Mariner Mission to Venus
Prepared for the National Aeronautics and Space Administration BY THE STAFF, Jet Propulsion Laboratory, California Institute of Technology COMPILED BY HAROLD J. WHEELOCK FOREWORD BY W. H. PICKERING, Director, Jet Propulsion Laboratory, California Institute of Technology
McGRAW-HILL BOOK COMPANY, INC. New York, San Francisco, Toronto, London
Copyright © 1963 by the Jet Propulsion Laboratory, California Institute of Technology. All Rights Reserved. Printed in the United States of America.
Library of Congress Catalog Card Number 63-17489.
This book describes one phase of the U. S. civilian space program—the journey of the Mariner spacecraft to the vicinity of Venus and beyond. It reports upon the measurements taken during the “flyby” on December 14, 1962, when Mariner reached a point 21,598 miles from the planet, and 36,000,000 miles from Earth (communication with the spacecraft was continued up to a distance of approximately 54,000,000 miles from Earth). The Mariner mission was a project of the National Aeronautics and Space Administration, carried out under Contract No. NAS 7-100 by the Jet Propulsion Laboratory, California Institute of Technology.
For many centuries scientific information about the planets and the vast void that separates them has been collected by astronomers observing from the surface of the Earth. Now, with the flight of Mariner II, we suddenly have in our hands some 90 million bits of experimental data measured in the region between Earth and the planet Venus. Thus, man for the first time has succeeded in sending his instruments far into the depths of space, and indeed, in placing them near another planet. A whole new area of experimental astronomy has been opened up.
This book is a brief record of the Mariner Project to date and is designed to explain in general terms the preliminary conclusions. Actually, it will be months or years before all of the data from Mariner II have been completely analyzed. The most important data were the measurements made in the vicinity of the planet Venus, but it should also be noted that many weeks of interplanetary environmental measurements have given us new insight into some of the basic physical phenomena of the solar system. The trajectory data have provided new, more accurate measurements of the solar system. The engineering measurements of the performance of the spacecraft will be of inestimable value in the design of future spacecraft. Thus, the Mariner II spacecraft to Venus not only looks at Venus but gives space scientists and engineers information helpful in a wide variety of space ventures.
Jet Propulsion Laboratory
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MARINER MISSION TO VENUS
FOREWORD
CONTENTS
ACKNOWLEDGMENTS
THE DOUBLE STAR OF THE ANCIENT WORLD
THE CONSENSUS PRIOR TO MARINER II
THE CYTHEREAN RIDDLE: LIVING WORLD OR INCINERATED PLANET
A PROBLEM IN CELESTIAL DYNAMICS
THE ORGANIZATION
NASA: FOR SCIENCE
JPL: JATO TO MARINER
GENERAL DYNAMICS: THE ATLAS
LOCKHEED: AGENA B
THE SPACEFRAME
THE POWER SYSTEM
TELECOMMUNICATIONS: RELAYING THE DATA
ATTITUDE CONTROL: BALANCING IN SPACE
PROPULSION SYSTEM
TEMPERATURE CONTROL
THE SCIENTIFIC INSTRUMENTS
THE ATLAS BOOSTER: POWER OF SIX 707’S
THE AGENA B: START AND RESTART
MARINER I: AN ABORTIVE LAUNCH
MARINER II: A ROLL BEFORE PARKING
THE PARKING ORBIT
ORIENTATION AND MIDCOURSE MANEUVER
THE LONG CRUISE
ENCOUNTER AND BEYOND
THE RECORD OF MARINER
DEEP SPACE INSTRUMENTATION FACILITY
THE GOLDSTONE COMPLEX
THE WOOMERA STATION
THE JOHANNESBURG STATION
MOBILE TRACKING STATION
COMMUNICATION CONTROL
THE OPERATIONS CENTER
CENTRAL COMPUTING FACILITY
DATA CONDITIONING SYSTEM
COSMIC DUST DETECTOR
SOLAR PLASMA EXPERIMENT
HIGH-ENERGY RADIATION EXPERIMENT
THE MAGNETOMETER
MICROWAVE RADIOMETER
INFRARED RADIOMETER
MARINER’S SCIENTIFIC OBJECTIVES
SPACE WITHOUT DUST?
THE UBIQUITOUS SOLAR WIND
HIGH-ENERGY PARTICLES: FATAL DOSAGE?
A MAGNETIC FIELD?
THE SURFACE: HOW HOT?
CLOUD TEMPERATURES: THE INFRARED READINGS
THE RADAR PROFILE: MEASUREMENTS FROM EARTH
FOOTNOTES
INDEX
Transcriber’s Notes