Walter S. Kiefer Lunar and Planetary Institute

Slides:



Advertisements
Similar presentations
© 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Advertisements

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.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 10.
Mercury = 5.4 g/cm 3 (Earth 5.5 g/cm 3 ) = 0.38 that of Earth Mass Radius Density Gravity = 3.3 x g = M Earth  = 2439 km = 0.38 R Earth Semimajor.
Interiors of Terrestrial Planets. Mercury MEAN RADIUS: km MASS: (Earth=1) DENSITY: 5.43 (g/cm^3) GRAVITY: (Earth=1) ORBIT PERIOD:
Mars. Some similarities between Mars & Earth Mars’ Bulk Properties Mars has days & seasons like Earth.
Mars Basics. Size & Distance Smaller than Earth (0.532x) Mars diam ~ 6779 km (4212 miles) Earth diam ~ 12,742 km (7918 miles) 8 Mars would fit inside.
Information of Mars Mars is the fourth planet from the Sun and is commonly referred to as the Red Planet. The rocks and soil have a red or pink hue due.
The Terrestrial Planets, Part III Mars. MARS The God of War.
M ARS By Danny and Kenny. W HAT IS M ARS ? Mars is the fourth planet in the solar system. It’s nick named the “Red Planet” Reddish in color Named after.
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.
Chapter Four The Moon: The Earth’s Closest Neighbor.
Your about to see a slide show of “Mars” By: Lindsey and Haley!
Early Spacecraft Exploration Early Spacecraft Exploration Mariner 3 & 4  “…these missions are being undertaken because Mars is of physical.
Observing Mars By Brad Jarvis. Overview Basic facts Orbits and distance Viewing Mars from Earth The view from space Current exploration Conclusion References.
Mars – The Last of the Inner Planets. Comparison of Mars and Earth in their correct relative sizes. Mars (diameter 6790 kilometers) is only slightly more.
1 Inner or Terrestrial Planets All the inner planets formed at the same time. Their composition is also very similar. They lack the huge atmospheres of.
MARS By: Charanjit, Richard & Cesar.
Bell Work: What is the name of the man who first invented the rocket? What are the names of the first four planets? What is the special name given to these.
The Inner Planets 20.3.
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.
The Solar System a1 Mercury Sun Venus Earth Mars Asteroids Jupiter Saturn Uranus Neptune Other objects Observe our solar system Four inner planets.
MARS. Where is Mars? 4 th planet in our solar system. Last of the rocky planets. Our solar system is in the Orion arm of the Milky Way Galaxy. Our sun.
Mars Monroe. Mons Olympus. Bigger than most states.
Chapter 10 Mars. Mars’s orbit is fairly eccentric which affects amount of sunlight reaching it 10.1 Orbital Properties.
Mars The Red Plant Mars is the fourth planet from the sun and the second smallest planet in the solar system. Named after the Roman god of war, it is often.
MARS.
Mars Images How We Know What We Know Current Spacecraft Mars Odyssey (’01-present) Mars Express (’03-present) Mars Exploration Rovers (’04-present) Mars.
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.
27-3OBJECTIVES Identify the basic characteristics of the inner planets. Compare the characteristics of the inner planets. Summarize the features that allow.
Surface Features of Mars. General Features Mars is a Desert World. Its surface is dominated by desert terrain dotted with Volcanoes and Craters. There.
Planets. The terrestrial planets and some large moons.
Curiosity Curiosity pictures Rover view Old Rover View form older rover.
Mars.
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
Exploring Mars.
Mars eccentricity = Mass = 0.11 MEarth
The Inner Planets.
© 2017 Pearson Education, Inc.
Week 3 Week January Out 18th Mars, Jupiter, Saturn.
THE INNER PLANETS.
Mars.
Early Exploration Mariner 3 & 4
Mars.
Lecture 12: Planetary Geology
Section 3 – pg 552 The Inner Planets
Planet Highlights.
A Report in Natural Science I
The Inner Planets.
Exploring Mars: The Inside Story
The Inner Solar System.
Planet Highlights.
Early Spacecraft Exploration
PLANET MARS Presented By: Samia Amir & Tauseef Saeed NCBA & E
Ask students which planet this is and ask them to name features they see in the image, e.g. clouds, water, etc.
All The Planets.
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
This imaginative painting shows a possible future human settlement on ___________. Settlers might live in domes to protect themselves from the harsh climate.
The Inner Planets of Our Solar System
Surface Features of Mars
Section 1: Earth’s Moon.
Craters on Mars Many craters Closer to asteroid belt No water erosion
The Solar System.
Information of Mars Mars is the fourth planet from the Sun and is commonly referred to as the Red Planet. The rocks.
The Inner Planets of Our Solar System
Lecture 12: Planetary Geology
Surface Features of Mars
Stephen Eikenberry 21 Feb 2019 AST 2037
Presentation transcript:

Walter S. Kiefer Lunar and Planetary Institute Next Stop: Mars! Walter S. Kiefer Lunar and Planetary Institute

Earth and Mars Earth and Mars at the correct relative size. The Earth view is of Africa (top) and Antarctica (bottom). Note the predominance of water, ice, and clouds on Earth, and the virtual absence of water on Mars.

