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The Universe Starring Man? The Impact of Scientific
The Universe Starring Man? The Impact of Scientific

... Also after Copernicus • Heat Death of the Universe? • The Big Crunch ...
Lecture6
Lecture6

... The night sky is dark This implies that the emission of starlight in the universe must be finite, in space, time or both. This is fundamental test for any cosmological model The Big-bang explains Olbers’s paradox with the finiteness of the lifetime of the Universe and hence of its stars: The univers ...
Course Expectations
Course Expectations

... 7. Galaxies are classified by shape 8. The Hubble Tuning Fork is the tool used to classify galaxies 9. The difference between active and inactive galaxies 10. Hubble’s Law is used to calculate the distance to other galaxies 11. The farther away the galaxy is the faster it is moving 12. The Big Bang ...
Answer Key: Big Bang Balloon Analysis Questions
Answer Key: Big Bang Balloon Analysis Questions

... What is the Universe? The universe is everything – planets, stars, galaxies, space, and even time! No one knows how big the universe is. In the past, many people thought the universe was infinite. Now, most cosmologists (astronomers who study the universe. “Kosmos” is a Greek word that means “the or ...
AstronomyQuotes
AstronomyQuotes

... See the world as it truly is, small and blue, beautiful in that eternal silence where it floats. ...
Astro-2: History of the Universe
Astro-2: History of the Universe

... The night sky is dark This implies that the emission of starlight in the universe must be finite, in space, time or both. This is fundamental test for any cosmological model The Big-bang explains Olbers’s paradox with the finiteness of the lifetime of the Universe and hence of its stars: The univers ...
PSCI 1414 General Astronomy
PSCI 1414 General Astronomy

... • Star system – A star and all the material that orbits it, including planets, dwarf planets like Pluto, and other small solar system bodies • Galaxy – A gravitationally bound system of stars, gas, and dust • Galaxy cluster (or group) – A collection of galaxies bound together by gravity • Superclust ...
About the Universe The Universe is everything that exists, including
About the Universe The Universe is everything that exists, including

... of the Universe, but nobody knows exactly how big it really is. However, astronomers have seen that the galaxies inside it are slowly moving away from each other. This must mean that the Universe is getting bigger all the time. Staring into space Staring into space is something people do all the tim ...
Document
Document

... 4. The Sun has a mass of about 2.0 x 1030 kg and a radius of 7.0 x 108 m. The Earth has a mass of about 6.0 x 1024 kg and a radius of 6.4 x 106 m. (a) Calculate the ratio of volume of the Sun to the volume of the Earth. ...
Y13 Cosmology HW booklet
Y13 Cosmology HW booklet

... 4. The Sun has a mass of about 2.0 x 1030 kg and a radius of 7.0 x 108 m. The Earth has a mass of about 6.0 x 1024 kg and a radius of 6.4 x 106 m. (a) Calculate the ratio of volume of the Sun to the volume of the Earth. ...
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 ...
Ch 1 Jan 17
Ch 1 Jan 17

... • A light-year is the distance light can travel in 1 year. It is not a measure of time. It is used to measure the distance to stars and galaxies. • It is about 10 trillion kilometers (6 trillion miles). • In the solar system, the AU (astronomical unit) is used. 1 AU is the average distance between t ...
PASS Content Standard 5.1
PASS Content Standard 5.1

... PASS Content Standard 5.1 ...
Inquiring minds want to know
Inquiring minds want to know

... Two detectors – one near, one far High statistics – challenge for accelerator and detector On and off axis ...
Chapter 10
Chapter 10

... nucleus of our Galaxy, and what is the probable explanation? 7. Describe the factors involved in galactic formation, including the role of collisions between galaxies. 8. Be able to identify a galaxy by its shape, according to the Hubble sequence. 9. Compare and contrast elliptical galaxies and spir ...
Section 19.3
Section 19.3

... in the past than it is today. It implies that the universe must have had a beginning. Astronomers today believe the universe exploded outward from a single point. This idea is known as the Big Bang theory. ...
understanding-the
understanding-the

... a. A group of people met together and decided to make it a theory. b. There is no other way to explain the formation of the universe. c. Distant galaxies were observed to be moving away from Earth. d. Edwin Hubble was an honest man. ...
The Universe and Galaxies - West Jefferson Local Schools
The Universe and Galaxies - West Jefferson Local Schools

... 2. ________ (fig. 26-16, pg. 832)  most ________ type of galaxy - spherical and ________ shaped  NO spiral arms, little dust and gas - generally have ________ stars (reddish in color) - Range of sizes a. ________ - trillions of stars, millions of light years in diameter b. ________ - millions of s ...
The Universe and Galaxies - West Jefferson Local Schools
The Universe and Galaxies - West Jefferson Local Schools

... 2. ________ (fig. 26-16, pg. 832)  most ________ type of galaxy - spherical and ________ shaped  NO spiral arms, little dust and gas - generally have ________ stars (reddish in color) - Range of sizes a. ________ - trillions of stars, millions of light years in diameter b. ________ - millions of ...
Quasars and Active Galaxies
Quasars and Active Galaxies

... Competing Cosmologies • “Big Bang”: 10 - 20 billion years ago the universe was much more dense than today (and therefore hot and unpleasant). • “Steady State”: As galaxies move apart from each other, new atoms are spontaneously created in empty space. These atoms coalesce to form new galaxies. The ...
ASTR100 Class 01 - University of Maryland Astronomy
ASTR100 Class 01 - University of Maryland Astronomy

...  Stellar collisions  galaxy evaporation and growth of central black hole. ...
lecture1
lecture1

... • Experiments and Observations can only be made from a very special point in space and time: Earth now. • Yet we would like to construct a scientific theory that describes the universe everywhere and at all times. ...
HW4 due - Yale Astronomy
HW4 due - Yale Astronomy

... than  the  Sun.  How  far  away  could  a  Type  Ia  supernovae  be,  and  still  be  detected  with   the  Hubble  Space  Telescope?    Express  your  answer  in  light  years.   ...
Galaxy map hints at fractal universe
Galaxy map hints at fractal universe

... And they say if the universe does become homogeneous at some point, it has to be on a scale larger than a staggering 300 million light years across. That's because even at that scale, they still observe large fluctuations – a cluster here, a void there – in the matter distribution. Most cosmologists ...
Cosmology – The Origin and Evolution of the Universe
Cosmology – The Origin and Evolution of the Universe

... cosmic time, every firecracker went off. • What would you hear? • --- one GiNormous ear-splitting “BANG”? • --- or, a continous ROAR that would never end? ...
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Expansion of the universe

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