Chapter 1 the water planet
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Chapter 1 The Water Planet. Origin of the Universe. Earth , a small, rocky planet, orbits the . . . the sun , a medium sized star, . . one of billions of stars in the Milky Way galaxy , . . one of billions of galaxies in the universe. Origin of the Universe.

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Chapter 1 The Water Planet

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Chapter 1 the water planet

Chapter 1The Water Planet


Origin of the universe

Origin of the Universe

Earth, a small, rocky planet, orbits the

. . . the sun, a medium sized star,

. . one of billions of stars in the Milky Way galaxy, . . one of billions of galaxies in the universe.


Origin of the universe1

Origin of the Universe

Brightness of pulsating stars – cepheid variables – was used to determine distance from Earth

Brighter stars = closer to Earth

Dimmer stars = farther from Earth

Repeated measurements determined cepheid variables were moving away from Earth

Interpretation  the universe is expanding

Size of the Universe: Luminosity


Origin of the universe2

Origin of the Universe

Size of the Universe: Doppler Effect

Doppler Effect:The apparent change in the frequency of sound waves or light waves due to the motion of a source relative to an observer

  • Example: change in frequency (pitch) of a siren from passing police car


Origin of the universe3

Origin of the Universe

Doppler Effect Example: The change in frequency (pitch) of a siren from passing police car

No change in frequency for sound waves when police siren and observer are stationary

Higher frequency when sound waves are compressed for objects moving toward an observer

Lower frequency when sound waves are stretched out for objects moving away from an observer


Origin of the universe4

Origin of the Universe

Light on Earth is a form of solar radiation and occurs at specific wavelengths from 380-750 nanometers

Size of the Universe: Doppler Effect

  • The color of light from distant stars is stretched (“shifted”) toward wavelengths at the red end of the spectrum

Shorter wavelength

Longer wavelength


Origin of the universe5

Origin of the Universe

Size of the Universe: Doppler Effect

  • Astronomers use the degree of “red shift” to determine the distance to far away galaxies

    • more than 13 billion light years (distance) from Earth


Origin of the universe6

Origin of the Universe

The Big Bang Theory

  • Reversing the expansion of the universe suggests the universe began with an episode of rapid expansion from a much more compact form

  • The almost instantaneous period of rapid expansion is known as the Big Bang

  • Within hours of the Big Bang, simple elements (hydrogen, helium) formed as subatomic particles combined

    • Hydrogen – 1 proton + 1 electron

    • Helium – 2 protons + 2 neutrons + 2 electrons


Stars and planets

Stars and Planets

  • Just 3 elements – hydrogen, oxygen, carbon - make up 90% of the human body (by weight)

    • Five more – nitrogen, calcium, phosphorus, potassium, sulfur – make up 9% more

    • Small amounts of many other elements needed for life

  • Hydrogen formed soon after the Big Bang

  • Other elements and complex compounds formed during the life cycle of stars


Stars and planets1

Stars and Planets

  • Gravity pulled together irregular clouds of gas and dust generated from the Big Bang to form galaxies (systems of stars)

Stars and galaxies in a small section of the universe. Image taken by Hubble space telescope


Stars and planets2

Stars and Planets

  • Gas and dust material clumped together to form millions of stars (ongoing process)

    • Very high temperatures and pressures in the interiors of stars fuses hydrogen atoms together – nuclear fusion – to form helium

    • Some stars burn out when hydrogen is used up. Others can fuse elements up to iron (Fe)

False color image from NASA Spitzer Space telescope showing cool gas and dust that are incubators for new stars.


Stars and planets3

Stars and Planets

  • Giant stars collapse over multiple stages, initially forming red supergiant stars

    • Collapse forms increasingly complex elements (e.g., carbon  oxygen)

  • Final stage is a massive explosion – supernova – that fuses elements together forming elements heavier than iron and blasts them through the universe

Kepler’s supernova. Astronomer Kepler noted the appearance of a new star (the supernova) on October 9, 1604.


