Bacterial spores and hydrocarbons in space
Danilo
Anton
Spectroscopic
studies of interstellar clouds of cosmic dust carried out by several
astronomical observatories in recent years have shown that
hydrocarbons are very abundant in the universe.
In
particular, English astronomer Fred Hoyle and other members of his
scientific team in British universities (Cambridge, Cardiff)
contributed transcendent data about various organic molecules found
in these clouds, including some, who had, the surprising spectral
behavior of certain bacteria spores.
In
1968 studies of interstellar dust detected polycyclic aromatic
molecules (Donn, 1968).
Four
years later, in another study (Johnson, 1972) confirmed the presence
of porphyrins in this space dust,
Wickramasinghe
in 1974 proved the existence of complex organic polymers in space
conditions, particularly polyformaldehydes. It
is noted that these molecules are related to cellulose and are
ubiquitous in terrestrial biochemistry.
Finally,
in 1975, Hoyle and Wickramasinghe concluded that organic polymers
constitute a significant proportion of the powder material in
interstellar dust clouds.
Hoyle
and Wickramasinghe continued their research work in the mid-1970s and
concluded that the light absorption spectrum of interstellar dust
could be explained if the grains had a certain size and were hollow.
In
1979, after comparing numerous substances with the data from the
interstellar dust these authors found a strong similarity with dry
bacterial spores which refract light as irregular hollow spheres and
have a range of proper grain size. Based on these data they
concluded that a significant proportion of interstellar dust grains
could consist of frozen bacterial spores.
This
finding was considered ridiculous in that time and even today is
generally ignored. There were even those who thought "poor
Fred Hoyle had lost its way".
Although
the interpretation of these research data were considered highly
speculative new information has been obtained in the last few years
ratifying those preliminary conclusions.
In
a recent paper Wickramasinghe found hetero-aromatic polymers in the
dust collected by the Stardust probe. According to the interpretation
of this author they would constitute fragments of broken cell walls
after impacts at 30 km per second against the surfaces of the
detectors.
In the last 15 years of his life, until his death in 2001, Hoyle was dedicated to study the implications of this hypothesis. His student and successor, Chandra Wickramasinghe and other disciples continue exploring these bold and innovative aspects of life in space.
In the last 15 years of his life, until his death in 2001, Hoyle was dedicated to study the implications of this hypothesis. His student and successor, Chandra Wickramasinghe and other disciples continue exploring these bold and innovative aspects of life in space.
From the book "Inexhaustible? Petroleum and Gas", Danilo Anton, Piriguazu Ediciones
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