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The Solar System

Presenting an issue on what is known about the sun and the bodies In orbit around it, with special reference to the knowledge gained In 18 years of exploration by space probes launched from the earth

By Carl Sagan

The Origin and Evolution of the Solar System

It is generally agreed that some 4.6 billion years ago the sun and the planets formed out of a rotating disk of gas and dust. Eactly how they did so remains a lively topic of investigation

By A. G. W. Cameron

The Sun

Recent spacecraft observations have revealed spectacular new features of the solar surface and atmosphere. What happens inside the sun, however, has lately become more mysterious

By E. N. Parker

Mercury

The remarkable pictures made by the spacecraft Mariner 10 have revealed a planetary paradox: Although Mercury is like the earth on the inside, it is like the moon on the outside

By Bruce C. Murray

Venus

It is cratered like the rest of the inner planets, but its surface has been transformed by its dense and cloudy atmosphere. The clouds trap sunlight to maintain a temperature of 900 degrees Fahrenheit

By Andrew and Louise Young

The Earth

The outstanding feature of our own planet is the dynamic activity of its atmosphere and its crust. Both have been substantially altered by the evolution of living organisms

By Raymond Siever

The Moon

Lacking an erosive atmosphere and geologically active outer layers, the earth's lifeless satellite has preserved a record of early events (but not the primordial events) in the history of the solar system

By John A. Wood

Mars

The first closeup photographs of it suggested that it was a cratered body as dead as the moon. Later pictures show a host of remarkable features indicative of a lively past

By James B. Pollack

Jupiter

More massive than all the other planets put together, it consists largely of hydrogen and helium. Below its turbulent atmosphere the hydrogen forms two liquid layers, one molecular and one metallic

By John H. Wolfe

The Outer Planets

Beyond Jupiter are the remote unexplored planets: Saturn, Uranus, Neptune and Pluto. Saturn has a composition much like Jupiter's; Uranus and Neptune appear to be rockier. Pluto is a small maverick

By Donald M. Hunten

The Smaller Bodies of the Solar System

They range in size from meteoroids no larger than a grain of sand to moons bigger than the planet Mercury. Many of them appear to be fragments resulting from collisions between growing planetesimals

By William K. Hartmann

Interplanetary Particles and Fields

A "wind" of charged particles blows out from the sun, punctuated by energetic bursts. These particles interact with the magnetic fields of the planets in intricate ways

By James A. Van Allen

Departments

  • 50 and 100 Years Ago, September 1975

  • Science and the Citizen, September 1975

  • Letters

    Letters to the Editors, September 1975

  • Recommended

    Books, September 1975

  • Mathematical Recreation

    Mathematical Games, September 1975

  • Amateur Scientist

    The Amateur Scientist, September 1975

  • Departments

    The Authors, September 1975

  • Bibliography, September 1975

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September 1975

See the World from a Different Perspective

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