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

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

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HEAO-1<br />

An X-ray astronomy satellite that surveyed the sky in the<br />

0.2 keV <strong>to</strong> 10 MeV energy band, providing nearly constant<br />

moni<strong>to</strong>ring <strong>of</strong> X-ray sources near the ecliptic poles.<br />

More detailed studies <strong>of</strong> a number <strong>of</strong> objects were made<br />

through pointed observations lasting typically three <strong>to</strong><br />

six hours. <strong>The</strong> spacecraft remained active until January 9,<br />

1979.<br />

HEAO-2<br />

<strong>The</strong> first fully imaging X-ray telescope <strong>to</strong> be placed in<br />

orbit; later renamed the Einstein Observa<strong>to</strong>ry <strong>to</strong> honor<br />

the centenary <strong>of</strong> the great physicist’s birth. Its angular resolution<br />

<strong>of</strong> a few arcseconds, field-<strong>of</strong>-view <strong>of</strong> tens <strong>of</strong><br />

arcminutes, and sensitivity several hundred times greater<br />

than any previous mission provided, for the first time,<br />

the capability <strong>to</strong> create images <strong>of</strong> extended objects and<br />

diffuse emission and <strong>to</strong> detect faint sources at such high<br />

energies (0.2–4.5 keV). It revolutionized astronomers’<br />

view <strong>of</strong> the X-ray sky. Observations ceased in April 1981.<br />

HEAO-3<br />

Like its predecessor HEAO-1, a survey mission operating<br />

in the hard X-ray and gamma-ray (50 keV–10 MeV) band.<br />

Its High Resolution Gamma-Ray Spectrometer Experiment,<br />

built by JPL (Jet Propulsion Labora<strong>to</strong>ry), was the<br />

largest germanium spectrometer placed in orbit at that<br />

time. <strong>The</strong> mission effectively ended when the cryogenic<br />

coolant for the germanium detec<strong>to</strong>rs ran out in May<br />

1981.<br />

Launch<br />

Vehicle: Atlas Centaur SLV-3D<br />

Site: Cape Canaveral<br />

heat barrier<br />

<strong>The</strong> speed above which friction with an atmosphere may<br />

damage a spacecraft. <strong>The</strong> heat barrier is <strong>of</strong> particular<br />

importance during reentry. Special systems are needed <strong>to</strong><br />

cool the spacecraft when it goes beyond the heat-barrier<br />

speed.<br />

heat-shield<br />

See reentry thermal protection.<br />

HEAO Missions<br />

Spacecraft Launch Date Orbit Mass (kg)<br />

HEAO-1 Aug. 12, 1977 429 × 447 × 22.7° 2,720<br />

HEAO-2 Nov. 12, 1978 526 × 548 × 23.5° 3,150<br />

HEAO-3 Sep. 20, 1979 487 × 503 × 22.7° 3,150<br />

heliopause 181<br />

heavy-lift launch vehicle (HLV)<br />

<strong>The</strong> most powerful type <strong>of</strong> space launch vehicle, sometimes<br />

defined as one having the capacity <strong>to</strong> place payloads<br />

<strong>of</strong> at least 10,000 kg in<strong>to</strong> low Earth orbit or<br />

payloads <strong>of</strong> 5,000 kg in<strong>to</strong> geostationary transfer orbit.<br />

Examples include the Space Shuttle, Atlas V, and Ariane<br />

5.<br />

helicon thruster<br />

A device that works in a similar way <strong>to</strong> the pulsedplasma<br />

thruster but with one important difference: a<br />

traveling electromagnetic wave interacts with a current<br />

sheet <strong>to</strong> maintain a strong force on a plasma moving<br />

along an axis. This circumvents the pulsed-plasma<br />

thruster’s problem <strong>of</strong> the force falling <strong>of</strong>f as the current<br />

loop gets larger. <strong>The</strong> traveling wave can be created in a<br />

variety <strong>of</strong> ways, and a helical coil is <strong>of</strong>ten used.<br />

heliocentric<br />

Related <strong>to</strong> or having the Sun as its center.<br />

heliopause<br />

<strong>The</strong> boundary <strong>of</strong> the heliosphere, where the pressure<br />

at the outer part <strong>of</strong> the heliosphere equals that <strong>of</strong> the<br />

heliopause <strong>The</strong> heliopause and other structures shown<br />

<strong>to</strong>gether with the exit trajec<strong>to</strong>ries <strong>of</strong> the twin Voyager and Pioneer<br />

probes. NASA

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