Ch. 8 Mars Flashcards

1
Q

Physical characteristics

  1. Diameter
  2. Avg dist from Sun
  3. Mass
  4. Orbital pd
  5. Rotational pd
  6. # of moons
  7. Magnitude
A
  1. Diameter = 1/2 X earth
  2. Avg dust from Sun = 1 1/2 X earth
  3. Mass = 1/10 X earth
  4. Orbital pd = 687 earth days
  5. Rotational pd = 24.6 earth hours
  6. # of moons = 2
  7. Magnitude = +1.8 - +2.9
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2
Q

Axial tilt

A

25 degrees

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3
Q

Seasons

A

Similar to earth ‘s seasons

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4
Q

Why is it red?

A
  • From iron oxide in soil

- literally rusty

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5
Q

Dark surface

A

“Canali” (channels)

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6
Q

What does Canali indicate?

A

Mars has a similar rotation pd to earth

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7
Q

Surface features (3)

A
  • currently dry
  • broad plains, shallow craters, extinct volcanoes, long canyons
  • bc mars has weaker gravity, it’s surface features = more extreme than earth’s
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8
Q

Vastitas borealis

A

Northern lowland

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9
Q

Southern highlands (2)

A
  • heavily cratered

- hilly plains

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10
Q

Mariner valley location (3)

A
  • between hemispheres
  • begins with heavily-fractured terrain in west
  • ends with ancient-cratered terrain in east
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11
Q

Mariner valley size

A

1/5 circumference of mars

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12
Q

Mariner valley origin

A

Believed to be a large crack that formed as planet cooled

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13
Q

Impact craters location

A

Most located in southern hemisphere

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14
Q

Location of volcanoes

A

Most in northern hemisphere

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15
Q

Olympus mons (2)

A
  • largest volcano in s.s.

- 3X height of mt. Everest

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16
Q

Other “artificial” features (3)

A

Photos have shown:

  1. Pyramids
  2. Skull
  3. Happy face
17
Q

Interior of mars (2)

A
  • evidence of ancient plate tectonics, but no activity today

- more solid than earth’s

18
Q

Magnetic field (2)

A
  • lacks a global magnetic field

- tectonic activity & magnetic field ended about 4b years ago

19
Q

Atmosphere Makeup (2)

A
  • 95% CO2

- 5% nitrogen, argon, and oxygen

20
Q

Atmosphere Characteristics (2)

A
  • composition similar to Venus and ancient earth

- Gravity = too weak to hold water vapor

21
Q

surface pressure

A

0.6% of earth’s

22
Q

Dust (2)

A
  • warm surface creates dust devils

- erodes surface features

23
Q

no water, but ice

A

w/e water that was left on mars, as it cooled, froze into ice

24
Q

watery past (3)

A
  • evidence there was once ocean in n. hemisphere
  • most ice in polar caps = water ice
  • rest is dry ice
25
Q

SNC meterorites

A

pieces of mars that land on earth

26
Q

Mar’s moons (2) and type of rotation

A
  1. Phobos (lg moon)
  2. Deimos (sm moon)
    • synchronous rotations
27
Q

Phobos (3)

A
  • larger, inner moon
  • orbits 3X/martian day
  • rises in west, sets in east
28
Q

Deimos (4)

A
  • smaller, outer moon
  • less heavily cratered
  • takes about 3 martian days to set
  • rises in east
29
Q

Spacecraft visitors (4) (altogether 8)

A
  1. mars 1 & 3
  2. Mariner 4 & 9
  3. Viking 1 & 2
  4. Phobos 1 & 2
30
Q

mars global surveyor (2)

A
  • launched by U.S.

- photos showed liquid water in 2 craters

31
Q

mars pathfinder

A

consisted of lander and lightweight wheeled robotic mars rover (Sojourner)

32
Q

mars exploration rover A (2)

A
  • 1st of 2 launched = spirit

- stuck in 2009

33
Q

mars exploration rover B (2)

A
  • 2nd of 2 launched = opportunity

- still active

34
Q

curiosity

A

-powered by radioisotope thermoelectric generator