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

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184 high mass fraction<br />

two S<strong>of</strong>t X-ray Imagers, which have 33-arcsecond resolution.<br />

This gives astronomers precise locations <strong>of</strong> gammaray<br />

bursts and allows detailed follow-up with optical<br />

instruments on the ground. <strong>The</strong> Massachusetts Institute<br />

<strong>of</strong> Technology operates the satellite, and the program is<br />

managed by the Goddard Space Flight Center as an<br />

Explorer Mission <strong>of</strong> Opportunity.<br />

Launch<br />

Date: Oc<strong>to</strong>ber 9, 2000<br />

Vehicle: Pegasus<br />

Site: Kwajalein Missile Range, Marshall Islands<br />

Orbit: 598 × 641 km × 1.9°<br />

high mass fraction<br />

A high value <strong>of</strong> the ratio <strong>of</strong> propellant mass <strong>to</strong> <strong>to</strong>tal<br />

mo<strong>to</strong>r mass. Values <strong>of</strong> 0.9 and greater characterize highmass<br />

fraction mo<strong>to</strong>rs.<br />

High Resolution X-ray Spectroscopy Mission<br />

A mission that would provide an exciting new approach<br />

<strong>to</strong> studying the origin <strong>of</strong> the chemical elements in stellar<br />

nucleosynthesis as well as active galaxies and galaxy clusters.<br />

It is identified in NASA’s Office <strong>of</strong> Space Science<br />

Strategic Plan as a potential mission beyond 2007 but<br />

remains in the early concept definition phase.<br />

high-energy radiation<br />

Penetrating particle or electromagnetic radiation with<br />

energies <strong>of</strong> more than a few thousand electron volts. It<br />

may include electrons, neutrons, pro<strong>to</strong>ns, mesons, X-rays,<br />

and gamma rays.<br />

high-gain antenna (HGA)<br />

A type <strong>of</strong> antenna used on board spacecraft <strong>to</strong> provide<br />

high amplification <strong>of</strong> either transmitted or received radio<br />

signals. HGAs typically consist <strong>of</strong> parabolic dishes and<br />

must be accurately pointed <strong>to</strong> be useful.<br />

Highwater<br />

Two suborbital tests <strong>of</strong> the Saturn I launch vehicle that<br />

resulted in the creation <strong>of</strong> massive ice clouds in the iono-<br />

Highwater Missions<br />

sphere. <strong>The</strong> second and third stages <strong>of</strong> the Saturn contained<br />

87,000 liters <strong>of</strong> water <strong>to</strong> simulate the mass <strong>of</strong> fully<br />

fueled stages. Following the successful launch <strong>of</strong> the first<br />

stage, the rocket was de<strong>to</strong>nated by explosives with a signal<br />

from the ground. <strong>The</strong> released water formed a massive<br />

cloud <strong>of</strong> ice particles several kilometers in diameter. By<br />

this experiment, scientists had hoped <strong>to</strong> obtain data on<br />

atmospheric physics, but poor telemetry made the results<br />

questionable. Highwater 2 marked the third straight<br />

launch success for the Saturn I and the first with maximum<br />

mass on board. (See table, “Highwater Missions.”)<br />

Himawari<br />

See GMS (Geostationary Meteorological Satellite).<br />

Hino<strong>to</strong>ri<br />

A Japanese satellite launched by ISAS (Institute <strong>of</strong> Space<br />

and Astronautical Science) principally <strong>to</strong> investigate X-rays<br />

from the Sun. It carried high-resolution s<strong>of</strong>t (longer wavelength)<br />

X-ray spectrometers and hard (shorter wavelength)<br />

X-ray instruments that obtained the first images <strong>of</strong> solar<br />

flares at energies above 25 keV and also observed celestial<br />

X-ray bursts. Hino<strong>to</strong>ri, whose name means “phoenix,” was<br />

known before launch as Astro-A.<br />

Launch<br />

Date: February 21, 1981<br />

Vehicle: M-3S<br />

Site: Kagoshima<br />

Orbit: 576 × 644 ×31°<br />

Mass: 188 kg<br />

Hipparcos<br />

An ESA (European Space Agency) astrometry satellite for<br />

measuring the position, brightness, and proper motion<br />

(movement against the distant stellar background) <strong>of</strong> relatively<br />

nearby stars <strong>to</strong> an unprecedented degree <strong>of</strong> accuracy.<br />

Its name is an abbreviation <strong>of</strong> High Precision<br />

Parallax Collecting Satellite and was chosen for its (somewhat<br />

strained) similarity <strong>to</strong> that <strong>of</strong> the Greek astronomer<br />

Hipparchus <strong>of</strong> Rhodes (190–120 B.C.). Although a faulty<br />

launch put Hipparcos in a highly elliptical orbit instead <strong>of</strong><br />

Launch site: Cape Canaveral<br />

De<strong>to</strong>nation<br />

Spacecraft Date Altitude (km) Time after Launch Length <strong>of</strong> Experiment<br />

Highwater 1 Apr. 25, 1962 105 2.5 min 1.62 days<br />

Highwater 2 Nov. 16, 1962 167 4 min 53 sec 1.46 days

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