Layers and Valley Networks By Nyan Cat: T. J. Kano Aery Kim Eunice Kim Mitsie Kim Hawon Koo Chandelle Pascual Valley Network Layers.

Slides:



Advertisements
Similar presentations
Changes to the Earth’s Surface
Advertisements

Channels By: Ryssa Asuncion Chance Kamaka Chance Kamaka Joshua Ramelb Joshua Ramelb Daisge Smith Daisge Smith
Rachelle A.~ Taylor B. ~ Alina N. ~ Aldrin O. ~ Brennen S. ~ Kit T.
HiRISE Image Targeting Challenge HiRISE (High Resolution Imaging Science Experiment) camera, orbiting Mars onboard the Mars Reconnaissance Orbiter, is.
Mars Activity Names: Ian Mecca and Robert Bell Howenstine High School, Mr. Martin, 9 th Grade, 4/18/07.
BY: Jared Flores | Zoe Garibay | Mia Iwanaga | Sabrina Martinez Jennifer Mills | Chandler Pascual.
Changes to Earth’s Surface Chapter 9
Martian Craters with Interior Deposits: Global Survey Results and Wind Model P21D-1875 Kristen A. Bennett 1 and Mark Schmeeckle 2 1 School of Earth and.
Modern Exploration Global Surveyor.  Objectives:  High resolution imaging of the surface  Study the topography and gravity  Study the role of water.
[Mars Polar Caps] By: Ryan and Reina. General Info About the Polar Caps Knowledge that the martian polar caps consist almost entirely of water ice goes.
PUT ON A HAPPY FACE The "Happy Face Crater" - officially named Galle Crater - puts a humorous spin on the "Face on Mars" controversy. This image was provided.
Yardangs on MARS!!! Period: 1 Big bang theory Amanda Hosino Christianne Jullian Jessica Luong Kelli Oyasato Leiala Okuda Megan Inouye-Ng.
Mars. Essential Points 1.Mars is about half the size of Earth 2.Mars has a thin carbon dioxide atmosphere 3.Mars has volcanoes and faults but no plate.
The Geology of Mars Flight into Valles Marineris.
What is inside Mars’ craters? Mary Dhel A., Mary Joy C., Aurelle D., Paul E., Paul G., Emlanta K., Jami K., Wisteria K., Taimane K., Shylo L., Ratu M.,
Streamlined Islands and Craters
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ Buried Glaciers at Mars Radar observations made from orbit reveal that nearly pure.
MARS ODYSSEY October 24, Thermal Emission Imaging System (THEMIS) Visible Imaging System –Visible-light images with 18 meters per pixel resolution.
This photograph shows channels in the sand on Mars and suggests that water created them. It also shows a picture if a water channel on Earth and the two.
Lesson4c Other processes on Mars. Dendritic (tree-like) drainage valleys EarthMars.
Looking at the Geology of Planets and Moons in Our Solar System PSC 121 Follow-up to Activity “Exploring the Geology of Several Worlds from Space”
Activity 4—Using Radar to Search the Darkness. Searching for clues… Mini-RF part 1 Mini-RF part 1 Mini-RF part 2 Mini-RF part 2.
Mars.  Focus Finding evidence of water on another planet. Using GIS to evaluate likelihood and determine best location.  Lesson Objectives Understand.
Study of bound water in the surface layer of Mars Workshop HEND-2002 “The First year of HEND operations on the NASA Odyssey Mars Orbiter” May 20-22, 2002.
Morphological Evidence for Water on Mars. Overview Pictorial comparison of features on Earth and Mars Gullies Alluvial fans Sedimentary layers Crossbedding.
JPL/NSTA Web Seminar: Inquire, Engage and Explore: The Mars Student Imaging Project LIVE INTERACTIVE LEARNING.
ASTRONOMY 340 FALL October 2007 Class #9. Salient Martian Features  R Mars = 3396 km (R Earth = 6378 km)  Higher surface area to mass ratio 
Early Spacecraft Exploration Early Spacecraft Exploration Mariner 3 & 4  “…these missions are being undertaken because Mars is of physical.
Mapping the Surface of Mars NOAO Science Education Group and Chris Martin from Howenstine Magnet High School.
LIVE INTERACTIVE YOUR DESKTOP December 19, 2011 Electromagnetic Spectrum: Remote Sensing Ices on Mars Presented by: Rudo Kashiri.
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
NASA’s Exploration Plan: “Follow the Water” GEOLOGY LIFE CLIMATE Prepare for Human Exploration When Where Form Amount WATER NASA’s Strategy for Mars Exploration.
“28 Seconds To Mars” Joshua Basuel, Makamae Caballero, Alyssia Fields, Marishell Gacuya, & Mark Kitano- Maguire Pd.6 Created by: Makamae Caballero.
Wind streaks Bibliography for Google images on windstreask Brooke Chinen, Graham Gibson, Howard Robinson, Justin Boin, Tamaria McDonald, Tyler Jordan Lacar.
1 There’s lots of evidence for water on Mars…in the past River beds and teardrop-shaped “perched” craters. Lake beds Minerals have been found that only.
Shaping Earth’s Surface
Interlude  Viking mission operations ended in the early 1980s  Viking missions gave scientists the most complete picture of Mars to date. What does this.
By: Calvin Arroyo, Alicia Bell-Reid, Nicholas Manago, Levias Peterson, Jorden Takushi & Taylor Torres
Age Estimation on Mars: Using Digital Surveying of Impact Craters
C.M. Rodrigue, 2014 Geography, CSULB Mars: Fourth Order Landscapes Geography 441/541 S/14 Dr. Christine M. Rodrigue.
Bradley Central High School
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ What Carved Martian Gullies? ‘Gullies’ are channels carved when material moves downhill.
Mission to Mars What to look for when you get there A Collection of Basic Earth Analogs.
Mars Science Laboratory 1st Landing Site Workshop Pasadena, CA — 31 May – 2 June Fine-layered Meridiani crater for the MSL Landing Site L. V. Posiolova,
Happy Halloween!. Homework #6 Due 6:00 pm today Exam #2 on Wednesday.
BACKGROUND MARS Research Presentation By Bradley Central Chemistry 3 rd Period Dr. Buckner.
Where are the longest wind streaks located on Mars? (The strongest winds on Mars) Why is your science question important? Why is your science question.
THE SOLAR SYSTEM By Reagan Herbek. The Inner Planets The inner planets are the four planets closest to the sun. They include: Mercury, the closest planet.
Mars Images How We Know What We Know Current Spacecraft Mars Odyssey (’01-present) Mars Express (’03-present) Mars Exploration Rovers (’04-present) Mars.
Yardangs Little dippers Audrey Mumford Allee Miral Darrian Lambert Micah Chang Taijah Jones Tyler Hauser Period 4.
Lakewood High School Mars Student Imaging Project MSIP.
Mars Student Imaging Project MSIP
Does the dark sand cascades area appear earlier in the year when the Sun has increased activity, especially more X-flares? Science Question This question.
By: Jacob, Chad, Breana, Kayla, Micah, Nick
Chapter Menu Lesson 1: Reading Maps
1.2: Observing the Surfaces of Mars and Earth
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
Early Exploration Mariner 3 & 4
Using Earth for Planetary Comparisons
Comparing Mars to Earth
4th period chemistry Dr.Buckner
Early Spacecraft Exploration
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
Earth vs. Mars Comparison
Surface Features on Mars
Yardang Investigation
Earth Science Jeopardy GA’s Landforms Changes to
Chaotic Terrains And Channels
During its two-year primary science mission, the Mars Reconnaissance Orbiter will conduct eight different science investigations at Mars. The investigations.
Earth.
Presentation transcript:

