Title: Early Exploration Mariner 3
1Early 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
2Early 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
3Early ExplorationMariner 4
4Early ExplorationMariner 4
5Early 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
6Early 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
7Early 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
8Early ExplorationMariner 6 7
- Launched February 23 (M6) March 27, 1969 (M7)
- Close approaches occurred July 31 (M6) August 5
(M7), 1969
9Early 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)
10Early ExplorationMariner 6 7
11Early ExplorationMariner 6 7
12Early 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
13Early 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
14CRATER BOXES!!!
15Early 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
16Early 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
17Early 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)
18Early ExplorationMariner 9
- Arrived at Mars only to find a global dust storm
blanketing the planet - Circular features peaking through the dust
19Early ExplorationMariner 9
20Early 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.
21Early 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
22Early 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
23Early ExplorationMariner 9
Credit NASA/Goddard Space Flight Center
24Early 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