home
***
CD-ROM
|
disk
|
FTP
|
other
***
search
/
No Fragments Archive 10: Diskmags
/
nf_archive_10.iso
/
MAGS
/
MEGA
/
MEGA_02A.MSA
/
ISSUE_2.PAK
/
MARS.PK1
/
MARS.PK1
Wrap
Text File
|
1998-03-24
|
18KB
|
294 lines
MARS SURFACE EXPLORATION
One question that is being asked by people is, "Why go to Mars"? The
reasons are very simple. People want to gain recognition of how they were the
first people who went to Mars and opened up a whole new world and most
importantly to move forward in economics.
As humans waste the precious materials and resources found on this planet
we have to consider going to other planets to explore for materials and energy
resources. Mars would be the first area for industrial development and mining
in the "new world".
There are talks that by the end of this century that a manned mission to
Mars should take place. We must start preparing ourselves properly in order to
explore Mars better. Scientists and researchers hopes when exploring Mars is to
find interesting minerals or matter that will help us understand what Mars was
like millions and millions of years ago.
The first manned mission to Mars will be more complex then that of the
first Moon landing which the main goal for going to the Moon was to just land
safely. The main thing that researchers and scientists are striving for is
exploratory, searching for useful raw materials such as water and at the same
time building up an extensive scientific picture of Mars-its state at the
present moment, its history and what the future developments are going to be.
As astronauts journey to Mars and finally reach there the main concern and
top priority when landing will be the astronauts safety. There will be more
flexibility when choosing a landing site. The astronauts will decide where they
want to land but must take into consideration that the roving vehicles would be
able to provide extended range when travelling on the surface of Mars. This most
probably would ensure that the sites that are in the scientists interest would
easily be accessible.
Possible landing sites must be chosen under one goal, that would be the
overall understanding of the surface and not by a place that looks attractive or
has special features even if they seem alluring. The things that have to be
taken in account for possible landing sites are:
- guaranteeing that the explorers will touch down at the place which is
specified; - choosing a place where possible interesting geological features may
be found; - choosing an area where rocks have recently been exposed; - a certain
area must be specified of where the roving vehicles may go.
Regions on Mars that have extensive dune fields and barely any bedrock, the
surface mobilities should be within a few kilometres to guarantee that samples
can be obtained without any difficulty. Landing sites that have easy access to
more than one type of interesting terrain has an advantage but unfortunately
these sites lean to be more on the rough side and might pose to be a weighty
hazard and obstacles might be in the way of roving vehicles.
There are a possible of ten prime landing sites that might be chosen when a
manned mission to Mars has taken place. The Kasei and Mangala valles are made
up of striking features which seem to have channels that are evidently engraved
by flowing water from the past. Extensive studies would provide significant
clues to why Mars lost reserves of water. These locations would offer and give
explorers a big advantage as this area is close to the large volcanoes and
volcanic plains that are near the equator, which will have affected their
geology a tremendous deal.
There are other riveting sites other than these, but they are difficult to
reach for a manned mission to Mars. The Polar region sites are precluded for
manned missions because fuel would be expensive to change form an initial
parking orbit to a tilted orbit in order to make it possible to land there. With
non-polar sites, it would be difficult to land on a gigantic volcanoes or
canyons. The problems with visiting the southern hemisphere regions is that it
is less attractive then the northern hemisphere and the terrain is much more
rougher. These areas are also the origin of dust storms and if a spacecraft
were to land there it would be foolish. Although these regions are not going to
be explored by explorers, at a later time or date they will be visited by
long-range vehicles, with men or without, sent from bases elsewhere.
Once the space craft has landed on the Mars and a go-ahead for a long stay
has been given the crew they will eat and rest for their venture on the surface
the next day. As walkers emerge onto Mars they will have to lower visors which
is coated with a thin, transparent layer of gold which eliminates unsafe
ultraviolet radiation.
As they emerge on the surface they will go around their spacecraft and look
for any damage done and then will grab soil samples in case the explorers have
to make a quick retreat. At the same time they will unload a roving vehicle in
which they will travel.
On foot, explorers would be able to cover a little more than a mile from
the base that they would have set up. If rovers (land vehicles) were taken
along then more area could be covered during exploring the planet and then would
easily be able carried back to their base.
When travelling across the Martian surface there will be many difficulties
encountered by the explorers when using the roving vehicles. On a manned mission
there will be two kinds of roving vehicles one for smooth surfaces and one for
not so smooth surfaces in an effort to increase the range of exploration.
