By: Jacob, Chad, Breana, Kayla, Micah, Nick

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Presentation transcript:

By: Jacob, Chad, Breana, Kayla, Micah, Nick Lava Flows on Mars By: Jacob, Chad, Breana, Kayla, Micah, Nick http://www.hoax-slayer.com/images/mars.jpg

Research Question Why is our Question Important? How will scientist benefit from this information? http://www.wired.com/images_blogs/photos/uncategorized/2008/03/18/mars_volcano.jpg

Research Question How far does lava flow from the volcanoes on Mars? We think our research question is important because it would determine how far the lava will flow whenever a volcano erupts. This will benefit scientist because it will determine how Mars grows and at what rate. http://www.wired.com/images_blogs/photos/uncategorized/2008/03/18/mars_volca no.jpg

Hypothesis

Hypothesis Group’s Hypothesis: The size of the volcano will determine how far the lava flows. For example if the volcano is big the lava flow will be big as well.

Background Information http://www.solarviews.com/raw/mars/olympus.jpg

How are volcanoes on Mars Formed? From countless eruptions overtime the lava creates layers of rock over and over and creates a large crater where the lava erupts from

Background information Mar’s has the largest shield volcanoes in the solar system. Volcanism occurs mostly within three regions of Mars these regions are Tharsis, Elysium, and the Hellas. Mars has a wide range of volcanic features. These volcanic features include large volcanic cones, unusual Patera structures, mare-like volcanic plains, and a number of other small features. Volcanism on Mars is very old. The most biggest volcanoes are located on huge uplifts or domes in the Tharsis and Elysium regions of Mars. Olympus Mons is the largest volcano in the Tharsis region. The Martian Volcanoes flows are much larger then terrestrial volcanoes

Background Information (cont.) Inside a volcano there is a pocket of magma beneath the surface and one or more cracks through which the magma forces its way out. The magma moves upward through a pipe or a long tube in the ground that connects to the magma chamber to the earths surface A lava flow is the area covered by lava as it pours out of the vents When a volcano erupts, the expanding gases pushes the magma from the magma chamber throughout the pipe until it explodes out

Methods

Methods Volcanoes and lava flows NASA’s Mars Odyssey THEMIS Camera 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 Volcanoes and lava flows Geographic regions we focused on All of Mars

THEMIS image is 18 km by 63 km we estimated the length Methods (continued) Sample Size We have 58 images total Categories of Data to be collected and “Why” THEMIS Image ID: this tells you exactly which image that is on Mars Latitude and longitude: We need them to describe exactly where a point is on Earth. Length of Lava Flow: We will need to use this information to determine the length of the lava flow from a volcano MISC. Observation: this shows some other characteristics the image had such as craters or channels. Measurements THEMIS image is 18 km by 63 km we estimated the length Of the lava flow.

Data Observations V27050006 258.8 -16.4 17 KM Craters in lava 257.3 14.5 18 KM Looks like tubes I03887002 242 -20 26 KM Destroyed Craters V11204010 147.2 24.3 Volcano V27100006 240.8 -21.1 63 KM Rocky Terrain V21995010 250 16 65 KM V05473001 248 17 64 KM Little Craters V101539002 159.711321 -20.123457 240km half of big craters on side V012267007 140.9 35.2 stream in middle one large line of lava in center

Data Observations cont. I07900011 243.5 -5.6 .1KM Very Clear VO5249002 207.6 -9.7 .O2KM Wind Streaks I03912002 241.9 -19.7 .1KM Craters V2453002 237 -8.3 .02KM Looks Like Desert V27773025 4.95 254.5 0.017 canyons and trenches near volcano V22171022 13.5 222.4 0.018 Whole area coverd in lava flows V19288013 227.6 16.1 0.018 Small crater in middle V05485002 240.9 -19.4 0.017 One crater and lava flows V07245501 246.2 -0.88 0.017 Carters and huge lava flow V11377001 221.8 -2.39 0.52 layers with lava flows V05908003 257.3 16.82 0.018 Craters with ejecta blanket V11085015 337.7 8.65 0.017 Layer near destroyed craters

Data Observations cont. V07881023 236.4 2.4 64km lava layers V03687003 226.9 18.2 66km lava streaks V27773025 254.6 4.9 65km mini volcano V1570001 242.9 -20.3 63km Big crater V03949003 255.8 -13.2 0.069431km Channels V05483002 240.1 -19.4 0.018516km has dust devils T25465002 264.7 -12.7 .1KM Channels VO3949003 255.8 -13.2 .1KM Channels V05483002 240.1 -19.4 .O2KM Dust Devils V20561007 226.3 15.9 .02KM Wind Streaks V05095012 305.18 29 .02KM Channels V06312021 126.8 19.5 .02KM Cracks

Mola Mars Map

Length of Lava Flow

Conclusion What did your group learn from the data collected? We learned that the average amount and the most common length of lava flow is around 18km. What would you do differently to make your investigation better? I would maybe take a better scale of the volume of the volcanoes so my answer would be more wholesome. Explain what scientific questions could branch off of this study to further scientific research about mars. Some scientific questions that could branch off of our research are “ Where are the safe areas in Mars?” This question could branch off of our study because obviously the areas with lava will kill you.

Bibliography http://www.solarviews.com/eng/marsvolc.htm http://volcano.oregonstate.edu/volcanoes/planet_volcano/mars/Overview.htm