Campbell has offered an explanation of the indications of water vapour
on Mars, apparent on Slipher’s photographs. An analysis of the latter’s
observations shows that the Moon was photographed about four hours
later in the night than was Mars. On all occasions except one, clouds
appeared in the sky. This indicates the presence of moisture in the
air, so that the humidity should change with the temperature which
latter rapidly falls in the course of the night. Campbell, himself,
found during the clear nights, when he made his observations, that
the humidity in the hours of the night up to midnight falls to a
fraction--a half or a third--of its original value an hour or so after
sunset. This rapid temperature drop is probably confined to the strata
immediately above the observation point but the moisture is strongly
concentrated downward so that this change in humidity undoubtedly
should have been taken into account. Or better, observations should
be avoided in the beginning of the night and the Moon and Mars
photographed as soon after each other as possible, precautions taken
by Campbell but not by Slipher. That the latter found less traces of
water on the lunar photos than on the martian ones is, therefore,
probably due to the fact that the former were taken about midnight but
the latter not long after sunset, when the atmosphere contained much
more water vapour. Thus, we learn how a small slip, more obvious to the
meteorologist than to the astronomer, may spoil a labour otherwise done
with extraordinary care.
To Campbell’s critique Very answered by the suggestion that the
meteorological conditions during the Mount Whitney observations should
have been exceptionally unfavourable. The entire south-west of the
United States and the north of Mexico were visited at that time by
cloudy weather and heavy downpours. Very contends that this humidity
should partly have extended to the high strata above Mount Whitney and
therefore rendered the calculation of the moisture content of the air
entirely unreliable.
Simultaneously (August, 1910) new measurements were published of
Slipher’s photo-plates from February, 1908, which Very had examined.
The result was now that the rain-band “A” was 2.5 times more pronounced
in the spectrum of Mars than in that of the Moon. Furthermore, the
oxygen absorption-band “B” was 1.5 times stronger for Mars than for the
Moon. Great quantities of water vapour and oxygen should, therefore,
undoubtedly exist in the atmosphere of Mars.
Public-domain text, read in full here on John Shaqi.
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