13.12.2012 Views

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

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

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

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

ERM ended in January 1990 (due <strong>to</strong> failures <strong>of</strong> both<br />

onboard tape recorders), more than three years <strong>of</strong> precise<br />

altimetry data were available <strong>to</strong> the scientific community.<br />

Launch<br />

Date: March 13, 1985<br />

Vehicle: Atlas E<br />

Site: Vandenberg Air Force Base<br />

Orbit: 775 × 779 km × 108.1°<br />

Mass: 635 kg<br />

geospace<br />

<strong>The</strong> domain <strong>of</strong> Sun-Earth interactions, also known as the<br />

solar-terrestrial environment. It consists <strong>of</strong> the particles,<br />

fields, and radiation environment from the Sun <strong>to</strong><br />

Earth’s space plasma environment and upper atmosphere.<br />

Geospace is considered <strong>to</strong> be the fourth physical<br />

geosphere, after solid earth, oceans, and atmosphere.<br />

geostationary orbit (GSO)<br />

A direct, circular geosynchronous orbit at an altitude <strong>of</strong><br />

35,784 km that lies in the plane <strong>of</strong> Earth’s equa<strong>to</strong>r. A<br />

satellite in this orbit always appears at the same position<br />

in the sky, and its ground-track is a point. Such an<br />

arrangement is ideal for some communication satellites<br />

andmeteorological satellites, since it allows one satellite<br />

<strong>to</strong> provide continuous coverage <strong>of</strong> a given area <strong>of</strong> Earth’s<br />

surface.<br />

geosynchronous orbit<br />

A direct, circular, low-inclination orbit around Earth<br />

having a period <strong>of</strong> 23 hours 56 minutes 4 seconds and a<br />

corresponding altitude <strong>of</strong> 35,784 km (22,240 miles, or 6.6<br />

Earth-radii). In such an orbit, a satellite maintains a position<br />

above Earth that has the same longitude. However,<br />

if the orbit’s inclination is not exactly zero, the satellite’s<br />

ground-track describes a figure eight. In most cases, the<br />

orbit is chosen <strong>to</strong> have a zero inclination, and stationkeeping<br />

procedures are carried out so that the spacecraft<br />

hangs motionless with respect <strong>to</strong> a point on the planet<br />

GEOS Missions<br />

geosynchronous/geostationary transfer orbit (GTO) 159<br />

Spacecraft Date<br />

Launch<br />

Vehicle Site Orbit Mass (kg)<br />

GEOS 1 Nov. 6, 1965 Delta E Cape Canaveral 1,114 × 2,273 km × 59.4° 175<br />

GEOS 2 Jan. 11, 1968 Delta E Vandenberg 1,079 × 1,572 km × 105.8° 209<br />

GEOS 3 Apr. 9, 1975 Delta 2918 Vandenberg 816 × 850 km × 115.0° 341<br />

below. In this case, the orbit is said <strong>to</strong> be a geostationary<br />

orbit.<br />

geosynchronous/geostationary<br />

transfer orbit (GTO)<br />

An elliptical orbit, with an apogee(high point) <strong>of</strong> 35,784<br />

km, a perigee (low point) <strong>of</strong> a few hundred kilometers,<br />

and an inclination roughly equal <strong>to</strong> the latitude <strong>of</strong> the<br />

launch site, in<strong>to</strong> which a spacecraft is initially placed<br />

before being transferred <strong>to</strong> a geosynchronous orbit<br />

(GSO). After attaining GTO, the spacecraft’s apogee<br />

kick mo<strong>to</strong>r is fired <strong>to</strong> circularize the orbit and thereby<br />

achieve the desired final orbit. Typically, this burn will<br />

also reduce the orbital inclination <strong>to</strong> 0° so that the final<br />

orbit is not only geosynchronous but also geostationary.<br />

Because the greater the initial inclination, the greater the<br />

velocity change (delta ν) needed <strong>to</strong> remove this inclination,<br />

it is important that launches <strong>of</strong> GSO satellites take<br />

place as close <strong>to</strong> the equa<strong>to</strong>r as possible. For example, in<br />

a Delta or an Atlas launch from Cape Canaveral, the<br />

transfer orbit is inclined at 28.5° and the required delta<br />

νincrement at apogee is 1,831 m/s; for an Ariane launch<br />

from Guiana Space Centre, the inclination is 7° and the<br />

deltaνis 1,502 m/s; while for a Zenit flight from the Sea<br />

Launch platform on the equa<strong>to</strong>r, the delta ν is 1,478<br />

m/s. By the rocket equation, assuming a (typical) specific<br />

impulse <strong>of</strong> 300 seconds, the fraction <strong>of</strong> the separated<br />

mass consumed by the propellant for the apogee<br />

maneuver is 46% from Cape Canaveral, 40% from<br />

Kourou, and 39% from the equa<strong>to</strong>r. As a rough guide,<br />

the mass <strong>of</strong> a geostationary satellite at the start <strong>of</strong> its<br />

operational life (in GSO) is about half its initial on-orbit<br />

mass when separated from the launch vehicle (in GTO).<br />

Before carrying out the apogee maneuver, the spacecraft<br />

must be reoriented in the transfer orbit <strong>to</strong> face in the<br />

proper direction for the thrust. This reorientation is<br />

sometimes done by the launch vehicle at spacecraft separation;<br />

otherwise, it must be carried out in a separate<br />

maneuver by the spacecraft itself. In a launch from Cape<br />

Canaveral, the angle through which the satellite must be<br />

reoriented is about 132°.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!