Unmanned rovers might have the same idea as the Soviet rover which has six
wheels, nuclear-powered design and weighing several hundred pounds and each
rover would be equipped with a standard set of sensors. Several rovers would be
dispatched and controlled possiblly by an orbiting satellite. After the crew has
left Mars the rover would still probe around Mars and collect samples. The rover
would be controlled from earth.
Larger manned rovers will also be needed for transporting up to six hundred
and eighty kilogram loads on forty kilometre journeys round trip. They should be
able to go over twenty degree slopes and be able to climb one foot boulders.
Even these rovers would be limited. For more vast exploration a vehicle with a
laboratory would be sent. The weight of the rover would be between four to five
tons but it would be able to transport two or three crew members for as long as
thirty days. The range of the rover would be 100 kilometres from their base and
reach speeds up to thirty-two kilometres per hour and carry two tons of
equipment. In the Soviet unmanned mission to Mars balloons will be essential
when the soviets arrive there. They have many advantages such as being simple,
cheap and light and would be able to cover thousands of kilometres of land in a
few weeks. After each balloon is unpacked the crew would test its instruments by
plugging it into standard test equipment and then attach a thin plastic object
to it and inflate it with helium which would be in a pressure bottle and then
release the balloon and let it drift independently. The heights that the
balloon could be able to reach would depend on its volume, the weight of the
payload that is in the balloon and the atmospheric temperature which changes
during the course of the day.
Later Manned Mars missions would have planes to explore the surface.
Studies have shown that a powered aircraft would be able to drop scientific
packages, penetrators and even deliver materials needed by parties that are
exploring the planet.
After landing on Mars the crew would bolt together the plane. It would
look like large powered glider and would be launched by a catapult or rockets.
The plane would have fifteen horse power engine and it would be driven by steam
which would be generated by the chemical breakdown of hydrazine.
The tremendous benefit of having a Mars plane is that it can be reused, it
would be easy to manoeuvre and the range the plane would be able to travel.
Maybe one day in a future mission planes would be able to glide over the surface
of the planet which would benefit scientific surface exploration.
When the explorers are on the planet their days will be long and
exhausting. Human explorers can explore more efficiently and more thoroughly
than robots can. Humans are more adaptable than robots. Humans would be able
to assess a huge assortment of situations faster and would be able to adjust to
their actions accordingly to what has to be done. A trained geologist with a
rock hammer can accumulate more samples that would be available around the
planet in an hour than an automated rover would be able to do in a year.
Humans will be extremely valuable in the search for life on the planet. A
professional astronaut would have the skills to easily spot a protected site
that would be favourable to life. An example of this would be a spot sheltered
by a rock. Equipment which is automatic that astronauts have is better for
things like, repetitive measurements which would be stretched over long periods
of time.
Scientific research will be divided into two main categories. There would
be a day to day exploration by the astronauts which would have more difficult
tasks. They would also be responsible for long-term monitoring by automatic
packages which would be left behind when they leave the planet.
The main concern for the astronauts would be geological investigation of
the planet. There might be one or more geologists in a mission to Mars. Teams
of geologists at mission control will plan exploration traverses by using the
orbiter's to take pictures of the surface. These pictures will produce a route
map that would help the astronauts while they are exploring the planet. The
astronauts will not be just responsible to collect samples and bring them home
but also they must study the rocks while on the planet and conduct some
analyses.
The things that astronauts are looking for is the chemical and mineral
composition of the rocks which would provide them with the information on the
geological history of Mars, at which places were the rocks formed, at which
temperatures and pressures were they formed, development of the atmosphere and
the history of water on Mars. Necessary information will be profited from the
rocks that are on the surface, but when drilling deep into the ground and
dislodging the rock, it will uncover the historical development of the regions
geology.
Each day the astronauts job will be to set on the surface in a rover which
would contain standard geological tools like hammers, chisels, rakes, sieves and
tongs which would enable them to pick up essential rocks even if they seem
awkward to pick up with their space suits on. Connected to their space suits
there will be a gnomon. This unique device is like a tripod with a free-hanging
central rod, which is able to photograph against each sample before it is
dislocated from the surface so the exact location is know to the astronauts.
This photograph shows the scale of each of the objects removed, slop of the
ground and its shadow that indicates the direction of the Sun. A colour pattern
will be attached to the photograph which allow scientists on Earth to
reconstruct the colours which surround the object removed. This is crucial
because cameras sometimes tend to distort the colour to some degree.
