�ݺ�ߣshows by User: tjmadigan

�ݺ�ߣshows by User: tjmadigan / http://www.slideshare.net/images/logo.gif �ݺ�ߣshows by User: tjmadigan / Fri, 29 Jul 2016 00:25:55 GMT �ݺ�ߣShare feed for �ݺ�ߣshows by User: tjmadigan SolarSID(Final Draft7) /slideshow/solarsidfinal-draft7/64494457 1c5de47c-e553-4bd5-a95e-7b4adfc1e973-160729002555
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]]> Fri, 29 Jul 2016 00:25:55 GMT /slideshow/solarsidfinal-draft7/64494457 tjmadigan@slideshare.net(tjmadigan) SolarSID(Final Draft7) tjmadigan <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/1c5de47c-e553-4bd5-a95e-7b4adfc1e973-160729002555-thumbnail.jpg?width=120&height=120&fit=bounds" />

SolarSID(Final Draft7) from Thomas Madigan

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0 Space Weather and Solar Flare Activity Research at Suffolk County Community College /slideshow/space-weather-and-solar-flare-activity-research-at-suffolk-county-community-college/64491798 solarsidfinaldraft7-160728214552
Integrated Space Weather and Solar Flare Research Exhibit Presented at Suffolk Community College, March 18, 2015 ]]>
Integrated Space Weather and Solar Flare Research Exhibit Presented at Suffolk Community College, March 18, 2015 ]]> Thu, 28 Jul 2016 21:45:52 GMT /slideshow/space-weather-and-solar-flare-activity-research-at-suffolk-county-community-college/64491798 tjmadigan@slideshare.net(tjmadigan) Space Weather and Solar Flare Activity Research at Suffolk County Community College tjmadigan Integrated Space Weather and Solar Flare Research Exhibit Presented at Suffolk Community College, March 18, 2015 <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/solarsidfinaldraft7-160728214552-thumbnail.jpg?width=120&height=120&fit=bounds" /> Integrated Space Weather and Solar Flare Research Exhibit Presented at Suffolk Community College, March 18, 2015

Space Weather and Solar Flare Activity Research at Suffolk County Community College from Thomas Madigan

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0 Kepler Mission /slideshow/kepler-39726900/39726900 kepler-140930185201-phpapp02
An overview of the Kepler mission, it's exciting new discoveries and the ever-growing variety of strange and wonderful worlds that populate our galaxy.]]>
An overview of the Kepler mission, it's exciting new discoveries and the ever-growing variety of strange and wonderful worlds that populate our galaxy.]]> Tue, 30 Sep 2014 18:52:01 GMT /slideshow/kepler-39726900/39726900 tjmadigan@slideshare.net(tjmadigan) Kepler Mission tjmadigan An overview of the Kepler mission, it's exciting new discoveries and the ever-growing variety of strange and wonderful worlds that populate our galaxy. <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/kepler-140930185201-phpapp02-thumbnail.jpg?width=120&height=120&fit=bounds" /> An overview of the Kepler mission, it's exciting new discoveries and the ever-growing variety of strange and wonderful worlds that populate our galaxy.

Kepler Mission from Thomas Madigan

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0 Fomalhaut B and Newton's General Solution to Kepler's Third law /slideshow/fomalhaut-b-and-newtons-general-solution-to-keplers-third-law/39574888 fomalhautbandnewtonsgeneralsolutiontokeplersthirdlaw-140926124039-phpapp01
The first direct observation of an exoplanet in orbit around its parent star was made by the Hubble Space Telescope. The observation is used to demonstrate the universal application and veracity of Newton's Universal Law of Gravitation, his general solution to Kepler's Third Law and Kepler's first 2 laws and that gravitation is the underlying driving principle behind it all.]]>
The first direct observation of an exoplanet in orbit around its parent star was made by the Hubble Space Telescope. The observation is used to demonstrate the universal application and veracity of Newton's Universal Law of Gravitation, his general solution to Kepler's Third Law and Kepler's first 2 laws and that gravitation is the underlying driving principle behind it all.]]> Fri, 26 Sep 2014 12:40:39 GMT /slideshow/fomalhaut-b-and-newtons-general-solution-to-keplers-third-law/39574888 tjmadigan@slideshare.net(tjmadigan) Fomalhaut B and Newton's General Solution to Kepler's Third law tjmadigan The first direct observation of an exoplanet in orbit around its parent star was made by the Hubble Space Telescope. The observation is used to demonstrate the universal application and veracity of Newton's Universal Law of Gravitation, his general solution to Kepler's Third Law and Kepler's first 2 laws and that gravitation is the underlying driving principle behind it all. <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/fomalhautbandnewtonsgeneralsolutiontokeplersthirdlaw-140926124039-phpapp01-thumbnail.jpg?width=120&height=120&fit=bounds" /> The first direct observation of an exoplanet in orbit around its parent star was made by the Hubble Space Telescope. The observation is used to demonstrate the universal application and veracity of Newton's Universal Law of Gravitation, his general solution to Kepler's Third Law and Kepler's first 2 laws and that gravitation is the underlying driving principle behind it all.

