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Facing the Heat Barrier - NASA's History Office

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<strong>Facing</strong> <strong>the</strong> <strong>Heat</strong> <strong>Barrier</strong>: A <strong>History</strong> of Hypersonics<br />

terous. The Teapot Committee drew on findings by Augenstein’s group at Rand,<br />

which endorsed a 1,500-pound warhead and a three-mile miss distance. The formal<br />

Teapot report, issued in February 1954, declared “<strong>the</strong> military requirement” on miss<br />

distance “should be relaxed from <strong>the</strong> present 1,500 feet to at least two, and probably<br />

three, nautical miles.” Moreover, “<strong>the</strong> warhead weight might be reduced as far<br />

as 1,500 pounds, <strong>the</strong> precise figure to be determined after <strong>the</strong> Castle tests and by<br />

missile systems optimization.” 17<br />

The latter recommendation invoked Operation Castle, a series of H-bomb tests<br />

that began a few weeks later. The Mike shot of 1952 had used liquid deuterium,<br />

a form of liquid hydrogen. It existed at temperatures close to absolute zero and<br />

demanded much care in handling. But <strong>the</strong> Castle series was to test devices that used<br />

lithium deuteride, a dry powder that resembled salt. The Mike approach had been<br />

chosen because it simplified <strong>the</strong> weapons physics, but a dry bomb using lithium<br />

promised to be far more practical.<br />

The first such bomb was detonated on 1 March as Castle Bravo. It produced 15<br />

megatons, as its fireball expanded to almost four miles in diameter. O<strong>the</strong>r Castle<br />

H-bombs performed similarly, as Castle Romeo went to 11 megatons and Castle<br />

Yankee, a variant of Romeo, reached 13.5 megatons. “I was on a ship that was 30<br />

miles away,” <strong>the</strong> physicist Marshall Rosenbluth recalls about Bravo, “and we had this<br />

horrible white stuff raining out on us.” It was radioactive fallout that had condensed<br />

from vaporized coral. “It was pretty frightening. There was a huge fireball with<br />

<strong>the</strong>se turbulent rolls going in and out. The thing was glowing. It looked to me like a<br />

diseased brain.” Clearly, though, bombs of <strong>the</strong> lithium type could be as powerful as<br />

anyone wished—and <strong>the</strong>se test bombs were readily weaponizable. 18<br />

The Castle results, strongly complementing <strong>the</strong> Rand and Teapot reports,<br />

cleared <strong>the</strong> way for action. Within <strong>the</strong> Pentagon, Gardner took <strong>the</strong> lead in pushing<br />

for Atlas. On 11 March he met with Air Force Secretary Harold Talbott and with<br />

<strong>the</strong> Chief of Staff, General Nathan Twining. He proposed a sped-up program that<br />

would nearly double <strong>the</strong> Fiscal Year (FY) 1955 Atlas budget and would have <strong>the</strong> first<br />

missiles ready to launch as early as 1958. General Thomas White, <strong>the</strong> Vice Chief of<br />

Staff, weighed in with his own endorsement later that week, and Talbott responded<br />

by directing Twining to accelerate Atlas immediately.<br />

White carried <strong>the</strong> ball to <strong>the</strong> Air Staff, which held responsibility for recommending<br />

approval of new programs. He told its members that “ballistic missiles were<br />

here to stay, and <strong>the</strong> Air Staff had better realize this fact and get on with it.” Then<br />

on 14 May, having secured concurrence from <strong>the</strong> Secretary of Defense, White gave<br />

Atlas <strong>the</strong> highest Air Force development priority and directed its acceleration “to<br />

<strong>the</strong> maximum extent that technology would allow.” Gardner declared that White’s<br />

order meant “<strong>the</strong> maximum effort possible with no limitation as to funding.” 19<br />

This was a remarkable turnaround for a program that at <strong>the</strong> moment lacked<br />

even a proper design. Many weapon concepts have gone as far as <strong>the</strong> prototype<br />

28<br />

Nose Cones and Re-entry<br />

stage without winning approval, but Atlas gained its priority at a time when <strong>the</strong><br />

accepted configuration still was <strong>the</strong> 440,000-pound, five-engine concept of 1953.<br />

Air Force officials still had to establish a formal liaison with <strong>the</strong> AEC to win access<br />

to information on projected warhead designs. Within <strong>the</strong> AEC, lightweight bombs<br />

still were well in <strong>the</strong> future. A specialized device, tested in <strong>the</strong> recent series as Castle<br />

Nectar, delivered 1.69 megatons but weighed 6,520 pounds. This was four times<br />

<strong>the</strong> warhead weight proposed for Atlas.<br />

But in October <strong>the</strong> AEC agreed that it could develop warheads weighing 1,500<br />

to 1,700 pounds, with a yield of one megaton. This opened <strong>the</strong> door to a new Atlas<br />

design having only three engines. It measured 75 feet long and 10 feet in diameter,<br />

with a weight of 240,000 pounds—and its miss distance could be as great as five miles.<br />

This took note of <strong>the</strong> increased yield of <strong>the</strong> warhead and fur<strong>the</strong>r eased <strong>the</strong> problem of<br />

guidance. The new configuration won Air Force approval in December. 20<br />

Approaching <strong>the</strong> Nose Cone<br />

An important attribute of a nose cone was its shape, and engineers were reducing<br />

drag to a minimum by crafting high-speed airplanes that displayed <strong>the</strong> ultimate<br />

in needle-nose streamlining. The X-3 research aircraft, designed for Mach 2, had a<br />

long and slender nose that resembled a church steeple. Atlas went even fur<strong>the</strong>r, with<br />

an early concept having a front that resembled a flagpole. This faired into a long and<br />

slender cone that could accommodate <strong>the</strong> warhead. 21<br />

This intuitive approach fell by <strong>the</strong> wayside in 1953, as <strong>the</strong> NACA-Ames aerodynamicists<br />

H. Julian Allen and Alfred Eggers carried through an elegant analysis<br />

of <strong>the</strong> motion and heating of a re-entering nose cone. This work showed that <strong>the</strong>y<br />

were masters of <strong>the</strong> simplifying assumption. To make such assumptions successfully<br />

represents a high art, for <strong>the</strong> resulting solutions must capture <strong>the</strong> most essential<br />

aspects of <strong>the</strong> pertinent physics while preserving ma<strong>the</strong>matical tractability. Their<br />

paper stands to this day as a landmark. Quite probably, it is <strong>the</strong> single most important<br />

paper ever written in <strong>the</strong> field of hypersonics.<br />

They calculated total heat input to a re-entry vehicle, seeking shapes that would<br />

minimize this. That part of <strong>the</strong> analysis enabled <strong>the</strong>m to critique <strong>the</strong> assertion that<br />

a slender and sharply-pointed shape was best. For a lightweight nose cone, which<br />

would slow significantly in <strong>the</strong> atmosphere due to drag, <strong>the</strong>y found a surprising<br />

result: <strong>the</strong> best shape, minimizing <strong>the</strong> total heat input, was blunt ra<strong>the</strong>r than sharp.<br />

The next issue involved <strong>the</strong> maximum rate of heat transfer when averaged over<br />

an entire vehicle. To reduce this peak heating rate to a minimum, a nose cone of<br />

realistic weight might be ei<strong>the</strong>r very sharp or very blunt. Missiles of intermediate<br />

slenderness gave considerably higher peak heating rates and “were definitely to be<br />

avoided.”<br />

29

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