CHAPTER VI
Life support
1 a. measuring radiation levels
Ionizing radiation in space comes in three main types. The
first is Galactic Cosmic Rays. Astronomers believe that these rays originate
mainly in supernovae, although they also appear to come from quasars and solar
flares from stars outside the Solar System. Every star reaches a point in its
lifetime when the hydrogen in its core has all been converted to helium. This
starts a series of reactions which forces the core to collapse in on itself.
When a star with a mass 10 times that of the Sun collapses, a vast amount of
energy is released in an explosion. A shock wave travels from the core and
blows apart the star. Positively charged nuclei of atoms are spewed into space.
These highly energetic nuclei travel through space almost as quickly as light.
The second type of radiation that astronauts and space colonists
must be concerned with is solar protons. The protons originate in the sun. For
reasons not fully understood by scientists, the sun sometimes ejects magnetic
energy in the form of solar flares. Solar flare activity is linked with
sunspots and the Sun's eleven year cycle. During a flare, temperatures range
from 10 to 20 million degrees Kelvin. The high temperatures accelerate
particles in the solar atmosphere. One of the most astounding things about
solar flares is the amount of energy released in a single eruption. A flare
usually releases 1027 ergs/sec. During the course of the entire
flare, the released energy would be the same as that given off by the
simultaneous explosion of several million, 100-megaton hydrogen bombs! This
energy takes the shape of many things, including solar protons. The protons
travel through space in the solar wind
which has a velocity of approximately 400 km/sec.
The third type of radiation is high energy electrons and
protons trapped by the Earth's magnetic field. The areas of trapped radiation
are called Van Allen belts. Protons surrounded by an inner and outer belt of
electrons form a belt which circles the Earth like a doughnut. NASA discovered
these belts in 1958 during the Explorer I mission. They are referred to as the
inner and outer Van Allen radiation belts, after James Van Allen who designed
Explorer I. The inner region is centered at about 3000 km above Earth and has a
thickness of about 5000 km. The outer region is centered at about 15,000 --
20,000 km above the surface of the Earth and has a thickness of 6,000 -- 10,000
km. Typically, manned space flight (such as the Shuttle) stays well below the
altitude of the van Allen radiation belts. Safe flight can occur below
altitudes of 400 km or so. The particles in Van Allen belts come from solar
flares, magnetic storms, and collisions of cosmic rays with particles in the
Earth's atmosphere.
All three forms of radiation can be extremely dangerous to
astronauts, especially when they are performing extravehicular and extra-colonial
activities (EVAs). The risk of radiation sickness will also increase on longer
voyages to places like Mars.
Ionizing
radiations in space
|
Name |
Energy
type (MeV) |
Charge |
RBE |
Location |
|
X-rays |
N/A |
0 |
1 |
Solar radiation, radiation belts and in
the secondaries made by stopping electrons and nuclear reactions |
|
Gamma
rays |
N/A |
0 |
1 |
|
|
Electrons |
1.0 |
1 |
1 |
Radiation belts |
|
0.1 |
1 |
1.08 |
||
|
Protons |
100 |
1 |
1-2 |
Inner radiation belts, cosmic rays,
solar cosmic rays |
|
1.5 |
1 |
8.5 |
||
|
0.1 |
1 |
10 |
||
|
Neutrons |
0.05 eV (thermal) |
0 |
2.8 |
Produced by nuclear interactions; found
near the planets and the Sun and other matter |
|
.0001 |
0 |
2.2 |
||
|
.005 |
0 |
2.4 |
||
|
.02 |
0 |
5 |
||
|
.5 |
0 |
10.2 |
||
|
1.0 |
0 |
10.5 |
||
|
10.0 |
0 |
6.4 |
||
|
Alpha
particles |
5.0 |
2 |
15 |
Cosmic rays |
|
1.0 |
2 |
20 |
||
|
Heavy
primaries |
N/A |
|
|
Cosmic rays |
The detection and measurement of radiation is
one of the most important functions the colonists will perform in determining
if radiation and/or radioactive contamination is present inside or outside the
settlement. Since humans can not sense ionizing radiation with their natural
senses, they will rely on instruments for detecting and measuring radiation.
They must be familiarized with the proper operation and use of the instruments
they have and intend to use even before reaching the orbital colony. That is
why both traditional and new radiation measurement methods will be used on the
Space colony.
Portable instruments, often called “survey meters”, will
play a major role in radiological protection inside the Settlement. They are
primarily used to detect contamination and to determine radiation field
intensities. Many radiation safety decisions, such as the need for
decontamination, shielding, personnel monitoring, change in work procedures,
etc., - will be based on radiological survey result using survey meters. The
majority of portable instruments are ionization chambers or Geiger-Mueller
counters.
Ion chambers are the simplest of all gas filled detectors.
Their normal operation is based on the collection of all the charges created by
ionization of radiation within the gas through the application of an electric
field. In the presence of an electric field, the drift of the positive and
negative charges represented by the ions and electrons constitutes an electric
current. Assuming that recombination is negligible, and all charges are
efficiently collected, the steady-state current which is produced is an
accurate measure of the radiation.
One of the important applications of ion chambers is in the
measurement of gamma ray exposure and exposure rate.
Portable ion chambers of many designs will commonly be used
as survey instruments for radiation monitoring purposes. The typically consist
of an air volume of several hundred cm3 from which the saturated ion current is
measured using a battery powered electrometer circuit. Walls are typically
air-equivalent, and are usually made of plastic or aluminum. These instruments
will give relatively accurate measurements of the exposure from gamma ray
energies inside the colony.
Another device efficient in measuring radiation levels is
the Geiger-Mueller (G-M) counter, which is probably the best known radiation
detector. It is popular because it is simple in principle, inexpensive to
construct and purchase, easy to operate, sensitive and reliable as a detector
of ionizing radiation. It will be particularly useful for radiation protection
surveys.
Simply constructed, a G-M counter consists of a type of gas
(usually helium, neon or argon). A positive high voltage source is then
connected between the shell and the wire. Any incident particle that ionizes at
least one molecule of the gas will initiate a succession of ionizations and
discharges in the counter.
These GM survey meters will be used for detecting alpha,
beta, and gamma radiation. With the detector window facing the radiation source
and held very close to it, all three radiations can be detected. With a solid
metal part of the detector (probe) facing the source of radiation, only
gamma radiation will be detected. The detection of either alpha and/or beta radiation
suggests the presence of radioactive
contamination.
X-ray imaging is also an important technique which will be
used in variety of applications such as nondestructive evaluation, radiology in
medicine, astronomical observations, X-ray diffraction for materials studies,
and others. The ability of X-rays to penetrate deep in to matter allows
investigation of interior components with possibility of real-time dynamic
studies. However, while significant advances have been made in X-ray sources as
well as image processing steps, the X-ray detectors will remain a limiting step
in many of applications. Important requirements for the X-ray detectors used in
such applications include large area (~ 20 cm x 20 cm), high resolution
(100-200 um), wide dynamic range (10~), high sensitivity, compact design, and
low cost. Ability to provide real-time images is an additional requirement in
some applications. To address this situation, we have proposed to develop a
solid state, large area, high resolution imaging detector by combining the
semiconductor film (lead iodide, PbI2) technology being developed at RMID with
the large format amorphous silicon (a-Si:H) readout technology. The detectors
would be capable of performing static as well as dynamic
imaging.
The Space Settlement will also serve as a huge laboratory
for conducting a variety of experiments concerning radiation and radiation
measurements technology. Some of these experiments will continue those of the
ISS scientists.A good way to measure exterior radiation levels and their
effects on astronauts is using a replica of human torso, similar to Fred, but
with improved characteristics. Fred is NASA's Phantom Torso traveling in the
International Space Station. This replica of a human torso is composed of 35
one-inch layers, each carrying passive dosimeters to measure the total
radiation that travels through the torso. Real-time radiation levels will also
be measured in the Phantom's brain, stomach, heart, colon, and thyroid. Fred's
"skin" is made of Nomex, a non-flammable material used in the suits
worn by NASCAR drivers. Two more passive dosimeters in the "skin"
measure external radiation doses. The data from the internal detectors can then
be compared with data from the external detectors. This experiment can provide
information on how to better protect the astronauts and can also be used in
measuring radiation levels in the immediate proximity of the space colony.
Two other solutions for measuring radiation, which are used
onboard the International Space Station (ISS), could serve very efficiently the
space settlement’s needs. One of them is the German Space Agency’s Dosimetric
Mapping System. An improved version of the system will be designed to measure the
different types of radiation that are penetrating the outside of the
Settlement. Dosimeters specific to various types of radiation will be placed in
the areas of major interest, such as residential and industrial areas. These dosimeters will record radiation levels
for long periods of time. High energy particles entering the Space Colony will
be measured by the tracks they leave behind in the Nuclear Tracking Detector
Packages. Two Dosimetry Telescopes will be placed in the industrial area, where
they will measure ions streaming into the Settlement, while 12
thermoluminescence dosimeters will measure the neutron dose.
The third measuring solution, the Bonner Ball Neutron
Detector, comes from the Japanese Space Agency, NASDA. Its primary function is
to measure neutron radiation. Because neutrons pass through an astronaut's skin
and may damage the bone marrow, we will dedicate experiments to recording data
on neutrons. The Bonner Ball consists of 6 spheres filled with Helium 3 and
connected to the control unit by a wire. Each sphere is covered with
polyethylene, the material used to protect sailors in nuclear submarines.
Neutrons enter each sphere where they react with the Helium to form electrons.
These electrons travel in a current down the wire into the control unit where
this current's strength is recorded. Scientists will collect information which
will allow them to assess the risk astronauts experience while traveling
through the exterior layers of the Space colony.
1 b. Effects
oflong term exposure to radiation
The radiation environments encountered in space are
different from the natural background radiation on Earth and are complex in
nature. Both bacteria and eukaryotes have evolved a series of mechanisms to
respond to similar damages on Earth.
As we have already shown, the space radiation environment
is largely comprised of positively charged particles such as protons and helium
ions and negatively charged electrons. The Earth's magnetic field serves as a
shield against charged particle radiations. The primary sources of radiation in
space are traditionally classified into trapped particle radiation, galactic
cosmic radiation, and solar particle radiation.
The galactic cosmic radiation (GCR) is the major radiation
in interplanetary space and is comprised primarily of charged particle
radiation. Of the different charged particles that make up the GCR, 87% are
protons, 12% are helium ions, and 1% are heavier ions that are of high
energies. Iron is the most important of these heavier ions due to its abundance
and the amount of energy each iron ion can deposit as it interacts with matter.
The sun contributes in a dynamic way to the space radiation
environment. Solar particle events (SPE) are large intermittent emissions of
protons, helium, and sometimes heavier ions from the sun. The frequency of SPE
varies within the solar cycle.
The different
charged particle radiations in space have biological consequences that are
dependent upon the spatial distribution of the energy they impart to the cell
or tissue. As charged particles pass through matter, they slow down. The energy
deposited is a function of the energy of a given particle, and the greatest
amount of energy deposited by a particle comes at the very end of its track.
Protons are generally sparsely ionizing radiations until they reach the very
end of their tracks, while the heavier ions are densely ionizing at the
beginning of their path and become more so as they slow down.
For short excursions outside the Space settlement, such as
have previously occurred, the small dose increments might be expected to have
little or no effect on astronauts. However, longer-duration space travel, such
as to the moon or different celestial bodies, may be another story. Radiation
doses may be sufficient to cause measurable increases in cancer or mutation
risk. However, radiation-induced cancer and mutations are rare effects at any
dose, and large populations are required to measure effects with statistical
reliability. It may be possible, though not terribly likely, that some
radiation doses in space may be sufficient to cause acute radiation sickness.
This is a deterministic effect of radiation, with a threshold dose for symptoms
of about 250 mSv at a high dose rate. For protracted exposure at a lower dose
rate in space, the threshold dose is substantially greater, perhaps up to 1 Sv.
The NCRP estimated that if a major solar particle event occurred during a visit
to the moon, it could give the astronauts doses to their skin of 6 Sv (600 rem)
with bone marrow doses of close to 0.9 Sv (90 rem).
Cells, tissues, and whole organisms have evolved a myriad
of responses to the types of damage that can be caused by charged particle
radiations. The early responses to charged particle exposures include
recruitment of DNA repair machinery, changes in gene expression, the initiation
of programmed cellular responses such as apoptosis, and alterations in the
tissue microenvironment.
Included among the initial types of damage that result in
DNA following exposure to charged particle radiations are base damage,
single-strand breaks, and double-strand breaks. Bacteria and eukaryotes have
highly complex systems for the repair of these alterations, which can also
result from naturally occurring errors in replication, changes that result from
ongoing oxidative metabolism, and exposure to chemicals of various kinds.
Following exposure to sparsely ionizing radiations, base damage and strand
breaks are widely scattered throughout the cell nucleus. For densely ionizing
radiations such as iron ions, the alterations are often clustered. Most of the
initial damage to DNA is efficiently removed prior to the next cell division
cycle by processes including nucleotide excision repair and double-strand break
repair. It has been suggested that the clustered damages associated with
densely ionizing radiation exposures may recruit multiple repair pathways to
the site of damage. The resulting "traffic jam" may lead to an
alteration of the efficiency of repair.
The programmed cell death pathway may be important in
maintaining tissue integrity in the space radiation environment by removing
damaged cells before they can divide. Virtually all cells in multicellular
organisms have evolved a system of altruistic suicide that is often referred to
as programmed cell death or apoptosis. This process is critical to normal
development and tissue homeostasis. Apoptosis is regulated by a series of
proteins that function as either effectors or suppressors of the process.
Through a complex series of heterodimeric and homodimeric interactions, these
proteins act as a "rheostat" to promote or suppress apoptosis. The
amounts of the various components of the "rheostat" are altered in
response to exposure to both sparsely and densely ionizing radiations. One of
the key players in the regulation of the apoptotic process is the p53 gene,
which has been referred to as the "guardian of the genome". P53 is
expressed in response to ionizing radiation exposures and serves to
downregulate one of the natural suppressors of apoptosis, bcl-2. Cells which
have lost the ability to initiate the normal apoptotic pathway appear to
accumulate mutations more readily following exposure to sparsely and densely
ionizing radiation.
In the context of organized tissues, there are additional
factors that mediate responses to charged particle radiations. The
extracellular matrix (ECM) and the cytokine environment provide signals that
help maintain tissue integrity and normal development of the organism. The ECM
influences cell morphology, mediates proliferative capacity, and regulates gene
and protein expression. The ECM can promote cancer progression and incidence.
Tissues respond to charged particle radiations by rapidly remodelling the ECM.
The time course and characteristics of the remodelling are different in
different tissue compartments. The long-term effects of this remodelling are
fertile areas of investigation.
In conclusion, biological systems have evolved a series of
mechanisms at the cell and tissue level to respond to the types of damages that
occur as a consequence of exposure to the various components of the space
radiation environment. In large part, these responses evolved to protect the
integrity of the organism.
Still radiation can cause immeasurable damage by
penetrating the skin and destroying cells. Many possible problems can ensue,
depending upon the severity of the damage. Temporary sterility in men and
women, bone-marrow damage, radiation burns, cancer, chromosome breakage, and
damage to the central nervous system are all possibilities. Although these run
the gamut from mild to serious for those of us on Earth, they all spell trouble
in space. If an colonist on the Space Settlement becomes ill, he may not be
able to complete all necessary tasks and may have impaired judgment. That is why
prevention and protection procedures must be efficiently conceived and fully
operable.
1 c. Radiation
prevention and protection
As said, a significant difficulty for manned missions
outside of the Earth's magnetosphere, including colonization related activities,
asteroid exploration, and space-based mining and manufacturing, is the hazard
of crew exposure to particulate radiation. Crew radiation shielding must become
an active problem for investigation.
Two types of radiation are particularly significant and
must be reduced as possible: solar flare protons, and high-energy galactic
cosmic rays (GCR). Solar flare protons come in bursts, lasting a day or so,
following an energetic solar event. The proton flux is omnidirectional;
although the source of the radiation is solar, the actual radiation comes from
all directions, and hence the orbital colony must be shielded in all
directions, and not just in the direction of the sun. In the absence of
shielding, a single large solar flare would likely be fatal to the crew, either
immediately or as a result of cancers induced by the radiation dose. Cosmic
rays are a continuous background consisting of extremely high energy heavy
nuclei, and are also omnidirectional. While the GCR background is not
immediately fatal, the integrated GCR dose over long missions will approach or
exceed the recommended maximum allowable whole-body radiation dose.
The dangerous components in both solar flare and GCR
radiation consists of positively charged particles. Neutral radiation (gammas,
neutrons) are a negligible component of the radiation ambient; negative
particles (electrons), while present, can be easily shielded. The positive
particles, however, are extremely penetrating, and require massive shields. In
the case of GCR, a small amount of mass shielding has no benefit, or even
negative benefit over no shielding at all, since the impact of GCR nuclei on a
light shield will produce secondary radiation considerably more intense than
the original GCR.
Since the particles involved are charged, an alternative
solution to the problem of shielding is the use of active electromagnetic
shields. The simplest such device would be the magnetic dipole shield. The
magnetic field of the Earth is a good example of a magnetic shield, and is responsible
for the relatively benign radiation environment on Earth. A magnetic shield
makes use of the fact that a charged particle's trajectory in a magnetic field
is curved. As a particle enters the region of high magnetic field, its
trajectory will curve away from the region to be protected. The advantages of a
magnetic shield to crew safety and health are obvious.
An additional advantage of the magnetic shield is that no
secondary radiation is produced by interaction of the shielded area with the
incident radiation.
The limit to the mass needed to produce a magnetic field is
determined by the tensile strength of materials required to withstand the
magnetic self-force on the conductors. For the minimum structure, all the
structural elements are tensioned, and from the virial theorem, the mass
required for withstand magnetic force can be estimated as:

