| Sunshine
State
Standards: |
|
| Objectives: |
|
| Materials: |
|
| Commit to an Outcome |
|
| Expose Beliefs |
|
| Confront Beliefs |
|
| Accommodate the Concept |
|
| Extend the Concept |
|
| Go Beyond |
|
What we learned from this activity:
The surface of the
Moon consists of light and dark areas.
There are types
of igneous rocks that have similar color (rhyolite-white; andesite-gray;
basalt dark gray to black) that relate to the colors on the Moon's surface
and could possibly exist on the surface of the Moon.
Amplifying Information:
During the Apollo missions which landed of the Moon, numerous 'Moon Rock' samples were returned to the Earth for study. These 'Moon Rocks' were similar to many types of igneous rocks we have on Earth including rhyolite, andesite, and basalt in addition to other types of igneous rocks. The dark areas of the Moon, Lunar Maria, were found to consist mostly of basalt. The the light colored areas of the Moon, the Lunar Highlands, were found to consist of light colored igneous rocks.
NASA is using an instrument (spectroscope) to investigate the surface of Mars from orbit and on the rovers. This instrument analyses the way a rock returns the various wavelenghts of light (colors) and that relationship with the composition of the rocks. The Mars Reconnaissance Rover (MRO) which was launched on August 12, 2005 is currently enroute to Mars will be in a stable orbit around Mars about September 2006. The MRO has an instrument onboard, CHRISM (Compact Reconnaissance Imaging Spectrometer for Mars), which will examine the composition of the Martian surface to determine desirable landing sites for later missions.