Observing Mars By Brad Jarvis. Overview Basic facts Orbits and distance Viewing Mars from Earth The view from space Current exploration Conclusion References.

Slides:



Advertisements
Similar presentations
The Terrestrial Planets
Advertisements

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.
PUT ON A HAPPY FACE The "Happy Face Crater" - officially named Galle Crater - puts a humorous spin on the "Face on Mars" controversy. This image was provided.
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.
Our Amazing Solar System
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.
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.
Earth Diameter 12756km Rotation Period 24 hours Orbital Period days Distance from Sun150 x 10 6 km Orbit Eccentricity/Tilt 0.02 / 23.3 degrees Temperature14C.
Mysteries of Earth and Mars Mars Facts and Exploration.
Mars. Information About Mars Mars is the 4 th planet from the sun. It is one of the inner planets because it is located inside the asteroid belt. Mars.
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”
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.
Brenda Herrera Bianei Rodrigues Stephanie Hayes.
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.
© 2011 Pearson Education, Inc. Venus and Mars. © 2011 Pearson Education, Inc. Venus.
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.
The Jetsons Go to “Mars”
NOTES: MARS 0.53 Diam(earth), -140 o C to 20 o C Atmosphere 95% CO2, 3% N2, 2% Ar 24 hr day, 25 o axial tilt like Earth 1. Small liquid core and magnetic.
4 th Grade. Sun Our Brightest Star Approximately one million Earths can fit inside the Sun. The center of the Sun, is made of helium. There are dark blotches.
Moon, Moon Phases & Eclipses. The Moon Calendar The current standard calendar is solar calendar (Gregorian calendar) – counting days The moon phases.
Mars: The Red Planet By Sarah Wolbach. What does Mars mean?  Roman god of war  Red color is associated with blood  Observed by Ancient Romans.
Early Spacecraft Exploration Early Spacecraft Exploration Mariner 3 & 4  “…these missions are being undertaken because Mars is of physical.
Unit 2 Lesson 4 The Terrestrial Planets Copyright © Houghton Mifflin Harcourt Publishing Company.
Innri Reikistjörnur Hvað heldur þú? Er hitastig á Merkúr, reikistjörnunni sem er næst sól, hærra en á jörðinni? Hver er samsetning skýja sem umlykja.
Mars Mars is a dry dead world. There are no Martian transits.
MARS By: Charanjit, Richard & Cesar.
Day and Night Phases of the Moon Planets
1. fluidized ejecta - liquid material expelled from meteor crater. Probably caused by permafrost melting when meteor hits.
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 Red Planet.
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.
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.
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.
The PLANETS and the SOLAR SYSTEM
Life on Mars Stephen Eikenberry 12 October 2010 AST
MARS.
Mars. When and where can you see it? Can be seen all night long. Sometimes undergoes apparent retrograde motion.
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.
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.
Our Whirling Planets 4th Grade Cherokee Elementary School.
The Terrestrial Planets Chapter 23, Section 2. Mercury: The Innermost Planet  Mercury, the innermost and smallest planet (not counting Pluto), is hardly.
By: Isabelle Saliba ~ Computer 4 th Period. All of the planets are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets.
Mars Mars is a dry dead world. There are no Martian transits.
Curiosity Curiosity pictures Rover view Old Rover View form older rover.
Mars The Red Planet.
Mars.
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
Mars eccentricity = Mass = 0.11 MEarth
Section 2: The Inner Planets
Surface Features Overview
Early Exploration Mariner 3 & 4
A Report in Natural Science I
The Inner Planets.
Section 2: The Inner Planets
Early Spacecraft Exploration
Mars - The Red Planet Image Courtesy of NASA/JPL-Caltech.
Craters on Mars Many craters Closer to asteroid belt No water erosion
Walter S. Kiefer Lunar and Planetary Institute
Stephen Eikenberry 21 Feb 2019 AST 2037
Presentation transcript:

Observing Mars By Brad Jarvis

Overview Basic facts Orbits and distance Viewing Mars from Earth The view from space Current exploration Conclusion References

