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Lab Observations

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Part 1: Recording Observations
In the following chart, record your observations of each test for the seven minerals. After you have completed all tests, name the minerals in Part 2 of this worksheet. An example of how to fill out the chart is illustrated follows.

|Recorded Observations for Minerals 1-7 |
|Tests |Example |Mineral 1 |
|Example: Fluorite |80% certain |I am almost certain this mineral is fluorite, but I am not completely sure. Fluorite and gypsum|
| | |are both white, shiny, have white streaks, cleave, and show no reaction to acid. However, the |
| | |specific gravity of this mineral is 3.18, which is higher than gypsum, so I am pretty sure it |
| | |is fluorite. |
|Mineral 1: Pyrite |100% certain |This mineral has more of gold color with only slight green undertone to it. While pyrite and |
| | |talk have similar attributes, such as the shiny specks and no reaction to acid, Pyrite is |
| | |heavier at 5.1, leaves a black streak and is much harder. |
|Mineral 2: Talc |70% certain |This mineral is similar to Pyrite, however, it is lighter at only 2.8, leaves a white streak, |
| | |however, when broke, I would categorize it as a cleavage, because the lines looked more smooth |
| | |than rough and bumpy to me. Its green color with the undertone of gold is what set it apart |
| | |from the Pyrite. |
|Mineral 3:Gypsum |50% Certain |This one has the appearance of Gypsum, in that it is white, leaves a white streak, is about the|
| | |same weight as that mineral at 2.7, however, mineral 3 reacted with acid, and Gypsum does not |
| | |do that. Also, while mineral 3 had some shine to it, it did not reflect a bunch of light so as |
| | |to create a sparkle, perhaps a slight glare, but not enough for me to say it was either pearly |
| | |or shiny. |
|Mineral 4:Orthoclase Feldspar |65% Certain |This mineral had a pink/orange color to it, left a white streak, appeared to have a shiny |
| | |luster, Scratched with a file and had no reaction to acid. It could very well be Corundum, |
| | |however, the specific gravity of mineral 4 is much lighter at only 2.6, whereas Corundum would|
| | |have a specific gravity of about 3.9-4.1 |
|Mineral 5: Quartz |75% Certain |Mineral 5 had a primary white color with a gold offset. When scratched on a surface, it left a |
| | |white streak. Its luster was shiny. However, its specific gravity was about .1 heavier than |
| | |listed. In our chart. Its hardness appeared to be more as well. |
|Mineral 6:Calcite |50%Certain |Mineral 6 showed all characters of Calcite, except for 2 factors, it was slightly lighter at |
| | |2.4, and it had no reaction to acid. It could pass off as Borax, however, it did not have a |
| | |dull luster and it is heavier than Borax. |
|Mineral 7:Graphite |80% Certain |Mineral 7 Had a black/burnt orange color, Left a brown streak, had shiny specks, when broken, I|
| | |thought it be smooth, or at least not bumpy enough to be considered a fracture. However, |
| | |Mineral 7 had no reaction to Acid, as Graphite would. |

Part 3: Evolutionary Processes
In the following table, identify two evolutionary processes of Earth. Include a 100- to 200-word explanation of each process.

|Evolutionary Process |Description |
|Nebular Hypothesis |The most popular and most used idea of how the solar system formed. This hypothesis states that a large mass of swirling |
| |interstellar dusted married with a gas called nebula. It begins to contract and expand, leaving behind a central bulge |
| |containing hydrogen that formed into helium, and thusly, becomes the sun. However, as it contracts, it continues to spin, |
| |forming a wide disk shape around the sun. The contractions rise the temperature which causes the beginning of fusion in the |
| |central bulge and gives the sun its shine. The outer disk begins to cool and is filled with chinks of debris. The larger |
| |chunks of debris pull in the smaller chunks by gravity, which are then very gradually formed into planets over a period of |
| |about tens of millions of years. |
|Planetary Accreation |This hypothesis is more of a sequel to the Nebular Hypothesis. The prior hypothesis mentions how the solar nebula cooled and|
| |flattened out into the disk made up of all that debris. Through random collisions, this debris grew into larger clumps, some|
| |large enough to have their own gravitational pull, which pulled in any debris with in their surrounding area. However, there|
| |were some rocks that managed to escape the pull. These rocks are what we know as meteorites. The idea of random collision |
| |and gravitational pulls leads to a hypothesis of how the moon came to be. The idea is that well over thousands of millions |
| |of years ago, while earth was still in the process of forming, another growing planet called Theia ran into the earth, Theia|
| |is completely destroyed by this impact and so is a portion of earth, leaving it look like a cookie with one bite taken out, |
| |which leaves earth’s axis tilted. The debris from this impact then forms a ring around earth and starts clumping together. |
| |The largest clump continues collecting debris and forms into what we know as the moon. Slowly, earth regains its shape and |
| |continues to evolve. |

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