mars-cratering-report

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School

Florida International University *

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Course

1002L

Subject

Geography

Date

Dec 6, 2023

Type

docx

Pages

3

Uploaded by ChefRook15093

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Name: Mars Cratering Activity 1 Use the web application shown in the video tutorial For this activity, you will be estimating the age of the Hadriaca Patera region (image 1) in the web appplication. Count the number of impact craters greater than 500 m in diameter for the square region of 15.42 km by 15.42 km. Non-impact craters for that square region should not be counted. Once you know the number of impact craters for that square region, use the following formula to estimate the number of craters per million square kilometers: Show all work: Image # 1 ( Hadriaca Patera ) Surface Density = 10 6 k m 2 × ( number of impact craters ) ( linear ¿ region ) 2 = ¿ 10 divided by 15.42^2 =0.042056318 x 10^6= 42,056 craters per million Age: 3 billion years
Name: Mars Cratering Activity 2 Use the same web application as before. For this activity, you will be estimating the age of the Nirgal Vallis region (image 5) & the Dao Vallis region (image 9) in the web application. Count the number of impact craters with different cut-off diameters for the different square regions. Non-impact craters should not be counted. Once you know the number of impact craters for that square region use the following formula to estimate the number of craters per million square kilometers: Show all work: Image # 5 ( Nirgal Vallis ) Surface Density = 10 6 k m 2 × ( number of impact craters ) ( linear ¿ region ) 2 = ¿ 17.39^2= 302.4121 divided by 10^6 x 11 = 100000= 11000000 divided by 302.4121 = 36374.20593 Age: 2 billion years Image # 9 ( Dao Vallis ) Surface Density = 10 6 k m 2 × ( number of impact craters ) ( linear ¿ region ) 2 = ¿ Age: 11.64^2= 135.4896 10^6 x 8 =8000000 divided by 135.4896 = 58914.67388
Name: If you skip the graphs, you will only earn credit for the Surface/Crater Density questions if you did them correctly. There are only three questions, so be careful.
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