Southeastern Imbrium Crater Age Dating and Ejecting Data Scientific Research March 30, Objectives Covered What we covered for Phase II Moon rocks from Houston, TX on loan Moon Zoo training GIS.
Download ReportTranscript Southeastern Imbrium Crater Age Dating and Ejecting Data Scientific Research March 30, Objectives Covered What we covered for Phase II Moon rocks from Houston, TX on loan Moon Zoo training GIS.
Southeastern Imbrium Crater Age Dating and Ejecting Data
Scientific Research
March 30, 2011
Objectives Covered
What we covered for Phase II Moon rocks from Houston, TX on loan Moon Zoo training GIS Imagery hits Red Bank High School How we set up our GIS Format Map analysis/craters Technical issue overcome in gaining imagery Cross section in Archimedes Trask method for Imbrium (Archimedes Crater) and Sea of Serenity Data Collection Conclusions
Moon rocks take out Red Bank High School -NASA mania hits
Lunar Sample from Apollo 16 Mission
Moon Rocks • Launch Pad: Florida, USA (Kennedy Space Center) • Launch Date: April 16, 1972 • Lunar Landing: April 21, 1972 • Mission Duration: 11 d 01 h 51 mins.
• The astronauts brought back 94.7 kg of lunar samples from the moon.
We used MoonZoo to help train our eyes to learn to identify craters. We mapped over 1251 images in 8 days.
How We Got the Imagery
To start: Imagery- how to capture the image, where to capture the image, and how to use the image.
We downloaded imagery from “LROC” and LO orbiters- this took a while and a lot of false starts. We finally found on the internet.
We used NASA Article technical paper from NASA to aid in our choice of imagery and how to proceed.
The Image!!!
Imbrium, you never looked so beautiful!
How We Stored Our Imagery Data
We used 24 memory flash drives to divide up the swathes.
19 swathes covering 9,630.4754304 square kilometers in the Southeastern Imbrium Basin
Ta!Da!- Mare Imbrium- Archimedes crater
12 11 1 5 2 3 4 6 8 9 13 10 14 15 16 17 18 19 7
Area Covered
Distance covered in 1 swathe is about 120 mile or 72 Km 120 miles
Randy Hale- GIS Guru that helped!
Geospatial Analyst at North River Geographic Systems Inc.
Vice President at Georgia URISA Member of the Board at TNGIC 1 st Vice President at ASPRS Owner at North River Geographic Systems, Inc
How we set up our GIS format
• Includes the name of our swathe, which is our work base • Also includes different names of objects found on the swathe • Includes names of objects found, distinguished in colors.
• Names are selected to identify objects of focus.
GIS Format – Part 2
• Used to identify craters detailed features • Used to shape certain objects in the way they are formed
Describes the object and its features
How To Edit a Compound Crater
This is Crater Analysis!
This is a compound crater. The rim walls are connected.
Compound Simple
With all of this information we created these!!! Left Right Swathe #4 With craters marked Combination to make corrected shift with GIS imagery Swathe #7 with only craters marked Swathe #6 with imagery behind it
How We Worked!!
Mrs. Keith is a real task master!
WORK! WORK! WORK!
Over 3 weeks 23 students (Scientific Research) & 1 teacher put in 30 hours we mapped over 55,000 craters At times it seemed like all we did at Red Bank was map craters on the moon.
GIS Hits Red Bank
But mayhem soon followed: 1. GIS crashed twice, and had to reload (which took 8 hours each).
2. We thought we had lost $30,000 of GIS Software-the search was on!
3. Power went out 4. Data crashed laptop 5. Data when printed took up over 1,100 sheets of paper, we stopped at 460.
6. Twitter knows about us! In England and Canada.
7. Data corruption on ‘stick’ 24 8. Can we take a picture and not have the Camera stolen!
9. 4 months of begging to get free software from Virginia GIS.
