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7/29/2019 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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7/29/2019 Alberghine Frayne Venus
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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.
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