edit
05-10-2007, 12:17 PM
Mars Virtual Olympics Summit Meeting (http://www.davis.ogsd.k12.ca.us/edenvale/mars1/summit.html)
http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/fossil.jpg
Background Information Research
Key Research Questions:
What are the characteristics of each of the planets in our solar system?
How far is each planet from Mars?
http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/travag.gif
Picture from HyperStudio™ http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/Sosyst.gif
Research Findings:
Our virtual athletes will travel in a specially constructed virtual Olympics shuttle.
The spectators will stay is a special booth above the stadium so they can see everything. There will be no bad seating.
http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/alien01.gif Astronomers (http://www.davis.ogsd.k12.ca.us/edenvale/mars1/astron.html)
Research Findings:
Venus is the 2nd planet from the sun. It is the 6th largest planet. It's orbit is108,200,000 km (0.72 AU) from the sun. It's the brightest object in the sky except for the sun and the moon. Venus's rotation is somewhat unusual in that it is both very slow (242 Earth days per Venus day. Venus is only slightly smaller that the earth (95% of the Earth's diameter, 80% of the earth's mass) It has few craters incating that is a relatively young surface. It's density and chemical composition is similiar to Earth's. Venus's atmospheric's pressure is 90 atmospheres on its surface. It is made up of mostly carbon dioxide. It has several cloud layers that are many km thick and made of supfuric acid. Venus has strong (350 kph) winds at the cloud tops, but only slow winds on the surface. Data from Magellen shows that Venus is covered by lava flows. There is no magnetic field on Venus. This may be because of it's slow rotation.
http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/fossil.jpg
Background Information Research
Key Research Questions:
What are the characteristics of each of the planets in our solar system?
How far is each planet from Mars?
http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/travag.gif
Picture from HyperStudio™ http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/Sosyst.gif
Research Findings:
Our virtual athletes will travel in a specially constructed virtual Olympics shuttle.
The spectators will stay is a special booth above the stadium so they can see everything. There will be no bad seating.
http://www.davis.ogsd.k12.ca.us/edenvale/mars1/gifs/alien01.gif Astronomers (http://www.davis.ogsd.k12.ca.us/edenvale/mars1/astron.html)
Research Findings:
Venus is the 2nd planet from the sun. It is the 6th largest planet. It's orbit is108,200,000 km (0.72 AU) from the sun. It's the brightest object in the sky except for the sun and the moon. Venus's rotation is somewhat unusual in that it is both very slow (242 Earth days per Venus day. Venus is only slightly smaller that the earth (95% of the Earth's diameter, 80% of the earth's mass) It has few craters incating that is a relatively young surface. It's density and chemical composition is similiar to Earth's. Venus's atmospheric's pressure is 90 atmospheres on its surface. It is made up of mostly carbon dioxide. It has several cloud layers that are many km thick and made of supfuric acid. Venus has strong (350 kph) winds at the cloud tops, but only slow winds on the surface. Data from Magellen shows that Venus is covered by lava flows. There is no magnetic field on Venus. This may be because of it's slow rotation.