This is a look at the Astrobiological occurance of life in the Universe, primarily derived through temperature and density.
The report takes a look at possibility of life on other planets from the stand point of size and nature of planets or stars, from which living
organisms may arise.
It is written that there is no definite information regarding the origin of life even on Earth, authorities generally agree that coacervates in an
aqueous medium, represent the earliest stage in the evolution of organic substances into living organisms.
That an atmosphere over the solid crust of the planet is important from allowing water to evaporate rapidly during the first stages of development.
Living organisms without the aid of some liquid medium would be virtually inconceivable. Stars and planets are conceived from interstellar medium
composed primarily of hydrogen. They theorize that in the early evolution of a star or planet the atmosphere is primarily hydrogen especially in its
outer envelope.Thus the hydrogen atmosphere then must be at least partially dissipated. The present atmosphere of the Earth must be a secondary one
formed as results of the process's of chemical reaction before the earth took formation as a planet.
Dissipation of hydrogen should not be so large a loss by a plant or protoplanet so as to change drastically its chemical content. On the other hand
hydrogen must be a dominant ingredient in the upper layers of in the early stages because of its high cosmic abundance and its lightness.
The conclusion is that the most likely radius of life sustaining planets would be between 10/8thcm and 2x10/9thcm
Conditions such as density and also bear upon the occurance of life thus
Tenatively they conclude that a habitable planet has most likely a radius between 10^8 and 2x10^9, admittedly a generous estimate since that range
includes the Moon and Mercury, both which are considered unfavorable for indegenious life due to their position in the solar system and their density.

