Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson.

Slides:



Advertisements
Similar presentations
Chapter 7 Earth and the Terrestrial Worlds
Advertisements

Atmospheres of the Terrestrial Planets. Atmospheres of the Moon and Mercury The Moon Mercury There is no substantial atmosphere on either body.
Space Exploration Mars Rovers, Apollo program, Voyager satellites, and SETI All Presented by the Peter C Period: 2 (two) As in 1+1=2 Or 2x1=2 ®
Centre of Planetary Science and Exploration University of Western Ontario.
Mars Pathfinder Mission Breakthrough on the Surface of Mars.
Modern Exploration Global Surveyor.  Objectives:  High resolution imaging of the surface  Study the topography and gravity  Study the role of water.
Mars ASTR-3040 Astrobiology Day 18. Homework Chapter 8 Due Thurs. March 31 3, 7, 13, 23, 30, 32, 41, 46, 51, 52 Plus (49 or 50) if you've read one of.
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.
ASTR100 (Spring 2008) Introduction to Astronomy Earth as a Planet Prof. D.C. Richardson Sections
Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 14 : Modern Mars Ty Robinson.
Astronomy190 - Topics in Astronomy
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
Second Quarter Questions. Concept Test The cores of the terrestrial worlds are made mostly of metal because ______. a.the terrestrial worlds as a whole.
Astronomy190 - Topics in Astronomy
Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 11 : Earth’s Habitability Ty Robinson.
Ch. 4 Study Guide Answers.
Mars Exploration Rovers and Mars. Evidence for Liquid Water on Mars (in remote past) Valley networks Outflow channels “Northern Ocean”
Modern Exploration Mars Pathfinder  “NASA’s Mars Pathfinder mission – the first spacecraft to land on Mars in more than 20 years and the first ever to.
The Rock Cycle.
Astronomy Tools and The Moon UNIT 11 STANDARDS: NCES 1.1.1, 1.1.2, 1.1.3, 1.1.4, 1.1.5, LESSON 2.
Mars & Venus: Space Exploration. INTRODUCTION  Humans have been curious about nature  Scientists send machines to explore other planets  Planets that.
Report: Astronomy Unit. The perfect planet… Earth is the only planet in our solar system that can sustain life.
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.
DO NOW Date: 5/18 Make a list of everything we (humans) need to stay alive.
The Goldilocks Problem?. Astronomical! Why is Venus so hot…
ASTRONOMY 340 FALL October 2007 Class #9. Salient Martian Features  R Mars = 3396 km (R Earth = 6378 km)  Higher surface area to mass ratio 
Intro to Soils. Objectives Define terms relating to soil. Describe factors affecting soil formation. Describe soil weathering factors. Describe the procedure.
Space unit Life in Space.
Mars Exploration Rovers. SpiritOpportunity Mars Exploration Rovers  Launch: June 10, 2003  Landed on Mars: January 4  Location: Gusev Crater  Planned.
Evolution of Mars Burton Gray. Introduction Comparison of Current Earth, Mars, and Venus Atmospheres Physical and Atmospheric Evolution of Mars.
Planetary Motion By Carol Greco. Why do planets move the around the sun the way they do? First you need to understand that scientists have discovered.
Lesson4d1 Working out the global history of Mars.
Destination Mars What Challenges do NASA Scientists face getting Rovers to safely land on Mars?
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.
ASTR Spring 2008 Joel E. Tohline, Alumni Professor 247 Nicholson Hall [Slides from Lecture30]
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
Planetary Terrestrial Surfaces and Exploring Mars Jaclyn and Carlton Allen Astromaterials Research and Exploration Science at Johnson Space Center.
The Solar System a1 Mercury Sun Venus Earth Mars Asteroids Jupiter Saturn Uranus Neptune Other objects Observe our solar system Four inner planets.
Chapter 10 Mars. Mars’s orbit is fairly eccentric which affects amount of sunlight reaching it 10.1 Orbital Properties.
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.
Mission to Pluto Using the satellites and missions described here, plan a mission to Pluto and choose the instruments.
Interlude  Viking mission operations ended in the early 1980s  Viking missions gave scientists the most complete picture of Mars to date. What does this.
Mission to Mars What to look for when you get there A Collection of Basic Earth Analogs.
Search for Life on MARS. Q: Why is water important for life? A: Because it’s such a great solute.
MARS.
Happy Halloween!. Homework #6 Due 6:00 pm today Exam #2 on Wednesday.
Introduction The 4 inner planets are Mercury, Venus, Earth, Mars The inner planets are composed mostly of rock, while the outer planets are gas giants.
Chapter 7c Mars: Freeze-dried Image from:
27-3OBJECTIVES Identify the basic characteristics of the inner planets. Compare the characteristics of the inner planets. Summarize the features that allow.
The Planets 7.3. What are some of the objects that make up our solar system? Planets Moons The Sun Comets Asteroids Stars.
Aim: How do increased carbon dioxide concentrations on our planet affect life?
Chapter 4 The Solar System.
Mars.
Exploring Mars.
DO NOW Pick up notes sheet. Get out Review half sheet.
Mars and Saturn II – What’s New?
Comparing the atmospheres of Venus, Earth, and Mars
Chatfield Senior High Department of Physics
Mars-2005.
WEATHER & CLIMATE.
Comparing the atmospheres of Venus, Earth, and Mars
Is/Was there life on Mars?
Information of Mars Mars is the fourth planet from the Sun and is commonly referred to as the Red Planet. The rocks.
11-2 Inner Planets.
Chapter 6 – Sedimentary and Metamorphic Rocks
The Rock Cycle.
The Rock Cycle.
Aim: What are rocks? Do Now: How are rocks related to minerals?
Is/Was there life on Mars?
Presentation transcript:

Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 15 : Ancient Mars Ty Robinson

Questions of the Day What is the evidence for liquid water on early Mars? What was different about early Mars that made it possible for liquid water to exist on its surface? What processes have subsequently affected Mars’ ability to sustain liquid water on its surface?

Surface Ages

Evidence from Space I Mars Earth Mars Riverbeds

Evidence from Space II Mars Earth Mars Sedimentary Layers

Evidence from Space III Flooding

Evidence for Water I Satellite Images –Riverbeds –Sedimentary layers –Flooding Evidence for Water

Follow the Water

Mars Pathfinder Launch: Dec Operation: Jul-Sep 1997 Instruments: - cameras - weather sensors - rock analysis tools

Pathfinder Landing landing video

Evidence for Water II Satellite Images –Riverbeds –Sedimentary layers –Flooding Pathfinder –Maghemite –Flood plain Evidence for Water

Mars Exploration Rovers Launch: Jun, Jul 2003 Operation: Jan ? Instruments: - cameras - weather sensors - rock analysis tools - microscope

Landing Sites

Gusev Crater

Extended Mission

Landing Sites

Minerals from Space

Opportunity Landing Site

Extended Mission

Chlorine and Sediments

Evidence for Water III Satellite Images –Riverbeds –Sedimentary layers –Flooding Pathfinder –Maghemite –Flood plain Spirit –Silica deposits Opportunity –Sediments –Blueberries –Chlorine concentration Evidence for Water

Questions? Liquid water is not stable on the surface of modern-day Mars because… temperatures are too low surface pressure is too low both surface temperatures and pressures are too low water does not exist on Mars

Questions? What must have been different about Mars in the past so that liquid water was stable on its surface? thicker atmosphere thicker atmosphere with more greenhouse gases Mars must have had a stronger magnetic field Mars must have been closer to the Sun

Greenhouse

Summary

Atmospheric Escape Impact Erosion Photolysis Solar Wind

Questions of the Day What is the evidence for liquid water on early Mars? What was different about early Mars that made it possible for liquid water to exist on its surface? What processes have subsequently affected Mars’ ability to sustain liquid water on its surface?

Quiz 3 - What is one thing you did not understand from today’s lecture? 2 - Explain why increasing chlorine concentrations with depth in a crater is evidence for the existence of water there in the past. 1 - What are three pieces of evidence that point to a wet early Mars which can be seen from space?