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RENEE M. CONDORI APAZA


     ARC – NASA
  2009 - CALIFORNIA
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 to the iron oxiode (rust) they contain.
Location
Mars -- the real planet
1.5 AU from Sun
Diameter ~ ½ Earth
                                          Cold, dry planet – weak greenhouse
Mass ~ 1/10 Earth
                                          Max 70F summer, Min -140F
Density 3.9 gm/cm   3


Period    687d ~ 2 yrs
Rotation 24h 37m
Inclination 24o
Atm – thin, low density

CO2      95%

N        3%
Ar        2%

H2O trace – clouds, ice caps
Earth and Mars Comparison
                 Earth          Mars
Radius           6378 km        3397 km
Density          5515 kg/m3     3933 kg/m3
Gravity          9.8 m/s2       3.72 m/s2
Year             365.25 days    686.98 days
Eccentricity     0.017          0.094
Day              24 hours       24 hr 39 min
Obliquity        23.45º         25.19º
Hubble Telescope Picture of Mars



                   This NASA Hubble Space
                   Telescope view provides
                   the most detailed complete
                   global coverage of the red
                   planet Mars ever seen
                   from Earth. This picture
                   was taken on February 25,
                   1995, when Mars was at a
                   distance of 65 million
                   miles.
Atmosphere on Mars




Mars has a rocky, dry terrain with huge volcanoes and
deep valleys. The atmosphere is much thinner than
Earth’s and is comprised primarily of carbon dioxide and
nitrogen. It’s gravity is about one-third of our own.
The surface on Mars




Surface Color: “Red”
Features
 – Impact Craters
 – Largest volcano in the
    solar system
    (Olympus Mons)
 – Largest Canyon in the
    Solar System
    (Valles Marineris)
 – Ancient river channels
 – Lava Rocks
 – Dust: Reddish from
    volcanic rock
Water on Mars?
Sinusoidal channels
Laminated terrain
Ice Caps
Largest Volcano on Mars



             The largest volcano in the
             solar system is Olympus
             Mons. It is 624 km (374
             miles) in diameter; about the
             same size as Arizona.
             The altitude of Olympus
             Mons is three times the
             altitude of the largest peak on
             Earth, Mt. Everest.
Gigantic Canyon



             Valles Marineris, or
             Mariner Valley, is a vast
             canyon system that
             runs along the Martian
             equator. Valles
             Marineris is 2500 miles
             long and reaches
             depths of up to 4 miles.
Gigantic Canyon


            For comparison, the
            Grand Canyon in
            Arizona is about 500
            miles long and 1 mile
            deep. In fact, the
            extent of Valles
            Marineris is as long as
            the United States and
            it spans about 20
            percent (1/5) of the
            entire distance around
            Mars.
Seasons on Mars




Like Earth, Mars has seasonal changes but the seasons last much
longer. In Winter, Mars’ polar ice cap can reach down to 45
degrees latitude and then rapidly shrink during Spring. Dust storms
are seasonal, also, as witnessed in this Hubble image.
Earth/Mars Comparison




                             Mars                   Earth
Distance from Sun       141.6 Million Miles       93 Million Miles
     Diameter               4222 Miles               7926 Miles
  Length of Year          687 Earth Days            365.25 Days
  Length of Day         24 hours 37 minutes     23 hours 56 minutes
     Gravity             .375 that of Earth    2.66 times that of Mars
   Temperature         Average -81 degrees F   Average 57 degrees F
Temperature Range          -127 C to 17 C           -88 C to 58 C
Number of Moons                  2                       1
Mars, the god of War


 The planet was named after Mars, the
 Roman God of War, who was one of the
 most worshipped and revered gods in
 ancient Rome. The god Mars held a
 special place in the Roman Pantheon not
 only for his patronly influence, but
 because of the importance of military
 achievement in the republic and the
 Roman Empire.
Early concepts




Before space exploration, Mars was considered the best
candidate for harboring extraterrestrial life. Italian
astronomer, Giovanni Schiaparelli thought he saw straight
lines crisscrossing its surface. This led to the popular belief
that irrigation canals on the planet had been constructed by
intelligent beings.
Mariner missions


         In July of 1965, Mariner
         4, transmitted 22 close-
         up pictures of Mars. All
         that was revealed was a
         surface containing many
         craters and naturally
         occurring channels but
         no evidence of artificial
         canals or flowing water.
Viking Landers


