Mars Mapping Mission St Joseph School Mr. Serra’s 7 TH Grade 4/19/2007 Presenter: Ms. Batchelder.

Slides:



Advertisements
Similar presentations
The Terrestrial Planets
Advertisements

Ch. 29 Sec. 2 Terrestial Planets. First four  Mercury, Venus, Earth, Mars  Solid, Rocky surfaces.
Mars Activity Names: Ian Mecca and Robert Bell Howenstine High School, Mr. Martin, 9 th Grade, 4/18/07.
WHY GO TO MARS Mars Base Mission Day 1. MARS AEROGRAPHY Mars is the 4 th planet from the sun. Mars is the 4 th planet from the sun. Water once flowed.
Mars. Some similarities between Mars & Earth Mars’ Bulk Properties Mars has days & seasons like Earth.
Class 3 : Craters in the solar system. Recap last class… Patterns in the solar system. Theory for solar system formation. How do we test this theory? Variety.
Our Country’s Geography
All About Volcanoes. Volcanoes can be quite scary, especially if they erupt when you least expect it! But what actually causes a volcano to form? Although.
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”
Landforms on Earth. What are Landforms? Landforms are Earth's physical features. The following are examples of Landforms: Volcanoes, Mountains, Valleys,
Earth’s surface has many natural shapes, or features called
Comparing the Sun, Earth, and Moon
Red Planet Mars Chapter Thirteen. Guiding Questions 1.When is it possible to see Mars in the night sky? 2.Why was it once thought that there are canals.
Chapter 6, Section 4 Volcanoes in the Solar System
Planet Highlights. Mercury Mercury Highest DensityHighest Density Thinnest AtmosphereThinnest Atmosphere Highest Temperature and Greatest Temperature.
Mars The latest mission to Mars touched down on the 6 August It is called the Mars Scientific Laboratory otherwise known as, Curiosity. This is a.
First Grade Science and Social Studies
Whenever you see me, click on me to learn more!
What are landforms?.
Fourth Grade Science and Social Studies
Landforms are the natural shapes or features of the land. There are many different types of landforms found on Earth.
Erupting Volcano Anak Krakatau. Is this a mud volcano on Mars? If so, could it be dredging up martian microbes? This strange possibility has been suggested.
The Inner Planets. The terrestrial planets 1.Mercury 2. Venus 3. Earth 4.Mars.
Third Grade Science and Social Studies
Our Solar System.. Astronomical unit is the distance between the Earth and the Sun X 10.
Volcanoes  Volcanoes form at weak spots in the Earth’s crust.  Magma is a molten mixture of rocky substances. It forms within the Earth in the Magma.
 Numerous amount of people have searched the ocean’s floor for many years  Although it has been explored there has been much that is still needed to.
In your table of contents…
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
Image Courtesy of NASA/JPL-Caltech.  Known to Babylonians 3,600 years ago as “Star that Wandered”  The Greeks referred to it as “Ares” the god of War.
W6 BY: Antonio, And Max Howenstine High School, Mr. Martin 6 th period class, 9 th grade, 4/20/07.
Mars Student Imaging Program The Three Principles Impact Craters Features you must know and understand. Ejecta – Material, from the crater, that was thrown.
Chapter 10 Mars. Mars’s orbit is fairly eccentric which affects amount of sunlight reaching it 10.1 Orbital Properties.
About The second planet from the Sun in the Earth's solar system. Venus has been know for millions of years. The planet Venus has long been one of the.
Landforms. A mountain is a landform higher than the land around it. Mountain.
Changes to Land. Landforms Features on the surface of the earth such as mountains, hills, dunes, oceans and rivers.
Astronomy 1010-H Planetary Astronomy Fall_2015 Day-29.
BY: KA’VARYA MCLAUGHLIN, INDICA MOSLEY, SAVANAH OZUNA.
Mission to Mars What to look for when you get there A Collection of Basic Earth Analogs.
Surface of the Red Planet. A reminder… we are looking at a smaller planet than the Earth.
CHAPTER 1.4 – EARTH’S MOON. IMPORTANT FACTS The first person to truly see the surface of the Moon was Galileo in Galileo used a compound telescope.
Space On Mars Reach Mars is the fourth planet  from the sun  and the second smallest planet in the S. Named after the Roman god of war it is often described.
SCIENCE REVIEW JAN A delta, the landform found at the mouth of a river, forms when - A. plants on the river bank cause erosion B. the river deposits.
Astronomy 1010 Planetary Astronomy Fall_2015 Day-29.
The Surface of the Moon. Surface Surface: The top or outside of something.
BACKGROUND MARS Research Presentation By Bradley Central Chemistry 3 rd Period Dr. Buckner.
The Mysteries of Mars Carlos, Chloe, Maria, Marisol, Melina and Oscar Utterback Middle School Ms. Copeland 6 th grade 4/19/07.
Exploring Geology on Earth and Mars Unit 2 By Jad Gaytan.
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.
Unit 11 Mars. Physical Properties Radius: 3400 km Moons: Deimos, Phobos Mass: 6.4 × kg Density: 3900 kg/m 3 Length of Day: 24.6 hours.
On the Surface of Mars Alma, Garron, Ivan, Paige Utterback Middle School Ms. Diana Ochoa and Ms. Deborah Copeland 6 th Grade 4/19/07.
Mars Presentation Angel, Bryan, Hayley, Alicia, Aarian, Jennifer, Imelda, Ben, Arnulfo, Yessica Utterback Magnet Middle School Ms.Ochoa 6 th grade April.
© 2010 Pearson Education, Inc. Chapter 9 Planetary Geology (abridged): Earth and the Other Terrestrial Worlds.
Organization  Our Solar System consists of: Comets orbiting the Sun Asteroids orbiting the Sun Planets orbiting the Sun ○ Moons orbiting the planets.
Oceanic -- Continental Match-Up. Abyssal Plain Continental shelfOce\ basin Continental Shelf The edges of the continents slope down from the shore into.
1.2: Observing the Surfaces of Mars and Earth
(Lots of pretty pictures. No math.)
Third Grade Science and Social Studies
Orbital and Physical Properties
VIRTUAL FIELD TRIP Physical Processes of Earth’s Surface
Planet Highlights.
Whenever you see me, click on me to learn more!
Comparing Mars to Earth
Planet Highlights.
6th Grade PBL Colonizing a Planet
Fourth Grade Science and Social Studies
Landform Notes.
This lesson will introduce some of the major kinds of landforms.
Continental Landforms
Science and Social Studies
Presentation transcript:

Mars Mapping Mission St Joseph School Mr. Serra’s 7 TH Grade 4/19/2007 Presenter: Ms. Batchelder

The most interesting result(s)we found from doing the activities We found there were impact craters, and volcanoes. We tried to estimate how old they were. We were surprised to find Earth-like features, as well as strange, weird formations. We found these results by evaluating the pictures. The method that we used was visual observation.

Olympus Mons

Results from the Part 2 Activity (with the HiRise Data) We found many interesting items like Impact Craters, Mountain Ranges, Volcanoes and River Beds. We found these results by studying the photographs carefully. It was hard to see the landforms sometimes. Were they raised or depressed? We used the method of Visual Observation to get our results. We think the craters were formed by meteors hitting the red Martian surface. We believe some mountain features and canyons were made by lava flows and liquid surface flows.

More Results from the Part 2 Activity (with the HiRise Data) Comparing Earth features with other features on Mars and/or to features on the Earth we see Volcanoes, Flowing River Beds, Deep Canyons and Titanic Mountains. Our Conclusion is that these features are similar because we have lava flows and volcanic eruptions on Earth. But we lack the many impact craters the red martian planet has.

Next Steps We don’t believe our site is a good place to land because there seems to be a very uneven surface with lots of mountains, crevices, and craters. We would like to know the type of terrain. Is it rough and rocky, sandy, or fairly stable? We would need to know this in order to evaluate a possible site. Our criteria for selecting a landing site would be mainly, a stable, flat surface. Our goal for sending a mission to Mars, would be to find out more about the planet, and search for evidence of water and life.

Continued… Based upon our observations, we would like to study the features that seemed to have been formed from interaction with water. These would include the bottom of canyons, and areas that seem to have been made by water. These areas look like dry arroyos or riverbeds.