The Earth in space: An essay on the origin of the Solar system
The origin of the sun and planets has been reviewed<br />from manifold considerations &mdash; nuclear, astrophysical, chemical and geophysical.<br />Basically, there are two schools of thought: monistic, which<br />postulates that the sun and the pla...
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Istituto Nazionale di Geofisica e Vulcanologia (INGV)
1964-06-01
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doaj-2fdb7d5e36d14996bdf27a04a8131fa62020-11-25T02:15:43ZengIstituto Nazionale di Geofisica e Vulcanologia (INGV)Annals of Geophysics1593-52132037-416X1964-06-0117341844710.4401/ag-5218The Earth in space: An essay on the origin of the Solar systemS. BURMANThe origin of the sun and planets has been reviewed<br />from manifold considerations &mdash; nuclear, astrophysical, chemical and geophysical.<br />Basically, there are two schools of thought: monistic, which<br />postulates that the sun and the planets formed from some primordial system<br />of gases; and dualistic, which holds that the planets and meteorites had<br />genesis in the sun's collision wtili another star. The extreme improbability<br />of collision almost discards this hypothesis.<br />The present day accepted theories are, hence, the monistic ones, and<br />the one particularly favored is the Dust &mdash; cloud hypothesis &mdash; that the sun<br />condensed into a star due to the gravitational collapse of a massive interstellar<br />gas-cloud, and subsequently gave birth to planets as further evolution<br />of the cloud progressed. Studies of extinct radioactivities, within the<br />framework of the above hypothesis, give clue to the early history of the<br />solar system and in particular indicate that the time interval between the<br />start of condensation and the formation of the meteorite parent-bodies is<br />less six million years (Cameron). In this context the origin of stars from<br />" globules " or proto-stars has been briefly discussed.<br />A somewhat " exotic " theory of the formation of planets from the<br />sun which hinged on the concept of secular decrease of the ' constant ' of<br />gravitation with the age of the universe (Dirac's hypothesis) has been discussed.<br />The earth (with expansion of its volume) and other celestial<br />bodies might provide empirical confirmation of the concept of diminishing<br />gravitation &mdash; an important problem of general relativity. This new idea<br />of physics might revolutionise fundamental concepts in geology and geophysics.http://www.annalsofgeophysics.eu/index.php/annals/article/view/5218 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
S. BURMAN |
spellingShingle |
S. BURMAN The Earth in space: An essay on the origin of the Solar system Annals of Geophysics |
author_facet |
S. BURMAN |
author_sort |
S. BURMAN |
title |
The Earth in space: An essay on the origin of the Solar system |
title_short |
The Earth in space: An essay on the origin of the Solar system |
title_full |
The Earth in space: An essay on the origin of the Solar system |
title_fullStr |
The Earth in space: An essay on the origin of the Solar system |
title_full_unstemmed |
The Earth in space: An essay on the origin of the Solar system |
title_sort |
earth in space: an essay on the origin of the solar system |
publisher |
Istituto Nazionale di Geofisica e Vulcanologia (INGV) |
series |
Annals of Geophysics |
issn |
1593-5213 2037-416X |
publishDate |
1964-06-01 |
description |
The origin of the sun and planets has been reviewed<br />from manifold considerations &mdash; nuclear, astrophysical, chemical and geophysical.<br />Basically, there are two schools of thought: monistic, which<br />postulates that the sun and the planets formed from some primordial system<br />of gases; and dualistic, which holds that the planets and meteorites had<br />genesis in the sun's collision wtili another star. The extreme improbability<br />of collision almost discards this hypothesis.<br />The present day accepted theories are, hence, the monistic ones, and<br />the one particularly favored is the Dust &mdash; cloud hypothesis &mdash; that the sun<br />condensed into a star due to the gravitational collapse of a massive interstellar<br />gas-cloud, and subsequently gave birth to planets as further evolution<br />of the cloud progressed. Studies of extinct radioactivities, within the<br />framework of the above hypothesis, give clue to the early history of the<br />solar system and in particular indicate that the time interval between the<br />start of condensation and the formation of the meteorite parent-bodies is<br />less six million years (Cameron). In this context the origin of stars from<br />" globules " or proto-stars has been briefly discussed.<br />A somewhat " exotic " theory of the formation of planets from the<br />sun which hinged on the concept of secular decrease of the ' constant ' of<br />gravitation with the age of the universe (Dirac's hypothesis) has been discussed.<br />The earth (with expansion of its volume) and other celestial<br />bodies might provide empirical confirmation of the concept of diminishing<br />gravitation &mdash; an important problem of general relativity. This new idea<br />of physics might revolutionise fundamental concepts in geology and geophysics. |
url |
http://www.annalsofgeophysics.eu/index.php/annals/article/view/5218 |
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