- published: 25 Apr 2012
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Stellar nucleosynthesis is the process by which the natural abundances of the chemical elements within stars change due to nuclear fusion reactions in the cores and overlying mantles of stars. Stars are said to evolve (age) with changes in the abundances of the elements within. Core fusion increases the atomic weight of its gaseous elements, causing pressure loss and contraction accompanied by increase of temperature. Stars lose most of their mass when it is ejected late in their stellar lifetimes, thereby increasing the abundance of elements heavier than helium in the interstellar medium. The term supernova nucleosynthesis is used to describe the creation of elements during the evolution and explosion of a presupernova star, as Fred Hoyle advocated presciently in 1954. One stimulus to the development of the theory of nucleosynthesis was the variations in the abundances of elements found in the universe. Those abundances, when plotted on a graph as a function of atomic number of the element, have a jagged sawtooth shape that varies by factors of tens of millions. This suggested a natural process other than a random distribution. Such a graph of the abundances can be seen at History of nucleosynthesis theory. Stellar nucleosynthesis is the dominating contributor to several processes that also occur under the collective term nucleosynthesis.
Steward Observatory is the research arm of the Department of Astronomy at the University of Arizona (UA). Its offices are located on the UA campus in Tucson, Arizona (USA). Established in 1916, the first telescope and building were formally dedicated on April 23, 1923. It now operates, or is a partner in telescopes at five mountain-top locations in Arizona, one in New Mexico, and one in Chile. It has provided instruments for three different space telescopes and numerous terrestrial ones. Steward also has one of the few facilities in the world that can cast and figure the very large primary mirrors used in telescopes built in the past decade.
Steward Observatory owes its existence to the efforts of American astronomer and dendrochronologist Andrew Ellicott Douglass. In 1906, Douglass accepted a position as Assistant Professor of Physics and Geography at the University of Arizona in Tucson, Arizona. Almost immediately upon his arrival in Tucson, Douglass established astronomical research programs using an 8-inch refracting telescope on loan from the Harvard College Observatory and actively began to pursue funding to construct a large research-class telescope in Tucson. Over the next 10 years, all of Douglass’ efforts to secure funding from the University and the Arizona Territorial (and later State) Legislatures ended in failure. During this time period, Douglass served the University of Arizona as Head of the Dept. of Physics and Astronomy, Interim President, and finally Dean of the College of Letters, Arts, & Sciences.
Creative Commons (CC) is a non-profit organization devoted to expanding the range of creative works available for others to build upon legally and to share. The organization has released several copyright-licenses known as Creative Commons licenses free of charge to the public. These licenses allow creators to communicate which rights they reserve, and which rights they waive for the benefit of recipients or other creators. An easy-to-understand one-page explanation of rights, with associated visual symbols, explains the specifics of each Creative Commons license. Creative Commons licenses do not replace copyright, but are based upon it. They replace individual negotiations for specific rights between copyright owner (licensor) and licensee, which are necessary under an "all rights reserved" copyright management, with a "some rights reserved" management employing standardized licenses for re-use cases where no commercial compensation is sought by the copyright owner. The result is an agile, low-overhead and low-cost copyright-management regime, profiting both copyright owners and licensees. Wikipedia uses one of these licenses.
Spaceflight (also written space flight) is ballistic flight into or through outer space. Spaceflight can occur with spacecraft with or without humans on board. Examples of human spaceflight include the U.S. Apollo Moon landing and Space Shuttle programs and the Russian Soyuz program, as well as the ongoing International Space Station. Examples of unmanned spaceflight include space probes that leave Earth orbit, as well as satellites in orbit around Earth, such as communications satellites. These operate either by telerobotic control or are fully autonomous.
Spaceflight is used in space exploration, and also in commercial activities like space tourism and satellite telecommunications. Additional non-commercial uses of spaceflight include space observatories, reconnaissance satellites and other Earth observation satellites.
A spaceflight typically begins with a rocket launch, which provides the initial thrust to overcome the force of gravity and propels the spacecraft from the surface of the Earth. Once in space, the motion of a spacecraft—both when unpropelled and when under propulsion—is covered by the area of study called astrodynamics. Some spacecraft remain in space indefinitely, some disintegrate during atmospheric reentry, and others reach a planetary or lunar surface for landing or impact.
Crash Course (also known as Driving Academy) is a 1988 made for television teen film directed by Oz Scott.
Crash Course centers on a group of high schoolers in a driver’s education class; many for the second or third time. The recently divorced teacher, super-passive Larry Pearl, is on thin ice with the football fanatic principal, Principal Paulson, who is being pressured by the district superintendent to raise driver’s education completion rates or lose his coveted football program. With this in mind, Principal Paulson and his assistant, with a secret desire for his job, Abner Frasier, hire an outside driver’s education instructor with a very tough reputation, Edna Savage, aka E.W. Savage, who quickly takes control of the class.
