The Red Planet.

Slides:



Advertisements
Similar presentations
The Terrestrial Planets
Advertisements

Chapter 7 Earth and the Terrestrial Worlds
Clicker Questions Chapter 6 The Terrestrial Planets Copyright © 2010 Pearson Education, Inc.
Earth to Mars Facts About the Planet Mars Earth Science.
© 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.
Red Planet Mars Chapter Thirteen.
Sun-Scorched Mercury Cloud covered Venus The Red planet Mars Chapters 11,12,13.
© 2010 Pearson Education, Inc. Chapter 10 Planetary Atmospheres (abridged): Earth and the Other Terrestrial Worlds.
ASTR100 (Spring 2008) Introduction to Astronomy Earth as a Planet Prof. D.C. Richardson Sections
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 10.
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
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.
April 11, 2006Astronomy Chapter 9 Earth-Like Planets: Venus and Mars Venus and Mars resemble Earth more than any other planets. Is it possible that.
Martian Meteorites Astronomy 315 Professor Lee Carkner Special Lecture.
Mars. Some similarities between Mars & Earth Mars’ Bulk Properties Mars has days & seasons like Earth.
Astronomy Picture of the Day. Mercury Mass = M Earth Radius = 0.38 R Earth  Surface Temp: K Average distance from Sun =.39 AU Moonlike:
Astronomy Picture of the Day. Mercury Mass = M Earth Radius = 0.38 R Earth  Surface Temp: K Moonlike: Surface craters, no atmosphere.
The Inner Planets  The inner planets are the 4 planets closest to the sun:  Mercury  Venus  Earth  Mars  The four inner planets are small and dense.
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.
The Inner and Outer Planets
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.
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.
The Terrestrial Planets, Part III Mars. MARS The God of War.
The Solar System.
© 2011 Pearson Education, Inc. Venus and Mars. © 2011 Pearson Education, Inc. Venus.
The Planets of Our Solar System
PLANETS. Solar System Our solar system consists of the sun, eight planets, moons, dwarf planets (or plutoids), an asteroid belt, comets, meteors, and.
The Goldilocks Problem?. Astronomical! Why is Venus so hot…
Mars. Moons of Mars Exploration of Mars ~1800: Herschel and others discover ice caps and clouds 1877: Phobos and Deimos discovered; also Schiaparelli.
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
Unit 2 Lesson 4 The Terrestrial Planets Copyright © Houghton Mifflin Harcourt Publishing Company.
(Terrestrial) Planetary Atmospheres II.  Atmospheres consist of exospheres only  Take either of their atmospheres, could “almost store them in a dorm.
Mars Mars is a dry dead world. There are no Martian transits.
The Terrestrial Planets. 2 Introduction  The four terrestrial planets – Mercury, Venus, Earth (The largest), and Mars – have similar sizes and structure.
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.
1. fluidized ejecta - liquid material expelled from meteor crater. Probably caused by permafrost melting when meteor hits.
The Inner Planets 20.3.
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
The Inner Planets Chapter Terrestrial Planets Mercury, Venus, Earth, Mars Mostly solid rock with metallic cores Impact craters.
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.
Intro to Our Solar System. Our Solar System Most of the planets in our solar system can be seen without a telescope. Uranus and Neptune are the only two.
PowerPoint for Mars. Mars Although its diameter is 1/2 and its mass 1/10 that of Earth, Mars is the planet that most resembles the Earth Mars extensively.
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.
Chapter 10 Mars. Mars’s orbit is fairly eccentric which affects amount of sunlight reaching it 10.1 Orbital Properties.
VENUS. “Twin” or “Sister” planet of the earth  similar size, mass, density; interior should also be similar with iron core, mantle, crust But totally.
Earth and the Other Terrestrial Worlds
Lecture 20. Outline For Today Venus review Mars The length of one solar day on Venus is A) about the same as that on Earth. B) much longer than that.
Chapter 7d Hothouse Venus. Venus Orbital distance: – km (0.72 AU) –NOT Eccentric Year: –224.7 d Day: – d –Retrograde rotation Temperature:
INNER PLANETS Terrestrial Planets are the Four planets closest to the sun. These planets have rocky terrain, and have higher temperatures due to receiving.
The Inner planets Section 28.2.
BY: KA’VARYA MCLAUGHLIN, INDICA MOSLEY, SAVANAH OZUNA.
Life on Mars Stephen Eikenberry 12 October 2010 AST
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
MARS.
Mars. When and where can you see it? Can be seen all night long. Sometimes undergoes apparent retrograde motion.
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.
Chapter 7c Mars: Freeze-dried Image from:
The Terrestrial Planets Chapter 23, Section 2. Mercury: The Innermost Planet  Mercury, the innermost and smallest planet (not counting Pluto), is hardly.
27-3OBJECTIVES Identify the basic characteristics of the inner planets. Compare the characteristics of the inner planets. Summarize the features that allow.
Our Solar System How it Formed & the Inner Planets Chapter 19 & 20.
Mars Mars is a dry dead world. There are no Martian transits.
Curiosity Curiosity pictures Rover view Old Rover View form older rover.
Unit 2 Lesson 4 The Terrestrial Planets
Mars eccentricity = Mass = 0.11 MEarth
Ask students which planet this is and ask them to name features they see in the image, e.g. clouds, water, etc.
11-2 Inner Planets.
Stephen Eikenberry 21 Feb 2019 AST 2037
Presentation transcript:

The Red Planet

Robotic Missions to Mars

Viking Lander

Martian landscape with frost

“Face” on Mars ?

