Jose Ribeiro
HET610, SAO
Whenever the Portuguese Navigators from the XV century found a desert island, they used to leave rabbits behind. Their aim was to verify whether the island had conditions for habitability or not. On their way back they would check if the rabbits’ population had grown. They did multiply! And today, farmers from Madeira and some islands in The Azores still fight sporadic rabbits plague.
“Invaders can change
ecosystems where they differ substantially from the natives in resource
acquisition or utilisation” (1).
Today, the new discoverers
enlarged their frontiers beyond Earth, sending exploratory probes and men to
space. Although manned spacecraft have
so far only landed on the moon, several robotics spacecraft already landed in
Mars, Venus, one entered Jupiter’s atmosphere, another landed on the asteroid
Eros, and one is now on its way to Titan. In the agenda are also under
preparation missions to collect and send to Earth samples from the Martian
soil, cometary matter, as well as to send an exploratory probe to Europa.
Very early, since the
preparation of the Apollo project, that the biologic risks began to be
discussed, as well as the respective prevention protocols against the
interplanetary biologic contamination. At first, works were mainly focused on
the risks of back contamination, i.e. the risk of lunar soil samples and
astronauts bringing extraterrestrial micro organisms, which might somehow
contaminate Earth. In 1967 the “Outer Space Treaty” was signed, which
“specifically requires that all space exploration must be done in a way that
avoids harmful contamination to celestial bodies or adverse changes in the
environment of the Earth from the introduction of extraterrestrial materials”
(2) (4).
Since then, the development
of Planetary Protection (PP) policies has been under the responsibility of the
Committee on Space Research (COSPAR) (2) (3), of the International Council of
Scientific Unions. In the USA the PP
policy is implemented by NASA, who is advised by the Space Studies Board (SSB)
(4).
Protocols were created for
the prevention of two types of cross-contamination:
-
back contamination, that is the introduction on
Earth of extraterrestrial contaminating agents brought by men, equipment or
samples.
-
forward contamination, that is the transport of
contaminating agents from Earth to space by spacecraft and men.
Due to an absolute lack of
information on extraterrestrial micro-organisms, measures for planetary protection have as parameters the study of
the extreme micro-organisms found on Earth (2); yet, this procedure can have
certain limitations, as the most extreme environmental conditions found on
Earth are soft compared to space environmental conditions. On one hand, our
extreme micro-organisms may not survive extraterrestrial environments (what is
highly probable), and on the other, extraterrestrial micro-organisms (should
they exist) may be highly resistant due to the inhospitable conditions they live in, thus representing an
increased risk to the ecosystem on Earth. As adverse as the environmental
conditions may be, the micro-organisms on Earth need liquid water in order to
survive (1). Therefore, forward contamination risks increase in regions where
liquid water exists, as in Mars and in Europa. Yet, there are confirmed
exceptions, as the case of the camera of the Surveyor 3 Lander, brought to
Earth by the astronauts of Apollo 12, which contained bacteria still viable
after two and a half years on the moon (5).
Not long ago, the existence
of extreme microbes would be considered scientific fiction, due to peculiar
environments they live in:
-
in volcanic areas live the extreme Thermophiles,
growing at temperatures exceeding 100ºC (6).
-
bacterial endospores, the resting stage of certain
bacteria, are known to survive for thousands of years, resisting to freezing
and vacuum, and resisting moderately to heat and to UV and ionising radiation
(6).
-
deep subsurface micro-organisms have been found at
700 meters below Earth surface. Some of these species have the capacity of
repairing their DNA, denoting great resistance to UV radiation and long-term
survival, even in space. Others, the extreme Halophiles are embedded in
crystals of salt dated approximately 200 million years old. The Barophilic
bacteria was isolated from the deep sea revealing great pressure resistance.
The Cryptoendolyth are found in the Antarctic, forming communities within
sandstone. They are adapted to extreme low temperatures, low moisture and high
winds (6).
-
the radiation-resistant bacteria can withstand large
doses of radiation. Some have been found within the course of radioactive
reactors (6).
Life adapts itself - so, one
should not ignore the contamination risks even in zones where survival is
highly improbable.
The report of SSB from 1978
“Recommendations on Quarantine Policy of Mars, Jupiter, Saturn, Uranus,
Neptune, and Titan” has been updated along the years, as scientific and
technologic knowledge develops. Recommendations regarding control of Mars
forward-contamination are as follows:
“1. Landers carrying
instrumentation for in situ investigation of extant Martian life should be
subject to at least Viking-level sterilisation procedures (...)”
“2. Spacecraft (including
orbiters) without biological experiments should be subject to at least
Viking-level presterilization procedures – such as clean-room assembly and
cleaning of all components – for reduction of bioload, but such spacecraft need
not be sterilised. (...)” (7).
The main reason for these
recommendations is linked to the fact that life detection experiments as well
as the equipment used in the experiments are extremely susceptible to
biological and chemical contamination by
agents on Earth. To detect life on a planet to then conclude that its
origin was from Earth, should not be the purpose of such expensive missions.
The Viking-level procedure
of sterilisation, first applied to the Viking missions, obeys to the four
following steps:
“1. Surfaces were rigorously
cleaned to reduce the starting bioburden on the spacecraft (...)”
