Title: Craters
1Craters
2Lunar Crater Categorization
- In 1978, Chuck Wood and Leif Andersson of the
Lunar Planetary Lab devised a system of
categorization of lunar impact craters. They used
a sampling of craters that were relatively
unmodified by subsequent impacts, then grouped
the results into five broad categories. These
successfully accounted for about 99 of all lunar
impact craters.
http//www.unm.edu/abqtom/images/Moon/Moon11-19-0
2b.jpg
3The LPC Crater Types
- ALC small, cup-shaped craters with a diameter
of about 10Â km or less, and no central floor. The
archetype for this category is 'Albategnius C'.
http//www.edwardroach.com/uploads/Albategnius_9-3
-07_504edt_300frames.jpg
4The LPC Crater Types
- BIO similar to an ALC, but with small, flat
floors. Typical diameter is about 15Â km. The
lunar crater archetype is Biot.
http//www.astrospider.com/images/moon/Biot_LAC98m
ap.jpg
5The LPC Crater Types
- SOS the interior floor is wide and flat, with
no central peak. The inner walls are not
terraced. The diameter is normally in the range
of 15-25Â km. The archetype is Sosigenes crater.
http//history.nasa.gov/ap15fj/photos/o/as15-97-13
288.jpg
6The LPC Crater Types
- TRI these complex craters are large enough so
that their inner walls have slumped to the floor.
They can range in size from 15-50Â km in diameter.
The archetype crater is Triesnecker.
http//www.damianpeach.com/lunartemp/triesnecker02
.jpg
7The LPC Crater Types
- TYC these are larger than 50Â km, with terraced
inner walls and relatively flat floors. They
frequently have large central peak formations.
Tycho crater is the archetype for this class.
http//upload.wikimedia.org/wikipedia/commons/7/7e
/Mooncrater.jpg
8The LPC Crater Types
- Beyond a couple of hundred kilometers diameter,
the central peak of the TYC class disappear and
they are classed as basins.
http//www.uwsp.edu/geo/projects/geoweb/participan
ts/dutch/Sudbury/schrodinger.gif
9Question
- How do the variables of velocity, size, and
meteor angle to surface affect the outcome of
resultant craters?
http//apod.nasa.gov/apod/image/0507/impact13sec_d
eepimpact_hri.jpg
10Hypothesis
- Develop a hypothesis about the outcome of your
experiment based on your observations, reading,
and experience
http//www.photoaxe.com/wp-content/uploads/2007/02
/droplet.jpg
11Your Lab
- You collected data on
- Speed of the impact (depending on height you
dropped your clay ball) - Angle of impact (depending on how far back you
were) - Size of meteor (depending on whether your clay
was 1, 2 or 3 pieces)
http//upload.wikimedia.org/wikipedia/en/c/c8/AS11
-42-6285.jpg
12Finish Collecting Data
- Collect your data
- Return all your equipment
- If you have finished your collection, you may
spend time with the resources
http//crism.jhuapl.edu/education/downloads/GUIDE_
Lesson2.pdf
13Analyze Your Data
- You collected 3 trials of a single variable, then
collected 3 trials of the next variable, and so
on. - Find the mean of each of your variables.
- Add three trials and then divide by 3
1.2 1.3 1.1 3.6 1.2
0.8 1.0 0.9 2.8 0.9 3.0
2.4 3.1 8.5 2.83
1.9 2.3 1.7 5.9 1.96
1.8 1.7 2.1 5.7 1.9 4.2
4.1 4.8 13.1 4.36
3.2 3.8 3.9 10.9 3.63
2.3 2.8 2.8 7.9 2.33 5.2
5.2 8.2 18.6 6.2
4.5 4.3 4.1 12.8 4.26
3.4 3.1 3.1 9.6 3.2 6.0
5.8 6.2 18.0 6.0
14Analyze Your Data
- First, lets look at how our data varies around
the mean
15Analyze Your Data
- Next, lets start picturing our data using
averages - Does this make sense?
16Analyze Your Data
17Analyze Your Data
18Conclusions
- What is your answer about the size, depth and ray
length as the velocity increases? - If you have any unusual data, give an education
guess what happened (most likely, human error)
19For This Lab
- Produce an 8½ x 11 or larger poster of this
experiment - Introduction Background on craters (tell me how
they are formed) - List your citations
- Methods Describe your experimental design
(include your hypothesis) - Results Include both a table and graph of your
data - Discussion Tell me what you learned
20Be Creative
21Have Fun
22What Did You Learn
23Include 4 Sections