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Venus

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... Venus come from the Babylonians on the famous Venus Tablet dated circa 1500 B.C. ... Shield Volcanoes. Pancake volcanoes. developed by thick lava. Coronae ... – PowerPoint PPT presentation

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Title: Venus


1
Venus
  • By James Menke
  • Kevin Mott
  • Travis Angell

2
Statistics
  • Mass (kg) 4.869e24
  • Mass (Earth 1) 81476
  • Equatorial radius (km) 6,051.8
  • Equatorial radius (Earth 1) .94886
  • Mean density (gm/cm3) 5.25
  • Mean distance from the Sun (km) 108,200,000
  • Mean distance from the Sun (Earth 1) 0.7233
  • Rotational period (days) -243.0187
  • Orbital period (days) 224.701
  • Mean orbital velocity (km/sec) 35.02
  • Orbital eccentricity 0.0068
  • Tilt of axis (degrees) 177.36

3
Statistics
  • Orbital inclination (degrees) 3.394
  • Equatorial surface gravity (m/sec2) 8.87
  • Equatorial escape velocity (km/sec) 10.36
  • Visual geometric albedo 0.65
  • Magnitude (Vo) -4.4
  • Mean surface temperature 482C
  • Atmospheric pressure (bars) 92
  • Atmospheric composition
  • Carbon dioxide 96
  • Nitrogen 3 
  • Trace amounts of Sulfur dioxide, water vapor,
  • carbon monoxide, argon, helium, neon,
  • hydrogen chloride, and hydrogen fluoride.  

4
Characteristics
  • Surface temperature 482 C (900 F)
  • This high temperature is primarily due to a
    runaway greenhouse effect caused by the heavy
    atmosphere of carbon dioxide.
  • Venus' surface appears to have been completely
    resurfaced 300 to 500 million years ago.
  • Liquid water does not exist on the surface.

5
Characteristics
  • Venus is scarred by numerous impact craters
    distributed randomly over its surface.
  • At least 85 of the Venusian surface is covered
    with volcanic rock.
  • Some features that are unique to Venus include
    coronae and arachnoids.

6
History
  • Venus is named after the Roman goddess of love
    and beauty.
  • The earliest recorded observations of Venus come
    from the Babylonians on the famous Venus Tablet
    dated circa 1500 B.C.

7
History
  • Venus has been observed in detail by both
    Aristotle and Ptolemy during the geocentric
    system era.
  • In 1610, Galileo Galilei was the first to observe
    the phases of Venus using his refractor.
  • The transit of Venus marked improvement in our
    knowledge of Venus and of our Solar System.

8
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9
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10
Internal Structure
  • Core Mostly Iron and Nickel
  • around 6000km
  • Mantel Made up of molten rocks
  • Little convection
  • Crust Made up of volcanic rock
  • Stronger and thicker than Earth, keeps getting
    thicker

11
Magnetic Field
  • What little magnetic field is from interaction
    between ionosphere and solar winds, not dynamo

12
Mantel Movement
  • Similar to convection
  • Generates heat through decay of radioactive
    materials
  • Results of movement
  • Might cause tectonic deformation
  • When crust breaks
  • lava flows - floods surface and becomes thicker

13
Atmosphere
  • Over 90 times more dense than Earths atmosphere
  • 96 Carbon Dioxide rest Nitrogen with small
    amounts of other
  • Clouds composed of sulfuric acid
  • Small amounts of water vapor high in atmosphere

14
Greenhouse Effect
  • Causes Venuss surface to be hotter than
    Mercury's surface
  • Average heat around 890 degrees Fahrenheit
  • Caused by the 96 CO2 in atmosphere
  • What caused the atmosphere to be composed of all
    this CO2?

15
High CO2
  • Venus formed too close to the sun and therefore
    water couldnt develop into oceans
  • Therefore plants couldnt form and CO2 couldnt
    be dissolved in water and stored in carbonate
    rocks
  • Since CO2 kept building up, it created a runaway
    greenhouse effect

16
Runaway Greenhouse Effect
  • High amounts of CO2 creates extreme heating.
  • Works just like Earth
  • Lets visible light in
  • Doesnt allow IR light in
  • Light hits surface and reradiates as IR
  • CO2 wont let heat out

17
Venuss surface
  • Scientist can only see using radio waves because
    clouds are too thick
  • 85 of surface is lowlands
  • 2 large continent areas

18
Venuss volcanoes
  • Rift Valleys
  • Meteor Craters
  • Faults with up/down motion
  • Shield Volcanoes
  • Pancake volcanoes
  • developed by thick lava
  • Coronae
  • collapsed domes over large magma chambers

19
Venuss plate tectonics
  • No plate tectonics
  • Smaller and therefore cooled off faster creating
    a thicker lithosphere that prevents plate
    tectonics
  • Although no plate tectonics, Venus still goes
    through a resurfacing of its own
  • 500 million yrs ago Venus resurfaced
  • Heat in mantle reaches limit where crust is weak
  • Over 100 million yrs, subducting occurs on large
    scale

20
  • Questions?
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