Stars and planets4

Stars and Planets

  • When stars form they are surrounded by a rotating disk of cosmic debris

  • Gravity pulls debris together to form planets that revolve in a consistent direction around star

    • Heavier, rocky planets closer to star

    • Lighter, gas-rich planets farther from star

  • Potentially thousands or millions of extra-solar planets revolve around other stars


Our solar system

Our Solar System

  • Solar system - sun and surrounding planets

  • Sun = 99.8% of total mass of the solar system

    • Sun 150,000,000 km from Earth

Sunspots – dark spots on surface of sun

Solar flare


Our solar system1

Our Solar System

  • The solar wind is a stream of charged particles emitted from sun’s magnetic field (1,600,000 km/hr)

  • The solar wind affects an volume of space known as the heliosphere

  • Earth’s magnetic field deflects the solar wind


Our solar system2

Our Solar System

  • Interactions of solar wind with Earth’s magnetic field generates aurora in the upper atmosphere of polar regions

  • Occasional solar eruptions can disrupt Earth’s magnetic field to produce electrical blackouts

    • Satellites in greater danger from solar flares than features on surface

Aurora from Earth

Aurora from space


Our solar system3

Our Solar System

  • Eight Planets

  • 4 terrestrial planets (Mercury, Venus, Earth, Mars)

  • Jovian planets (Jupiter, Saturn, Uranus, Neptune)


Our solar system4

Our Solar System

  • What about Pluto?

  • Improved technology resulted in recent discoveries of several distant objects that were similar size or larger than Pluto

  • International Astronomical Union (IAU) could either

    • Consider the new objects as new planets

    • OR

    • Classify the new objects – and Pluto – as a new group of objects

  • IAU chose option #2


Pluto

Pluto

  • What about Pluto?

  • IAU adopted a new definition of the term planet:

  • A planet is an object that orbits a star and is massive enough (~400 km radius) for gravity to pull its material into an approximately spherical shape. A planet would have cleared the neighborhood around its orbit.

  • Pluto does not meet the last part of the definition and was considered a founding member of a new class of objects - dwarf planets


Our solar system5

Our Solar System

  • Terrestrial Planets

  • Composed of rocks

  • Divided into compositional layers

    • Crust – composed of lighter elements (e.g., silicon, oxygen)

    • Mantle

    • Core – composed of heavier elements (e.g., iron, nickel) found in metallic meteorites

The Good Earth, Chapter 2: Earth in Space


Our solar system6

Our Solar System

  • Jovian Planets

  • Large, gas giants

  • Much of the volume of the planets is a thick atmosphere overlying oceans of liquid gases

  • Characterized by many moons and ring systems

Jupiter and four of its largest moons.

Saturn’s ring system. The gravitational pull of the moon’s keep the ring systems in place.


The unique composition of earth

The Unique Composition of Earth

Earth shares many features with other planets, so what makes it so special?

  • Liquid water

  • Gravity and a protective atmosphere

  • Life-sustaining gases

  • A strong magnetic field


The unique composition of earth1

The Unique Composition of Earth

Earth’s size is sufficient to produce enough gravity to hold a thick atmosphere of gases in place

  • Atmosphere protects us from:

  • Incoming small asteroids/comets

  • Harmful solar radiation (x-rays, UV)


The unique composition of earth2

The Unique Composition of Earth

Earth’s biosphere has altered the composition of the atmosphere to add oxygen and extract toxic carbon dioxide

  • Atmosphere composition effects temperature:

  • Higher carbon dioxide content on Venus produces temperatures of 464oC


The unique composition of earth3

The Unique Composition of Earth

Composition of Earth’s atmosphere just right to absorb enough heat to keep average temperature of 15oC

  • Greenhouse effect:

  • Water vapor, carbon dioxide (0.038%) gases absorb heat

  • Without greenhouse effect, temperatures would be -18oC


The unique composition of earth4

The Unique Composition of Earth

Earth’s magnetic field protects Earth from harmful solar wind that would strip away atmosphere

Magnetic field due to molten rocks in the outer core and relatively rapid planetary rotation:

  • Smaller planets or slowly rotating planets have lost heat and have weak magnetic fields


Earth s moon

Earth’s Moon

Four theories for Moon formation:

Fission: Rapid spin spun moon from Pacific Ocean. Improbable.

Capture: Moon formed elsewhere in solar system but was gravitationally captured. Improbable.

Condensation: Moon condensed close to earth in solar nebula formation. Improbable.

Giant Impactor: Mars-sized body (Theia) impacted Earth 50 million years after initial formation. Best accounts for Earth-Moon characteristics.


Earth s moon1

Earth’s Moon


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