where
is the density of the
structural material, S is the tensile strength, B the magnetic field, V the characteristic
volume of the field, and
the permeability of
vacuum.
An alternative to the magnetic shielding is to use an
electrostatic shield. Since both solar flare protons and heavy nuclei in GCR
radiation are positively charged, shielding would simply require adding a
positive charge to the object to be shielded sufficient to repel the particles.
To shield against solar flare protons would require an electrostatic potential
of on the order of 1 E8 volts; shielding against cosmic ray nuclei as well
would require as much as 1 E10 volts.
Unfortunately, the situation is complicated by the
interplanetary plasma. Attempting to simply charge the colony in Earth orbit
would result in electrons being attracted by it. This would discharge the
settlement very quickly. In this case, to maintain a charge of 2.E8 volts would
require a power of 1 E7 kilowatts.
Con-centric spheres of opposing charge to repel both
positive and negative particles, would reduce the discharging, but maintaining
the required voltage difference over a small distance is beyond the range of
current technology.
Another solution would be using a hybrid of the magnetic
shield and the electrostatic shield, the "plasma shield." An
electrostatic charge is applied to the vehicle (or habitat) shell to repel the
positively charged radiation; a magnetic field then prevents the plasma
electrons from discharging the vehicle. At large distances the shield is charge
neutral, since the magnetically confined electrons exactly neutralize the
charge on the shell. Since electrons are lighter than protons by a factor of
1860, the magnetic field required for the plasma shield is reduced over that
for a simple magnetic shield by the same ratio, and hence the weight associated
with the field generation and structure. This ratio is even more favorable for
shielding from cosmic rays.
The required electron confinement time tau to maintain the
charge, assuming a maximum allowable energy expenditure of 10 kW (for the 5m.
radius torus assumed), is 100 minutes. With the assumed plasma density n of
2.E9 e-/cm3, the confinement product n tau is 1 E13/cm3-sec. Magnetic
containment systems for fusion applications have demonstrated n tau products in
excess of E14 /cm3-sec at considerably higher temperature, so maintaining the
charge is not unreasonable.
The plasma shield will be made even more effective if it is
used in combination with a passive mass shield, since the mass shield is most
effective for low energy particles.
Still the most efficient and simple way of protecting
against radiations and solar flares is using an electromagnetic shield. This
topic is detailed in the next chapter (“Electromagnetic shielding”).
The choice of material and thicknesses for best radiation
blocking are dictated primarily by structural and thermal considerations.
Metals (which meet all these considerations) are generally opaque to UV, X-ray
and gamma-ray radiation.
Recent advances in high-temperature superconductors mean
that it is reasonable to consider superconductors operating at 77K or higher on
the orbital colony. This is a range which will allow use of passive cooling,
where the temperature is achieved by directly radiating excess heat to space, a
considerable advantage over use of superconductors requiring liquid He
temperatures.
Extremely high strength to weight composite materials could
be the best solution. Since the limit to magnetic field strength is produced by
the tensile strength of materials required, composite materials with strength
to weight ratios five times (Kevlar 49) to 7 times (PBO) higher than that of
steel allow considerable weight reduction in the tension members.
The most important enabling technology, which must be
available on the orbital colony, will be the ability to form high-temperature superconductors
into wires, process which will take place deep inside the industrial core of
the settlement. While magnetic shielding can be done using conventional (low
temperature) superconductors, the pay-off in simplicity and weight of higher
temperatures is so great as to be mission-enabling. Clearly, advances in the
critical current and the transition temperature will also allow significant
gains to be made as well. A second required technology which must be
demonstrated is the cooling of wires to the superconducting transition
temperature using passive cooling, essentially shielding the wire from the sun
and allowing it to radiate to deep space.
However, the skin of the forward fuselage of the orbital or
mining modules will be made of
'conventional 2024 aluminum alloy', while the crew compartment will be
constructed of 2219 aluminum alloy plate. The windows will be comprised of
either 2 or 3 panes of glass, depending on the window location, with the panes
between 0.25 and 1.3 inches and made of either aluminosilicate or fused silica,
similar to those found on today’s shuttles.
Spacesuit and spacecraft windows will be specifically
designed to block most of the UV radiations that pass through.
An important requirement is that little or no magnetic field
should penetrate into the inhabited region, due to concern about the hazardous
effects of long-term exposure to magnetic fields. However, considerably simpler
engineering designs can be made if some magnetic field is allowed to penetrate
into the shielded region.
In cases of emergency, well-shielded areas that can sustain
life for a few days until the particles die down can work as shelter from
unusual powerful solar flares. A good place for such special radiation-isolated
areas would be in the center of the ship, surrounded by the water tanks.
The moon may also represent a source of radiation which
must be taken into account during the mining operations. The majority of
radiation on the moon is in the form of charged particles (protons and helium
nuclei) from the sun. Most of the rest is ultraviolet radiation (UV). UV, of
course, will not penetrate even a small thickness of lead, and neither will
charged particles. On the other hand, these radiations will not penetrate other
materials, such as rock, plastic, and so forth. It's not necessary to use lead
for shielding on the moon because it's too heavy. The use plastic will be more
efficient. As for the thickness, it depends on the energy of the incoming
protons—a few cm may suffice, or maybe as much as a few tens of cm.
d.
Electromagnetic shielding
As we said before, electromagnetic shielding is the most
convenient way of protecting against ionizing radiations in space. The
principle is in fact simple: the magnetic shield is based on the fact that a
charged particle's trajectory in a magnetic field is curved. When the particle
enters the region of high magnetic field, its trajectory will be curved away
from the region we want to protect from radiation.
For example, let’s consider
the Alpha particles (
) as radiating factor. They represent 8% of the maximum
amount of ionizing particles found in space. Their mass (m1) is 4
, their speed (v) is of approximately 1000 Km/s and their
electric charge (q) is 2e. The figure below shows the particle’s change of
trajectory when entering a magnetic field zone.

