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10 Scientific Laws and Theories You Really Should Know
10 Scientific Laws and Theories You Really Should Know

... some of the other (i.e., E=mc²). • Second Law - You can't break even- Due to everincreasing entropy, you can't return to the same energy state. Energy concentrated in one place will always flow to places of lower concentration. • Third Law - You can't quit the game – which refers to absolute zero, t ...
Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... • A light year (ly) is the distance light travels in a year – About 1016 m (~6 trillion miles) • Speed of light is 3  108 m/sec or 186,000 mi/sec ...
Chapter 1 - A Modern View of the Universe
Chapter 1 - A Modern View of the Universe

... Kessel Run in less than twelve parsecs." ...
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... 14. In what part of their life cycle are most stars in the universe? ...
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... Velocity = = 500 km/s = 0.508 Mpc/Gyr ...
Evolution and the Big Bang, ET Life Lec. 6, Jan 18, 2002
Evolution and the Big Bang, ET Life Lec. 6, Jan 18, 2002

... After one half-life 4lbs remain, after two halflives 2lbs remain and after 3 half-lives only one lb is left. Thus only ¼ of the initial # of neutrons will be left after 20 minutes because the neutron half-life is 10 minutes. ...
Standard EPS Shell Presentation
Standard EPS Shell Presentation

... The universe continued as a giant cloud of gas until about 300 million years after the Big Bang. Parts of the gas cloud began to collapse and ignite to form clusters of stars—the first galaxies. ...
4th Six Weeks Review key
4th Six Weeks Review key

... 31. Fusion occurs when ___hydrogen_ atoms fuse to form __helium____ with the resulting change in mass releases energy. 32. What type of star is our sun? (circle one) MASSIVE or AVERAGE 33. Our sun is a _____main sequence star and is the color ___yellow___. 34. Where is our sun located within the Mil ...
Tour of the Universe
Tour of the Universe

... center of a galactic bulge, there is a black hole.  Other galaxies are elliptical in shape and are ovoid and spherical. These galaxies contain much  less gas and dust than spiral galaxies and are thought to have been formed from collisions  between spiral galaxies. Irregular galaxies are shapeless a ...
Polarimetry & Star
Polarimetry & Star

... Gravitational collapse of some of these “structures” produces the first stars and galaxies. ...
What is a Scientist? - Cockeysville Middle School
What is a Scientist? - Cockeysville Middle School

... information you have gathered. http://hubblesite.org/gallery/album/galaxy/ ...
INDESCRIBABLE: Listening Guide with Louie Giglio
INDESCRIBABLE: Listening Guide with Louie Giglio

... 7. We live in a subdivision of the universe called the “Milky Way Galaxy.” 8. The “Milky Way Galaxy” itself is so big that we have to use “light years” to get around in it. 9. Light goes 5.88 trillion miles in a year… that is a “light year.” 10. The “Milky Way Galaxy” consists of billions of stars. ...
PHS 111 Test 3 Review Chapters 26-28
PHS 111 Test 3 Review Chapters 26-28

... Most of the stars in colliding galaxies: do not make contact with one another. coalesce into larger stars. exchange amounts of material in proportion to their masses. end up as binaries. undergo accelerated collapse. Cosmology is the study of the overall structure and evolution of: the universe. sta ...
PHS 111 Test 3 Review Chapters 26-28
PHS 111 Test 3 Review Chapters 26-28

... Most of the stars in colliding galaxies: do not make contact with one another. coalesce into larger stars. exchange amounts of material in proportion to their masses. end up as binaries. undergo accelerated collapse. Cosmology is the study of the overall structure and evolution of: the universe. sta ...
Sample pages 2 PDF
Sample pages 2 PDF

... the earth indicates that, approximately 14 billion years ago (the exact time remains in some dispute) the universe as we observe it was confined to a very small region of space and has been expanding from that confined space ever since (the ‘Big Bang’) (More precisely, the space itself has been expa ...
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Lecture

... Hot objects emit more and at shorter wavelengths (higher frequencies) ...
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... 57. Scientists believe that the universe is not a constant size but is ____________________ 58. When light coming from an object has longer wavelengths than expected (called a red shift), it means that object is moving _______________from us. The greater the red shift, the _______________________it ...
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Macro\micro

... (Milky Way), our galaxy. ...
The Universe: Big, weird and kind of scary!
The Universe: Big, weird and kind of scary!

... universe has always existed in more or less its current state, and always will. (most accepted until 1960s-1970s)) 2. Big Bang (Inflation) Theory: The universe began as a singularity, and suddenly expanded outwards (currently most accepted theory). ...
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Unit 1 The Universe

... atmosphere expanding after active fusion ends. – Planetary nebula -forms when a star can no longer support itself by fusion reactions in its center – White dwarf -hot, dense core of matter that remains from the collapse of a low-mass star. It is about the size of Earth. – Black dwarf-white dwarf tha ...
What Does an Astronomer Do?
What Does an Astronomer Do?

... across. A light-year is the distance it would take for light to travel in one year. Since light travels at a speed of about 186,000 miles per second, a light-year is a huge distance! The universe is made up of an uncountable number of galaxies. Only the nearest objects in our solar system can be rea ...
dark - The Institute of Mathematical Sciences
dark - The Institute of Mathematical Sciences

... composed of protons, neutrons, and electrons that we learn about in school. It comprises gas, dust, stars, planets, people, etc. Dark Matter: This makes up about 25% or about a quarter of our Universe. This is the so-called "missing mass" of the Universe. It comprises the dark matter halos that surr ...
Astronomy 110G Review Sheet for Exam #3 The
Astronomy 110G Review Sheet for Exam #3 The

... Einstein’s and Newton’s theories have been in conflict, the former have prevailed.) • The radiation from the “big bang” is seen today as the “cosmic background radiation” which peaks at microwave frequencies. This is 10,000°K radiation “cooled” to about 3°K by the redshift associated with the univer ...
Structure of the Universe
Structure of the Universe

... massive stars, but rather a white dwarf that accretes mass from a companion until it exceeds the Chandrasekhar limit (1.4 Msun) ...
Macro\micro - shoukath.net
Macro\micro - shoukath.net

... (Milky Way), our galaxy. ...
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Chronology of the universe



The chronology of the universe describes the history and future of the universe according to Big Bang cosmology, the prevailing scientific model of how the universe developed over time from the Planck epoch, using the cosmological time parameter of comoving coordinates. The model of the universe's expansion is known as the Big Bang. As of 2015, this expansion is estimated to have begun 13.799 ± 0.021 billion years ago. It is convenient to divide the evolution of the universe so far into three phases.
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