Basic Facts about Mars Diameter: Mars Day: Mars Year: Mass: Gravity: Atmosphere: Atmospheric Pressure: Surface Temperature: 6,794 km (53% of Earth) 24 hours 37 minutes 687 Earth days 11% of Earth 38% of Earth 95% Carbon Dioxide < 1% of Earth at sea level -125 to +20 Celsius The image on the left is from the Hubble Space Telescope in 1999. Note the large storm system near the North Polar cap (1600 kilometers, or 1000 miles across).

Giant Volcanos Many of the geologic features on Mars occur on a very large scale, a fact that often fascinates school children. This three-dimensional perspective view shows the martian volcano Olympus Mons. It is the largest volcano known in the Solar System, at 640 kilometers (400 miles) across and 22 kilometers (14 miles) high.

Valles Marineris Valles Marineris is a giant trough on Mars, more than 4000 kilometers (2500 miles) long and up to 10 kilometers (6 miles) deep. It is long enough that it would reach from California to Washington D.C. on Earth! Valles Marineris formed in the middle part of martian history, roughly 2.5 to 3.5 billion years ago, when forces in the crust of Mars stretched the surface and created massive faults, resulting in the deep valley that crosses the center of this image.

An Impact Scarred Surface This image shows the Argyre impact basin, 1850 kilometers (1150 miles) across and 5 kilometers (3.1 miles) deep, which formed by the impact of a large asteroid or comet.. It has a deep, relatively smooth floor and is surrounded by a high, rough blanket of ejecta. Ejecta is the material which was blasted out of the basin by the impact and lands in the area surrounding the impact crater or basin. The Argyre basin probably formed around 3.8 to 4 billion years ago. Numerous smaller impact craters are also seen in this image.

Ancient Floods The surface of Mars has been scoured in many places by giant floods of water. This image shows Ravi Vallis, a region 300 kilometers (190 miles) across. The flood erupted from the depression at the left center and flowed to the right, creating the scoured channel floor seen in this image. 50 km

Phobos and Deimos Mars has two very small moons. Phobos (upper left) is 27 by 19 kilometers (17 by 11 miles) across. Deimos (lower right) is 15 by 11 kilometers (9.5 by 7 miles) across. Both moons may be captured asteroids. If so, they were probably captured early in martian history.

A Desert World Mars is a desert world, with no liquid water at its surface. This view, showing rust-colored dust and gray, basaltic (lava) rocks, was taken by NASA’s Spirit rover in early 2004.

A Geologic Time Machine Because rock layers are laid down bit by bit, the layer at the bottom of this cliff must be older than the layer at the top of the cliff. (This is similar to the stack of papers on your desk, or pile of clothes in your dirty clothes hamper – the papers at the bottom of the stack have been there longer than those at the top of the stack). By examining the rocks layer by layer, geologists can read the history of Mars. Because Mars has been geologically less active than Earth in the last 3 billion years, the early part of martian history is better recorded than the early history of Earth. In that sense, exploring Mars is like being in a geologic time machine.

Life on Mars? Look for evidence of respiration, response to nutrients. Results probably indicate unusual soil chemistry. No evidence for organic molecules at the parts per billion level. Claimed evidence for life in martian meteorite is not generally accepted. NASA looked for evidence of life in 2 places on Mars with the Viking spacecraft in 1976. Although a small number of the tests were ambiguous, the general consensus of scientists who have examined the data is that no evidence of life was found. Similarly, no evidence for organic molecules (the chemical building blocks of life) was found. A small number of scientists claimed in 1996 to have found evidence for fossil life in a meteorite from Mars (including the “fossil” shown in the image here), but these claims have not been generally accepted by the science community. For a summary of this issue see an article by Allan Treiman, “Microbes in a Martian Meteorite?” in the April 1999 issue of Sky and Telescope magazine. However, none of these findings are sufficient to prove that life does not (or did not) exist on Mars.