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Osservatorio Astronomico di Palermo Giuseppe S. Vaiana |
The study of the origin, evolution and
distribution of life in the universe is the groundwork of
Astrobiology/Astrochemistry. This is a multidisciplinary science in
which astrophysics, physics, chemistry, biology and geology work in
synergy to answer the following questions: How did life originate on
Earth and how did it evolve? Is there life in space and how can we
find evidence of it? There is increasing consensus among the
scientific community on the hypothesis that we cannot understand the
origin and evolution of life unless our scenario goes far beyond the
restrictive limits of our own planet. This new perspective has its
foundations on the ever-increasing amount of discoveries of organic
molecules in interstellar clouds, and amino acids and other
biologically relevant material - i. e. molecules that are commonly
found in proteins - in meteorites.
Observations and theoretical models suggest
that planetary systems like ours came from dense inter- stellar
clouds made of gases and dust particles which, because of gravity,
collapsed to form a central star, the planets and a large amount of
minor celestial objects such as small grains, meteorites and comets,
relicts of the primordial nebula. In the newly formed planetary
system, planets undergo heavily bombarded by such relicts receiving
an enormous amount of organics.
For instance, over the first 320 million
years of its life, more than a thousand times the actual biomass
settled on Earth. Hundreds of organics molecules have been so far
detected in space and some of them very important for life including
amino acids found in meteorites, and some of them are of biological
relevance, i.e commonly found in proteins.
From this hypothesis other questions arise: what kind of processes has led to the formation, in space, of complex molecules such as amino acids? And how could they survive the ionizing solar radiation? Solar radiation, if on one hand can cause damage to prebiotic material, on the other is crucial in supplying the energy required for the synthesis of prebiotic molecules in interplanetary space. Although several models have been recently proposed to explain amino acid formation in space, we still do not know what role exogenous prebiotic molecules play in the origin-of-life process.
Moreover, amino acids, and more in general
organic material, are easily photo-degradable and with lack any
suitable protective mechanism, it is unlikely that they could have
survived in harsh interplanetary space and on Earth primordial
environment.
So, although the hypothesis that basic life
molecules are exogenous is well observed and experimented, it is far
from representing a co-coherent and complete theory for the origin of
life.
The OAPa LIFE (Light Irradiation Facility for Exochemistry) laboratory.
In 2006 a laboratory for
astrobiology/astrochemistry was set up, in order to study the role of
X and UV radiations coming from young Sun-like stars, in the
synthesis of organic molecules, particularly amino acids, in space.
The interplanetary space conditions are
simulated by means of a ultra high vacuum chamber (10^-11 mbar),
provided with a pumping system, a cryostat through which temperatures
of 10 K (about -263 C) can be reached, X and UV radiations sources
simulating emissions from the young sun, and several measuring
instruments. Although the laboratory is still under development a
series of experiments have been performed so far. Studies of the
effects of soft X-ray radiation on DNA molecules (Ciaravella et al
2004) and amino acids (Ciaravella et al 2010) have shown the
competing processes, e.g. destruction versus formation of new
structures (dual role of radiation). In particular, DNA molecules
from Bacillus Subtilis were irradiated in water solution at room
temperature, simulating terrestrial environment, with and without
presence of clays in the solutions.
The results have pointed out the important
role of clay, a key component in the formation of complex molecular
structure, in protecting the molecules from the radiation damage. In
the amino acids experiment along with the destruction of the
tryptophan molecules large molecular structures, such as tryptophan
dipeptide and tripeptide have been observed. Studies of soft X-ray
irradiation of interstellar ice analogues have shown that X-rays are
more efficient than typical used, HI Ly (121.6 nm), ultraviolet
radiation in producing new complex species (Ciaravella et al 2010,
Ciaravella et al. 2011).
Involved people:
Marco Barbera - barbera at astropa.unipa.it
Angela Ciaravella - ciarave at astropa.inaf.it
Alfonso Collura - collura at astropa.inaf.it
Giusi Micela - giusi at astropa.inaf.it
1) Ciaravella A., Scappini F., Franchi M., Cecchi-Pestellini C., Barbera M.Candia R., Gallori E., Micela G., Role of Clay on Adsorbed DNA against X-ray Radiation, 2004, International Journal of Astrobiology, Vol.3 (1), 31.
2) Ciaravella A., Muñoz Caro, G., Jimenez Escobar, A., Cecchi Pestellini, C., Giarrusso, S., Barbera, M., Collura, A. Soft X$-$ray Irradiation of a Methanol Ice: Implication for H2CO Formation in Interstellar Regions, 2010, ApJL, 722, 45
3) Ciaravella A., Bongiorno, D., Cecchi-Pestellini, C., Testa, M.L.,Indelicato, S., Barbera, M., Collura, A., La Barbera, A., Mingoia, F.,The Young Hard Active Sun: Soft X-ray Irradiation of Tryptophan in Water Solutions, 2011, Int. J. of Astrobiology, 10(1), 67
4) Ciaravella A., Jimenez Escobar, A., Muñoz Caro, G., Cecchi Pestellini, C., Candia, R., Giarrusso, S., Barbera, M., and, Collura, A. Soft X-ray Irradiation of Pure Carbon Monoxide Interstellar Ice Analogues, 2011, ApJL, in press