“2 .Instruments were cleaned
and assembled in cleanrooms by workers in surgical attire (...). Both the
lander and orbiter were treated in this way.”
“3. The entire lander and
its payload were assembled under the same conditions. (...)”
“4. The lander was then placed
in an oven and subjected to dry heat in cycles (...)” (8).
Since the Viking mission, NASA has been
concerned in practice with the forward-contamination; for example, in the Mars
Pathfinder Mission Status from 4th February 1997, it is reported: “The
spacecraft will not be placed on a Mars atmospheric entry trajectory until
after TCM-3 because of planetary quarantine requirements” (9).
Prevention practice to
back-contamination goes back to the Apollo mission, and was under the
responsibility of the Lunar Receiving Laboratory (LRL). In this Laboratory the
astronauts, a physician, a technician, as also the lunar soil samples, remained
under quarantine. The astronauts were submitted to a three week quarantine
(10). The astronaut quarantine practice was discontinued after the Apollo 14
mission, as from the outcome of the studies from Apollo 11 and 12 missions,
they reached the conclusion that it was not a necessary procedure (11).
Lunar soil samples were all
submitted to quarantine. In this case, the protocol aimed to “permit assessment
of lunar material so that samples could be released within 30 days from their
arrival at the LRL, unless some evidence of extraterrestrial organisms
appeared.” (12)
Planetary protection today
is so important as any other phase of a space mission. The respect for the
ecosystems will be culturally consolidated in developed countries in the next
few generations. Earth, as well as other celestial bodies, are not free from an
alien contamination. It belongs to NASA History that some engineers and
scientists from the Manned Spacecraft Center “felt that the quarantine facility
and its elaborate precautions were unnecessary impediments to Apollo
operations” (13). Fortunately for mankind, the USA is a country with a
financial budget to space exploration. Yet, the risk that poor countries, with
access to space technology, neglecting the prevention procedures is dangerously
high.
On the other hand, human
error is an existing factor: risk evaluation errors and procedure
simplification (the urgent deadlines may lead to simplification of certain
aspects, which otherwise would be more thoroughly considered).
And, obviously, there may be
contamination risks in case panspermia is a reality. The entry in the
atmosphere of a contaminated meteor may start an infestation (14); yet this
fact is inevitable.
Scientists can also opt to
colonise planets with Earth biomass, in order to study the conditions of
habitability of those ecosystems. But before, they should take into account the
outcome of the “rabbits experiment” of the Portuguese Navigators from the XV
century....
References
1- Elliot Levinthal, “Search for the Evidence of Live: Caution and Humility: Where
There’s Water”
http://calspace.uscd.edu/marsnow/library/science/exobiology/
2- Race,M.S. , Rummel, J.D., “Bring Em Back Alive-Or At Least Carefully
http://www.astrobiology.com/adastra/bring.em.back.html
3- “Planetary Protection for Mars Missions”
http://cmex-www.arc.nasa.gov/Exo_Strat/Docs/protection.html
4- “Biological Contamination of Mars-Issues and Recommendations”-Summary
http://www.nas.edu/ssb/bcmarsmenu.htm
5- Daniel Pendick, “The Real Men in Black”, Astronomy mag., July 99, pp.36
6- “Biological Contamination of Mars-Issues and Recommendations”-Chap.4
http://www.nas.edu/ssb/bcmarsmenu.htm
7- “Biological Contamination of Mars-Issues and Recommendations”-Chap.5
http://www.nas.edu/ssb/bcmarsmenu.htm
8- “Biological Contamination of Mars-Issues and Recommendations”-Chap.4
http://www.nas.edu/ssb/bcmarsmenu.htm
9- “Mars Pathfinder Mission Status”, 4 February 1997
http://www.xtec.es/recursos/astronom/mars/mpf/mpfstatus_020497.htm
10- “Primary Mission Accomplished: 1969 – The Astronauts in Quarantine”
http://www.hq.nasa.gov/office/pao/History/SP-4214/ch9-7.html
11- “First Phase of Lunar Exploration Completed: The end of Quarantine”
http://www.hq.nasa.gov/office/pao/History/SP-4214/ch12-9.html
12- “Setback and Recovery: 1967 – Complexities of Quarantine”
http://www.hq.nasa.gov/office/pao/History/SP-4214/ch7-9.html
13- “Handling Samples from the Moon – Staffing the Lunar Receiving Laboratory”
http://www.hq.nasa.gov/office/pao/History/SP-4214/ch4-6.html
14- Paul Davies – “Interplanetary Infestation” – Sky & Telescope Mag., Sep. 99,pp.32
Other Readings:
- “Handling Samples from the Moon – Completing Design and Starting Construction”
http://www.hq.nasa.gov/office/pao/History/SP-4214/ch4-5.html
- “Handling Samples from the Moon – The Specter of “Back-Contamination””
http://www.hq.nasa.gov/office/pao/History/SP-4214/ch4-3.html
- “Preventing the Forward Contamination of Europa – Microbial Detection and
Identification”
http://www.nas.edu/ssb/europamenu.htm
- E.C. Levinthal and J. Lederberg, “Relationship of Planetary Quarantine to Biological Search Strategy” – Life Sciences and Space Research – North-Holland, Amsterdam (1968)