the “twin planet” of earth by daniel barraza and michael taylor per. 2 mrs.ducharme

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Venus THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

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Page 1: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

VenusTHE “TWIN PLANET” OF EARTH

BY DANIEL BARRAZAAND MICHAEL TAYLOR

PER. 2Mrs.Ducharme

Page 2: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

Venus is the second planet from the Sun, making it hotter than our planet.

It is part of the milky way galaxy, between two “arms” of the spirals.

In Our Galaxy

Not this one

Page 3: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

TEMPERATURE

The temperature on Venus is about 860 degrees Fahrenheit, Because it is close to

the sun.

Page 4: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

NAMING THE PLANET

Venus got its name from the Roman goddess of love.In Greek, the goddess of love is Aphrodite. In Babylonian, her name is Ishtar.

Page 5: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

ORBIT

Venus’ orbit is elliptical and counter-clockwise.

Venus takes approximately 243 days to orbit the Sun.

Page 6: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

COMPOSITIONVenus' atmosphere is nearly 100 times as massive as Earth's, and its thick cloud layers block the surface from view. It exerts a pressure of approximately 92 bars at the surface. Its composition is nearly all CO2. The density at the surface is 65,000 g/m3. Wind speeds range from 1-4 km/sec at the surface. The scale height of the atmosphere is about 15.9 km.

Page 7: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

Life on Venus

Life cannot be supported on Venus, unless it was very tough and could withstand high gravity, could use CO2 like we use oxygen, and have a slow metabolism.

Page 8: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

M OOOOOOONS

Sorry but Venus has no moons.

Page 9: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

PHYSICAL CHARACTERISTICS

Venus has no water on its surface, and very little water vapor in its atmosphere. Scientists think that the runaway greenhouse effect that makes Venus so hot today boiled away its oceans long ago. Since Venus lacks a planetary magnetic field, the Sun’s solar wind was able to blast the hydrogen atoms out of Venus’ atmosphere and into space. Venus can never be cool again.Most of the surface of Venus is covered by smooth volcanic plains, and its dotted with extinct volcanic peaks and impact craters. Venus has much fewer impact craters than other planets in the Solar System, and scientists have estimated that some event resurfaced Venus between 300-500 million years ago, wiping out all of the old impact craters and volcanoes.

Page 10: THE “TWIN PLANET” OF EARTH BY DANIEL BARRAZA AND MICHAEL TAYLOR PER. 2 Mrs.Ducharme

A LONG, LONG TIME AGO, IN A CLASSROOM JUST DOWN THE HALLWAY, WE STARTED THIS

POWERPOINT.NOW IT IS OVER.

THANK YOU FOR YOUR ATTENTION, AND WE HOPE YOU LEARNED

SOMETHING FROM US.