Fomalhaut B and Newton's General Solution to Kepler's Third law from Thomas Madigan

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0 The Unprecedented Rosetta mission to Comet 67P/Churyumov�CGerasimenko /slideshow/the-unprecedented-rosetta-mission-to-comet-67-p-final-draft/39295115 therosettamissiontocomet67pfinaldraft-140919105235-phpapp02
After almost 11 years in transit and 4 gravitational assists from the Earth and Mars, the European Space Agency��s Rosetta probe has arrived at the Jupiter-family comet 67P/Churyumov�CGerasimenko. Arriving on Wednesday, August 6th, the probe went into a 100 km-high orbit around the comet, both of which are now in common orbit around the sun. Depending on the comet��s activity, Rosetta will come as close as 10 km to the comet��s nucleus over the course of the mission. With a high orbital eccentricity (the orbit��s deviation from a perfect circle) of 0.640, a perihelion of 1.2 AU and an aphelion of 5.68 AU, 67P/Churyumov�CGerasimenko is now in common orbit around the sun with Rosetta. Rosetta is a cornerstone mission of the European Space Agency (ESA). It is an unprecedented landmark achievement in human history and the history of science. Humankind has placed a sophisticated instrument of science in orbit around a comet's nucleus and has placed a robotic lander in the surface of that nucleus! Rosetta will chase down, go into orbit around, and land on the object of interest. It will study 67P/Churyumov-Gerasimenko with a combination of remote sensing and in situ measurements. The mission has 2 phases, the ongoing orbital phase and the landing phase. During the ongoing orbital phase, the spacecraft will examine the comet up close with its suite of 11 instruments. During the landing phase, the orbiter will release the Philae lander which carries an onboard suite of 10 instruments for imaging and sampling the comet��s nucleus. The mission will track the comet through perihelion, its closest approach to the sun, examining its behavior before, during and after. Providing an introductory retrospective of comets, sometimes regarded as harbingers of doom, Prof. Madigan discusses this historic mission, a mission that includes study of the comet from the surface of its nucleus! This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on September 18th, 2014.]]>
After almost 11 years in transit and 4 gravitational assists from the Earth and Mars, the European Space Agency��s Rosetta probe has arrived at the Jupiter-family comet 67P/Churyumov�CGerasimenko. Arriving on Wednesday, August 6th, the probe went into a 100 km-high orbit around the comet, both of which are now in common orbit around the sun. Depending on the comet��s activity, Rosetta will come as close as 10 km to the comet��s nucleus over the course of the mission. With a high orbital eccentricity (the orbit��s deviation from a perfect circle) of 0.640, a perihelion of 1.2 AU and an aphelion of 5.68 AU, 67P/Churyumov�CGerasimenko is now in common orbit around the sun with Rosetta. Rosetta is a cornerstone mission of the European Space Agency (ESA). It is an unprecedented landmark achievement in human history and the history of science. Humankind has placed a sophisticated instrument of science in orbit around a comet's nucleus and has placed a robotic lander in the surface of that nucleus! Rosetta will chase down, go into orbit around, and land on the object of interest. It will study 67P/Churyumov-Gerasimenko with a combination of remote sensing and in situ measurements. The mission has 2 phases, the ongoing orbital phase and the landing phase. During the ongoing orbital phase, the spacecraft will examine the comet up close with its suite of 11 instruments. During the landing phase, the orbiter will release the Philae lander which carries an onboard suite of 10 instruments for imaging and sampling the comet��s nucleus. The mission will track the comet through perihelion, its closest approach to the sun, examining its behavior before, during and after. Providing an introductory retrospective of comets, sometimes regarded as harbingers of doom, Prof. Madigan discusses this historic mission, a mission that includes study of the comet from the surface of its nucleus! This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on September 18th, 2014.]]