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CENTRAL TEXAS COLLEGE
CENTRAL TEXAS COLLEGE

... time keeping, and navigation. Nowadays, astronomy is adding other practical applications, such as addressing vital questions about climate change on Earth. It is further expanding our knowledge of the solar system and space, where there are potentially unlimited supplies of energy and materials. Ove ...
Lecture Topics 1023
Lecture Topics 1023

... ASTR 1023 Lecture Topics These are the headings of the paragraphs into which ASTR 1023 lectures are divided. Use them to check your notes for completeness, and to see how the course is organized. It is also a good idea to cross-check these topics with your reading assignments, because some topics ar ...
The Search for the Earliest Galaxies
The Search for the Earliest Galaxies

... was a critical watershed in the evolving universe. It was when the intergalactic medium became substantially ionized as we see it today. This reionization was completed approximately 1 billion years after the Big Bang. ...
Quasar Formation and Energy Emission in Black Hole Universe
Quasar Formation and Energy Emission in Black Hole Universe

... black holes were formed when the universe was merely 1-2 billion years after the big bang had taken place [5, 21]. How the supermassive black holes with billions of solar masses were formed so rapidly during the early universe is a great mystery raised by astronomers recently [22]. Theoretically, su ...
Chapter 26: Stars, Galaxies, and the Universe Stars
Chapter 26: Stars, Galaxies, and the Universe Stars

... against its true brightness or magnitude. For stars on the main sequence, the hotter they are, the brighter they are. The length of time a star is on the main sequence depends on how long a star is able to balance the inward force of gravity with the outward force provided by the nuclear fusion goin ...
Chapter 15 Stars, Galaxies, and Universe
Chapter 15 Stars, Galaxies, and Universe

... •Irregular – smaller than other galaxies •Young stars, lots of gas and dust •Located close to larger galaxies. ...
The Cosmological Distance Ladder
The Cosmological Distance Ladder

... distances) and in the Tully-Fisher and HII region methods (too low) and that best overall value for H0 was Ho = 67 +_ 12 km/s/Mpc Feb 8th 2008 ...
No Slide Title
No Slide Title

... • BUT Sigurdsson et al. (2003, Science, 301, 193) claim that a millisecond pulsar in globular M4 has a Jupiter size companion – Claim based on timing anomalies – If true, then planets may have been forming 12 billion years ago in a very metal-poor environment (<0.1 x solar) – Alternatively, planet m ...
Staff Application - University of Utah School of Computing
Staff Application - University of Utah School of Computing

... sulfur, S) required to form these compounds. Chemical bonds are broken between oxygen (O) and carbon (C), hydrogen (H), nitrogen, and sulfur, and new bonds are formed in products that include gaseous oxygen (O2) and organic compounds.” 13 Light energy provides the necessary additional energy to brea ...
A Brief History of Time - Stephen Hawking
A Brief History of Time - Stephen Hawking

... to explain the existence of the universe. (Within the universe, you always explained one event as being caused by some earlier event, but the existence of the universe itself could be explained in this way only if it had some beginning.) Another argument was put forward by St. Augustine in his book ...
“Here Comes the Sun” How the new
“Here Comes the Sun” How the new

... are equivalent and the choice is arbitrary. The same could be said not just for the Earth but for any object in the universe. General Relativity is the current best physical theory of gravitation and it might incorporate Mach’s Principle, although this is still a matter of debate. However, invoking ...
The Big Bang
The Big Bang

... In the distant past, many large galaxies emitted a large amount of light from processes associated with the supermassive black holes at their centers (“Active” Galaxies) ...
The quest for the size of the universe in early relativistic cosmology
The quest for the size of the universe in early relativistic cosmology

... radius of space-time. We then examine the different works in this field by Ludwik Silberstein (1872-1948) and Knut Lundmark (1889-1958). Finally, we give an overview of further investigations on the topic carried out before the discovery of the expanding universe. The variety of methods to obtain th ...
Section 6 The Expanding Universe The Doppler Effect
Section 6 The Expanding Universe The Doppler Effect

... determine the mass of a galaxy (or a cluster of galaxies). By measuring the amount of light reaching the Earth, scientists can estimate the number of stars in the galaxy. Knowing the number of stars in the galaxy, scientists can mathematically determine the mass of the galaxy. Fritz Zwicky used both ...
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... * A long time ago, astronomers thought that the Earth was the centre of the Universe. This was called the geocentric model. The evidence for this model came from observations of the sky using the naked eye. After the telescope was invented, astronomers quickly gathered evidence which showed that the ...
transcript - Bright Star Ministries
transcript - Bright Star Ministries