We notice that in all cases the trajectory of the particle
is tangent to the magnetic field zone in point P. This can also be shown using
a geometrical demonstration, based on the drawing below:

Knowing the electromagnetic induction of the field (
), the mass (
), the speed (
) and the charge (q) of the Alpha particle, we can determine
the
) and the radius of the particle’s circular trajectory (
).

![]()
Let’s assume that
R=R0 (the radius of the magnetic field). For generating and
maintaining a certain magnetic field around the torus we will use a series of
close wound bobbins placed on the exterior margins of the torus, powered by
photovoltaic panels. The distance between coils can be calculated by taking into account the
electromagnetic induction we wish to generate.

We can determine the
inductance of a singe-layer coil according to the Wheeler formula, which
states:
![]()
We can also find the amperage
needed to maximize the efficiency of the electromagnetic field.
;
- the Solar power per
square meter
;
- the radius of the electromagnetic field

Taking into account that the
coils will be entirely exposed to the ionizing radiations, we have chosen the
radius of a coil (R0) to be half of its length (l).
![]()
; S- the surface of the coil face to the Sun
; P – the power generated on a coil;
- the efficiency of the photovoltaic panel
; n – the number of turns (n=104)
![]()
The determined amperage is
very low and thus it is very easy to generate. The electromagnetic field
created by the sysem of coils will be functioning at satisfactory efficiency
and will protect the torus from ionizing radiations.
For obtaining a more intense
electromagnetic induction using the same amperage and without having to increase the length of the
coil systems we could use multi-layered coils, which consist in a number of
concentric common coils. We will be able to generate a more intense electromagnetic
field with almost the same use of energy.
Still there will be points
found in less intense electromagnetic field somewhere between the coils, but
they will not raise any problem because of their simetric repartition.

2. Artificial
gravity
a. Means of
creating pseudogravity
After studying the effects of the 0 gravity habitats, we
reached the conclusion that artificial gravity is extremely necessary for the
health and the normal life course of the colonists.
|
Constant |
Significance |
|
R |
radius from rotation axis |
|
r |
radius of floor |
|
|
angular velocity of habitat |
|
Acent |
centripetal acceleration |
|
ACor |
Coriolis acceleration |
|
acent |
relative centripetal acceleration, for circumferential motion
in the habitat's plane of rotation |
|
X,Y,Z |
inertial Cartesian coordinates |
|
x,y,z |
relative Cartesian coordinates, tied to the rotating
habitat |
|
T |
elapsed time |
|
|
tangential velocity |
|
|
normal velocity |
|
|
composed velocity |
While the Space Settlement is spinning, the floor of the
space station would apply a centripetal force on the persons to keep them
traveling in a circular path, thus an object
in circular motion with and angular velocity
around a circle of
radius R experiences a centripetal acceleration
which will be the
pseudo constant g, similar on Earth.
Abnormalities in free-fall motion reveal abnormalities in
the gravity itself. To facilitate a side-by-side comparison of various gravity
environments, it's useful to specify a few standard tests:
Drop

The figure shows the motions of an observer and of a
particle which drops from a height h.
In the inertial frame:
Before striking the floor, the particle travels a linear
distance in the inertial frame:
, and subtends an angle of:
![]()
If the observer had not dropped the particle it would have
traveled the same distance on a circular path subtending an angle of:
This is the angle that the observer subtends while the
particle is falling.
In the observer's rotating frame of reference, the particle
will strike the floor at an arc distance from the observer:
, where positive is east (prograde) and negative is west
(retrograde). The particle always deflects to the west, because:
![]()
The angles
and
depend only on the
initial height h and the floor radius r. If the expressions are
rewritten in terms of the ratio
, they become:

Smaller ratios of h to r result in smaller
angles, smaller angle differences, and a more vertical path as seen from the
rotating frame.
The angular velocity
and centripetal
acceleration Acent influence the speed at which the particle
falls, but not the path it follows. The elapsed time will be: ![]()
Hop
The figure below shows the motion of a particle that hops
vertically from the floor with an initial relative velocity v.

First we write the tangential velocity dependency of the
radius

The resultant force is 0 thus,
![]()
![]()
For our particular case:

From here we calculate the normal velocity:
![]()
Now we can calculate the composed velocity from:

