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AstronomyQuotes
AstronomyQuotes

... star lost in a galaxy tucked away in some forgotten corner of a universe in which there are far more galaxies than people. ...
White Dwarf Stars
White Dwarf Stars

... How much longer / shorter is the lifetime of a 5 Msun star main sequence compared to the lifetime of a 1 Msun main sequence star? A. 5 times longer B. 5 times shorter C. 50 times shorter D. 50 times longer E. They both have the same lifetime ...
Expansion of the Universe
Expansion of the Universe

...  Time, space and matter all began with the Big Bang. In a fraction of a second, the Universe grew from smaller than a single atom to bigger than a galaxy and it kept on growing at a fantastic rate It is still expanding today After the big bang, the universe expanded quickly (and continues to expa ...
All these different energies are classified according to wavelength
All these different energies are classified according to wavelength

... blue or red? If a galaxy is moving away from earth, is it blue or red? ...
Galaxies - Wallkill Valley Regional High School
Galaxies - Wallkill Valley Regional High School

... - Range from dwarf to giant galaxies based on number of stars ...
The Ever Expanding Universe
The Ever Expanding Universe

... Herculean task that involved over 2000 years of work! The Greeks knew how to do it using their mathematical invention trigonometry (the mathematics of right triangles), but a telescope precise enough to measure extremely tiny angles was not available until the 19th century when Friedrich Bessel succ ...
Watch the episode titled “The Milky Way” from the series “The
Watch the episode titled “The Milky Way” from the series “The

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Milky Way galaxy - Uplift North Hills Prep
Milky Way galaxy - Uplift North Hills Prep

... universe, its origin, and its future. foundation: Einstein’s general theory of relativity and its theory of gravitation—for in the large-scale structure of the universe, gravity is the dominant force. ...
~Crowfoot
~Crowfoot

... a) arises from the Balmer γ transition. b) is due to preferential scattering of blue light as in Earth’s sky. c) is the light from an embedded blue star. 3)2 The “Pillars of Creation” on this image Eagle Nebula a) show the destruction of a nebula by a supernova explosion b) are the jets from a young ...
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... _____ 5. A scientist can identify a star’s composition by looking at a. the star’s prism. b. the star’s continuous spectrum. c. the star’s absorption spectrum. d. the star’s color. _____ 6. If the universe expands forever, a. the universe will collapse. b. the universe will repeat itself. c. the uni ...
Date - Penn Physics
Date - Penn Physics

... The movies and tutorials can be previewed on Astronomy Place at www.astronomyplace.com The tutorials in boldface should be completed and submitted prior to class. The movies are strongly recommend. The other online materials and materials from the SkyGazer CD Rom are optional. (The recommended SkyGa ...
III. Contents of The Universe
III. Contents of The Universe

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Astronomy - Wappingers Central School District
Astronomy - Wappingers Central School District

... conference. I will be updating it to reflect the changes in content in this years rules. I’m not sure yet how to test 50 teams at States on the use of DS9 image viewing software, and won’t ...
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Cosmic Landscape Introduction Study Notes About how

... The Weak Force - This force is responsible for nuclear beta decay and other similar decay processes involving fundamental particles. The Gravitational Force - This is the force that holds us onto the Earth. It could be important in our daily life, but on the scale of atomic world it is of negligible ...
Problem Set # 8: The Last Problem Set Due Wednesday, December
Problem Set # 8: The Last Problem Set Due Wednesday, December

... 1) [20 points] The dim little star Proxima Centauri, the Sun’s nearest neighbor among the stars, has a mass M = 0.12Msun , where Msun is the Sun’s mass. It has a luminosity L = 0.00014Lsun , where Lsun is the Sun’s luminosity. Like the Sun, Proxima Centauri is powered by the fusion of hydrogen into ...
Chapter 8, Lesson 5, pdf
Chapter 8, Lesson 5, pdf

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Slide 1

... The Universe contains billions of galaxies, each containing millions or billions of stars. The space between the stars and galaxies is largely empty. ...
Chapter 26 Book Questions
Chapter 26 Book Questions

... 29. Astronomers theorize that the universe came into being in an event called the _________________. 30. Circle the letter of each sentence that is true according to the big bang theory. A. The matter and energy in the universe was once concentrated in a very hot region smaller than a sentence perio ...
ASTRONOMY 1303 Syllabus Fall 2015
ASTRONOMY 1303 Syllabus Fall 2015

... explore heavenly objects like clusters, double stars and nebulas. The date of this lab is dependent upon the weather and phase of the Moon. This fall we will also have an opportunity to view a total lunar eclipse. It is happening in the evening of the 27th of September. Weather permitting the observ ...
Astrophysics Presentation
Astrophysics Presentation

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Lec12
Lec12

... move into spiral arms 2. Squeezing of clouds triggers star formation 3. Young stars flow out of spiral arms ...
Historical Overview of the Universe
Historical Overview of the Universe

... In the nineteenth century, distances to nearby stars were measured, nebulae were catalogued, and the spectroscopic decomposition of light was learned as the first astrophysical method. In the twentieth century, stellar spectroscopy was developed as a way of determining stellar parameters, in particu ...
THE COSMIC DANCE
THE COSMIC DANCE

... This coming together creates of electrons and protons to make Hydrogen gives off light we call… MICROWAVES. This is how we know what the lumps of matter look like At 380,000 years after the Big Bang—The Recombination Era. ...
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... Biophysics: Imaging  Spectroscopy • Spectroscopy is far more powerful than imaging “A spectrum is worth a thousand pictures” • Every element or object in the Universe has unique spectral signature (like DNA) • Radiation absorption and emission highly efficient at resonant energies corresponding to ...
Astronomy
Astronomy

... Astronomy Vocabulary ...
< 1 ... 35 36 37 38 39 40 41 42 43 >

Structure formation

In physical cosmology, structure formation refers to the formation of galaxies, galaxy clusters and larger structures from small early density fluctuations. The Universe, as is now known from observations of the cosmic microwave background radiation, began in a hot, dense, nearly uniform state approximately 13.8 billion years ago. However, looking in the sky today, we see structures on all scales, from stars and planets to galaxies and, on still larger scales still, galaxy clusters and sheet-like structures of galaxies separated by enormous voids containing few galaxies. Structure formation attempts to model how these structures formed by gravitational instability of small early density ripples.The modern Lambda-CDM model is successful at predicting the observed large-scale distribution of galaxies, clusters and voids; but on the scale of individual galaxies there are many complications due to highly nonlinear processes involving baryonic physics, gas heating and cooling, star formation and feedback. Understanding the processes of galaxy formation is a major topic of modern cosmology research, both via observations such as the Hubble Ultra-Deep Field and via large computer simulations.
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