... astray at times. Scripture is unfortunately subject to the same flaw: what we read and how we interpret what we read can lead us into different directions. If God created both nature and inspired the Bible to be written, then these two disciplines must cohere. If they don’t, something must be wrong ...
The Comprehensible Universe
The Comprehensible Universe

... gravity. The outside region was very cold, dark, and ...
Stars, Galaxies, and the Universe Section 1
Stars, Galaxies, and the Universe Section 1

... • The second and longest stage in the life of a star is the main-sequence stage. During this stage, energy continues to be generated in the core of the star as hydrogen fuses into helium. • A star that has a mass about the same as the sun’s mass stays on the main sequence for about 10 billion years. ...
What is a planet? - X-ray and Observational Astronomy Group
What is a planet? - X-ray and Observational Astronomy Group

... • BUT Sigurdsson et al. (2003, Science, 301, 193) claim that a millisecond pulsar in globular M4 has a Jupiter size companion – Claim based on timing anomalies – If true, then planets may have been forming 12 billion years ago in a very metal-poor environment (<0.1 x solar) – Alternatively, planet m ...
Test 4 Review Clicker Questions
Test 4 Review Clicker Questions

... The Doppler shifts of 21-cm radiation from hydrogen in the spiral arms provides astronomers with a tool to map out the Galaxy’s structure. Copyright © 2010 Pearson Education, Inc. ...
Chapter 1 - Pearson Education
Chapter 1 - Pearson Education

... system by sending probes to the planets, and many of our most powerful observatories, including the Hubble Space Telescope, reside in space. On the ground, computer design and control have led to tremendous growth in the size and power of telescopes, particularly in the past decade. Many of these ef ...
Lecture 2: ppt, 5 MB
Lecture 2: ppt, 5 MB

... Supernovae: Massive stars end in glorious explosions. Hubble found three mysterious rings of material encircling a doomed star that exploded as a supernova in 1987. During the years since the eruption, Hubble spied brightened spots on the ...
Gone in a flash: supernovae in the survey era
Gone in a flash: supernovae in the survey era

... brighter than a Type Ia supernova). The first of SLSN (Gal-Yam 2012), commonly defined as CFHT, or DECam on the Cerro Tololo Interevent, SCP 06F6, was identified in 2009 and had being brighter than –21 in absolute magnitude American Observatory 4 m Blanco telescope), broad, unexplained spectral abso ...
Galaxies - SD43 Teacher Sites
Galaxies - SD43 Teacher Sites

... galaxy. A galaxy forms when gravity causes a large, slowly spinning cloud of gases, dust, and stars to contract. All the stars in the universe were formed in galaxies. To get a better idea of just how many stars 100 billion is, imagine a star being the size of a grain of sand. The number of stars yo ...
A Brief History of Time
A Brief History of Time

... outermost sphere carried the so-called fixed stars, which always stay in the same positions relative to each other but which rotate together across the sky. What lay beyond the last sphere was never made very clear, but it certainly was not part of mankind’s observable universe. Ptolemy’s model prov ...
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Fine-tuned Universe

The fine-tuned Universe is the proposition that the conditions that allow life in the Universe can only occur when certain universal fundamental physical constants lie within a very narrow range, so that if any of several fundamental constants were only slightly different, the Universe would be unlikely to be conducive to the establishment and development of matter, astronomical structures, elemental diversity, or life as it is understood. The proposition is discussed among philosophers, scientists, theologians, and proponents and detractors of creationism.Physicist Paul Davies has asserted that ""There is now broad agreement among physicists and cosmologists that the Universe is in several respects ‘fine-tuned' for life"". However, he continues, ""the conclusion is not so much that the Universe is fine-tuned for life; rather it is fine-tuned for the building blocks and environments that life requires."" He also states that Template:"" 'anthropic' reasoning fails to distinguish between minimally biophilic universes, in which life is permitted, but only marginally possible, and optimally biophilic universes, in which life flourishes because biogenesis occurs frequently"". Among scientists who find the evidence persuasive, a variety of natural explanations have been proposed, such as the anthropic principle along with multiple universes. George F. R. Ellis states ""that no possible astronomical observations can ever see those other universes. The arguments are indirect at best. And even if the multiverse exists, it leaves the deep mysteries of nature unexplained.""
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