        Finally, in July and September
        1976, Viking Landers 1 and 2
        touched down on the surface of
        Mars. The three biology
        experiments aboard the
        landers discovered unexpected
        and enigmatic chemical activity
        in the Martian soil, but provided
        no clear evidence for the
        presence of living
        microorganisms in the soil near
        the landing sites.
Viking Landers




According to scientists, Mars is self-sterilizing. They believe
the combination of solar ultraviolet radiation that saturates the
surface, the extreme dryness of the soil and the oxidizing
nature of the soil chemistry prevent the formation of living
organisms in the Martian soil. The question of life on Mars at
some time in the distant past remains open.
The First Rover




Mars Pathfinder was the first instrumented lander and robotic rover to study
the surface of Mars. Findings from the investigations carried out by scientific
instruments on both the lander and the rover suggest that Mars was at one time
in its past warm and wet, with water existing in its liquid state and a thicker
atmosphere.
Mars Exploration Rovers




 Artist’s Concept Image: NASA



The Mars Exploration Rovers, Spirit and Opportunity, are
currently studying how past water activity on Mars has
influenced the red planet's environment over time.
Spirit



         In March 2005, Spirit
         studied rocks in the “Paso
         Robles” area that have a
         high sulfur content. Much
         of the high sulfur is
         contained in a hydrated
         iron-sulfate mineral that
         can only have formed in
         the presence of liquid
         water.
Opportunity



        Opportunity’s spectrometer
        and microscopic imager
        found that rocks near the
        lower slopes of Endurance
        Crater were affected by
        water both before and after
        the crater formed.
Curiosity
NASA's Curiosity Mars Rover
To handle this science toolkit, Curiosity is
twice as long and five times as heavy as Spirit
or Opportunity. The Gale Crater landing site
places the rover within driving distance of
layers of the crater's interior mountain.
Observations from orbit have identified clay
and sulfate minerals in the lower layers,
indicating a wet history.


NASA's Mars Science Laboratory
Curiosity rover, a mobile robot for
investigating Mars' past or present
ability to sustain microbial life.
Curiosity    is  being   tested    in
preparation for launch in the fall of
2011.
Future Exploration of Mars