Basic Facts about Mars Location is fourth from the Sun Day is about the same as an Earth day Year is nearly two Earth years long Size is half Earth’s, with about the same land area Gravity is about 1/3 that of Earth Atmosphere is mostly CO 2 at less than 1% the air pressure on Earth Temperature is -125°F to -13°F Two moons are possibly captured asteroids

Orbits and Distance Mars is: million miles away from Earth at opposition million miles away from the Sun

Viewing Mars from Earth

Viewing Mars from Earth Apparent Size The apparent size of Mars varies between 14 and 25 arcseconds at opposition (1/133 and 1/75 the apparent size of the Moon)

Viewing Mars from Earth Albedo Features Common types of features: Lacus (lake), Mare (sea), Regio (region), Sinus (bay) Map courtesy Daniel Troiani (producer), Carlos Hernandez (named features), ALPO

Viewing Mars from Earth The Colors of Mars Red is the color of iron-rich dust Dark gray is the color of volcanic rock White is the color of ice

Viewing Mars from Earth Changes in Appearance Apparent tilt of poles varies with relative positions of Earth and Mars Sizes of polar regions get smaller in summer and larger in winter Clouds can be white (water and CO 2 ice) or red (dust) Dust storms usually occur in southern summer and may engulf the planet Features appear dark or light depending on presence of dust

The View from Space Dust storm from Hubble Space Telescope

The View from Space A Confusion of Orientation Earth-based photos and maps are oriented so that south is up Space-based photos and maps are oriented so that north is up There have been two different longitude references for space- based maps since 2002

The View from Space Mapping the Surface Common types of features: Chasma (chasm), Fossa (long valley), Mons (mountain), Patera (crater), Planitia (plain), Planum (plateau), Terra (land), Tholus (hill), Vallis (valley), Vastitas (lowland)

The View from Space Martian Geology

The View from Space: Martian Geology Cratered Terrain Older parts of Mars are heavily cratered Typically in the southern hemisphere Noachis Terra (Noachis)

The View from Space: Martian Geology Northern Plains Younger parts of Mars are lightly cratered Typically in the northern hemisphere

The View from Space: Martian Geology Channels and “Canals” Water likely carved channels in the surface Some of the famous “canals” seen from Earth may have dust blown by the wind Xanthe Terra (Oxia Pallus)

The View from Space: Martian Geology Valles Marineris Valles Marineris is the largest canyon in the Solar System. It is the width of the lower 48 states of the U.S. and up to four miles deep. It is a fracture caused by the uplift of volcanoes in the Tharsis region.

The View from Space: Martian Geology Tharsis and Olympus Mons Tharsis is a region where the crust has uplifted. It is about 2,500 miles across and six miles high. Sitting atop this uplift are shield volcanoes, the largest of which is Olympus Mons. It is over 300 miles across, and 15 miles high.

The View from Space: Martian Geology Hellas Hellas Planitia is one of two large impact basins (Argyre Planitia is the other). It is 1,100 miles across and five miles deep. It is full of fast-cooling dust. It has been seen with frost and haze in the mornings.

Current Exploration Two Mars Exploration Rovers (left) will land on opposite sides of Mars in January They will study rocks over a maximum range of about 3/4 mile per day. Mars Express (including an orbiter and lander, right) will arrive at Mars in December It is the first mission since Viking to look for life.

Conclusion Mars is an entire world, with the same amount of land as Earth, and it is only six months away. It is an interesting place that can be explored by telescope, by robot, and eventually by people.

References Books: Boyce, J. (2002). The Smithsonian Book of Mars. Washington: Smithsonian Institution Press. Beatty, J., Petersen, C., Chaikin, A., eds. (1999). The New Solar System, 4th Ed. Cambridge: Sky Publishing Corp. Hartmann, W. (2003). A Traveler’s Guide to Mars. NY: Workman Publishing. Web: ALPO Albedo Map [ Mars Exploration Rover [ Mars Express [ Mars Gazetteer [ Mars Section Observing Alert and Images Page [ Mars Society [ Software: Starry Night Pro (Space.com) The Guide (Project Pluto)

Photos Courtesy: Tim Brown