> Fri, 19 Sep 2014 10:52:35 GMT /slideshow/the-unprecedented-rosetta-mission-to-comet-67-p-final-draft/39295115 tjmadigan@slideshare.net(tjmadigan) The Unprecedented Rosetta mission to Comet 67P/Churyumov�CGerasimenko tjmadigan After almost 11 years in transit and 4 gravitational assists from the Earth and Mars, the European Space Agency��s Rosetta probe has arrived at the Jupiter-family comet 67P/Churyumov�CGerasimenko. Arriving on Wednesday, August 6th, the probe went into a 100 km-high orbit around the comet, both of which are now in common orbit around the sun. Depending on the comet��s activity, Rosetta will come as close as 10 km to the comet��s nucleus over the course of the mission. With a high orbital eccentricity (the orbit��s deviation from a perfect circle) of 0.640, a perihelion of 1.2 AU and an aphelion of 5.68 AU, 67P/Churyumov�CGerasimenko is now in common orbit around the sun with Rosetta. Rosetta is a cornerstone mission of the European Space Agency (ESA). It is an unprecedented landmark achievement in human history and the history of science. Humankind has placed a sophisticated instrument of science in orbit around a comet's nucleus and has placed a robotic lander in the surface of that nucleus! Rosetta will chase down, go into orbit around, and land on the object of interest. It will study 67P/Churyumov-Gerasimenko with a combination of remote sensing and in situ measurements. The mission has 2 phases, the ongoing orbital phase and the landing phase. During the ongoing orbital phase, the spacecraft will examine the comet up close with its suite of 11 instruments. During the landing phase, the orbiter will release the Philae lander which carries an onboard suite of 10 instruments for imaging and sampling the comet��s nucleus. The mission will track the comet through perihelion, its closest approach to the sun, examining its behavior before, during and after. Providing an introductory retrospective of comets, sometimes regarded as harbingers of doom, Prof. Madigan discusses this historic mission, a mission that includes study of the comet from the surface of its nucleus! This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on September 18th, 2014. <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/therosettamissiontocomet67pfinaldraft-140919105235-phpapp02-thumbnail.jpg?width=120&height=120&fit=bounds" /> After almost 11 years in transit and 4 gravitational assists from the Earth and Mars, the European Space Agency��s Rosetta probe has arrived at the Jupiter-family comet 67P/Churyumov�CGerasimenko. Arriving on Wednesday, August 6th, the probe went into a 100 km-high orbit around the comet, both of which are now in common orbit around the sun. Depending on the comet��s activity, Rosetta will come as close as 10 km to the comet��s nucleus over the course of the mission. With a high orbital eccentricity (the orbit��s deviation from a perfect circle) of 0.640, a perihelion of 1.2 AU and an aphelion of 5.68 AU, 67P/Churyumov�CGerasimenko is now in common orbit around the sun with Rosetta. Rosetta is a cornerstone mission of the European Space Agency (ESA). It is an unprecedented landmark achievement in human history and the history of science. Humankind has placed a sophisticated instrument of science in orbit around a comet's nucleus and has placed a robotic lander in the surface of that nucleus! Rosetta will chase down, go into orbit around, and land on the object of interest. It will study 67P/Churyumov-Gerasimenko with a combination of remote sensing and in situ measurements. The mission has 2 phases, the ongoing orbital phase and the landing phase. During the ongoing orbital phase, the spacecraft will examine the comet up close with its suite of 11 instruments. During the landing phase, the orbiter will release the Philae lander which carries an onboard suite of 10 instruments for imaging and sampling the comet��s nucleus. The mission will track the comet through perihelion, its closest approach to the sun, examining its behavior before, during and after. Providing an introductory retrospective of comets, sometimes regarded as harbingers of doom, Prof. Madigan discusses this historic mission, a mission that includes study of the comet from the surface of its nucleus! This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on September 18th, 2014.