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Mars Planet

  • 1. RENEE M. CONDORI APAZA ARC – NASA 2009 - CALIFORNIA
  • 2. 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 to the iron oxiode (rust) they contain.
  • 4. Mars -- the real planet 1.5 AU from Sun Diameter ~ ½ Earth Cold, dry planet – weak greenhouse Mass ~ 1/10 Earth Max 70F summer, Min -140F Density 3.9 gm/cm 3 Period 687d ~ 2 yrs Rotation 24h 37m Inclination 24o Atm – thin, low density CO2 95% N 3% Ar 2% H2O trace – clouds, ice caps
  • 5. Earth and Mars Comparison Earth Mars Radius 6378 km 3397 km Density 5515 kg/m3 3933 kg/m3 Gravity 9.8 m/s2 3.72 m/s2 Year 365.25 days 686.98 days Eccentricity 0.017 0.094 Day 24 hours 24 hr 39 min Obliquity 23.45º 25.19º
  • 6. Hubble Telescope Picture of Mars This NASA Hubble Space Telescope view provides the most detailed complete global coverage of the red planet Mars ever seen from Earth. This picture was taken on February 25, 1995, when Mars was at a distance of 65 million miles.
  • 7. Atmosphere on Mars Mars has a rocky, dry terrain with huge volcanoes and deep valleys. The atmosphere is much thinner than Earth’s and is comprised primarily of carbon dioxide and nitrogen. It’s gravity is about one-third of our own.
  • 8. The surface on Mars Surface Color: “Red” Features – Impact Craters – Largest volcano in the solar system (Olympus Mons) – Largest Canyon in the Solar System (Valles Marineris) – Ancient river channels – Lava Rocks – Dust: Reddish from volcanic rock
  • 9. Water on Mars? Sinusoidal channels Laminated terrain Ice Caps
  • 10. Largest Volcano on Mars The largest volcano in the solar system is Olympus Mons. It is 624 km (374 miles) in diameter; about the same size as Arizona. The altitude of Olympus Mons is three times the altitude of the largest peak on Earth, Mt. Everest.
  • 11. Gigantic Canyon Valles Marineris, or Mariner Valley, is a vast canyon system that runs along the Martian equator. Valles Marineris is 2500 miles long and reaches depths of up to 4 miles.
  • 12. Gigantic Canyon For comparison, the Grand Canyon in Arizona is about 500 miles long and 1 mile deep. In fact, the extent of Valles Marineris is as long as the United States and it spans about 20 percent (1/5) of the entire distance around Mars.
  • 13. Seasons on Mars Like Earth, Mars has seasonal changes but the seasons last much longer. In Winter, Mars’ polar ice cap can reach down to 45 degrees latitude and then rapidly shrink during Spring. Dust storms are seasonal, also, as witnessed in this Hubble image.
  • 14. Earth/Mars Comparison Mars Earth Distance from Sun 141.6 Million Miles 93 Million Miles Diameter 4222 Miles 7926 Miles Length of Year 687 Earth Days 365.25 Days Length of Day 24 hours 37 minutes 23 hours 56 minutes Gravity .375 that of Earth 2.66 times that of Mars Temperature Average -81 degrees F Average 57 degrees F Temperature Range -127 C to 17 C -88 C to 58 C Number of Moons 2 1
  • 15. Mars, the god of War The planet was named after Mars, the Roman God of War, who was one of the most worshipped and revered gods in ancient Rome. The god Mars held a special place in the Roman Pantheon not only for his patronly influence, but because of the importance of military achievement in the republic and the Roman Empire.
  • 16. Early concepts Before space exploration, Mars was considered the best candidate for harboring extraterrestrial life. Italian astronomer, Giovanni Schiaparelli thought he saw straight lines crisscrossing its surface. This led to the popular belief that irrigation canals on the planet had been constructed by intelligent beings.
  • 17. Mariner missions In July of 1965, Mariner 4, transmitted 22 close- up pictures of Mars. All that was revealed was a surface containing many craters and naturally occurring channels but no evidence of artificial canals or flowing water.
  • 18. Viking Landers Finally, in July and September 1976, Viking Landers 1 and 2 touched down on the surface of Mars. The three biology experiments aboard the landers discovered unexpected and enigmatic chemical activity in the Martian soil, but provided no clear evidence for the presence of living microorganisms in the soil near the landing sites.
  • 19. Viking Landers According to scientists, Mars is self-sterilizing. They believe the combination of solar ultraviolet radiation that saturates the surface, the extreme dryness of the soil and the oxidizing nature of the soil chemistry prevent the formation of living organisms in the Martian soil. The question of life on Mars at some time in the distant past remains open.
  • 20. The First Rover Mars Pathfinder was the first instrumented lander and robotic rover to study the surface of Mars. Findings from the investigations carried out by scientific instruments on both the lander and the rover suggest that Mars was at one time in its past warm and wet, with water existing in its liquid state and a thicker atmosphere.
  • 21. Mars Exploration Rovers Artist’s Concept Image: NASA The Mars Exploration Rovers, Spirit and Opportunity, are currently studying how past water activity on Mars has influenced the red planet's environment over time.
  • 22. Spirit In March 2005, Spirit studied rocks in the “Paso Robles” area that have a high sulfur content. Much of the high sulfur is contained in a hydrated iron-sulfate mineral that can only have formed in the presence of liquid water.
  • 23. Opportunity Opportunity’s spectrometer and microscopic imager found that rocks near the lower slopes of Endurance Crater were affected by water both before and after the crater formed.
  • 24. Curiosity NASA's Curiosity Mars Rover To handle this science toolkit, Curiosity is twice as long and five times as heavy as Spirit or Opportunity. The Gale Crater landing site places the rover within driving distance of layers of the crater's interior mountain. Observations from orbit have identified clay and sulfate minerals in the lower layers, indicating a wet history. NASA's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011.

Hinweis der Redaktion

  1. http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-mars.html
  2. http://mars.jpl.nasa.gov/mep/science/olympus_mons.html
  3. http://mars.jpl.nasa.gov/mep/science/vm.html
  4. http://www.the-planet-mars.com/mars-earth-comparison.html
  5. http://www.meridiangraphics.net/mars.htm
  6. http://www.solarviews.com/eng/mars.htm
  7. http://www.solarviews.com/eng/mars.htm
  8. http://mars.jpl.nasa.gov/MPF/ops/prm-thmb.html
  9. http://www.the-planet-mars.com/pathfinder/pathfinder-pictures.html
  10. http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20050307a/Sol381A_P2543_True_RAD-A418R1_br.jpg
  11. http://spaceflight1.nasa.gov/mars/