Layers and Valley Networks By Nyan Cat: T. J. Kano Aery Kim Eunice Kim Mitsie Kim Hawon Koo Chandelle Pascual Valley Network Layers

Research Question Aery, Hawon, Chandelle, TJ How are layers and valley networks related? Why is your science question important? Why is your science question important? We think it is important because they both relate to certain things (possibly) and how it relates to Mars today. Why is your science question interesting? Why is your science question interesting? It is interesting because it combines our group’s two main ideas that we wanted to do.

Background Information Layers Valley Networks

Background Information Layers Layers are formed by dust particles and water sediments piling on top of each other pressing down on each other because of its own weight. Over time, the layers got thicker and thicker. A Picture of a layer Aery, Eunice, Mitsie, T.J., Chandelle, Hawon

Backround Information Valley Networks Valley networks maybe formed by recurrent floods during a long period when the Martian climate may have been much like that of some arid or semiarid regions on Earth. Valley networks maybe formed by recurrent floods during a long period when the Martian climate may have been much like that of some arid or semiarid regions on Earth. Valley Networks

Background Information Other Information It is thought that valley networks were run by ground flows instead of rain, like the ones on Earth is. It is thought that valley networks were run by ground flows instead of rain, like the ones on Earth is. Layers are found usually near polar ice caps and is not commonly known (as a topic). Layers are found usually near polar ice caps and is not commonly known (as a topic). Hawon, Chanelle

Hypothesis Mitsie, Aery, T.J., Eunice, an Chandelle’s hypothesis: Mitsie, Aery, T.J., Eunice, an Chandelle’s hypothesis: If there are many samples of layers, then by looking at pictures of layers to see if there are valley networks, it will show that the layers were made by the valley networks because the water would flow from the valley networks and create layers.