The plot focuses mostly on the students and their interactions with their teachers and each other. In the beginning, Rico is the loner with just a few friends, Chadley is the bookish nerd with few friends who longs to be cool and also longs to be a part of Vanessa’s life who is the young, friendly and attractive girl who had to fake her mother’s signature on her driver’s education permission slip. Kichi is the hip-hop Asian kid who often raps what he has to say and constantly flirts with Maria, the rich foreign girl who thinks that the right-of-way on the roadways always goes to (insert awesomely fake foreign Latino accent) “my father’s limo”. Finally you have stereotypical football meathead J.J., who needs to pass his English exam to keep his eligibility and constantly asks out and gets rejected by Alice, the tomboy whose father owns “Santini & Son” Concrete Company. Alice is portrayed as being the “son” her father wanted.
A narrated video of my Stellar Nucleosynthesis presentation made for a college astronomy course. Watch this and you will have a good understanding of where stars get their energy, why they explode, and how the heavier elements of the universe are formed.
Explanation of element formation through Big Bang Nucleosynthesis, Stellar Nucleosynthesis, and Supernovae Nucleosynthesis. The elements that are formed in each type of Nucleosynthesis and the characteristics required for each type. More videos like this: http://www.youtube.com/playlist?list=PLMWvfa0XiLmmqM7ehBVA_u9bU2D_i7KNo "Electrodoodle" Kevin MacLeod (incompetech.com) Licensed under Creative Commons: By Attribution 3.0 http://creativecommons.org/licenses/by/3.0/
"Stellar nucleosynthesis" is the process by which the natural abundances of the chemical elements within stars vary due to nuclear fusion reactions in the cores and overlying mantles of stars. Stars are said to evolve with changes in the abundances of the elements within. Core fusion increases the atomic weight of its gaseous elements, causing pressure loss and contraction accompanied by increase of temperature. Structural changes of the star become necessary to stabilize it. Stars lose most of their mass when it is ejected late in their stellar lifetimes, thereby increasing the abundance of elements heavier than helium in the interstellar medium. The term supernova nucleosynthesis is used to describe the creation of elements during the evolution and explosion of a presupernova star, a...
Joni Mitchell was right, we are stardust. Get your own Space Time t-shirt at http://bit.ly/1QlzoBi Tweet at us! @pbsspacetime Facebook: facebook.com/pbsspacetime Email us! pbsspacetime [at] gmail [dot] com Comment on Reddit: http://www.reddit.com/r/pbsspacetime Stars are our stellar alchemists. They spend their entire lifespan creating and molding elements. In their final moments, a supernova spreads these elements out into the universe, providing the building blocks for new stars, planets, and even us! 'The Recipe For Life…' by It's Okay To Be Smart http://bit.ly/1UJbRkn Colliding neutron stars produce heavy elements Berger, Fong & Chornock 2013 http://arxiv.org/abs/1306.3960 https://www.cfa.harvard.edu/news/2013-19 Stellar Alchemist song by Kim Boekbinder http://kimboekbinder.band...
My talk at Nerd Nite San Francisco on August 15th, 2012 on stellar nucleosynthesis and the origin of all the elements in the Universe.
What is STELLAR NUCLEOSYNTHESIS? What does STELLAR NUCLEOSYNTHESIS mean? NUCLEOSYNTHESIS meaning - NUCLEOSYNTHESIS pronunciation - NUCLEOSYNTHESIS definition - NUCLEOSYNTHESIS explanation - How to pronounce NUCLEOSYNTHESIS? Source: Wikipedia.org article, adapted under https://creativecommons.org/licenses/by-sa/3.0/ license. Stellar nucleosynthesis is the process by which the natural abundances of the chemical elements within stars change due to nuclear fusion reactions in the cores and overlying mantles of stars. Stars are said to evolve (age) with changes in the abundances of the elements within. Core fusion increases the atomic weight of its gaseous elements, causing pressure loss and contraction accompanied by increase of temperature. Stars lose most of their mass when it is ejected ...
Presented by Anna Simon
Fusion, which occurs when atomic nuclei combine to form new elements, is extremely powerful. All the stars in the universe, including the Sun, are nuclear furnaces fueled by fusion. Through fusion, stars are responsible for forming all the naturally occurring elements heavier than hydrogen and helium -- before stellar nucleosynthesis, only the lightest elements existed in the universe. This video segment adapted from NOVA illustrates the critical role that stars play in creating the elements.