Oppositions of Mars (Best Viewing) The best time to view a superior planet is at Opposition, whereas the best time to view an inferior planet is at maximum elongation

Opposition and Retrograde motion

Mars – Vital Statistics Mass ~ 1/10 Earth’s Diameter = 4200 mi, ½ Earth’s Density = 3.9 x water Year = 1.9 Earth years Day = 24 hr 37 min Distance to Sun = 1.5 AU (227 million Kms) Surface gravity (g) = 0.38 Earth’s Tilt of rotation axis = 25 degrees (seasons!) Surface T: Max 70 F, but usually -100 to -220 F Large variations in T (thin atmosphere)

Martian Gravity Although Mars almost certainly had a primordial atmosphere similar to Earth’s, most of it was lost primarily because of low gravity Gravitational acceleration g(Mars) = 0.38 g(E) M (Mars) ~ 1/10 M(E); R(Mars) ~ ½ R(E) g(Mars) = G M(Mars) / R2(Mars)  g(Mars) / g(E) = (1/10) / (1/4) = 0.4 Objects on Mars fall 2 ½ times slower

Mother of all canyons: Valles Marineris 5000 Kms (coast-to-coast if in US)

Polar “dry ice” caps (CO2) Northern Southern Polar icecaps are dry ice on top and water ice underneath

Polar cap with dust lanes

Evidence of ancient water flows on Mars “Canal” type features (dried up riverbeds); Martian climate was warm and wet in the past. Why did it change to the barren environment today ? The atmosphere evaporated ! Anti-greenhouse Effect !! Opposite of Venus !!!

More evidence of water

Ancient volcanic flows Recent volcanic activity (~ 100 million yrs) with huge runny lava flows (why?) Low gravity !

Mother of all volcanoes: Olympus Mons 24 Kms high (3 times Mt. Everest), 600 Kms across (as big as Missouri)

Volcanic Plains – Giagantic Shield Volcanoes Summits capped with “Calderas” – flat, broad, collapsed craters

“Mud-splash” crater

Topography: Warmer, Volcanic Northern Hemisphere and colder, cratered Southern Hemisphere

Some Basic Features of Mars First superior planet, best seen at opposition Most like Earth (season like on Earth, but twice as long) Eccentricity = 0.09, 4.5 times that of Earth’s orbit; Mars is 20% closer to the Sun at perihelion; receives 44% more sunlight Perihelion occurs during southern summers, which are shorter but hotter than northern summers, but southern winters are much longer; large variations in southern polar ice caps (may extend halfway to equator) North is warmer than the south !

Recycling heavy compounds H2O and CO2 and the Greenhouse Effect H2O, N2 remain in the atmosphere; CO2 is recycled on earth via photosynthesis EARTH H2O breaks up from UV; H2, N2, O2 escape; CO2 freezes on Mars as permafrost, or on polar icecaps MARS Martian atmosphere (0.007 bars) is 95% CO2

Anti-Greehnouse Effect ! Whereas Venus displays one extreme, the “runaway” greenhouse effect which retains most of the re-radiated energy (heat) in the infrared, Mars has the manifestation of the opposite effect How ? Violent dust storms prevent sunlight from reaching the surface, and temperature inversion in atmosphere

Steps to a Martian Dust Storm: Convection between night and day sides produces 50-200 MPH winds Dust blown into upper atmosphere (no rain to clear!) Sunlight blocked by dust  upper air gets warmer, surface cooler  “anti-greenhouse effect” Temperature difference makes convection worse, so more dust blown into atmosphere Nuclear Winter (nuclear war!) Extinction of Dinosaurs (asteroid impact!)

Life on Mars Viking Landers, Pathfinder, Rover and Spirit robotic missions TV  Nothing big seen moving around (at least so far) No organic compounds (C,H,O molecules) found No micro-organisms found Biological tests by robotic experiments are sensitive enough to have detected life in Antarctica

Terra-forming Altering a planet’s environment to create a climate simulating Earth’s Prescription for Mars: Melt polar CO2 to start greenhouse effect Raises the temperature so rest of ice melts Plant algae, etc. for photo-synthesis: CO2  O2 (Voila !) How does one start step 1?

Small Moons of Mars Moons of Mars are about the size of Columbus I-270 beltway