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The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity

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ora<strong>to</strong>ry from 1935 <strong>to</strong> 1958, during which time he earned<br />

his Ph.D. In 1955, he became direc<strong>to</strong>r <strong>of</strong> the Vanguard<br />

satellite program. When that program became part <strong>of</strong><br />

NASA on Oc<strong>to</strong>ber 1, 1958, he remained chief <strong>of</strong> the<br />

NASA Vanguard division and then became assistant<br />

direc<strong>to</strong>r <strong>of</strong> spaceflight development (1958–1960). In February<br />

1960, he became direc<strong>to</strong>r <strong>of</strong> NASA’s <strong>of</strong>fice for the<br />

United Nations conference and, later, assistant direc<strong>to</strong>r<br />

<strong>of</strong> NASA’s <strong>of</strong>fice <strong>of</strong> plans and program evaluation. In<br />

1962, Hagen returned <strong>to</strong> higher education as a pr<strong>of</strong>essor<br />

<strong>of</strong> astronomy at Pennsylvania State University, becoming<br />

head <strong>of</strong> the department in 1975.<br />

Hagoromo<br />

A small (12-kg) lunar orbiter ejected from the Japanese<br />

Hiten spacecraft on March 19, 1990; its name means<br />

“angel’s robe.” Contact with the probe was lost after its<br />

release.<br />

Haise, Fred Wallace, Jr. (1933–)<br />

An American astronaut who served as Lunar Module<br />

pilot on the ill-fated <strong>Apollo</strong> 13 mission. Haise received<br />

a B.S. in aeronautical engineering from the University<br />

<strong>of</strong> Oklahoma in 1959 and joined the Navy in 1962, subsequently<br />

serving as a fighter pilot in the Oklahoma<br />

National Guard. He was the Aerospace Research Pilot<br />

School’s outstanding graduate <strong>of</strong> Class 64A and served<br />

with the Air Force from 1961 <strong>to</strong> 1962 as a tactical fighter<br />

pilot. NASA then tapped him as a research pilot at its<br />

Flight Research Center at Edwards, California, and at its<br />

Lewis Research Center. Haise was one <strong>of</strong> 19 selected by<br />

NASA in its fifth class <strong>of</strong> astronauts in April 1966. He<br />

was backup Lunar Module pilot for <strong>Apollo</strong> 8 and<br />

<strong>Apollo</strong> 11 before being named <strong>to</strong> that slot on <strong>Apollo</strong><br />

13. <strong>From</strong> 1973 <strong>to</strong> 1976, Haise was technical assistant<br />

<strong>to</strong> the manager <strong>of</strong> the Space Shuttle Orbiter Project.<br />

He was commander <strong>of</strong> one <strong>of</strong> the two-man crews that<br />

piloted Shuttle approach and landing test flights in<br />

1977. <strong>The</strong>se flights evaluated the Shuttle’s capabilities<br />

after the test vehicle Enterprise was released from the<br />

back <strong>of</strong> a Boeing 747 jet above the California desert.<br />

Haise retired from NASA in June 1979 and held several<br />

managerial positions with Grumman Aerospace Corporation<br />

before retiring in 1996.<br />

Hakucho<br />

<strong>The</strong> first Japanese X-ray astronomy satellite; it was named<br />

“swan” in Japanese because one <strong>of</strong> the most powerful<br />

cosmic X-ray sources is Cygnus X-1. Like many other<br />

X-ray satellites deployed around this time, Hakucho was<br />

designed <strong>to</strong> study and moni<strong>to</strong>r transient (quick-changing)<br />

phenomena, with special emphasis on X-ray bursts in the<br />

energy range <strong>of</strong> 0.1 <strong>to</strong> 100 keV. It was known prior <strong>to</strong><br />

Hale, Edward Everett 177<br />

launch as Corsa-B. Hakucho s<strong>to</strong>pped operating in April<br />

1985.<br />

Launch<br />

Date: February 21, 1979<br />

Vehicle: M-3S<br />

Site: Kagoshima<br />

Orbit: 543 × 566 km × 29.8°<br />

Mass: 96 kg<br />

HALCA (Highly Advanced Labora<strong>to</strong>ry for<br />

Communications and Astronomy)<br />

A Japanese satellite that forms the first spaceborne element<br />

<strong>of</strong> the VSOP (VLBI Space Observa<strong>to</strong>ry Program),<br />

led by ISAS (Institute <strong>of</strong> Space and Astronautical Science)<br />

in collaboration with the National Astronomical<br />

Observa<strong>to</strong>ry <strong>of</strong> Japan. HALCA’s main instrument is an<br />

8-m-diameter radio telescope. <strong>The</strong> satellite’s highly elliptical<br />

orbit facilitates VLBI (Very Long Baseline Interferometry)<br />

observations on baselines up <strong>to</strong> three times<br />

longer than those achievable on Earth. Observations are<br />

made at 1.6 GHz, 5 GHz, and 22 GHz. HALCA is also<br />

known by the national name Haruka (“far away”)—a reference<br />

<strong>to</strong> its great distance from Earth at apogee (the<br />

highest point <strong>of</strong> its orbit). Before launch, the satellite was<br />

called MUSES-B.<br />

Launch<br />

Date: February 12, 1997<br />

Vehicle: M-5<br />

Site: Kagoshima<br />

Orbit: 569 × 21,415 km × 31.4°<br />

Hale, Edward Everett (1822–1909)<br />

A prolific American writer, a contributing edi<strong>to</strong>r <strong>to</strong> <strong>The</strong><br />

Atlantic Monthly, and almost certainly the only science fiction<br />

writer <strong>to</strong> serve as chaplain <strong>to</strong> the U.S. Senate; he<br />

appears <strong>to</strong> have been the first <strong>to</strong> describe an artificial Earth<br />

satellite. His short s<strong>to</strong>ry “<strong>The</strong> Brick Moon” (1869) and its<br />

sequel, “Life on the Brick Moon,” 140 both published in <strong>The</strong><br />

Atlantic Monthly, tell <strong>of</strong> a 200-foot diameter sphere (built <strong>of</strong><br />

bricks <strong>to</strong> “stand fire very, very well”) that is due <strong>to</strong> be<br />

launched in<strong>to</strong> an orbit 4,000 miles high. Since its purpose<br />

is <strong>to</strong> provide a longitude fix for naviga<strong>to</strong>rs who will see it<br />

from the ground as a bright star, Hale reasons correctly<br />

that a polar orbit is needed. In effect, the Brick Moon will<br />

move around a giant Greenwich meridian in the sky, fulfilling<br />

the same role for the measurement <strong>of</strong> longitude that<br />

the Pole Star does for latitude. Two huge, spinning flywheels<br />

are set up <strong>to</strong> throw the artificial moon in<strong>to</strong> its correct<br />

orbital path—but something goes wrong. <strong>The</strong> brick<br />

sphere rolls prematurely down “upon these angry flywheels,

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