Massive stars fuse heavier elements in their cores than lower mass stars. This leads to the creation of heavier elements up to iron. Iron robs critical energy from the core, causing it to collapse. The shock wave, together with a huge swarm of neutrinos, blast through the star’s outer layers, causing it to explode. The resulting supernova creates even more heavy elements, scattering them through space. Also, happily, we’re in no danger from a nearby supernova. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Massive Stars Fuse Heavier Elements Up To Iron 1:15 Iron Uses High Amounts of Energy, Thus Making Stars Collapse 3:58 The Resulting Supernova Creates Even Heavier Elements 10:00 Relax, Something Else Will Kill You 9:04 ...
Afterschool Universe is an out-of-school-time astronomy program for middle school students that explores basic astronomy concepts through engaging hands-on activities and then takes participants on a journey through the Universe beyond the Solar System. This video shows a simple activity with clay that demonstrates the stages of fusion within the core of a star. Depending on its mass, a star can fuse and create many different elements before it finally runs out of fuel. If you are interested in the Afterschool Universe program, visit their website at http://universe.nasa.gov/afterschool/ This video is public domain and can be downloaded at: http://svs.gsfc.nasa.gov/vis/a010000/a010100/a010116/index.html Like our videos? Subscribe to NASA's Goddard Shorts HD podcast: http://svs.gsfc...
A narrated video of my Stellar Nucleosynthesis presentation made for a college astronomy course. Watch this and you will have a good understanding of where stars get their energy, why they explode, and how the heavier elements of the universe are formed.
Explanation of element formation through Big Bang Nucleosynthesis, Stellar Nucleosynthesis, and Supernovae Nucleosynthesis. The elements that are formed in each type of Nucleosynthesis and the characteristics required for each type. More videos like this: http://www.youtube.com/playlist?list=PLMWvfa0XiLmmqM7ehBVA_u9bU2D_i7KNo "Electrodoodle" Kevin MacLeod (incompetech.com) Licensed under Creative Commons: By Attribution 3.0 http://creativecommons.org/licenses/by/3.0/
"Stellar nucleosynthesis" is the process by which the natural abundances of the chemical elements within stars vary due to nuclear fusion reactions in the cores and overlying mantles of stars. Stars are said to evolve with changes in the abundances of the elements within. Core fusion increases the atomic weight of its gaseous elements, causing pressure loss and contraction accompanied by increase of temperature. Structural changes of the star become necessary to stabilize it. Stars lose most of their mass when it is ejected late in their stellar lifetimes, thereby increasing the abundance of elements heavier than helium in the interstellar medium. The term supernova nucleosynthesis is used to describe the creation of elements during the evolution and explosion of a presupernova star, a...
Joni Mitchell was right, we are stardust. Get your own Space Time t-shirt at http://bit.ly/1QlzoBi Tweet at us! @pbsspacetime Facebook: facebook.com/pbsspacetime Email us! pbsspacetime [at] gmail [dot] com Comment on Reddit: http://www.reddit.com/r/pbsspacetime Stars are our stellar alchemists. They spend their entire lifespan creating and molding elements. In their final moments, a supernova spreads these elements out into the universe, providing the building blocks for new stars, planets, and even us! 'The Recipe For Life…' by It's Okay To Be Smart http://bit.ly/1UJbRkn Colliding neutron stars produce heavy elements Berger, Fong & Chornock 2013 http://arxiv.org/abs/1306.3960 https://www.cfa.harvard.edu/news/2013-19 Stellar Alchemist song by Kim Boekbinder http://kimboekbinder.band...
My talk at Nerd Nite San Francisco on August 15th, 2012 on stellar nucleosynthesis and the origin of all the elements in the Universe.
What is STELLAR NUCLEOSYNTHESIS? What does STELLAR NUCLEOSYNTHESIS mean? NUCLEOSYNTHESIS meaning - NUCLEOSYNTHESIS pronunciation - NUCLEOSYNTHESIS definition - NUCLEOSYNTHESIS explanation - How to pronounce NUCLEOSYNTHESIS? Source: Wikipedia.org article, adapted under https://creativecommons.org/licenses/by-sa/3.0/ license. Stellar nucleosynthesis is the process by which the natural abundances of the chemical elements within stars change due to nuclear fusion reactions in the cores and overlying mantles of stars. Stars are said to evolve (age) with changes in the abundances of the elements within. Core fusion increases the atomic weight of its gaseous elements, causing pressure loss and contraction accompanied by increase of temperature. Stars lose most of their mass when it is ejected ...
Presented by Anna Simon
Fusion, which occurs when atomic nuclei combine to form new elements, is extremely powerful. All the stars in the universe, including the Sun, are nuclear furnaces fueled by fusion. Through fusion, stars are responsible for forming all the naturally occurring elements heavier than hydrogen and helium -- before stellar nucleosynthesis, only the lightest elements existed in the universe. This video segment adapted from NOVA illustrates the critical role that stars play in creating the elements.