Here we calculate the distance between detachment and the
landing points:
![]()
The time between the detachment and the landing moment:
![]()
![]()
and
![]()
We can calculate ![]()
![]()
b.
The effects of artificial gravity and zero-gravity on human metabolism
Zero
gravity has diverse effects on the human body, some of which lead to
significant health concerns. We can easily conclude that it would be much
healthier for crews to provide artificial gravity for long duration space
habitation. This means rotating the habitat to produce artificial gravity by
use of the centrifugal force.
For
very small habitats, rotating them produces artificial gravity which results in
some very noticeable differences with real gravity due to the Coriolis Effect.
When you drop an object, it does not fall straight now, but falls by a curve
(according to the perspective of the person inside the rotating habitat).
While
standing up, your upper body will find itself significantly leaned over if you
are in a small habitat rotating fast. For larger habitats, these effects are
diluted to where they are humanly unnoticeable. If we want artificial gravity
in spacecraft or small habitats and strive for a most economical design, then
we need to understand the significance of rotation on humans. The analogy to
the comfort of sailors on ships at sea is appropriate. Large ships are more
comfortable than small ones.
Based
on experiments on people in centrifuges and slow rotation rooms, it appears
that the maximum rotation rate appears to be around 4 revolutions per minute.
The
main reason for lowering radius would be simply economics in an early space
habitat in that lower radius means less material needed, including designs for
stress. However, in a scenario using asteroidal or lunar material whereby the
costs of material in orbit is much lower; we will opt for larger habitats and
Earth-normal gravity.
Space
stations in low Earth orbit have not used artificial gravity for several
reasons: so that they could be smaller and cheaper; many of the experiments to
be conducted by the station were in microgravity.
For
connecting the spent fuel tanks to produce a space station situated in orbit,
we can just put a long cable between them and rotate the structure.
Studies
indicate that familiarity with gravity is learned in infancy. An infant at 4
months begins to realize that a rolling ball cannot pass through an obstacle,
but are not yet aware that an unsupported ball will fall. When they have 5
months, they discriminate between upward and downward motion. At 7 months, they
show sensitivity to gravity and the “appropriate” acceleration of a ball
rolling upward or downward. By adulthood, falling objects are judged to move
naturally only if they accelerate downward on a parabolic path. These judgments
are based not on mathematical reasoning, but on visual experience.
These
common-sense ideas, rooted in the experience of terrestrial gravity, permeate
architectural theory. A habitat design for a gravitational environment
distinctly different from Earth’s requires a fundamental reexamination of
terrestrial design principles. The goal is not to mimic Earth, but rather, to
help the inhabitants adapt to the realities of their rotating habitat. In
artificial gravity, the effects of Coriolis acceleration and cross-coupled
rotation arise only during relative motion within the rotating habitat.
One
phenomena which is taken for granted on Earth but cannot be in space, is
vestibular perception. It might be possible, through experience in a properly
designed habitat, to acquire a transformation tendency to vestibular perception
from visual, acoustic, haptic, or other perceptions. The goal is not to induce
motion sickness by the mere sight of some visual cue. Rather, it is to provide
visual or other reminders that motion relative to these cues will result in
certain inescapable side effects, inherent in the artificial gravity. These
perceptual cues would act as signals, triggering adaptive coordination in the
inhabitants. From the designer’s point of view, a consistent vocabulary of such
signals would have to arise from convention. From the inhabitants’ point of
view, these conventions might to some extent be taught, but the unconscious
transformation to a vestibular image would rely on association based on direct
experience.
It is
ironic that, having gone to great expense to escape Earth gravity, it may be
necessary to incur the additional expense of simulating gravity in orbit
because the consequences of long-term exposure to weightlessness.
(*)
|
Effect |
Description |
|
fluid redistribution |
Bodily fluids shift from the lower extremities toward the head |
|
fluid loss |
The brain interprets the increase of fluid in the cephalic area
as an increase in total fluid volume. In response, it activates excretory
mechanisms. This compounds calcium loss and bone demineralization. Blood
volume may decrease by 10 percent, which contributes to cardiovascular
deconditioning. Space crew members must beware of dehydration |
|
electrolyte imbalances |
Changes in fluid distribution lead to imbalances in potassium
and sodium and disturb the autonomic regulatory system |
|
cardiovascular changes |
An increase of fluid in the thoracic area leads initially to
increases in left ventricular volume and cardiac output. As the body seeks a
new equilibrium, fluid is excreted, the left ventricle shrinks and cardiac
output decreases. Upon return to gravity, fluid is pulled back into the lower
extremities and cardiac output falls to subnormal levels. It may take several
weeks for fluid volume, peripheral resistance, cardiac size and cardiac
output to return to normal |
|
red blood cell loss |
Blood samples taken before and after American and Soviet flights
have indicated a loss of as much as 0.5 liters of red blood cells. Scientists
are investigating the possibility that weightlessness causes a change in
splenic function that results in premature destruction of red blood cells. In
animal studies there is some evidence of loss through microhemorrhages in
muscle tissue as well |
|
muscle damage |
Muscles
atrophy from lack of use. Contractile proteins are lost and tissue shrinks.
Muscle loss may be accompanied by a change in muscle type: rats exposed to
weightlessness show an increase in the amount of "fast-twitch"
white fiber relative to the bulkier "slow-twitch" red fiber. In
1987, rats exposed to 12.5 days of weightlessness showed a loss of 40 percent
of their muscle mass and "serious damage" in 4 to 7 percent of
their muscle fibers. The affected fibers were swollen and had been invaded by
white blood cells. Blood vessels had broken and red blood cells had entered
the muscle. Half the muscles had damaged nerve endings. which is independent
of weightlessness. |
|
bone damage |
Bone
tissue is deposited where needed and resorbed where not needed. This process
is regulated by the piezoelectric behavior of bone tissue under stress.
Because the mechanical demands on bones are greatly reduced in micro gravity,
they essentially dissolve. While cortical bone may regenerate, loss of
trabecular bone may be irreversible. Diet and exercise have been only
partially effective in reducing the damage. Short periods of high-load
strength training may be more effective than long endurance exercise on the
treadmills and bicycles commonly used in orbit. Evidence suggests that the
loss occurs primarily in the weight-bearing bones of the legs and spine.
Non-weight-bearing bones, such as the skull and fingers, do not seem to be
affected |
|
hypercalcemia |
Fluid
loss and bone demineralization conspire to increase the concentration of
calcium in the blood, with a consequent increase in the risk of developing
urinary stones |
|
immune system changes |
There
is an increase in neutrophil concentration, decreases in eosinophils,
monocytes and B-cells, a rise in steroid hormones and damage to T-cells. In
1983 aboard Spacelab I, when human lymphocyte cultures were exposed in vitro
to concanavalin A, the T-cells were activated at only 3 percent of the rate
of similarly treated cultures on Earth. Loss of T-cell function may hamper
the body's resistance to cancer -- a danger exacerbated by the high-radiation
environment of space |
|
interference with medical procedures |
Fluid redistribution affects the way drugs are
taken up by the body, with important consequences for space pharmacology.
Bacterial cell membranes become thicker and less permeable, reducing the
effectiveness of antibiotics. Space surgery will also be greatly affected:
organs will drift, blood will not pool, and transfusions will require
mechanical assistance |
|
vertigo and spatial disorientation |
Without
a stable gravitational reference, crew members experience arbitrary and
unexpected changes in their sense of verticality. Rooms that are thoroughly
familiar when viewed in one orientation may become unfamiliar when viewed
from a different up-down reference. There is evidence that, in adapting to
weightlessness, the brain comes to rely more on visual cues and less on other
senses of motion or position. |
|
space adaptation syndrome |
About
half of all astronauts and cosmonauts are afflicted. Symptoms include nausea,
vomiting, anorexia, headache, malaise, drowsiness, lethargy, pallor and sweating.
Susceptibility to Earth-bound motion sickness does not correlate with
susceptibility to space sickness. The sickness usually subsides in 1 to 3
days |
|
loss of exercise capacity |
This
may be due to decreased motivation as well as physiological changes.
Weightlessness also makes it clumsy: equipment such as treadmills, bicycles
and rowing machines must be festooned with restraints. Perspiration doesn't
drip but simply accumulates. |
|
degraded sense of smell and taste |
The
increase of fluids in the head causes stuffiness similar to a head cold.
Foods take on an aura of sameness and there is a craving for spices and
strong flavorings such as horseradish, mustard and taco sauce |
|
weight loss |
:
Fluid loss, lack of exercise and diminished appetite result in weight loss.
Space travelers tend not to eat enough. Meals and exercise must be planned to
prevent excessive loss |
|
flatulence |
Digestive
gas cannot "rise" toward the mouth and is more likely to pass through
the other end of the digestive tract |
|
facial distortion |
The
face becomes puffy and expressions become difficult to read, especially when
viewed sideways or upside down. Voice pitch and tone are affected and speech
becomes more nasal |
|
changes in posture and stature |
The
neutral body posture approaches the fetal position. The spine tends to
lengthen. Each of the Skylab astronauts gained an inch or more of height,
which adversely affected the fit of their space suits |
|
changes in coordination |
Earth-normal
coordination unconsciously compensates for self-weight. In weightlessness,
the muscular effort required to reach for and grab an object is reduced.
Hence, there is a tendency to reach too "high" |
A conclusion after all these is that artificial gravity can
approach Earth-normalcy within any non-zero tolerance, provided that the radius
and tangential velocity are large and the
angular velocity is small.
3. Atmosphere
a.Effects of the artificial gravity on the
atmosphere

