical and infrared ...
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Slide 1

... Amino Acids are the building blocks of life (make up proteins/enzymes). They are found naturally in space! ...
universalgravitation
universalgravitation

... The constant of proportionality (G) in the above equation is known as the universal gravitation constant. Henry Cavendish determined the precise value of G experimentally in the century after Newton's death. The value of G is found to be G = 6.673 x 10-11 N m2/kg2 The units on G may seem rather odd ...
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P1 - The Earth in the Universe

... • Information about distant stars and galaxies comes only from the radiation astronomers can detect • Light pollution interferes with observations of the night sky ...
Unpacking Outcomes - NESD Curriculum Corner
Unpacking Outcomes - NESD Curriculum Corner

... Key vocabulary – ray, refraction, reflection, critical angle, total internal reflection, refractive index, medium converging/diverging lenses, ray diagram, type (real or virtual), attitude, orientation (upright or inverted), position (relative to optical center), fibre optics, polarization, wave, bo ...
Modern physics
Modern physics

... Almost the same energy for l=n-1, and for high n. ...
Astronomy Solar System Formation Sun and Stellar Evolution
Astronomy Solar System Formation Sun and Stellar Evolution

... 9. Be prepared to visually identify these layers. 10. What affects do these above characteristics have on the Earth (if any)? 11. How is the Sun’s magnetic field related to the above characteristics? 12. The Sun’s Interior a. What is the source of energy production? Have a rough idea how this proces ...
What`s in the sky tonight - Forsyth Astronomical Society
What`s in the sky tonight - Forsyth Astronomical Society

Lots of free resources!
Lots of free resources!

... Accessible Astronomy Resources “The International Astronomical Union (IAU) has recognized the potential of astronomy to contribute to education and creating a better world. To fulfill this potential, however, astronomy must be accessible to everyone, regardless of background, learning styles or abil ...
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Lecture 5: Matter Dominated Universe: CMB Anisotropies and Large

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Going to the End of the Earth to Learn About the Beginning of the

Physics 161 Homework 1 - Solutions Friday August 26, 2011
Physics 161 Homework 1 - Solutions Friday August 26, 2011

The Modern Origins Story: From the Big Bang to Habitable Planets
The Modern Origins Story: From the Big Bang to Habitable Planets

Telescope - St John Brebeuf
Telescope - St John Brebeuf

... Reflecting telescopes do not suffer from Chromatic Aberration. All wavelengths will reflect off the mirror in the same way. Reflecting telescopes can be made very large because the mirrored surfaces have plenty of support. Thus, reflecting telescopes can greatly increase in light gathering and resol ...
Document
Document

... Reflecting telescopes do not suffer from Chromatic Aberration. All wavelengths will reflect off the mirror in the same way. Reflecting telescopes can be made very large because the mirrored surfaces have plenty of support. Thus, reflecting telescopes can greatly increase in light gathering and resol ...
Telescope
Telescope

... Reflecting telescopes do not suffer from Chromatic Aberration. All wavelengths will reflect off the mirror in the same way. Reflecting telescopes can be made very large because the mirrored surfaces have plenty of support. Thus, reflecting telescopes can greatly increase in light gathering and resol ...
Lesson 16.3
Lesson 16.3

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Gravitational lens

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