The Unprecedented Rosetta mission to Comet 67P/Churyumov�M��erasimenko from Thomas Madigan

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0 Exploding stars 2011 Nobel Prize in Physics /slideshow/exploding-stars-2011-nobelprize-37103523/37103523 explodingstars-2011nobel-prize-140717154240-phpapp02
views In 1929 Edwin Hubble discovered that the universe is expanding. Ever since, we have been striving to fully comprehend the implications of his discovery. Our understanding of the universe and our place in it has evolved from an anthropocentric, static, earth-centered model to a dynamic, evolving cosmos where galaxies are flung across time and space, where the cosmic horizon is quickly receding and the discoveries that await us are limited only by our imagination. Based on Edwin Hubble��s discovery that the universe is expanding, a study was begun in 1998 to determine the expansion rate of the universe at great distances. Culminating with the 2011 Nobel Prize in Physics being awarded to 2 Americans and an Australian, it was determined that the expansion rate of the universe is not decreasing but increasing at great distances, a finding that was quite unexpected and had far-reaching implications for our cosmological models and understanding of the expanding universe. In this presentation, I discuss this discovery in detail and how a specific type of exploding star (supernova) was used to make this discovery. This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on July 9th, 2014.]]>
views In 1929 Edwin Hubble discovered that the universe is expanding. Ever since, we have been striving to fully comprehend the implications of his discovery. Our understanding of the universe and our place in it has evolved from an anthropocentric, static, earth-centered model to a dynamic, evolving cosmos where galaxies are flung across time and space, where the cosmic horizon is quickly receding and the discoveries that await us are limited only by our imagination. Based on Edwin Hubble��s discovery that the universe is expanding, a study was begun in 1998 to determine the expansion rate of the universe at great distances. Culminating with the 2011 Nobel Prize in Physics being awarded to 2 Americans and an Australian, it was determined that the expansion rate of the universe is not decreasing but increasing at great distances, a finding that was quite unexpected and had far-reaching implications for our cosmological models and understanding of the expanding universe. In this presentation, I discuss this discovery in detail and how a specific type of exploding star (supernova) was used to make this discovery. This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on July 9th, 2014.]]> Thu, 17 Jul 2014 15:42:40 GMT /slideshow/exploding-stars-2011-nobelprize-37103523/37103523 tjmadigan@slideshare.net(tjmadigan) Exploding stars 2011 Nobel Prize in Physics tjmadigan views In 1929 Edwin Hubble discovered that the universe is expanding. Ever since, we have been striving to fully comprehend the implications of his discovery. Our understanding of the universe and our place in it has evolved from an anthropocentric, static, earth-centered model to a dynamic, evolving cosmos where galaxies are flung across time and space, where the cosmic horizon is quickly receding and the discoveries that await us are limited only by our imagination. Based on Edwin Hubble��s discovery that the universe is expanding, a study was begun in 1998 to determine the expansion rate of the universe at great distances. Culminating with the 2011 Nobel Prize in Physics being awarded to 2 Americans and an Australian, it was determined that the expansion rate of the universe is not decreasing but increasing at great distances, a finding that was quite unexpected and had far-reaching implications for our cosmological models and understanding of the expanding universe. In this presentation, I discuss this discovery in detail and how a specific type of exploding star (supernova) was used to make this discovery. This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on July 9th, 2014. <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/explodingstars-2011nobel-prize-140717154240-phpapp02-thumbnail.jpg?width=120&height=120&fit=bounds" /> views In 1929 Edwin Hubble discovered that the universe is expanding. Ever since, we have been striving to fully comprehend the implications of his discovery. Our understanding of the universe and our place in it has evolved from an anthropocentric, static, earth-centered model to a dynamic, evolving cosmos where galaxies are flung across time and space, where the cosmic horizon is quickly receding and the discoveries that await us are limited only by our imagination. Based on Edwin Hubble��s discovery that the universe is expanding, a study was begun in 1998 to determine the expansion rate of the universe at great distances. Culminating with the 2011 Nobel Prize in Physics being awarded to 2 Americans and an Australian, it was determined that the expansion rate of the universe is not decreasing but increasing at great distances, a finding that was quite unexpected and had far-reaching implications for our cosmological models and understanding of the expanding universe. In this presentation, I discuss this discovery in detail and how a specific type of exploding star (supernova) was used to make this discovery. This public event was hosted at the Ross School (East Hampton, NY) by the Montauk Observatory on July 9th, 2014.

Exploding stars 2011 Nobel Prize in Physics from Thomas Madigan

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0 https://cdn.slidesharecdn.com/profile-photo-tjmadigan-48x48.jpg?cb=1523550042 Professional Astronomer and educator. Associate professor for the city and state universities of New York, NASA/ JPL Solar System Ambassador, Associate of the American Astronomical Society, Fellow of the Royal Astronomical Society, Professional Speaker, Technologist, Technology Manager and Entrepreneur. https://cdn.slidesharecdn.com/ss_thumbnails/1c5de47c-e553-4bd5-a95e-7b4adfc1e973-160729002555-thumbnail.jpg?width=320&height=320&fit=bounds slideshow/solarsidfinal-draft7/64494457 SolarSID(Final Draft7) https://cdn.slidesharecdn.com/ss_thumbnails/solarsidfinaldraft7-160728214552-thumbnail.jpg?width=320&height=320&fit=bounds slideshow/space-weather-and-solar-flare-activity-research-at-suffolk-county-community-college/64491798 Space Weather and Sola... https://cdn.slidesharecdn.com/ss_thumbnails/kepler-140930185201-phpapp02-thumbnail.jpg?width=320&height=320&fit=bounds slideshow/kepler-39726900/39726900 Kepler Mission