The spinning motion of the Settlement around its symmetry axis
causes different atmospheric pressure values in different points of the colony,
depending on their distance to the center of the torus. The atmospheric
pressure will decrease from the exterior circumference of the torus to its
center, following the law deduced in this chapter.
Towards the OY axis we consider a very thin disc of air of
mass dm, found in mechanical equilibrium
under the action of the forces of pressure which simulate the effects of
gravity on the atmosphere. The “disc” is shown in the figure below:
We can apply the fundamental principle of dynamics for the
state of equilibrium:
[1]
We can also express the dm mass as:
[2]
The equation of state for the gaseous disc is:
[3]
resulting in
[4].
According to relations [2], [3] and [4], relation [1]
becomes a differential equation:
[5]
In the mathematical relation above, p is the
air pressure at distance y towards
the center of the Settlement, dp –
the pressure rise according to the dy
dsitance, μ – the molar mass of
the air, ω – the angular speed
of the torus around its axis, T – the
average termodinamic temperature inside the colony, which is assumed to be
constant and equal to 293 K (corresponding to 20oC), Rg - the universal
gas constant (8310 J Kmol-1 K-1). The equation can be
solved by performing an integral calculus:
,
[6],
C is an integration constant.
Its value can be determined by requiering the pressure at ground level (y=R;, R – the major radius of the torus;
R=4011m) to be similar to that on Earth (p = p0
105 Pa).
resulting
in
[7]
By interpolating relation [7]
in relation [8] we obtain:
[8]
We can transorm the
logarithmic function into a exponential dependency. Therefore, relation [8]
becomes:
[9],
Relation [9] puts forward in an adequate form the variation
of the air pressure inside the Settlement according with the distance from the
residential surface, measured towards the center of the torus, along a
transport column leading to the center of the orbital station.
We notice that the pressure
inside the 0 gravity body is not null.
[10]
Trot is the
rotation period of the settlement around its simmetry axis (Trot=127s).
It appears that the pressure
inside the central body of the colony is eligible for sustaining life in case
part of the population is evacuated and sheltered there, as it exceeds the air
pressure on top of the highest mountains on Earth.
Phisiological implications of atmosphere
Creating an atmosphere that can sustain life is extremely
important, but at the same time extremely difficult, because there are many
problems to consider.
Pressure and its influence on blood absorption of gasses is
one of the major problems, because of its’ physiological implications.
High pressures create embolia, the gass absorption being
stopped and we do not need that. This is the reason why we calculated a normal
air pressure in the settlement of ½ atmospheres, in order to make the blood gas
absorption easier. This also creates a smaller amoung of gass that has to be
generated or imported to the station.
Atmosphere Composition
In order to preserve acceptable living conditions we have
to recreate Earth’s atmospheric pressure, keeping the molar fractions of the
gasses constant.
Earth’s atmosphere consists of: 20% O2 , 78 %N2,
and 2% other gasses (volumes).
Oxygen’s molar fraction is:
20/100=0.2 (volume percents equal mole percents because a mole of any
gas in the same environment conditions occupies the same volume; for example:
in normal conditions at 0o Celsius (273K) and 1 atm a mole of any
gas occupies a volume of 22.4 L or dm3
according to Avogadro’s law). Nitrogen’s molar fraction is 0.78,
and other gasses’ molar fraction is 0.02.
The total volume of
the space station is 19754175000 m3 (the volume of the torus) + 815125000 m3 (the central
body’s volume), for a total of 20569300000 m3.
- number of moles
- number of moles of air needed in the settlement’s
conditions
of air
Oxygen’s molar fraction is: xO2=0.2
Number of kmoles of oxygen is : ![]()
kmoles of oxygen
Nitrogen’s
molar fraction is : xN2=0.78
Number of kmoles of nitrogen needed :
kmoles of nitrogen
Number of kmoles of other gasses:
kmoles of other gasses
Chemical generation of Oxygen
In order to preserve
the gaseous pressure in the station, we will have to constantly monitor the
oxygen, nitrogen balance and volume.
Some of the Station’s oxygen will be generated different ways, from two different types of
substances: from lunar and asteroidal ores that contain metal oxides, using the
separation methods presented in chapter 3, and from heated lunar ice water, by
its electrolysis:
2* |cathode (-)
2H2O(liquid) +2e-=> H2 (gas)+2OH-(aqueous)
[reduction]
anode (+) 2H2O(liquid) -4e-
=> O2(gas)+4H+ (aqueous) [oxidation]
Total process:
2H2O
=> 2H2 + O 2
This reaction needs 285,5 kJ per mole of water. ∆Hreaction=
571 kJ
This is also a source of hydrogen.
Oxygen is also used for the fabrication of ozone (ozein= to
smell), it’s triatomic allotropic state O3.It can be obtained with
UV lamps or by the cryogenic liquefaction of air. This can have a plentitude of
uses: medical uses and water disinfectant (see waste management). It’s a very
powerful oxidizing agent, and it must be produced close to its source of
application.
Hydrogen generation
Hydrogen generation is made from thermal extraction and
electrolysis (see separation methods). Another method would be from large
ammonia transports, by decomposing it into elements: 2 NH3=>N
2 +3 H 2, altering the equilibrium created with the reverse
reaction (by Le Chatelier’s principle). Asteroids contain also hydrogen
volatiles from which we can obtain the hydrogen.
Nitrogen generation
This gas is extremely important (a little rare), being one
on the gasses we have to transport in large amounts from Earth, under the form
of ammonia, so that we will be able to use the entire cargo.
Lunar ice water which was newly discovered to have amounts
of nitrogen dissolved in it. This is another source of N 2. The reason for this
surprising fact could be the meteor and asteroidal impacts in the past; another
space nitrogen source is asteroid volatiles containing nitrogen gas along other
gasses.
The lack of some volatiles can determine major problems.
Nitrogen is one of the most important because nitrogen sources are few and the
necessary quantities are great. Once created the biogeoecosystem the import of
ammonia will stop, because the circuit will be closed, and matter will not be
lost any more.
f.
CO2
concentration control and removal
Carbon Dioxide Elimination
Biological elimination is made by plants, which take the
carbon dioxide form the atmosphere and they use it as their own food.
We are aware of the importance of photosynthesis in the
carbon dioxide elimination process, but we have to take safety measures, and
find a backup system of elimination of CO2.Accidents may happen with
the plant population. We can use the dioxide to form water and methane with
hydrogen, and the compounds formed can be used to form water and in this manner
to reform the cycle.
Carbon Dioxide Reduction System (CRS)
In this cycle, CO2 reacts with hydrogen and
forms methane and water:
CO2 + 4H2 => CH4 + 2H2O + Q
This reaction can happen in a reactor, in catalytical
conditions. The water vapour formed in this manner is condensed on a cold
surface, so that the gas stream is composed only by methane. Water obtained
this way can be collected and the methane separated in a combustible gas
chamber or pipe.
The water can support the process of electrolysis, and it
is decomposed in Oxygen and hydrogen. Oxygen is released at the anode and is
collected and seprated, and hydrogen molecules are formed at the cathode. This
last gas is used at the restart of the cycle.
METAL OXIDES
Silver oxide reacts with CO2 and forms a silver
carbonate. Also Magnesium and lithioum oxides are viable to take part in this
process, but the highest chemisorbtion of CO is made by Ag.
Ag2O + CO2 => Ag2CO3 (in an aqueous environment)
SOLID AMINE WATER DESORBED
This is an elimination method that uses an ion exchange
resin that has the proprety of being able to chemically bond CO2
molecules to its structure. The total elimination of the gas can be made in
vacuum or even space, when tha dioxide molecules are dispersed.
ION EXCHANGE ELECTRODIALYSIS
This method has the same principle as the ne mentioned
above, but it is at the same time different. The compounds formed at the
surface contact between the ion-exchange resin and the dioxide are carbonates,
that can be easily eliminated in an electrical field, and at the same time the
resin is regenerated.
THE 4 BED MOLECULAR SIEVE (4BMS)
This device has a water side and a chemically active side.
In the active side, on of the beds has the function of actively adsorbing water
molecules, and at the same time the air is passed to the bed and the CO2
is adsorbed. The other beds have the
purpose of desorbing the water, which is eventually returned to the first phase
of the cycle.
THE SABATIER PROCESS
This process is based on the burning of CO2 in H
to produce Oxygen and methane gas. The process is exothermic (323K/mole CO2)
because of the destruction of the two double C=O bonds.
CO2
+ H2 =>CH4 + O2 + Q
THE BOSCH PROCESS
This is another process of transforming CO2 in
other products. In this case the products are solid black C and gaseous O2.
This reaction generates 431K per mole of CO2.
CO2
=> C + O2 + Q
Preventing contamination involves eliminating the risk
factors which could lead to the incapability of the organisms to function
within their normal adaptation limits.
Measuring toxicity levels inside a fully operative
ecosystem will surely not be an easy thing to achieve. For estimating the
distribution and level of toxicity we must first study the response of the
different communities of humans, animals and plants based on a specific
biochemical, physiological or behavioral endpoint.
For determining if exposure to a certain toxicant substance
will result in adverse responses for the Settlement’s biotope we must first
calculate the dose, the time and the frequency of exposure.
Therefore all habitats onboard the Space Settlement must be
permanently monitored and carefully studied. To achieve this, periodical tests
must be conducted upon both aquatic and terrestrial organism, including plants,
invertebrates and vertebrates. This complex monitoring system will be based on
highly sensitive chemo-sensors which will constantly examine the chemical
composition of air and water vapors and send the precise results to the central
data logger (trace contaminant control) for further analysis.
Still the best way of preventing contamination and thus
endangering the artificial ecosystem will be creating a strict set of rules
concerning the use, waste and recycling of the different materials onboard the
Settlement. Therefore, the distribution, exploiting and dumping of materials
will have to respect a certain cycle; meanwhile, several norms concerning the
industrial activities and the industrial waste management will help in
preventing chemical contamination.
The different substances onboard the Settlement will have
to follow the cycle presented below:

|
Diagram inspired from
http://science.nasa.gov/ |
e.
Ventilation and ventilation devices
Because
we have a perfect isolated habitat we need a very good ventilation to replenish
oxygen, dilute the concentration of carbon dioxide and water vapor, preventing
the infiltration of dust and atmospheric pollutants, and minimize unpleasant
odors. Thereby we will stop the effects of a poor air quality which can lead to
headaches, respiratory difficulties, sinus congestion, fatigue, throat and eye
irritation and poor concentration. For the houses’ interior we can use the
Indian Teepee principle.
The
exhausted air will be replaced with fresh air found at the temperature of the
torus, which is drawn into the building via low level louvers and doorways,
thus providing vertical air movement, which is the most natural and efficient
way to ventilate buildings.
Vertical air movement occurs due to lower density, warm air rising as it
expands becoming more buoyant. As cool air, which is dense and therefore
heavier, enters the building at low level it pushes the warm air upwards thus
developing convection currents. For the artificial “wind”, in the residential
zone and also in the
agricultural one, we can use common fans with aluminium
palettes for high efficiency.

