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388 <strong>Suppressed</strong> <strong>Inventions</strong> <strong>and</strong> Other <strong>Discoveries</strong><br />

opposition between those who were open <strong>and</strong> accepting <strong>of</strong> the new knowledge<br />

about space, <strong>and</strong> those who worked to prevent the truth from coming<br />

out<br />

Along with the later observations <strong>of</strong> mysterious clouds <strong>and</strong> lights, the<br />

cryptic radio signals led some independent astronomers to conclude that<br />

we were being given rudimentary signals from Mars to challenge our<br />

thinking about life beyond the Earth. Regarding habitability, there was<br />

even more scientific certainty in <strong>other</strong> telescopic studies. As early as 1926,<br />

photographs were taken in ultraviolet light that clearly showed a substantial<br />

atmosphere on Mars. Compared with infrared photographs taken at the<br />

same time, the pictures proved that there is a dense atmosphere, possibly<br />

40 miles in depth. There are undoubtedly more rarefied layers above this<br />

altitude, much like the upper, tenuous atmosphere around the Earth, that<br />

would be too thin to be recorded by photography. It has been suggested that<br />

the top <strong>of</strong> the Martian atmosphere might reach 400 miles, by the British<br />

scientist-writer Earl Nelson, author <strong>of</strong> There Is Life on Mars (1956).<br />

The early photographs showing the Martian atmosphere were taken by<br />

G. E. Hale <strong>of</strong> the Mount Palomar Observatory [Southern California] <strong>and</strong> are<br />

reproduced in Nelson's book. There are two immediate <strong>and</strong> important conclusions<br />

that can be drawn from these observations. The surface gravity on<br />

Mars must be substantially higher than has been taught, for a low gravity<br />

would not be sufficient to retain such a sizable atmosphere. Secondly, with<br />

such a dense atmosphere, the sun's energy would interact much differently<br />

than orthodox theories suggested, <strong>and</strong> the temperatures on Mars would be<br />

considerably warmer, more moderate, <strong>and</strong> more Earth-like.<br />

Although the length <strong>of</strong> the Martian year is nearly double our 365-day year,<br />

the seasons on Mars vary <strong>and</strong> alternate just like on Earth. When the northern<br />

hemisphere is in its summer cycle, the southern hemisphere has its winter.<br />

The length <strong>of</strong> the Martian day is 24 hours <strong>and</strong> 37 minutes, <strong>and</strong> the inclination<br />

<strong>of</strong> its axis is 25 degrees, which is very close to Earth's 23 degrees.<br />

Both the northern <strong>and</strong> southern polar caps extend nearly half way to the<br />

Martian equator during their respective winters. With the onset <strong>of</strong> spring<br />

in either hemisphere, its ice cap recedes <strong>and</strong> a wave <strong>of</strong> darkening over<br />

broad areas spreads slowly towards the equator. This cyclic surface darkening<br />

was widely considered to be seasonal vegetation growth as water<br />

was liberated from the polar caps. Each polar cap will shrink considerably<br />

during its respective summer cycle. Sometimes the southern polar cap<br />

melts completely.<br />

The broad areas near the equator, such as Mare Serpentis, Mare<br />

Sirenium, <strong>and</strong> Syrtis Major, change from their winter shade <strong>of</strong> brown, to<br />

light green <strong>and</strong> then to dark green. This latter stage has <strong>of</strong>ten been<br />

described as a dark blue-green. Astronomers also noted that as the seasons

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