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BIO 10 Lecture 2

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Title: BIO 10 Lecture 2


1
BIO 10 Lecture 2
  • THE UNIVERSE AND ITS CHEMISTRY WHAT IS LIFE?

2
Setting the Stage for Life
  • The prevailing scientific theory for how the
    Universe came into being (i.e. the theory that
    explains the most facts and has the best
    predictive power) is that the Universe began with
    a Big Bang explosion 13.7 billion years ago.
  • Time, space, and matter came into existence with
    this event
  • Since an act of creation implies space and time,
    most scientists do not believe it is even
    meaningful to talk about a Creator or Creation
    Event
  • The Universe is not expanding into anything! All
    we can really say is that space and time are both
    increasing

3
  • 300,000 years after the Big Bang, protons
    captured electrons to form the first hydrogen
    atoms.
  • Hydrogen (H) is the simplest element it has only
    one proton and one electron
  • The Big Bang also created a small amount of
    Helium (He), Lithium (Li) and Beryllium (Be)
  • All elements with higher molecular weights were
    created later, in the bellies of massive stars

4
A PERIODIC TABLE OF THE ELEMENTS

5
  • 600 million years after the Big Bang, the first
    generation of galaxies and stars fell together
    by gravity
  • Early stars were comprised entirely of H and He
    (with traces of Li and Be) and had no rocky
    planets
  • They might have had gaseous planets like our own
    outer planets (Jupiter, Saturn, Uranus, and
    Neptune)

6
  • Stars are nuclear fusion furnaces
  • H is being converted to He in the core
  • 4 H ? 1 He, so pressure drops with fusion and
    gravity squeezes harder
  • As gravity increases, temp increases, levels of
    radiation increase, and star is pushed outward,
    maintains size
  • When all the H is used up, the star will begin to
    convert He to C (carbon), the most important
    element for life

7
Small stars The smallest stars only convert
hydrogen into helium. Medium-sized stars (like
our Sun) Late in their lives, when the hydrogen
becomes depleted, will begin to convert helium
into oxygen and carbon. Massive stars (greater
than five times the mass of ourSun) When their
hydrogen becomes depleted, high mass stars
convert helium atoms into carbon and oxygen,
followed by the fusion of carbon and oxygen into
neon, sodium, magnesium, sulfur and silicon.
Later reactions transform these elements into
calcium, iron, nickel, chromium, copper and
others.
8
  • Up to iron (Fe), fusion creates energy. After
    iron, fusion requires energy.
  • When the core of a massive star turns to iron,
    gravity can no longer be stopped
  • A sudden and massive implosion creates a neutron
    star or black hole where the core of the star had
    once been
  • The implosion is accompanied by a massive
    explosion that fuses elements beyond iron and
    scatters heavy elements into space

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  • 5 billion years ago, our star, the Sun formed
    out of a cloud of H and He contaminated with
    the heavier elements produced by the supernova of
    another star
  • 4.5 billion years ago, The Earth formed from
    the same spinning disk that formed the Sun.
  • Metals and other heavy elements remained closer
    to the sun gaseous planets like Jupiter and
    Saturn formed farther out

12
  • Thus, the solar system, and particularly the
    inner planets in the solar system, were rich in
    heavier elements
  • The chemistry of life relies mostly on the
    following elements
  • Hydrogen
  • Carbon
  • Oxygen
  • Nitrogen
  • Phosphorous

Created in supernovas
13
From Muck to Microbes
  • Formation of the Solar System
  • The oldest rocks on are just slightly younger
    than the sun 4.5 billion years old
  • Nebular Hypothesis The solar system was born out
    of a swirling (rotating) cloud of hydrogen and
    helium, with a smattering of heavier elements
  • Most of the H and He are found in the sun rocky
    planets made of heavier elements (like Earth) are
    found close to the sun, while gaseous planets
    (Jupiter, Saturn, Uranus, Neptune) are found
    further out
  • Earth formed as an accretion of smaller
    asteroid-like bodies

14
In the Nebular Hypothesis, a cloud of gas and
dust collapsed by gravity begins to spin faster
because of the conservation of angular momentum
15
The collapsing, spinning nebula begins to flatten
into a rotating pancake
16
As the nebula collapses further, local regions
begin to contract gravitationally on their own
because of instabilities in the collapsing,
rotating cloud
17
  • The Moon formed as a result of an early
    catastrophic collision between Earth and another
    planetoid, which also created the tilt in Earths
    axis
  • The heat of early bombardments and impacts kept
    Earth hot and enabled heavier elements
    (principally iron) to flow to the core, where
    they remained molten
  • Over time, the crust of the Earth cooled and
    became solid

18
  • The Nebular Hypothesis is considered to be a good
    scientific theory because it explains many facts
    about the solar system
  • All of the planets revolve around the sun in the
    same direction
  • the axes of most planets are at right angles to
    their plane of orbit
  • all the planets revolve around the sun in roughly
    the same plane
  • All evidence to date suggests that the planets
    and sun are roughly the same age

19
Earths Early Environment
  • Molecules present on early Earth included
    nitrogen, water vapor, and carbon dioxide the
    same gases currently produced by volcanoes
  • Other minor contributors included methane,
    ammonia, carbon monoxide, sulfur dioxide, and
    hydrogen cyanide NO OXYGEN!
  • Comet impacts may have contributed large amounts
    of water vapor, helping to form the early oceans
  • Earths age can be estimated from levels of
    radioactive 238U versus 206Pb in rocks, and the
    age of the Moon can be accurately determined
    using this method

20
What is Life?
  • What is Life?
  • In-class Exercise
  • How is life distinguished from non-life? How do
    we know that something is ALIVE?

21
Some Definitions for Life
  • Krogh (2004)
  • Living things
  • Can assimilate and use energy
  • Can respond to the environment
  • Can maintain a relatively constant internal
    environment
  • Possesses an inherited information base
  • Can reproduce
  • Are composed of one or more cells
  • Are highly organized

22
  • Dawkins (1995)
  • Living things are the survival machines for a
    stream of digital information that changes over
    time
  • Living beings are just temporary hosts for the
    information molecule (DNA) and exist for the sole
    purpose of enabling that molecule to be
    perpetuated
  • DNA is ultimately the only thing that survives
    through time

23
  • Schroedinger (1944)
  • Life directs a stream of negative entropy upon
    itself to create order from chaos
  • Entropy (disorder) in the Universe is always
    increasing
  • Life works against entropy by borrowing energy
    from the Sun
  • In the end, however, entropy always wins

24
  • BUDDHA and the man with 84 problems
  • Dr. Seuss and trying to get to Solla Sollew
    (where there arent any problems, or else just a
    few )

25
Short Review of Lecture 2
  • What is the best current scientific theory for
    the origin of the Universe?
  • Why does the Big Bang theory make the idea of a
    "Creator" or "Creation Event" a meaningless thing
    to discuss?
  • What is space expanding into?
  • What elements were formed in the Big Bang?
  • How were other (heavier) elements (including
    carbon, the basis for life chemistry) formed?
  • What are the common characteristics shared by all
    living things but not by non-living things?
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