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By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero, Aija Blue, Kristian Yap.
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By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

Apr 01, 2015

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Page 1: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero, Aija Blue, Kristian Yap.

Page 2: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

“Our research question is important because Ejecta may be a geological feature related to water, and by figuring out the location of rampart Ejecta craters, we may discover where the most rampart craters are located.”

The importance to finding out our research question is because we want to find where exactly or where is the closet spot that rampart craters hit. By this we can find out why they hit?, their impact, and what is the Ejecta made out of?.

space.y2u.co.uk/Photo/Picture_Solar_System.jpg

Page 3: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

blogs.coventrytelegraph.net/thegeekfiles/ufo.jpg

In our group we came up with a hypothesis that we all agreed on.

In our group we all said that if the bottom of Earths atmosphere is cold then so must Mars’ atmosphere be cold there for if the Rampart Craters Ejecta is made out of ice it may hit the bottom because of the coldness.

We could go into further information such as if Mars’ has some type of rotation exactly like Earth then the Sun would hit some what the same way as how it hits Earth because the reflection of sun light.

Page 4: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

www.galaxyimages.com/moon8.jpg

We think our research question is important because we can find out if life on Mar’s is actually possible.

I Hope there is life on Mars’!

Page 5: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

www.astronomy-blog.com/.../9-2007/mars-9810.jpg

*Rampart craters are formed by impact and liquid

*It has a special Ejecta that looks like a flower when it hits on the surface of Mars.

*The reason why scientist think that there is water on Mars is because the Ejecta is supposedly made up of frozen water.

Page 6: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

By Impact

Either by asteroid,

meteorites,

comets

The transfer of the Meteorite strikes

on to the surface.

After impact it may cause a

flower type that is called an Ejecta

Deposition of platesboundaries

Then……..BOOM!A crater is formed!

This is how craters are formed and

what happens after impact.

Page 7: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

Space Craft Themis Camera

Camera THEMIS Camera

Image Type Visible Images- to see details within the craterMOLA- to see context of image and depth

Geologic Features Studied

Crater types and the presence of Rampart Craters within the crater to answer our question, “so , Where are the most Rampart Craters are located? “

Geographic regions we focused on

http://www.allbestwallpapers.com/computer-mac_x_leopard_space_wallpapers.html

Page 8: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

http://www.allbestwallpapers.com/computer-mac_x_leopard_space_wallpapers.html

Sample Size Themis images used to gather data.

Categories of data to be collected and “why” Image Id#- Keep track of the specific image analyzed.Latitude/longitude- keep track of location and their proximityMisc Data- to record any other interesting into not warranted by our necessary data categories but certainly important to our study.

Measurements Rough estimation relative to image parameters based on THEMIS camera visible image range of 18km

Page 9: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

Sample Size Themis images used to gather data.

Categories of data to be collected and “why”

Image Id#- Keep track of the specific image analyzed.Latitude/longitude- keep track of location and their proximityMisc Data- to record any other interesting into not warranted by our necessary data categories but certainly important to our study.

Measurements Rough estimation relative to image parameters based on THEMIS camera visible image range of 18km

Page 10: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

Themis Image ID Longitude Latitude Crater Type Ejecta Observations

V125835006 24.990547 -50.946266 Modefied 0 it looks sort of new

V27741031 97.19646 1.125312 Modefied 0 Crater is starting go away

V29739009 59.73448 36.846558 Modefied 0 Half of crater is gone

V07909002 175.4821 -14.579002 Modefied 0

V26781003 307.48706 46.746387 Modefied 0

V07749004 107.11201 -30.916529 Modefied 0 LOTS OF CANYONS

V07405003 307.20694 -34.140217 Modefied 0

V07450004 84.7302 -57.48426 Modified 0 CALM SURFACE

V25479007 72.49171 26.56626 Modified 0 craters is forming

V28283015 65.44393 46.746387 Modified 0 a lot of details in the crater

101539002 275.9255 -30.201267 modified no Channels and many small craters

V28834009 246.54414 17.275997 Modified no Lava Flows

V28683012 291.92386 63.618855 modified no One big crater

V26781003 100.26607 -10.072057 modified no One Dark Slope streak

V27555023 69.932816 45.251007 Modified NO One modified crater

V27741031 97.19646 1.125312 Modified NO Lumpy cratersV29739009 59.73448 36.846558 Modified NO Old craters

Page 11: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

I08658002 175.73853 -13386349 Destroyed 0

V02304003 175.6335 -15.30991 Destroyed 0

I03028002 176.224 14.519147 Destroyed YES

V27189024 187.8202 39.948097 Destroyed 0 Crater is broken

V27086631 279.55432 41.016296 Destroyed 0 Crater is almost gone

V32945001 74.15295 -27.47532 Destroyed 0 Crater is almost gone

V27555023 69.932816 45.251007 Destroyed 0 Crater is broken

V04582011 338.43616 24.356598 Destroyed 0 LOTS OF PRESERVED CRATERS

V07658005 211.70448 -29.652924 Destroyed 0 GULLIES,CHANNELS

V26695024 5.792714 11.019984 Destroyed 0 crater is destroyed

v28683012 291.92 63.61 Destroyed 0 Gullies

v28632014 318.38 44.037 Destroyed 0 Collapsed Lava tubes

V27021044 349.50726 4.981852 Destroyed No Dunes

V28283015 307.48706 46.746387 Destroyed No One Huge crater

V28479007 49.54766 26.516626 Destroyed NO Dark Slopes

Page 12: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

v28479007 49.64 26.51 Preserved Yes

V28834009 246.54414 17.725997 Preserved 0 The crater is a full circle

V01605003 174.74019 -14.731401 Preseved 0

V02691003 175.04747 -14.726359 Preserved 0

I04963002 175.0108 -12.414344 Preseved 0

V0496586 174.7492 -13.946566 Preseved 0

V010580003 175.79373 -14.4756 Preserved 0

V01243002 175.21605 -14.816523 Preserved Yes

V26781003 100.26607 10.072057 Preserved 0

V07742002 309.30127 -28.964914 Preserved 0 NONE

V07798008 132.54744 -40.325314 Preserved 0 CHAOTIC TERRAIN

V07404005 334.90967 -41.13456 Preserved 0 LOTS OF BLACK DOTS

V28632014 318.38208 44.037617 Preserved no many small craters in a group

V27086031 279.55432 41.016296 Preserved no collapsed features

V27189094 187.8208 39.948097 Preserved YES 1 big ejecta on one of the preserved crateres

V25483003 81.21938 -14.4283 Preserved YES 1 big ejecta on one of the preserved crateres

V10947001 26.167135 -8.060469 Preserved & Modified YES Ejecta looks faded

V33072002 -23.451626 9.823448 Preserved YES Lots of preserved craters wwith ejecta

V32945001 74.15295 -27.47532 Preserved NO There was channels

V01256001 63.340282 10.882847 Preserved YES Only one ejecta was found

Page 13: By: Jordan Alejo, Brandon Bersola, Lauren Bonga, Raquel Crawford, Michael Gray, Matthew Juntilla, Bryson Miyasato, Zachary Mon, Hugo Nimoto, & Mervin Obrero,

V27189024 187.82 39.94 Rampart 0 bumpy

V27086031 279.55 41.0162 Rampart Yes Channels and craters

V2883409 246.544 17.27 Rampart 0 Smooth

V26781003 100.266 -10.07 Rampart Yes Bumpy

v27021044 349.5 4.981 Rampart 0 Dust Devil

v28283015 307.487 46.746 NONE 0

v26695024 35.364 11.0199 NONE 0 Bumpy