Massive stars fuse heavier elements in their cores than lower mass stars. This leads to the creation of heavier elements up to iron. Iron robs critical energy from the core, causing it to collapse. The shock wave, together with a huge swarm of neutrinos, blast through the star’s outer layers, causing it to explode. The resulting supernova creates even more heavy elements, scattering them through space. Also, happily, we’re in no danger from a nearby supernova. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Massive Stars Fuse Heavier Elements Up To Iron 1:15 Iron Uses High Amounts of Energy, Thus Making Stars Collapse 3:58 The Resulting Supernova Creates Even Heavier Elements 10:00 Relax, Something Else Will Kill You 9:04 ...
Afterschool Universe is an out-of-school-time astronomy program for middle school students that explores basic astronomy concepts through engaging hands-on activities and then takes participants on a journey through the Universe beyond the Solar System. This video shows a simple activity with clay that demonstrates the stages of fusion within the core of a star. Depending on its mass, a star can fuse and create many different elements before it finally runs out of fuel. If you are interested in the Afterschool Universe program, visit their website at http://universe.nasa.gov/afterschool/ This video is public domain and can be downloaded at: http://svs.gsfc.nasa.gov/vis/a010000/a010100/a010116/index.html Like our videos? Subscribe to NASA's Goddard Shorts HD podcast: http://svs.gsfc...
My talk at Nerd Nite San Francisco on August 15th, 2012 on stellar nucleosynthesis and the origin of all the elements in the Universe.
A narrated video of my Stellar Nucleosynthesis presentation made for a college astronomy course. Watch this and you will have a good understanding of where stars get their energy, why they explode, and how the heavier elements of the universe are formed.
Presented by Anna Simon
The Origin, History, Evolution & Future of the Universe. The Universe is all of time and space and its contents. The Universe includes planets, stars, galaxies, the . A brief history of the universe, from the big bang to the origin of mankind. Big Bang: Stellar Nucleosynthesis: . Get the song on iTunes: // A tapestry of footage tracing the cosmic and biological origins of our . Backed by stunning illustrations, David Christian narrates a complete history of the universe, from the Big Bang to the Internet, in a riveting 18 .
From www.geoset.info and www.geoset.fsu.edu Abstract The Astrophysicist Fred Hoyle who is well known for his work on Stellar Nucleosynthesis of the Chemical Elements and the Steady State Theory also proposed that he had evidence that there were bacteria in space. In this "Blackboard Lecture" (actually a whiteboard) this evidence is analysed carefully and the claim is shown to be wanting. Other aspects of scientific methods and integrity are discussed.
Sir Fred Hoyle FRS was an English astronomer noted primarily for the theory of stellar nucleosynthesis and his often controversial stances on other scientific matters—in particular his rejection of the "Big Bang" theory, a term coined by him on BBC radio. While Hoyle was well-regarded for his works on nucleosynthesis and science popularization, his career was also noted for the controversial positions he held on a wide range of scientific issues, often in direct opposition to the prevailing theories supported by the majority of the scientific community. In addition to his work as an astronomer, Hoyle was a writer of science fiction, including a number of books co-written with his son Geoffrey Hoyle. Hoyle spent most of his working life at the Institute of Astronomy at Cambridge and served ...
A star is a luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun. Other stars are visible from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of stars have been assembled by astronomers, which provide standardized star designations. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Once the hydrogen in the core of a star is nearly exhausted, almost all naturally occu...
---=== Our World on HD ===--- star is a luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun. Other stars are visible from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of stars have been assembled by astronomers, which provide standardized star designations. For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Once the hydrogen in the core of a star is nearly exhaus...
What Is The Largest Star In The Universe? - Full Documentary HD A star is a luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, the brightest of which gained proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. However, most of the stars in the Universe, including all stars outside our galaxy, the Milky Way, are invisible to the naked eye from Earth. Indeed, most are invisible from Earth even through the...
Jump to specific chapter using table of contents below or just LISTEN to the full article! Hans Albrecht Bethe (July 2, 1906– March 6, 2005) was a German and American nuclear physicist who, in addition to making important contributions to astrophysics, quantum electrodynamics and solid-state physics, won the 1967 Nobel Prize in Physics for his work on the theory of stellar nucleosynthesis. TABLE OF CONTENTS: 0. Introduction (00:00:00) 1. Early years (00:01:39) 2. Early work (00:05:16) 3. United States (00:11:49) 4. Manhattan Project (00:17:30) 5. Hydrogen bomb (00:20:53) 6. Later work (00:22:35) ............6.1. Lamb shift (00:22:37) ............6.2. Astrophysics (00:25:06) 7. Political stances (00:28:09) 8. Personal life (00:30:02) 9. Honors and awards ...