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Early Exploration Mariner 3

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... and geological interest and offers the best opportunity in our solar system for shedding light on the possibility of extraterrestrial life. – PowerPoint PPT presentation

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Title: Early Exploration Mariner 3


1
Early ExplorationMariner 3 4
  • these missions are being undertaken because
    Mars is of physical and geological interest and
    offers the best opportunity in our solar system
    for shedding light on the possibility of
    extraterrestrial life. (They), however, are not
    designed to provide answers to the question of
    life on Mars.

Mariner 4 Press Kit, October 29, 1964
2
Early ExplorationMariner 4
  • Launched November 24, 1964 closest approach
    occurred on July 14, 1965
  • Took 22 pictures w/ a TV camera viewing through a
    reflecting telescope

3
Early ExplorationMariner 4
4
Early ExplorationMariner 4
5
Early ExplorationMariner 4
  • Notable observations from Mariner 4
  • Images returned showed a Moon-like cratered
    terrain
  • Surface atmospheric pressure of 4.1 to 7.0 mb
    (accepted values ranged from 10 100 mb)
  • Daytime temperatures of -100 C (-148 F) were
    estimated
  • No magnetic field was detected

6
Early ExplorationMariner 4
  • How did Mariner 4 advance scientific
    understanding of Mars?
  • Mars looked more like the Moon
  • Life far less likely
  • IMPORTANT Mariner 4 only imaged 1 of the
    surface of Mars, mostly in the southern
    hemisphere
  • What technological advance(s) did Mariner 4
    carry?
  • The Mariner 4 spacecraft

7
Early ExplorationMariner 6 7
  • Study the surface and atmosphere of Mars to
    establish the basis for future experiments in the
    search for extra-terrestrial life and to develop
    technology for future Mars missions. The 1969
    flights will not determine the presence of life
    on Mars but will help establish whether or not
    the Martian environment is suitable for life.

Mariner (6 7) Press Kit, July 18, 1969
8
Early ExplorationMariner 6 7
  • Launched February 23 (M6) March 27, 1969 (M7)
  • Close approaches occurred July 31 (M6) August 5
    (M7), 1969

9
Early ExplorationMariner 6 7
  • Two TV cameras medium high resolution, IR
    radiometer (surface temps, is southern cap CO2 or
    H2O?), UV spectrometer (atmospheric composition),
    IR spectrometer (surface near-surface
    composition)

10
Early ExplorationMariner 6 7
11
Early ExplorationMariner 6 7
12
Early ExplorationMariner 6 7
  • Notable observations from the Mariner 6 7
    missions report
  • Temps range between -73 C (-100 F) 15 C (60
    F)
  • The polar caps were crusted with frozen carbon
    dioxide
  • Features with a dimension of 900 (ft.) could be
    identified.
  • The so-called Martian canals were not in
    evidence.
  • At a location called Nix Olympicawas a huge
    crater 300 miles in diameter.
  • No indications of volcanism were found.
  • Mariner 6 7 imaged 20 of the surface of Mars,
    mostly in the southern hemisphere

13
Early ExplorationMariner 6 7
  • How did Mariner 6 7 advance scientific
    understanding of Mars?
  • Temperature range
  • South polar cap composed of CO2 temp reading of
    -123C (-190F)
  • NO CANALS
  • What technological advance(s) did Mariner 6 7
    carry?
  • Spacecraft with higher resolution cameras
    spectrometers

14
CRATER BOXES!!!
15
Early ExplorationMariner 8 9
  • Study the surface and atmosphere of Mars in
    detail, and over a period of time, to provide a
    broad picture of the history of the planet and
    natural processes currently shaping the Martian
    environment. To accomplish this, one spacecraft
    will map 70 of the planet and the other will
    repeatedly study selected areas on Mars to
    observe changes on the surface and in the
    atmosphere.

Mariner (8 9) Press Kit, April 30, 1971
16
Early ExplorationMariner 8 9
  • Launched May 8 (M8) May 30, 1971 (M9)
  • Mariner 8 failed 4.5 minutes after launch,
    Mariner 9 arrived at Mars on November 14, 1971

17
Early ExplorationMariner 8 9
  • Narrow-angle and wide angle TV cameras, IR
    radiometer (surface temps), UV spectrometer
    (composition of upper atmosphere), IR
    interferometer spectrometer (provide a picture of
    the circulation of the atmosphere composition
    of the surface)

18
Early ExplorationMariner 9
  • Arrived at Mars only to find a global dust storm
    blanketing the planet
  • Circular features peaking through the dust

19
Early ExplorationMariner 9
20
Early ExplorationMariner 9
  • Notable results from Mariner 9
  • Global mapping (imaging) of the surface of Mars
  • The first detailed views of the Martian
    volcanoes, Valles Marineris, the polar caps, and
    the satellites Phobos and Deimos
  • Provided information on global dust storms, the
    planets rugged gravity field, and evidence for
    surface aeolian (wind) activity.

21
Early ExplorationMariner 9
  • Olympus Mons
  • 27 km tall (16.8 miles), 600 km (373 miles) wide
  • Shield volcano composed of basalt
  • Largest (known) volcano in the solar system

22
Early ExplorationMariner 9
  • Valles Marineris
  • 4,000 km long (2,500 miles), 200 km (124 miles)
    wide, 7 km (4 miles) deep
  • Large crack resulting from uplift of Tharsis
    bulge
  • Named after Mariner 9

23
Early ExplorationMariner 9
  • Tharsis Bulge

Credit NASA/Goddard Space Flight Center
24
Early ExplorationMariner 9
  • How did Mariner 9 advance scientific
    understanding of Mars?
  • Mars is more geologically diverse than had ever
    been presumed
  • Evidence water once flowed on the surface, not in
    artificial canals, but natural river channels
  • What technological advance(s) did Mariner 9
    carry?
  • Spacecraft orbited Mars, first unmanned planetary
    orbiter in history
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