|1||Lecture 44: The Future Of Life In The Solar System||55:49|
These lecture podcasts are audio recordings of daily lectures from Prof. Richard Pogge's Autumn Quarter 2009 section of Astronomy 141 at The Ohio State University. They were recorded live, unscripted and unedited.
This file was recorded after lecture because of a recorder malfunction.
What is the future of life on Earth and in our Solar System The Sun is the source of energy for life on the Earth, but it will not shine forever. This lecture looks at the impact of the various stages of the evolution of the Sun on is the future of life on Earth and in our Solar System The Sun is the source of energy for life on the Earth, but it will not shine forever. This lecture looks at the impact of the various stages of the evolution of the Sun on the habitability of the Solar System, with particular emphasis on the continued habitability of the Earth. NOTE: Due to a recorder malfunction this lecture was re-recorded later in the day on 2009 Dec 2, rather than being live from the class room in Smith Laboratory. As such, it is about 10 minutes longer than usual my pacing is off when not in front of class. Tune in. Dirty Disco Kono Vidovic. In five billion years, the Suns going to evolve into a red giant. Thats bad news for Earth, but exciting for some of the worlds a little farther album was released on the label Not On Label Richard Pogge Self-released catalog number none. This album was released in 2009-12-02 year. Format of the release is. File , MP3. Date of Copyright: C 2009-12-02. Track list: Track title. Find mp3 free Lecture 44: The Future Of Life In The Solar System. mp3 player of Richard Pogge - Lecture 44: The Future Of Life In The Solar System: mp3 Player. Music video: Watch now Richard Pogge's video clip of album Lecture 44: The Future Of Life In The Solar System. See also releases of Richard Pogge: Click to release co. Best Richard Pogge Podcasts For 2020. Latest was Lecture 46: This View of Life Course Finale. Listen online, no signup necessary. Best Richard Pogge podcasts we could find updated April 2020. Best Richard Pogge podcasts we could find Updated April 2020. Related podcasts: Podcasting Education Science Natural Sciences Higher Education. Sign up on web. Lecture 44: The Future of Life in the Solar System 55:49. Richard Pogge, MTWThF 2:30. Lecture 46: Are We Alone Life in the Universe. Key Ideas: Basic requirementsconditions for life. The best future hopes seems to be direct imaging searches around nearby stars using techniques of interferometry and coronography, with follow-up spectroscopy to study any likely candidate habitable planets. Two proposed but not yet fully funded missions being designed to accomplish this are: Darwin: Multi-satellite ESA interferometerplanet finder. Terrestrial Planet Finder TPF - NASA imaging interferometer and coronographic imager missions. The main goals of these projects are . Computer simulations of the Solar System's evolution over the next five billion years suggest that there is a small less than 1 chance that a collision could occur between Earth and either Mercury, Venus, or Mars. During the same interval, the odds that the Earth will be scattered out of the Solar System by a passing. The planet could remain at an obliquity of 60 to 90 for periods as long as 10 million years. Pangaea was the last supercontinent to form before the present. Посмотреть сведения об участниках альбома, рецензии, композиции и приобрести альбом 2012 VBR File от Strange New Worlds: The Properties Of Exoplanets на free to Richard Pogge Lecture 27: Deep Time: The Age of the Earth 2006 Oct 30 Lecture 27: Deep Time: The Age of the Earth 2006 Oct 30. 1 track 44:55. Artist images. Richard Pogge. 298 listeners. Learn about the science behind the current exploration of the solar system in this free class. Use principles from physics, chemistry, biology, and geology to understand the latest from Mars, comprehend the outer solar system, ponder planets outside our solar system, and search for habitability in our neighborhood and beyond. And then in the infrared part of the wavelength, for water vapor in the atmosphere. Water vapor in the atmosphere has absorptions here, here, here, here, here, here. You see plenty of it out in then the infrared at three microns, this whole de, depression of this spectrum is because of the water vapor. There's a lot of other stuff in there too