|
General scheme of a common ventilation fan |
f.
Temperature and humidity control
We
must have automatic temperature control systems all over the torus and the
central body for maintaining a constant
normal temperature. A sensor will monitor the temperature inside the habitable
area and the agricultural area. If a temperature variation appears it
communicates with the controller, which will be linked to a microchip which is
able to increase or decrease the required temperature with a margin of safety
of maximum +/- 0.5°C.
A
Dehumidifier is an appliance that removes moisture from the air. Most of the
dehumidifiers work like refrigerators and air-conditioners. They have cooling
coils. Water vapor is condensed and removed from the air going through the
dehumidifier. This requires a lot of energy to condense water vapor and the
higher the background humidity level, the more energy it takes.
Other
types of dehumidifiers are made with the help of a silica gel impregnated on a
desiccant wheel with a fast heating coat made out of paper or fiber-glass. This
wheel is like a deep porous material that forces the air to get to the
desiccant substance. This chemical compound attracts the water molecules in its
pores, taking all the moisture from the air and incorporating it.
Low
humidity also can be harmful since excessive evaporation can irritate the
mucous membranes of the nose and bronchi, thus we need a device for creating
humidity. Studies show that for a person wearing light clothes, the ideal
conditions of well-being occur when the environmental temperature is between
23...25°C, and the relative humidity is between 40...60%. Also, in some
industrial processes the humidity favors we can avoid various inconveniences
consisting in the formation of electrical charges.
Besides
the natural humidification which has lot sources, we must use artificial ones
too. A type of artificial humidifier would be the one which nebulizes the water
producing a fine mist that is blown into the torus by a small fan incorporated
in the machine. The mist then evaporates immediately, humidifying the air. The
mist outlets can be orientated in every horizontal direction.
All these features will make an efficient and versatile
atmosphere control, suitable for creating an agreeable way of life.
VI.4.
Flora
a.
Plant growing and maintaining process
Plants
will be needed to produce O2 and food from simple substances like CO2
and H2O and they are essential for life support on the station. But plants also
need themselves conditions to live. The most important factors that influence
plant growth are nutrients (minerals, C, H, N, O, P, S), the soil and
climateric conditions (temperature, light, humidity, atmosphere composition).
Plant processes (like photosyntesis, circulation and respiration) are of major
interest for plant growing as well as for humans (photosyntesys produces oxygen
and organic compound such as glucose, intense respiration consumes oxygen etc.
*see nutrition in plants). If one of these functions is altered, the result
will be abnormal growing or even death.
The
soil is very important to plants, because it offers both support and almost all
nutrients. Because natural soil takes millions of years of development making
manufacturing almost impossible and its transportation from Earth would be very
expensive, artificial soil will be used with similar properties as the natural
one. The soil is in fact a solution; which contains both organic and inorganic
molecules.
Since
nutrients are by nature inorganic, the organic component is not strictly
necessary ( in nature is a continuous source of inorganic compounds, but the station
will be a closed system, so the organic detritus will be recycled and
transformed in simple, inorganic substances, which will be returned back to the
soil).
The
artificial soil will have two components: a biotic one (plant roots and other
organisms, needed to maintain the soil balance) and an abiotic component. The
abiotic component will comprise a polymer (which will have a structure and
consistency resembling with a sponge - like the natural soil- providing support and space for water and
other dissolved compounds -like nutrients), sand (silica)-small quantities,
calcar (CaCO3)-small quantities, nutrients and organic detritus (in
small quantities). An average depth of 5-7 meters will be sufficient for all
type of plants grown on the station. The soil will stay on a bed of rubber (10
cm deep), which is impenetrable for all substances solved in earth. Water will
be held in small spaces by capillarity (all spaces with a diameter smaller than
0.5 mm). Nutrients will be held by solving in water and by their attraction to
the negative charged membrane of the root absorbing cells.
The nutrients are divided into two major groups:
macronutrients (which are required in large amounts - approx. 1 mg per gram of
dry mass: C, H, O, N, P, S, K, Ca) and micronutrients (100 microg per gram of
dry mass: Cl,Fe,Mn,B,Zn,Cu,Ni,Molybdeum). These nutrients can be obtained
initially from the Moon and the Earth and then integrated into natural cycles
to be reused by the plants.
1. Sources of nutrients
2. Carbon source: => plants use CO2 as
source of carbon. CO2 will be obtained from respiration of humans, animals and
plants.
3. Oxygen source: => for glucose
(monozaharide) and polyzaharides or derivates (fructose) obtained from it the
main source of oxygen is CO2. In respiration, oxygen is taken from O2 -
produced by plants themselves. Even if O2 is consumed during
plant respiration and pho torespiration (a special type of respiration that
occurs when photosynthesis is blocked), the quantity of oxygen produced during
water hydrolysis (first part of photosynthesis) is much higher than the
quantity used for respiration, thus resulting a surplus that may be used by
humans and animals.
4. Hydrogen source: => the main source of hydrogen is water or the
free H+ ions from the soil.
5. Phosphorus source: => acids :(H2PO4)-
, (HPO4)2-;
salts: K3PO4, Na2PO4.
6. Potassium source: => K+ from potassium salts:
KCl, K2SO4 , KI solved in water
(Ionized form; e.g. for potassium
and clorure, free ions of K+
and Cl-).
7. Calcium source: => Ca2+ from salts (CaSO4, CaCl2)
or fine divided Ca.
8. Nitrogen source : => nitrogen will be taken from (NO3)-,
(NH4)+, NH3 and from the artificial atmosphere through nitrogen
fixation.
9. Iron, Zinc, Copper, Nickel, Manganese, Magnesium : => from fine
divided metal or their salts (FeCl2, FeCl3,
CuSO4, ZnSO4 etc.).
10. Boron source: => (BO3)3-, B4O7.
11. Molybdenum source: => fine divided molybdenum.
12. Chlorine source: => chlorine will be obtained from salts in their
ionized forms (K+, Cl-, Na+- Cl-).
13. Sulfur source : => (SO4)2-,
from salts or acids, solved in water.
Nutrients
are absorbed by plants in their ionized form (K+, Cl-, Mn2+,
Mg2+, Fe2+, Fe3+, Cu2+, Ca2+, (NO3)-, (SO4)2- or as gases (CO2,O2)
or liquids (H2O) through osmosis. Generally, nutrients are available for
plants in their most oxidized form (carbon as CO2,
hydrogen as water, phosphorous as phosphate, nitrogen as nitrate, and sulfur as
sulfate). In addition to CO2 and O2, plants are able to take up other compounds through their
leaves such as some sulfur oxides from the atmosphere. Plants can also be
fertilized by spraying their leaves with a nutrient solution (copper, manganese
and iron are more efficiently absorbed from such foliar spraying than from the
soil), but the pH of the solution and the concentration of nutrient ions within
must be carefully adjusted (in very large quantities, iron is toxic for plants
and a very low pH prevents ion absorption), and the plants must be sprayed at
the right “time of day”. Plants can adapt to nutrient - deficient soils by
directing their roots to patches of soil where the nutrients they lack can be
found.
Plant roots manifest a certain degree of selectivity.
However, the mineral composition of plants often reflects the composition of
the soil and water in which they grow, meaning that some minerals that are not
necessary for plants can accumulate in their body. Plants growing on mine
tailings, for instance, may contain gold or silver, and the nutritional value
of fruits and vegetables may vary depending on the composition of the soil. But
that means also that some elements that humans and animals need (like selenium
or natrium) can be absorbed by the plants from the soil and then used in
alimentation; they can provide a plentiful source of elements (provided that
the soil contains these elements).
|
Needed quantities and deficiency
symptoms of major plant nutrients |
|
ELEMENT |
FRACTION
(percent)% |
MAJOR USES DEFICIENCY SIMPTOMS |
|
Carbon |
45 - 50 |
In all organic molecules
retarded or abnormal growth |
|
Hydrogen |
5 - 7 |
In all organic molecules
retarded or abnormal growth |
|
Oxygen |
27 - 33 |
In most organic molecules;
respiration retarded or abnormal
growth |
|
Nitrogen |
8 - 10 |
In proteins, nucleic acids,
coenzymes, Chlorosis of leaves, beginning with lower leaves |
|
Phosphorus |
2 - 3 |
In nucleic acids and
phospholipids; in Retarded growth, blue green or dark green color; coenzymes
of energy metabolism; protein red, purple or brown pigments along
veins,regulatorbegining on underside of leaf |
|
Sulfur |
0.5 |
In proteins, coenzymes Chlorosis
of whole plant, retarded growth |
|
Potassium |
4 - 5 |
Major divalet cation in cytosol;
in chlorophyll; Dieback of growing points; blue-green or dark enzyme
activator green color, necrotic spots; leaf margins necrotic |
|
Calcium |
2 - 3 |
Cell wall component; maintains
membrane Dieback of growing points; affects meristems structure; regulates
cytoskeleton; second
(undeveloped terminal buds); stunted root growth; messenger in signal-transduction
pathway leaves curl |
|
Magnesium |
1 |
Major divalent cation in
cytosol; in clorophill; Marginal chlorosis and red, purple, or brown Enzyme
activator pigments in mature leaves first, with green venation |
|
Micronutrients |
Parts per million |
|
|
Chlorine |
500 ppm |
Photosyntesis; ionic balance in
cytosol Young leaves blue-green color and shiny, then become chlorotic, necrotic,
bronzed |
|
Iron |
500 ppm |
Enzyme activator; electron
carrier of ETS Chlorosis of young
leaves, but larger veins remaining green; short, slender stems |
|
Manganese |
250 ppm |
Enzyme activator; especially
Krebs cycle and Stunted, interveinal chlorosis in leaves; pale amino acid biosynthesis enzymes
overall coloring; leaves malformed, with necrotic |
|
Boron |
100 ppm |
Cofactor in chlorophill
synthesis; may act in Tissues hard, brittle; stems rough and cracked; carbohydrate transport; not well
understood growing tips damaged; flowering inhibited; heart rot of root
crops; poor legume nitrogen fixation |
|
Zinc |
100 ppm |
Enzyme activator; auxin
synthesis” Little leaf", rosette formation; leaves necrotic, twisted,
misshapen; late summer mottling leaves |
|
Copper |
30
ppm |
Enzyme activator, especially
redox reactions Dieback of growing points; leaves chlorotic or and lignin
biosynthesis; electron carrier blue-green
in color, elongated; leaf margins curl or roll |
|
Molybdeum |
0.5 ppm |
Enzyme activator, especially in nitrogen
Interveinal chlorosis; pale, distorted, yellow fixation and nitrate reduction
leaves, with margins that curl or roll; stunting |
|
Nickel |
|
Enzyme activator, nitrogen
metabolism |
As it
results from the table, nutrients deficiencies may cause severe disturbances in
plant metabolism. Any deficiency should be treated immediately after observed,
otherwise the plant will die.
Light
is essential for plants and they cannot live without it. It influences
circulation and its absence prevents photosynthesis.Light is one type of