Methods Spacecraft NASA’s Mars Odyssey Camera THEMIS Camera Image Type Visible Images-to see details within the crater MOLA-to see context of image and depth Geologic Features Studied How are layers and valley networks related? This relates because we have to look at the geologic features on layers and valley networks This relates because we have to look at the geologic features on layers and valley networks Geographic regions we focused on All parts of Mars with layers Themis Camera

Methods continued Sample Size 61 THEMIS Images used to gather data Categories of Data to be collected and “Why” Image ID#- To see if it was a duplicate images Latitude/Longitude- To know where to graph it and know where it is located Misc. data- To record other interesting information not warranted by necessary data categories but certainly important to our study Features- To see if valley networks are nearby Measurements Picture Diameter- Rough estimation relative to image parameters based on THEMIS Camera’s Visible Image range of 18km x 30km

Methods Continued Website List: Website List: 1. website; 2. Search “layers” 3. Click on pictures of “layers” 4. Log Latitude,Longitude 5. Log any other features 6. Log image #

Data

Data Image#LatitudeLongitudeFeatures V Wind streaks &preserved craters V Craters &sand dunes &mountains &chaotic terrain N/A Chaotic terrain &modified craters V Crater

N/A Chaotic terrain N/A15.8 S210.2Craters, Channels and streamlines N/A Channels &craters N/A Chaotic terrain N/A Chaotic terrain

V Chaotic Terrain V Chaotic Terrain V Destroyed Craters Hebes Chasma Canyons &Landslide V Dust devil Tracks

V Craters V Craters, Chaotic Terrain &Dust devil tracks V Dust devil Tracks Craters V Destroyed Craters

V Dust devil Tracks V Destroyed Craters &Mountains V Modified Craters V Windstreaks &Destroyed craters N/A-8097Modified Craters

V Thin Coating of dust V N/A V Modified Craters V N/A V Sand Dunes

V Wind streaks V Destroyed Craters V Wind streaks N/A Preserved &Modified Craters V Modified Craters &Sand Dunes

V Wind streaks &Modified Craters V Preserved Craters &Wind streaks V Polar Ice Caps V Sand Dunes V Clouds

V Ice Caps V Landslide V ONLY LAYERS V Small Dunes &basaltic Sands V Destroyed Craters

N/A V N/A V Sand Dunes V Landslide V N/A

V Sand Dunes V Landslide N/A Sand Dunes V Chaotic Terrain V N/A

V N/A V N/A -8097Craters &Chaotic Terrain V Mountains V Preserved Craters

V Landslide &Craters V Craters &Canyons

Discussion

Discussion This data chart is a bar graph which tells us the amount of each sixteen geological features near layers. About half of the sixteen features are below three and the rest are above- craters being the highest with the amount of about thirty. There were five features that showed up only once.

Discussion This graph is a scatter plot, showing us the 60 locations of layers. This graph shows the latitude and longitude of layers we have found. We’ve figured out that most layers are on the edges of the MOLA Map and the latitudes are usually ranging from negatives to positive 80’s. The longitude is mostly positive going up to more than 300 and there are no negatives at all.

Bibliography Baldwin, Emily. " Episodic Not Catastrophic Flooding on Mars." Astronomy Now Online. 11 Sept Web. 20 Nov Baldwin, Emily. " Episodic Not Catastrophic Flooding on Mars." Astronomy Now Online. 11 Sept Web. 20 Nov "Layers of Mars." NASA Science Web. 23 Nov "Layers of Mars." NASA Science Web. 23 Nov Dickinson, David. "May 2009 News and Notes." Astro Guyz. Genesis Frame, Education Theme, 1 May Web. 29 Nov Dickinson, David. "May 2009 News and Notes." Astro Guyz. Genesis Frame, Education Theme, 1 May Web. 29 Nov Layers-Period 2 (typo): Layers-Period 2 (typo): "Mars Global Surveyor MOC2-262 Release." Space Cameras, Operations, and Science - Malin Space Science Systems. Malin Space Science System, NASA, 4 Dec Web. 01 Dec "Mars Global Surveyor MOC2-262 Release." Space Cameras, Operations, and Science - Malin Space Science Systems. Malin Space Science System, NASA, 4 Dec Web. 01 Dec Valley Networks: Valley Networks: "An Odyssey Of Mars Science: Part 3." Space News From SpaceDaily.Com. 18 Dec Web. 01 Dec "An Odyssey Of Mars Science: Part 3." Space News From SpaceDaily.Com. 18 Dec Web. 01 Dec VN: VN: "MARSIS." CO.RI.S.T.A. Ed. Stefania Mattei. Consorzio Di Ricerca Su Sistemi Di Telesensori Avanzati. Web. 01 Dec "MARSIS." CO.RI.S.T.A. Ed. Stefania Mattei. Consorzio Di Ricerca Su Sistemi Di Telesensori Avanzati. Web. 01 Dec mars_layers...: mars_layers...: Riding with Robots: Archive. NASA, 23 June Web. 1 Dec "Mars Global Surveyor MOC2-262 Release." Space Cameras, Operations, and Science - Malin Space Science Systems. Malin Space Science System, NASA, 4 Dec Web. 01 Dec "Mars Global Surveyor MOC2-262 Release." Space Cameras, Operations, and Science - Malin Space Science Systems. Malin Space Science System, NASA, 4 Dec Web. 01 Dec