Technical Issues We Faced With Imagery
1.
Figure 1
1.) Lining up pictures with dots to make swaths 2.) Issues when we were downloading data from LROC was compression data to make swathes and from them not to pixilate or become fuzzy 3.) Last 2 swathes from Sea of Serenity had Long and Lat problems
Original Image
Download Flipping
When we downloaded the crater imagery in order to use the images we had to first turn pictures
90°
Clockwise
Image after 1 st rotation Final Image
Then we had to turn an additional
180° 90°
Clockwise again until the original image had been rotated a total of Clockwise from its original position
Projection Issues matter:
We put swathes in the southern part of the Imbrium basin to make the projection more rectangular. Better data in the long run!
Still swathes were smaller at the top and wider at the bottom more due to curvature of the moon even with cylindrical projections to lessen long/lat issues.
Sinusoidal Projections allow us to have true and accurate diameters of craters.
Imbrium
Ileminite Rock
(Fe² TiO³) - Formula Has a melting point of 1800ºC or 3272ºF The name for the place of the discovery is Ilem mountains in Russia Metallic to sub metallic metal generally iron black meaning that the lava that formed the south eastern portion of Imbrium had to be around 1800ºC or greater during eruption.
Cross sectional Data for Archimedes Crater
1 3 4 5 6 7 2
Cross Sections
Overall Data Table Read Out Trask 1 – Imbrium Type of Crater Compound Bright Compound Dark Compound Compound Heavy Eroded Compound Light Eroded Simple Total Number 865 102 21 28 565 Simple Bright Dark Simple Simple Heavy Eroded 11468 **highest concentration** 4180 2165 1520 Simple Light Eroded Total of all the craters Combined 20073 **highest concentration** 40987 Square Meters 109,935,726.105555
17,070,670.00716
25,131,823.880641
17,733,033.61608
32,980,290.983086
456,327,831.5276
260,828,060.8237
89,358,083.170547
79,469,488.0927
964,838,198.3933
2,053,673,206.600369
So, what is trask?......
What is the Trask Method?
The Trask Method is a way of determining the ages of craters based on these assumptions: Newly formed craters appear sharp with raised rims and rayed ejecta.
Craters are subdued and destroyed eventually by meteorite impacts.
Small craters are eroded faster and disappear in less time than large craters.
62 Trask Method Pages Done by hand!!! Only 1038 to go…..UGH!
A Trasking We Will Go!!! (Counting Crater Diameters) We added, Counted, Divided, Rechecked Then 62 Pages in we Found The Microsoft Excel Program
Trask Method 1 Data-Via Excel
( Interior Imbrium/ Archimedes / Archimedes)
Diameter (ft)
0-32.8
32.8-164 164-328 328-1640.4
1640.4-3280.8
3280.8-16,404.2
16,404.2-32,808.4
Diameter (m)
0-10 10-50 50-100 100-500 500-1000 1000-5000 5000-10,000
Amount
20 7,316 14,572 17,435 1277 361 6
Percentages
.049
17.85
35.55
42.53
3.11
.88
.014
The Relative date of our swathes was: we found craters in the Copernican time interval of 1 and 3. the majority of our impact craters (32,007) were between 50 and 500 meters in diameter at 78.1%. 17.9% of our craters fell between 10 to 50 meters.
