Significant Achievements in Space Bioscience 1958-1964United States. National Aeronautics and Space Administration
Science
Significant Achievements in Space Bioscience 1958-1964
United States. National Aeronautics and Space Administration
Biology; Space flight
Studies by Davis and Libby ([ref.32]) on the atmosphere of Jupiter
support the possibility of the production of organic matter in its
atmosphere in a manner analogous to the processes which may have led to
the synthesis of organic molecules in the Earth’s early history. It is
difficult to assess the possibility that life has evolved on Jupiter
during the 4- or 5-billion-year period in which the planet has retained
a reducing atmosphere.
The question of extraterrestrial life and of the origin of life is
interwoven. Discovery of the first and analysis of its nature may very
well elucidate the second.
The oldest form of fossil known today is that of a microscopic plant
similar in form to common algae found in ponds and lakes. Scientists
know that similar organisms flourished in the ancient seas over 2
billion years ago. However, since algae are a relatively complex form of
life, life in some simpler form could have originated much earlier.
Organic material similar to that found in modern organisms can be
detected in these ancient deposits as well as in much older Precambrian
rocks.
Although the planets now have differing atmospheres, in their early
stages the atmospheres of all the planets may have been essentially the
same. The most widely held theory of the origin of the solar system
states that the planets were formed from vast clouds of material
containing the elements in their cosmic distribution.
It is believed that the synthesis of organic compounds preceding the
origin of life on Earth occurred before its atmosphere was transformed
from hydrogen and hydrides to oxygen and nitrogen. This theory is
supported by laboratory experiments of Calvin ([ref.16]), Miller
([ref.33]), and Oró ([ref.34]).
The Earth’s present atmosphere consists of nitrogen and oxygen in
addition to relatively small amounts of other gases; most of the oxygen
is of biological origin. Some of the atmospheric gases, in spite of
their low amounts, are crucial for life. The ultraviolet-absorbing ozone
in the upper atmosphere and carbon dioxide are examples of such gases.
Significant in the search for extraterrestrial life are the data (e.g.,
planet’s temperature) transmitted by Mariner II, which was launched from
Cape Canaveral on August 27, 1962, and flew past Venus on December 14,
1962. Mariner II’s measurements showed temperatures on the surface of
Venus of the order of 800° F, too hot for life as known on Earth.
Public-domain text, read in full here on John Shaqi.
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