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Exploring the Unknown: Selected Documents in ... - The Black Vault

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50<br />

First Steps <strong>in</strong>to Space: Projects Mercury and Gem<strong>in</strong>i<br />

Document I-2<br />

Document Title: H. Julian Allen and A. J. Eggers, Jr., NACA, “Research<br />

Memorandum: A Study of <strong>the</strong> Motion and Aerodynamic Heat<strong>in</strong>g of Missiles<br />

Enter<strong>in</strong>g <strong>the</strong> Earth’s Atmosphere at High Supersonic Speeds,” 25 August 1953.<br />

Source: Folder 18674, NASA Historical Reference Collection, NASA History<br />

Division, NASA Headquarters, Wash<strong>in</strong>gton, DC.<br />

In <strong>the</strong> later 1940s aerodynamicists began research on <strong>the</strong> best means of reentry to Earth from<br />

space, where <strong>the</strong> high speeds caused atmospheric heat<strong>in</strong>g <strong>in</strong> excess of 1,800°F. <strong>The</strong>se <strong>in</strong>vestigations<br />

found that a blunt-nose body experienced much less heat<strong>in</strong>g than a po<strong>in</strong>ted body,<br />

which would burn up before reach<strong>in</strong>g Earth’s surface. <strong>The</strong> blunt reentry body, discovered <strong>in</strong><br />

1951 by H. Julian Allen, an eng<strong>in</strong>eer with NACA’s Ames Research Center, created a stronger<br />

shock wave at <strong>the</strong> nose of <strong>the</strong> vehicle and dumped a good deal of <strong>the</strong> reentry heat <strong>in</strong>to <strong>the</strong><br />

airflow, mak<strong>in</strong>g less heat available to heat <strong>the</strong> reentry vehicle itself. Allen’s work led to <strong>the</strong><br />

design of wide-body bases for spacecraft, giv<strong>in</strong>g <strong>the</strong> capsules <strong>the</strong>ir characteristic “teardrop”<br />

shape, and to <strong>the</strong> use of <strong>the</strong> ablative heat shields that protected <strong>the</strong> Mercury, Gem<strong>in</strong>i, and<br />

Apollo astronauts as <strong>the</strong>ir space capsules reentered Earth’s atmosphere. This document represents<br />

one of Allen’s earliest contributions to understand<strong>in</strong>g <strong>the</strong> reentry problem. Coupled with<br />

his later contributions, as well as with <strong>the</strong> research of o<strong>the</strong>rs <strong>in</strong>clud<strong>in</strong>g his early collaborator<br />

Alfred Eggers, Allen’s research made possible human spaceflight <strong>in</strong> <strong>the</strong> 1960s.<br />

NACA<br />

RESEARCH MEMORANDUM<br />

A STUDY OF THE MOTION AND AERODYNAMIC HEATING OF MISSILES<br />

ENTERING THE EARTH’S ATMOSPHERE AT HIGH SUPERSONIC SPEEDS<br />

By H. Julian Allen and A. J. Eggers, Jr.<br />

Ames Aeronautical Laboratory<br />

Moffett Field, Calif.<br />

August 25, 1953<br />

SUMMARY<br />

A simplified analysis is made of <strong>the</strong> velocity and deceleration history of missiles<br />

enter<strong>in</strong>g <strong>the</strong> earth’s atmosphere at high supersonic speeds. It is found that,<br />

<strong>in</strong> general, <strong>the</strong> gravity force is negligible compared to <strong>the</strong> aerodynamic drag force<br />

and, hence, that <strong>the</strong> trajectory is essentially a straight l<strong>in</strong>e. A constant drag coefficient<br />

and an exponential variation of density with altitude are assumed and generalized<br />

curves for <strong>the</strong> variation of missile speed and deceleration with altitude<br />

are obta<strong>in</strong>ed. A curious f<strong>in</strong>d<strong>in</strong>g is that <strong>the</strong> maximum deceleration is <strong>in</strong>dependent<br />

of physical characteristics of a missile (e.g., mass, size, and drag coefficient) and

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