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Innri Reikistjörnur Hvað heldur þú? Er hitastig á Merkúr, reikistjörnunni sem er næst sól, hærra en á jörðinni? Hver er samsetning skýja sem umlykja.

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Presentation on theme: "Innri Reikistjörnur Hvað heldur þú? Er hitastig á Merkúr, reikistjörnunni sem er næst sól, hærra en á jörðinni? Hver er samsetning skýja sem umlykja."— Presentation transcript:

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2 Innri Reikistjörnur

3 Hvað heldur þú? Er hitastig á Merkúr, reikistjörnunni sem er næst sól, hærra en á jörðinni? Hver er samsetning skýja sem umlykja Venus? Er fljótandi vant á Mars í dag? Er líf á Mars í dag?

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6 Myndir frá Mariner 10 sýna hve líkt yfirborð Merkúr er því sem er á Tunglinu MercuryMoon

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8 Caloris Basin Note the edge of a huge crater on the left, mostly in shadow.

9 Unusual, Hilly Terrain The tiny, fine-grained wrinkles are actually closely spaced hills.

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11 Mercury has an iron core and a magnetic field like Earth Mercury rotates in 176 Earth days, barely enough to have a dynamo created magnetic field -- yet, Mercury still has a magnetic field. Its source is a great mystery.

12 Mercury’s temperature range is the most extreme in the solar system Mercury’s slow 176 day rotation and the lack of an appreciable atmosphere means temperatures vary enormously from one side of the planet to the other. Daytime with the Sun overhead reaches 700K (or 800°F) Midnight with the Sun completely obscured is 100K (or -280°F) Earth typically has temperature differences between day and night of about 11K (or 20°F)

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14 The surface of Venus is completely hidden beneath permanent cloud cover

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16 Venus Atmosphere is 96% CO 2 Temperature is 750K –much higher than Mercury –daytime AND nightime –caused by the greenhouse effect

17 The greenhouse effect heats Venus’s surface

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19 Venus is covered with gently rolling hills, two “continents,” and numerous volcanoes

20 The Venusian Surface

21 Impact Craters on Venus

22 Mars as viewed from Earth

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25 Like Earth, Mars has polar ice caps that grow and shrink with the changing seasons.

26 Valles Marineris is many times larger than the Grand Canyon Enormous shield volcanoes

27 Olympus Mons - the largest volcano in the solar system has a base larger than the state of Colorado

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29 Early space probes to Mars found no canals but did find some controversial features

30 Surface features indicate that water once flowed on Mars Ohio River valley on Earth River channels on Mars

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32 Viking I Lander Picture from 1976

33 1999 Picture from the Mars Pathfinder Lander - Sagan Station Note the remote- control rover, Sojourner, next to a Martian rock

34 Martian air is thin and often filled with dust Mars’ thin atmosphere is 95% CO 2 Mars’ atmospheric pressure is about 1% as high as Earth’s Mars’ coldest temperatures occur at the poles at about 160K (-170°F) Typical Mars temperatures range between 50°F and -80°F

35 The Martian meteorite found in Antarctica has not provided conclusive evidence about life on Mars

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37 Mars’ two moons, Phobos and Deimos, look more like potatoes than spheres

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39 What did you think? Is the temperature on Mercury, the closest planet to the Sun, higher than the temperature on Earth? The temperature on the daytime side of Mercury is much higher than on Earth, but the temperature on the nighttime side of Mercury is much lower than on Earth because Mercury rotates so slowly and has little atmosphere to retain heat. What is the composition of the clouds surrounding Venus? The clouds are composed primarily of sulfuric acid. Does Mars have surface liquid water today? No, but there are strong indications that it had liquid water in the distant past. Is life known to exist on Mars today? No life has yet been discovered on Mars.

40 Self-Check 1: Compare and contrast the atmospheres of the terrestrial planets in terms of temperature, pressure, and chemical composition. 2: List the properties that Mercury has in common with the other terrestrial planets with the Moon. 3: Compare and contrast the surfaces of Mercury, Mars, and Venus with that of the Earth in terms of geologic structures and evidence regarding tectonic activity. 4: Describe plausible explanations for the absence of water vapor in the Venusian and Martian atmospheres. 5: Discuss the contributions of the various spacecraft missions to our understanding of the terrestrial planets. 6: Discuss the evidence for the existence of water on Mars surface in the past and the location and form of that water today. 7: Compare the magnetic fields of Mercury, Venus, and Mars with that of Earth.


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