Astronomy 141 - Life in the Universe - Autumn Quarter 2009

Astronomy 141 - Life in the Universe - Autumn Quarter 2009

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Astronomy 141 - Life in the Universe - Autumn Quarter 2009 episodes

  • Lecture 26: The Deserts of Mars
    For many, the most likely place in the Solar System to search for life
    beyond the Earth is Mars. This lecture describes the properties of
    Mars, a desert world with a thin, dry, cold carbon dioxide atmosphere.
    I will review evidence that has begun to point unequivocally to the
    conclusion that Mars had flowing and standing liquid water on its
    surface in the past, perhaps during the first billion years or so.
    If Mars had a warm, wet past, did life also get a start there?
    Recorded live on 2009 Oct 30 in Room 1005 Smith Laboratory on the
    Columbus campus of The Ohio State University.
    48 min
  • Lecture 25: The Requirements for Life in the Solar System
    Having completed our tour of the Solar System, we now turn to a
    discussion of the requirements for life, and where those requirements
    might be satisfied elsewhere in the Solar System. Some - energy,
    complex chemistry, and liquid water - seem obvious, but they are not the
    only possibilities or considerations. At the end, we will have a short
    list of possible places to look, some expected, others surprising.
    Recorded live on 2009 Oct 29 in Room 1005 Smith Laboratory on the
    Columbus campus of The Ohio State University.
    48 min
  • Lecture 24: The Jovian Planets
    We turn our attention to the Giant Planets of the outer Solar System:
    the gas giants Jupiter and Saturn, and the ice giants Uranus and Neptune.
    We will review their structure and properties, and then examine their
    systems of moons, with special attention to the giant moons. While the
    Jovian planets themselves seem unlikely places to hunt for life in our
    Solar System, a few of their largest moons may be more promising than
    appears at first sight. We'll explore this further in subsequent lectures
    in this unit. Recorded live on 2009 Oct 28 in Room 1005 Smith Laboratory
    on the Columbus campus of The Ohio State University.
    48 min
  • Lecture 23: Terrestrial Worlds in Comparison
    We follow our tour of our Solar System with an in-depth comparison of
    the Terrestrial Planets. In particular, we want to contrast and compare
    their geological and atmospheric histories. This will inform our
    inquiry into whether or not we expect to find life on these worlds.
    Recorded live on 2009 Oct 27 in Room 1005 Smith Laboratory on the
    Columbus campus of The Ohio State University.
    47 min
  • Lecture 22: The Family of the Sun
    This first lecture of Unit 4 - Life in the Solar System - is a quick
    tour of our Solar System reviewing the planets, dwarf planets, moons,
    and small bodies that make up our celestial home. This lecture will
    introduce many of the places we will be considering in detail over the
    next two weeks, and which we'll find around other stars. Recorded live
    on 2009 Oct 26 in Room 1005 Smith Laboratory on the Columbus campus of
    The Ohio State University.
    47 min
  • Lecture 21: Impacts and Extinction
    We end our exploration of life on the Earth with a look at death in the
    fossil record. This lecture looks at the role asteroidal impacts have
    played in the history of the Earth, and their possible role in mass
    extinction events in the fossil record. We will discuss near-earth
    asteroids, historical impacts, and the K-T event in which a massive
    asteroid impact caused a mass extinction of species that included all
    non-avian dinosaurs among its victims, opening up the biosphere to the
    dominance of mammals. We'll look at other mass extinctions during the
    past 500Myr, and talk about whether extinction-class impacts are in our
    future. Recorded live on 2009 Oct 22 in Room 1005 Smith Laboratory on
    the Columbus campus of The Ohio State University.
    47 min
  • Lecture 20: The History of Life on Earth
    In this lecture we step back and look at the history of life on Earth
    from the first signs of life at start of the Archaean Eon 3.5 billion
    years ago to just up to the present day. We will review the appearance
    of photosynthesis and the rise of oxygen in the atmosphere in the
    Proterozoic, the appearance of the first eukaryotes and sexual
    reproduction, and the Cambrian explosion of plant and animal species at
    the start of the Phanerozoic Eon, and briefly review the changes in life
    to the present day from the Cambrian Explosion to the colonization of
    land by plants and then animals. Most of the lecture will be where most
    of the time was spent, in the early, microbiological Earth. Recorded
    live on 2009 Oct 21 in Room 1005 Smith Laboratory on the Columbus campus
    of The Ohio State University.
    48 min
  • Lecture 19: The Origin of Life on Earth
    How did life arise from non-life? Frankly, we don't know, but current
    experimental work is aimed at trying to understand how it might work in
    biochemical terms. This lecture sets out the problem of "abiogenesis",
    and describes our current thinking about the likely origins of life on
    Earth. We will review the classic Miller-Urey experiment, and look at
    its insights and limitations, discuss meteoritic sources of amino acids,
    and the basic requirements needed for protolife. I will then describe
    in outline two scenarios that are active areas of origins research: the
    RNA World model and the Metabolism First model. Finally, I will very
    briefly mention Exogenesis and Panspermia, which don't really address
    the problem of abiogenesis so much as move it elsewhere. Recorded live
    on 2009 Oct 20 in Room 1005 Smith Laboratory on the Columbus campus of
    The Ohio State University.
    47 min
  • Lecture 18: The First Living Things on Earth
    What are the first recognizable forms of life that we find in the
    geological record? How far back can we go in geological time and still
    find life? This lecture reviews three lines of evidence that have
    emerged in recent years to suggest that life may have emerged very early
    on the young Earth, perhaps within a few hundred million years of the
    end of the epoch of heavy bombardment. I will describe fossil
    stromatolites, microfossils, and carbon isotope data that are used to
    explore these questions. Recorded live on 2009 Oct 19 in Room 1005
    Smith Laboratory on the Columbus campus of The Ohio State University.
    47 min
  • Lecture 17: Life on the Edge
    Extremophiles are organisms that are adapted to survive in extreme
    environments. This lecture describes the challenges that
    extremes of heat, cold, acidity, salinity, and radiation pose to
    organisms, and show examples of how evolution has nonetheless allowed
    some organisms to adapt to not just survive but thrive in such extreme
    conditions. Finally, we will explore the possible limits of life on
    Earth, and find that while you can make things pretty extreme and still
    have organisms adapt, you reach the limit if there is no water. Rather
    than being oddballs, these organisms give us important insights into the
    origins of life on Earth, and widens the possibilities for life on other
    worlds. Recorded live on 2009 Oct 16 in Room 1005 Smith Laboratory on
    the Columbus campus of The Ohio State University.
    47 min

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