Diameter of Craters
Summary of GIS Trask 1 Data – Imbrium Crater Object ID in meters Frequency SUM Diameter MEAN Diameter MIN Diameter MAX Diameter RANGE Diameter COUNT Diameter 10-50m 7282 267931.7848
36.791236
10.115496
49.998206
39.88271
7282 50-100m 14556 1062589.975
73.000135
50.004989
99.995138
49.0149
14556 100-500m 17435 3423917.212
196.38183
100.01442
499.95944
399.94502
17435 500-1000m 1277 848423.892
664.389
500.246
997.025
496.779
1277 1000-5000m 361 579381.532
1654.796
1000.258
4835.843
3835.584
361 5000-10000m 6 37005.17863
6167.529771
5192.508224
8873.401565
3680.893341
6
Trask 1 Data
Trask 2 Data
New Trask Images
Two Swathes Red - Imbrium
Two Blue Swathes - Serenity
Two Red Swathes – Inbrium Trask 2
Object ID in Meters Frequen cy SUM Diameter MEAN Diameter MIN Diameter MAX Diameter RANGE Diameter COUNT Diameter 10-50m 293 10833.039
36.972
6.305
49.925
43.619
293 50-100m 1003 75321.4
75.096
9.608
100-500m 1717 331161.074
192.87
100.34
99.955
499.4
90.346
399.06
500-1000m 94 62756.743
667.625
503.306
997.025
493.71
1000-5000m 38 74044.464
1948.539
1003.458
4835.843
3832.385
1003 1717 94 38 5000-10000m 1 5698.2002
5698.2002 5698.2002
5698.2002
0 1
Two Blue Swathes – Serenity Trask 2
Object ID in meters Frequency SUM Diameter MEAN Diameter MIN Diameter MAX Diameter RANGE Diameter COUNT Diameter 10-50 m 50-100 m 100-500 m 4616 6107 3867 160715.7
435917.6
670878.7
34.82
71.38
173.49
10.06
50 100 49.999
49.995
499.76
39.94
49.992
399.76
4616 6107 3867 500-1000 m 191 1000-5000 m 72 5000-10000 m 2 129632.3
678.7
0 0 500.31
0 996.06
0 445.75
110372.6
1532.95
1003.26
3569.09
2565.82
0 191 72 2
New Swathe’s Location
What Did We Learn?
The age of the Archimedes crater inside the south eastern Imbrium 1.8-2.75 Copernican The age of the western Serenity crater 2.5-4.3 Copernican 55,000 craters mapped The different types of craters: Bright Whites, Dark Haloed, Compound, Simple.
Area mapped totals: Imbrium 9,630.46 sq Km (5,778.4 sq. miles) Serenity 2,156.5 sq Km (1,293.9 sq miles) All areas mapped total: 11,786.9 sq Km (7,o72.11 sq miles) The type of rocks in the Archimedes crater is ILeminite The melt temperature of rocks on the moon in Archimedes 1800ºC or 3272ºF How to use GIS to map the moon Most craters in both areas fell between 50-500m-wih 78.1% in Imbrium and 67.1% in serenity Cross Sections: 1,500 ft rim walls in the southern portion of Imbrium Comparing like areas for best data: Old Area: 2012.4 km New Area:2156.5 km
Where do we go from here?
1.
2.
3.
4.
5.
Develop a DM Model of swathes that went through the rim wall of Archimedes to see elevation and slump patterns Get Data for 3-D Modeling, 50% overlap needed Get swathes outside the Imbrium. The whole perimeter! We had to stop at 2! For times sake Look at statistical data for more trends to answer questions of why so few craters in 500-1000m? 1000m-5000m?
the 0-10 – we think our resolution or picture would not let us see and the 5000-10000m are really rare.
Bibliography
http://www.lpi.usra.edu
http://www.the-moon.wikispaces.com
http://www.apollo.sese.edu
http://www.tappedin.org
http://www.thunderbolts.info/tpod/2006/archog/060315/srille.html
l http://www.homepage.ntlworld.com/peterlloyd3/moon/craters/membrium050423.htm
http://www.nasa.gov
http://www.moontoday.net
http://www.moonzoo.org
http://www.onlinecharttool.com
(slide 36) http://astrogeology.usgs.gov/Projects/LunarOrbiterDigitization/Pilot/lunorbWebovervu .html
http://www.galleries.com/minerals/oxides/ileminite/ileminite.html
Http://www.mindat.org
Thank You!!!
Red Bank High School 2011