electromagnetic radiation, a form of energy that behaves like both a particle
and an oscillating wave, straining the human ability to represent natural
phenomena realistically.
As a particle, each unit of EM radiation is
called a photon. It travels at a velocity (c), which is 3x(10)8 meters/sec in
vacuum; the radiation also vibrates with a frequency of a vibration per second
and has a wavelength of lambda. The photon may be considered a packet or
quantum of energy. But not all the light is used by plants. Only red ad blue
light is absorbed and the rest is reflected (that’s why the color of the plant
is green - the only visible color which is not absorbed).
The
optimum intensity for plants is around 20,000 - 25,000 Lx, higher or smaller
values lowering photosynthesis. To the plants from the station only red and
blue light will be given, by filtering normal light through red or blue glass.
b.
Fluorescent plants
There
are two types of light that may be used: artificial and natural light, each one
with is advantages and disadvantages. Artificial light can be obtained from
illuminating systems such as ordinary lightballs and has a high intensity, but
consumes a lot of energy. Natural light can be obtained from some bacteria,
mushrooms, fishes and coelenterates (only the bacteria are of interest) or from
the plants themselves if they are genetically modified. The light produced by
bacteria (from genus Photobacterium: Photobacterium phosphorous and
Photobacterium leiognath) is withe-green and cold (it doesn’t contain infrared
and ultraviolet rays) and of small intensity, so a huge quantity of such
bacteria would be needed and is an oxygen consumer. The mechanism which will
produce light is the following: a substance (called generically luciferin) is
oxidized with molecular oxygen to luciferase, from this process resulting
light. Substances from the luciferin
group are: luciferil-sulphate, 2-benzil luciferin etc.
luciferil-sulfokinase
Luciferil-sulphate
+ O2 ——————————————————————> LH2
luciferin
+ATP (cofactor)
So,
the bacterium grown on a nutritive medium (glucose and nutrients) in presence
of oxygen can be used to produce inexpensive, small intensity light.
The light producing plants are genetically manipulated
plants to which the luciferase enzyme (responsible for glowing) gene has been
added. The nature of the light is similar to the light produced by the
bacterium from the Photobacterium genus. The technique used is cloning the gene
into a plasmid which permits their expression in plants treated with it. Plants
obtained from the genetically modified plant will have the same properties as
their parents (they will glow too).
VI.5.
Food factor and Agriculture
In
order to be able to conceive a permanent existence of a rather dense population
on our proposed Space Settlement we began by imagining the model of a
microclimate similar to that found on Earth. We then tried to artificially
compensate for the lack of all those elements which are not to be naturally
found on our station.
a.
Food composition and preparation
Correct
nourishment is a basic condition for a healthy population. Health does not mean
only “not being ill”, but also a physical, mental and social state of
well-being.
Nourishment
is the first among the eight principles which define a healthy way of living.
That’s why achieving a project of such magnitude implies special care and
studies in order to find solutions to all human necessities.
Agriculture
is the field which provides the essential raw materials to the food industry,
therefore only by creating the conditions for getting quality produce can we
ensure the necessary base of the food processing.
In
this respect, we could also get rid of everything that has been harmful to
people on Earth (tobacco, alcohol etc.) and direct our attention to healthy
produce.
The
nutritive substances are divided after their function in:
· nutrients with energetic role:
glucids and proteins, which provide the vital energy
· nutrients with plastic role: proteins,
used to repair cellular structures
· nutrients with catalytic role:
vitamins, minerals, that influence metabolic reactions.
The
optimal proportion between proteins, lipids and glucids (or carbohydrates) is
1:2.5-3.5:0.8. The quantity needed by a person varies after the “due body
weight “. Due body weight, in kilograms, is equal to person’s height in
centimeters minus 100 (+-10%) - for men and minus 110 for women. Thus, for a
person 160 cm tall, a due body weight is 60 kg +- 6kg. A correct amount of
protein to be consumed in a day is approx. 1g per kg of due body weight. Thus,
a person with 60kg needs to consume about 60+-6 g of protein to satisfy body’s
daily needs. Any excess of protein is converted to fat, provided energy
requirements are met by other components. Using the ratio 1:2.5-3.5:0.8, the
required quantity of lipids and carbohydrates can be calculated: 150-210 g of
fat and 30 to 50 g of carbohydrate.
The
needed energy is expressed in calories (1 cal = the quantity of heat required to
raise the temperature of 1g of water with 1 grade). All body activities require
energy, and daily needs vary with people due body weight and activities. For
example, an adult with less activity needs about 2500 kcal, while a worker
needs 5000 kcal and a performance sportive 8000 kcal. Energetic requirements
are also higher for children: 4000-4500 kcal.
How
much a healthy human requires protein per day? Opinions are divided: while the
WHO protein figure translate into 56g of protein a day for a (75 kg) man and
48g for a(64 kg) woman, the recommendations of the UK Department of Health and
Social Security (DHSS) are slightly higher: 68g a day for a sedentary or
moderately active men, and 54g a day for women, but the quality is important.
The quality of protein is measured by comparing the proportions of essential
amino acids in a food with the proportions required for good nutrition. The
closer the 2 numbers are, the higher the protein quality. Egg and milk proteins
are high - quality proteins that are efficiently used by the body and are used
as reference standards against which other proteins can be compared. Meat
protein is of high protein quality, whereas several proteins from plants used
as major food sources are relatively deficient in certain essential amino
acids, e.g., tryptophan and lysine in maize (corn), lysine in wheat, and
methionine in some beans. In a mixed diet, a deficiency of an amino acid in one
protein is made up by its abundance in another; such proteins are described as
complementary; e.g., the protein of wheat and beans combined provides a
satisfactory amino acid intake. Under such circumstances, a greater total
amount of protein must he consumed to satisfy requirements.
Regardless
of their source, aminoacids that are not immediately incorporated into new
protein are rapidly degraded and they are not stored.
All
dietary proteins (proteins that can be used by humans) are digested and
absorbed in the bloodstream as individual aminoacids. The body requires 20
different aminoacids, and only 8 can be synthesized. The daily needs of protein
are calculated based on body weight, extra growth on infants require larger
quantities. Pregnancy, lactation, tissue repair after injury, recovery from
ilness, increased physical activity is other conditions requiring more dietary
protein. Generally, a diet where 12% of the energy is supplied as protein is
adequate.
Fats-or
lipids-are a class of organic substances that are not soluble in water. In
simple terms, fatty acids are chains of carbon atoms with hydrogen atoms
filling the available bonds. Most fat in our bodies and in the food we eat is
in the form of triglycerides, that is, three fatty-acid chains attached to a
glycerol molecule.
Fat’s
value as a “fuel” for our body increases with the increase in the amount of
hydrogen per gram of carbon in its molecule, with the increase in the
energy-contributing constituents. Chemically, the best are long-chain fully
saturated fatty acids, that is to say, solid fats of animal origin. Only fats
with the length of the chain above 10 carbon atoms are suitable to be utilized
by our cells and tissues without conversion. These fats are directed straight
to the blood stream via the lymphatic system, and they do not have to be
converted and made suitable by the liver, as is the case with inferior fats
(with shorter chains), or all other constituents of consumed and digested
foods. Long chain fatty acids are the best medication for those suffering from
liver diseases. Chemically and factually long chain fatty acids are the best
“fuel” for our bodies.
By eating animal fats we not only receive concentrated energy, but we also
receive all the fat- accompanying elements needed to obtain this energy, in the
necessary quantity and proportion. The human body metabolizes animal fats
easily and such metabolism is energetically economical. The digestive system is
designed to slowly deliver the building blocks and energy containing matter.
Carbohydrates
are widely distributed in plants and animals, where they fulfill both structural
and metabolically functions. In plants, glucose C6H12O6 is
synthesized during photosynthesis, while animals obtain it from plants or other
animals. Animals can synthesize some carbohydrates from fat and protein but
these quantities are much under their needs.
Most carbohydrates in the food form glucose, galactose and
fructose. These are transported to the liver via the portal vein, where
galactose and fructose are converted into glucose. Glucose is specifically
required by many tissues, but does not have to be provided directly from food
since other compounds like starch, fructose, galactose are transformed in
glucose either during digestion (starch) or in liver (fructose, galactose). A
minimum daily intake of carbohydrates is about 50g to prevent ketosis and loss
of muscle protein.
Vitamins
are substances that act as catalytic substances. In their absence, some
products cannot be synthesized, producing severe diseases to humans (loss of
nocturnal sight, heart diseases, anemia, etc.)
The
necessary vitamins are: A, B1, B2, B6, B12, C, D, E, K, and PP. Some can be
solved in water (B1,B2,B6,B12,PP,C) and others in fats (A,D,E,K). Vitamin A can
be found in fresh vegetables (especially carrots), milk, liver, butter, cheese
and eggs; 12mg are required daily. Vitamin B1 is found in meat, cereals,
vegetables, milk, liver; 1-2mg/day. Vitamin B2 can be found in almost all
foods; 1-2mg/day. Vitamin B6 can be found in cereals, vegetables, and meat.
Vitamin B12 is found in pork and beef meat, eggs and fish; 2mg/day. Vitamin C
can be found in fresh fruits and vegetables (tomatoes); 70mg/day. Vitamin D is
found in cheese, yogurt, milk, cream, liver, eggs, fish, fish oil; 1-2 mg/day.
Vitamin E can be found in margarine, seeds, fresh vegetables, wheat, vegetal
oils; 20mg/day. Vitamin K is found in fresh vegetables, liver, produced by
intestinal bacteria; 4mg/day. Vitamin PP can be found in dried vegetables,
cereals, eggs, milk, and liver. Vitamins are generally present in plants and
they are less abundant in animals.
Although
water isn’t a nutrient, it has a very high importance because it represents the
medium were all reactions take place and in which most substances are solved.
The daily need of water is around 1.5-2 l/person, but this value can be much
higher if transpiration is high (for example, when temperature is high). Water
can be taken directly or from other products (the value required comprises the
total water ingested).
Minerals have catalytic proprieties or they
take part as components in some compounds (like iron in hemoglobin). Minerals
