posted on Mar, 3 2008 @ 08:19 PM
This brief report on the limiting size of planets that would be conducive to life forming is based on the planet's ability to retain an atmosphere.
This is based on the assumption that the planet is within the temperate orbital zone of a main sequence star, which is a star that is of a medium size
and long life. The estimate is that hydrogen being the predominant element would be retained as an atmosphere if the planet was large enough and dense
enough to have enough gravity to keep the gas from escaping out into space. Then later the planet might produce oxygen that would be suitable for life
to form.
Being written in 1960, this was probably the best estimate of the time, but we now know that a planet also need to be geologically active with a
molten core, which gives it the magnetosphere that protects the planet from high energy particles and keeps an atmosphere from being blown away by the
solar wind. This is what probably happened on Mars, although it still has some atmosphere, the planet was too small and too far from the Sun to remain
geologically active. Over time the core cooled off and the magnetosphere weakened and Mars lost most of it's atmosphere.
This document brings up a whole host of questions as to why this report was requested and by whom. Granted this time frame was the beginning of the
space race and the government was interested in everything about space, but it still makes me wonder if there was some other reason.