After each sample is photographed their locations would be carefully
written down. The astronaut will then place the samples in hermetically sealed
containers. Geologists would highly recommend that a percentage of the sample
be kept refrigerated at Marslike temperatures to prevent the soil sample to
change on the way back to earth. The astronauts rover would stop every few
hundred feet and soil samples would be tested automatically.
Drilling around the planet would be carried out on a regular basis. This
would be one of the astronauts most vigorous activities. The rover of the
astronaut will carry electrical powered drills and a supply of aluminium tube
sections. The drill will be similar to jack-hammers used in construction on
Earth. The drill will be powered by a compressor using Mars' carbon dioxide
atmosphere.
Mars' internal structure will be better understood when scientists find out
the rate of heat flow from the interior. A method of doing this is by
thermometers which would be placed at different depths of Mars. Little heaters
would be positioned near thermometers which would reveal how heat flows through
the material that makes up the surface layers.
Most probably on a trip to Mars there will be complicated apparatus' for
extensive analyses of soil. An electron scanning microscope would probably be
used to look for any tiny fossils and aid in hopes of distinguish any minerals.
An X-ray fluorescence spectrometer will be used to record the X-rays emitted by
materials when they are irradiated by a radioactive source which will discover
the materials present. There also will be a combined gas chromatography and a
mass spectrometer which will separate and measure the gases that is driven off
when a sample is heated
When humans and rovers finally get to the poles, their top priority will be
to get samples of the core which will be taken from the layers of deposits of
ice and dust (which is millions of years old). This would probably have a
record of how the climate has changed over hundreds of million of years.
There are numerous fascinating surface structures of Mars and when
explorers do go to Mars it will be interesting to see what information they
bring back about the places that have already been identified and the things and
places that remain a mystery to us. These places include the volcanoes, the
north and south poles of Mars, the equatorial canyons, the unique craters,
basins etc. All these places when studied will help us get a better
understanding of the planet which has amazed us from pictures that were taken
from non manned missions.
The volcanoes on the planet are the most startling features of Mars. There
are many volcanoes on Mars but the most sensational is found near the equatorial
region of Tharsis. On the planet, volcanoes have been around much of the
planet's history. The general shape hints that eruptions of fluid lava has very
small amounts of ash in it. The chemical composition of the terrestrial
volcanoes on the planet shows that lava and the rate at which the volcanoes
erupted affected the volcanoes's final structure.
The craters of Mars have a huge ranges from little as a several meters
across to huge broad basins which are up to hundreds of kilometres in diameter.
The southern hemisphere contains hardly any craters which is visible but in the
northern hemisphere there an abundant amount of craters.
There are about sixteen basins on Mars each one larger than0 two hundred
and fifty kilometres in diameter somewhere on the surface of Mars. Each basin
appears to be vast and multi-ringed. Some basins are fairly new but the others
are significantly old which look considerable eroded
There are many striking features of Mars but we must understand the dilemma
that is on Mars about the water. There are many things on the surface of Mars
that look like water channels. Many years ago scientists thought that these
channels were made by erosion, by lava, or the wind might have made these
channels but this no longer holds true today. Scientists know that water did
once exist in huge quantities by the visible channels of Mars.
We have found out that water did once exist on Mars but where has it all
gone? Unfavourable scientists can only take a guess by what is know about the
planet and then estimate at how much water Mars once had, how much of the water
escaped on the surface and how much of it is hidden to the naked eye.
The amount of water that is on Mars is negligible. The polar caps of Mars
contain some water but they are mixed with frozen carbon dioxide and dust so the
quantity of water is not known. The permafrost underground is another water
supply. The colder the conditions of Mars then the more chance of finding
permafrost under the surface of Mars. There are estimates that at the poles the
permafrost is well up to eight kilometres thick and lie just a few centimetres
below the surface. Near the equator the permafrost is estimated to be up to,
two to three kilometres thick and just a few metres deep.
When a trip to Mars takes place and in the near future it will many
scientist, researchers and the people will be excited to learn what the planet
is like. There are many fascinating things on Mars that still remain a mystery
today and a manned mission to Mars will help us unravel these mysteries.
BIBLIOGRAPHY Asimov, Isaac. MARS, The Red Planet. New York: Lothrop, Lee and
Shepard Company. 1977
Asimov, Isaac. MARS: Our Mysterious Neighbor. Milwaukee: Gareth Stevens
publishing. 1988
Simon, Seymour. MARS. New York: William Morrow and Company. 1987
Frank Miles and Nicholas Booth. Race to Mars. New York: Harper and Row
publishers. 1988