are: P, Ca, Fe, Zn, Cu, Cl, Na, K, S, Se, Ni, Mn, and Mg.
As no
single food contains all these elements, we have to use a variety of
foodstuffs. In the case of living on a space station, there are two
possibilities of ensuring the nourishment of the population.
One
could be the classical way similar to that which we are familiar with on Earth.
This presents, however, a variety of problems, connected to the diversity of
the required technical means, complex methods and storage facilities. Another
way would be a balanced vegetarian diet, without cholesterol and fats for the
benefit of the human body. Furthermore, as the evolution of civilization aims
at the creation of a new type of man, with higher aspirations but less time, we
suggest a re-thinking and re-designing of the food industry, so that it would
serve the interests of the individual, offering him the necessary state of
health and comfort.
In
this respect, we recommend the use of Soya as the basic raw material to obtain
various foodstuffs ranging from diary produce to those having the taste of
meat. Millet paste could successfully replace eggs.
A
vegetarian diet can offer man the benefit of protein of superior quality such
as glucose and lipids which are not harmful, nut-oil, seeds, olives, fiber,
vitamins and total mineral salts.
This
is the ideal we should pursue to avoid many of the causes of illness nowadays.
Setting as our objective a healthy diet, the designing and construction of the
technical facilities helps to achieve the above purpose.
On as
pace station, crops an be grown on the seven levels used for agriculture,
provided with red spectrum lights, adequate ventilation, system of keeping
constant temperature and air humidity, as well as the polymer texture used as
crop supports.
Crops
must be treated with natural and synthetic fertilizers to get quality produce.
Once the plants have grown, they are harvested and stored in appropriate
spaces, until they are processed.
But,
people’s mentality being what it is, perhaps some may experience frustration in
the absence of those useful domestic animals with whom they were used on Earth
(poultry, livestock). Fish breeding facilities are also possible and from a
psychological point of view.
In
conclusion, the diet onboard L.E.D.A. will comprise a mixture of aliments from
the following classes:
· Fruits and
vegetables
· Cereals
· Milk and
milk products
· Meat and
eggs
|
Product |
Values are taken from 100g/100ml of product, and they are
expressed in g |
|
sunflower seeds |
P: 24.4 L: 43.7 C: 24.6; 566kcal |
|
walnut |
P:16 L:60.3 C:18.0;651 kcal |
|
apples |
P: 0.4 L:0.4 C: 12.1; 47 kcal |
|
avocados |
P:2 L:15.3 C:7.4; 161 kcal |
|
pears |
P:0.6 L:0.2 C:14.4; 55 kcal |
|
soya beans |
P: 34.3 L: 19.6 C: 32.7; 385 kcal |
|
kidney-beans |
P: 21.4 L: 1.6 C:61.6;
290 kcal |
|
carrots |
P:1 L:0.4 C:8.7; 27 kcal |
|
potatoes |
P:1.9 L:0.1 C:20.5; 86 kcal |
|
tomatoes |
P:0.9 L:0.2 C:3.6; 15kcal |
|
mushroom |
P:2.7 L:0.4 C:2.6; 17 kcal |
|
bread (white) |
P: 8.1 L:1.5 C:51.6; 240 kcal |
|
flour |
P:9.4 L:1.6 C: 74.1; 346 kcal |
|
rice |
P: 6.7 L:0.7 C:78.9; 347 kcal |
|
butter |
P:0.7 L:82.5 C:0.7;742kcal |
|
full cream milk |
P:3.2 L:3.7 C:4.7; 66 kcal |
|
eggs |
P:12.5 L:10.7 C:1; 151 kcal |
|
beef |
P:20.9 L:3.6 C:0; 116 kcal |
|
chicken |
P:16 L:2.2 C:0; 122kcal |
|
pork |
P:21 L:10 C:0; 175 kcal |
Since cultivation will be reduced on the station, only the foods
with the best quality will be grown.
b. Food depositing
and quality control
In the area designed for industrial activities, the
technical equipment for processing the agricultural and animal produce will be
of major importance. They will ensure the mechanical and thermal treatment used
in the process of getting both raw materials and the final produce.
We
must design this equipment having in view the special conditions required when
working in a space station environment, the necessity of recycling the
residues, eliminating the effect of vibrations, noise, and odor pollution. The
final products must be properly stored in special locations from which they
will be delivered according to the demand.
The quality
of the products is reflected in the quality of the population’s state of
health, therefore monitoring quality is essential during the entire production
cycle.
VI.6.
Water management
Most
forms of life require water for their survival. On the Space Settlement, we
will need to find ways of producing and effectively recycling the water for
plants and humans.
|
INPUTS - kg/person/day |
|
|
Oxygen |
0.83 |
|
Dry Food |
0.62 |
|
Water in Food |
1.15 |
|
Food Preparation Water |
0.79 |
|
Drinking Water |
1.61 |
|
Oral Hygiene Water |
0.36 |
|
Hand and Face Wash |
1.81 |
|
Shower Water |
5.44 |
|
Clothes Wash Water |
12.47 |
|
Dish Wash Water |
5.44 |
|
Urinal/Comode Flush Water |
0.49 |
|
Total: |
31.0 kg |
|
OUTPUTS - kg/person/day |
|
|
Carbon Dioxide |
1.00 |
|
Water from Respiration and
Perspiration |
2.28 |
|
Urine |
1.50 |
|
Urine Solids |
0.06 |
|
Hygiene Water |
7.18 |
|
Latent (Evaporated) Hygiene
Water |
0.44 |
|
Clothes Wash Water |
11.87 |
|
Latent (Evaporated) Clothes Wash
Water |
0.60 |
|
Latent (Evaporated) Food
Preparation Water |
0.04 |
|
Dish Wash Water |
5.41 |
|
Latent (Evaporated) Dish Wash
Water |
0.03 |
|
Feces Solids |
0.03 |
|
Feces Water |
0.09 |
|
Sweat Solids |
0.02 |
|
Urinal and Commode Flush Water |
0.49 |
|
Total |
31.0 kg |
From:
Wydeven, T., and Golub, M.A., Generation Rates and Chemical Compositions of
Waste Streams in a Typical Crewed Space Habitat, NASA Ames Research Center, Moffett Field, CA (1990)
and Webb, P., Ed., Bioastronautics Data Book, NASA SP-3006, National
Aeronautics and Space Administration, Washington, D.C. (1964).
a.
Water Production
Initially,
water will have to be extracted from the Moon, in the form of ice, the ice
melted using solar energy and then purified. Also, the first spaceships
arriving at the station will need to carry water supplies. On the settlement,
water will be constantly recycled, since there are no viable water sources in
space, apart for The Moon and The Earth, and the cost of supplying the station
with all the necessary water from these places is too great.
Plants and animals eliminate water through breathing and
excretion.
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Excess humidity in
the air will need to be condensed and the water recycled.
b. Water storage
Water will be stored in a cluster of interconnected tanks
located at the center of the space station. The connections of the tanks will
be fitted with valves and pumps. When water from the tanks is used, the
remaining water must be distributed evenly in order to avoid oscillations due
to inertia.
The storage area will need to be large enough to hold a few
days’ supply of water in the case of an emergency (about 54250 tons for a week,
which means that the whole storage area should have a volume of 54250 cubic
meters).
Since “gravity” increases as we advance towards the outer
regions of the station (the inhabited area), water will flow naturally (or with
little energy consumption) to where it is needed. However, sewage water will
have to be pumped to the purification plant and then into the storage tanks
using electric pumps.
c. Water quality
control
A water processing facility will be placed next to the
storage tanks. It should be able to handle a flow of 7750 cubic meters a day. Water
purification methods include physical, chemical and biological purification and
each method will be used at different stages of the process.
1. Physical purification involves the removal of solids
from liquids using filters. Water is forced through a membrane under pressure,
leaving impurities behind. Cross flow membrane filtration methods will be used
to separate salts and organic matter from the water. The finest membranes will
be able to filter particles as small as 0.001 microns (reversed osmosis). That
includes most salts, bacteria, viruses, and metal ions.
2. Chemical purification consists of adding chemicals to
the water. The chemicals act as biocides or prevent the formation of certain
reaction products. Oxidizing agents can be added for disinfection or to
neutralize reducing agents and reducing agents should be added to reduce
oxidizing agents.
The most common chemical used for disinfection is chlorine.
However, it is not a suitable solution for the space station because of its
tendency to form toxic chlorine gas or to react to chloramines and chlorinated
hydrocarbons. To prevent this, we could add chlorine dioxide (ClO2) to the
water, as it is an effective biocide in very low concentrations. It reacts to
amino-acids in the cytoplasm and kills the microorganism. The by-product of
this reaction is chlorite.
Ultra-violet radiation can be used for disinfection, as
well as ozone, iodine or silver. UV radiation treatment should be applied to
water being stored in the tanks, since it prevents the division of cells and
therefore the multiplication of microorganisms.
3. Biological purification involves the use of
microorganisms, mainly bacteria to decompose remaining organic materials
dissolved in the water.
4. A very useful method for preventing the water
contamination by removing organic constituents and residual disinfectants is
the activated carbon filter. This is a favored technique because of its
multifunctional nature and the fact that it adds nothing detrimental to the
treated water. Another advantage is that this method not only improves taste
and minimizes health hazards; it also protects other water treatment units such
as reverse osmosis membranes and ion exchange resins from possible damage due
to oxidation and organic fouling. There are two principles by which activated
carbon removes contaminants from water: absorption and residual disinfectants
removed by catalytic reduction.
Water quality will be monitored to ensure against disease.
The supply will conform to regulations concerning chemical, inorganic and
organic matter concentration.
The EPA current drinking water standards (units are
milligrams per liter (mg/L) unless otherwise specified):
|
Microorganisms |
||
|
Contaminant |
MCLG (mg/L) |
MCL or TT (mg/L) |
|
Cryptosporidium |
zero |
TT |
|
Giardia lamblia |
zero |
TT |
|
Heterotrophic plate count |
n/a |
TT |
|
Legionella |
zero |
TT |
|
Total coliforms |
zero |
5.0% |
|
Viruses (enteric) |
zero |
TT |
|
Disinfection Byproducts |
||
|
Contaminant |
MCLG (mg/L) |
MCL or TT (mg/L) |
|
Bromate |
zero |
0.010 |
|
Chlorite |
0.8 |
1.0 |
|
Haloacetic acids (HAA5) |
n/a |
0.060 |
|
Total trihalometanes (TTHMs) |
none |
0.10 |
|
Disinfectants |
||
|
Contaminant |
MRDLG (mg/L) |
MRDL (mg/L) |
|
Chloramines (as Cl2) |
4 |
4.0 |
|
Chlorine (as Cl2) |
4 |
4.0 |
|
Chlorine dioxide (as ClO2) |
0.8 |
0.8 |
|
Anorganic Chemicals |
||
|
Contaminant |
MCLG (mg/L) |
MCL or TT (mg/L) |
|
Antimony |
0.006 |
0.006 |
|
Arsenic |
0 |
0.010 |
|
Asbestos (fiber>10
micrometers) |
7 million fibers per liter |
7 MFL |
|
Barium |
2 |
2 |
|
Beryllium |
0.004 |
0.004 |
|
Cadmium |
0.005 |
0.005 |
|
Chromium (total) |
0.1 |
0.1 |
|
Copper |
1.3 |
TT Action Level=1.3 |
|
Cyanide (as free cyanide) |
0.2 |
0.2 |
|
Fluoride |
4.0 |
4.0 |
|
Lead |
zero |
TT Action Level=0.015 |
|
Mercury (inorganic) |
0.002 |
0.002 |
|
Nitrate (measured as Nitrogen) |
10 |
10 |
|
Nitrite (measured as Nitrogen) |
1 |
1 |
|
Selenium |
0.05 |
0.05 |
|
Thallium |
0.0005 |
0.002 |
|
Organic Chemicals |
||
|
Contaminant |
MCLG (mg/L) |
MCL or TT (mg/L) |
|
Atrazine |
0.003 |
0.003 |
|
Benzene |
zero |
0.005 |
|
Carbofuran |
0.04 |
0.04 |
|
Chlorobenzene |
0.1 |
0.1 |
|
Dalapon |
0.2 |
0.2 |
|
Dichloromethane |
zero |
0.005 |
|
Dinoseb |
0.007 |
0.007 |
|
Diquat |
0.02 |
0.02 |
|
Endothall |
0.1 |
0.1 |