Alberghine Frayne Venus

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    Sydney Frayne

    Briana Alberghine

    THE PLANET VENUS

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    APPEARANCE OF VENUS

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    History of Venus

    Venus is the Roman

    Goddess of Love and

    Beauty. In Greek

    Mythology, she is alsoknown as Aphrodite.

    This is the sign for

    Venus.

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    BASIC FACTS OF VENUS

    Venus was first discovered by a caveman who mistook it for astar. Ancient Greeks also wanted to learn more about Venus asa star

    Venus is the second planet from the Sun

    Venus is nearly the same size as Earth

    12,102 km in diameter(12,756 km for Earth)

    82% the mass of Earth

    Similar density, 5.3 g/cm3 (5.5 g/cm3 for Earth)

    Venus takes 223 days to orbit the Sun

    Venus takes 2,243 days to rotate on it axis and it rotates theopposite direction of Earth

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    EARTHS SISTER

    Venus is sometimes called

    Earths twin orsisterbecause the planets are so

    much alike. They are almost

    the same size and they both

    have relatively young

    surfaces. They also are

    similar in chemical anddensity compositions.

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    LAYERS OF VENUS

    Crust-the Venusian crust is comparably thin, extending a depth of 30 miles. The surface is

    remarkably flat, with on 10% of the planet having a relief. The thin crust is one of the

    reasons why Venus was geographically active in the recent past.

    Mantel-below the crust is a rocky mantel, again solid, extending almost from the surface

    to a depth of about 2,000 miles

    Core-large metal core, probably composed of the metal nickel and iron, which takes up

    about half of its radius. The planet has a weak magnetic field, so its core could possibly

    be solid.

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    VOLCANOES

    Venus is a planet with wide-scale volcanic activity

    In the lowland plains, lava renews the surface anderases craters

    The are many volcanoes associated with surface hotspots

    The largest volcano on Venus is Sif Mons

    3 km high, 500 km across

    Caldera is 40 km across

    These volcanoes result from magma reaching thesurface

    Pressure under the surface can cause bulges calledcoronae

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    TEMPERATURE OF VENUS

    Venus is very hot. It can heat up to over 867

    degrees F. The cause is the thick yellow

    clouds (formed from a poison called Sulfuric

    Acid) all around the planet. It is cal led the

    greenhouse effect. The clouds trap the

    heat, causing the planet to get hotter and stayhot.

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    Visitations to Venus

    More than 20spacecraft's havevisited Venus. The veryfirst one was Mariner 2,

    which visited Venus in1962. Some of the otherspacecraft's includePioneer Venus, Venera7, and Magellan.

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    THE MAGELLAN MISSION TO VENUS

    The Magellan mission to Venus was launched May 4, 1989 and arrived at Venus onAugust 10, 1990

    Magellan used a high resolution radar to map the surface of Venus through theopaque clouds

    Magellan worked for 4 years and mapped 98% of the surface of Venus

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    MAPPING SURFACE OF VENUS

    The Magellan data can be processed into 3-D views of the surface of Venus

    False color picture of Venus constructed

    from radar images from the Magellan

    space craft

    3-D view of three impact crater on

    the surface of Venus

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    GRAVITATIONAL FORCE

    If a 150 pound person went on Venus. They would weigh 132 pounds.

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    VENUSS ATMOSPHERE

    The atmosphere of Venus causes a very high surface temperature and gives thesurface a perpetual red twilight

    The weather at the surface is hot, dry, calm

    The pressure at the surface is 90 times the Earths atmospheric pressure

    Carbon Dioxide 96%

    Nitrogen 3.2

    Other .8%

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    VENUS: LOCATION & ORBIT

    This close proximity to the Sun accounts for the average surface temperature on Venus of

    482 degrees Celsius. It takes 0.62 Earth years, or 225 Earth days, to complete one

    revolutionary period and 243 Earth days to complete a rotational period. This makes a

    Venus day longer than a Venus year! At an orbital inclination of 3.39 degrees and an

    eccentricity of 0.0068, the planet's orbit about the Sun is almost perfectly circular.

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    PHASES OF VENUS

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    TIME ON VENUS

    One day on Venus would be 243

    Earth days. One year on Venus

    would be 224 Earth days. That

    means that a day is longer than a

    year on Venus.

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    BIBLIOGRAPHY

    spaceodyssey.dmns.org/media/12607/ venus.ppt

    www.uen.org/.../downloadFile.cgi?file... venus.ppt...venus.ppt

    www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_...

    www.oocities.org/shivabhava333/ VENUS.ppt

    http://library.thinkquest.org/C005921/Venus/venuLocOrb.htm

    Garlick, Mark A. Astronomy: A Visual Guide Richmond Hill, Ont: Firefly, 2004. Print.

    http://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.oocities.org/shivabhava333/VENUS.ppthttp://www.oocities.org/shivabhava333/VENUS.ppthttp://www.oocities.org/shivabhava333/VENUS.ppthttp://www.oocities.org/shivabhava333/VENUS.ppthttp://library.thinkquest.org/C005921/Venus/venuLocOrb.htmhttp://library.thinkquest.org/C005921/Venus/venuLocOrb.htmhttp://library.thinkquest.org/C005921/Venus/venuLocOrb.htmhttp://library.thinkquest.org/C005921/Venus/venuLocOrb.htmhttp://www.oocities.org/shivabhava333/VENUS.ppthttp://www.oocities.org/shivabhava333/VENUS.ppthttp://www.oocities.org/shivabhava333/VENUS.ppthttp://www.oocities.org/shivabhava333/VENUS.ppthttp://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.powershow.com/.../The_Planet_Venus_powerpoint_ppt_http://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppthttp://www.uen.org/.../downloadFile.cgi?file...venus.ppt...venus.ppt