Themes > Science > Astronomy > Astronautics > History before sputnik (1957)

People dreamed of spaceflight for millennia before it became reality. Evidence of the dream exists in myth and fiction as far back as Babylonian texts of 4000  BC. The ancient Greek myths of Daedalus and Icarus also reflect the universal desire to fly. As early as the 2nd century AD, the Greek satirist Lucian wrote about an imaginary voyage to the moon. In the early 17th century the German astronomer Johannes Kepler wrote Somnium (Sleep), which might be called a scientific satire of a journey to the moon. The French writer and philosopher Voltaire, in Micromégas (1752), told of the travels of certain inhabitants of Sirius and Saturn; and in 1865 the French author Jules Verne depicted space travel in his popular novel From the Earth to the Moon. The dream of flight into space continued unabated into the 20th century, notably in the works of the British writer H. G. Wells, who published The War of the Worlds in 1898 and  The First Men in the Moon in 1901. More recently, fantasies of spaceflight have been nourished by science fiction.
 
Early Developments
During the centuries when space travel was only a fantasy, researchers in the sciences of astronomy, chemistry, mathematics, meteorology, and physics developed an understanding of the solar system, the stellar universe, the atmosphere of the earth, and the probable environment in space. In the 7th and 6th centuries BC, the Greek philosophers Thales and Pythagoras noted that the earth is a sphere; in the 3rd century BC the astronomer Aristarchus of Sámos asserted that the earth moved around the sun. Hipparchus, another Greek, prepared information about stars and the motions of the moon in the 2nd century BC. In the 2nd century AD Ptolemy of Alexandria placed the earth at the center of the solar system in the Ptolemaic system.
 
Scientific Discoveries
Not until some 1400 years later did the Polish astronomer Nicolaus Copernicus systematically explain that the planets, including the earth, revolve about the sun . Later in the 16th century the observations of the Danish astronomer Tycho Brahe greatly influenced the laws of planetary motion set forth by German astronomer Johannes Kepler. Italian scientist Galileo and British scientists Edmund Halley, Sir William Herschel, and Sir James Jeans were other astronomers who made contributions pertinent to astronautics.


Celestial Models by Ptolemy and Copernicus
Currently, most people consider it obvious that the sun is at the center of the solar system, but the sun-centered (heliocentric) concept was slow to evolve. In the 2nd century AD, Claudius Ptolemy proposed a model of the universe with the earth at the center (geocentric). His model (shown left) depicts the earth as stationary with the planets, moon, and sun moving around it in small, circular orbits called epicycles. Ptolemy's system was accepted by astronomers and religious thinkers alike for several hundred years. It was not until the 16th century that Nicolaus Copernicus developed a model for the universe in which the sun was at the center instead of the earth. The new model was rejected by the church, but it gradually gained popular acceptance because it provided better explanations for observed phenomena. Ironically, Copernicus' initial measurements were no more accurate than Ptolemy's, they just made more sense.
 
Physicists and mathematicians also helped to lay the foundations of astronautics. In 1654 the German physicist Otto von Guericke proved that a vacuum could be maintained, refuting the old theory that nature "abhors" a vacuum. In the late 17th century English mathematician and physicist Sir Isaac Newton formulated the laws of universal gravitation and motion. Newton's laws of motion established the basic principles governing the propulsion and orbital motion of modern spacecraft.
Despite the scientific foundations laid in earlier ages, however, space travel did not become possible until the advances of the 20th century provided the actual means of rocket propulsion, guidance, and control for space vehicles.
 
Rocket Propulsion
The techniques of rocket propulsion also originated long ago. Ancient rockets used gunpowder as fuel, very much as in fireworks today. In AD 1232 in China, the city of Kaifeng was reportedly defended against the Mongols by the use of rockets. From the Renaissance onward, references were made to the proposed or actual military use of rockets in European warfare. As early as 1804 the British army established a rocket corps equipped with rockets that had a range of about 1830 m (about 6000 ft).
 
In the United States, the foremost pioneer in rocket propulsion was Robert Goddard, a professor of physics at Clark College (now Clark University). He began experimenting with liquid fuels for rocketry in the early 1920s. He launched the first successful liquid-propelled rocket on March 16, 1926. During the same general period, studies on spaceships and rocket propulsion were being conducted in several parts of the world. About 1890 Herman Ganswindt, a German law student, conceived of a solid-propellant spaceship that demonstrated a marked awareness of the stability problem. Konstantin Tsiolkovsky, a Russian schoolteacher, published in 1903 A Rocket into Cosmic Space, which proposed the use of liquid propellants for spaceships. In 1923 a German mathematician and physicist, Hermann Oberth, published Die Rakete zu den Planetenräumen (The Rocket into Interplanetary Space). The book was supplemented by Walter Hohmann, a German architect, who published in 1925 Die Erreichbarkeit der Himmelskörper (The Possibility of Reaching Celestial Bodies), which contained the first detailed calculation of interplanetary orbits.
 
World War II (1939-1945) provided the impetus and motivation for the development of long-range suborbital rockets. The United States, the USSR, Great Britain, and Germany simultaneously developed rockets for military purposes. The most successful were the Germans, who developed the V-2 (a liquid-propellant rocket used in the bombardment of London) at Peenemünde, a village near the Baltic coast. At the close of the war, the U.S. Army brought back a number of the V-2s, which were then used in the United States for experimental research in vertical flights. Some German engineers went to the USSR after the war, but the leading rocket experts went to the United States, including Walter Dornberger, and Wernher von Braun
 
Spacecraft
Spacecraft that do not have to carry humans can be of a great variety of sizes, from a few centimeters to several meters in diameter, and many shapes, depending on the purposes for which they are designed. Spacecraft that do not carry a crew have radio-transmitting equipment, both to relay information back to earth and to signal the position of the spacecraft.


Saturn 5 Rocket
A Saturn 5 rocket rises slowly from its launch pad in the early stages of the Apollo 17 mission. More than 110 m (363 ft) tall, the multistage rockets are fueled by kerosene and liquid hydrogen. In addition to being used extensively in the Apollo Space Program, one of the massive Saturn 5 rockets was used to launch NASA's Skylab in 1973.
 
Manned spacecraft must fulfill more exacting requirements than unmanned vehicles because of the needs of the human occupants. A manned space vehicle is designed to provide air for the astronauts, food and water, navigation and guidance equipment, seating and sleeping accommodations, and communication equipment so the astronauts can send and receive information from the control center on earth. A distinctive feature of manned spacecraft is the heat shield that protects the vehicle as it reenters the atmosphere
 
Propulsion
The rocket engines that launch and propel spacecraft are of two main types: solid-propellant rockets, which use chemicals that burn in a fashion similar to gunpowder, and liquid-propellant rockets, which use liquid fuels and oxidizers carried in separate. Most of the rockets that have launched American spacecraft have had several separate rocket stages; each stage is separately powered with its own fuel. After the fuel in each stage is consumed, the empty stage drops away from the spacecraft.
Because the technology to build space-launch vehicles is closely akin to that for long-range ballistic missiles, the United States and the USSR were the only two countries that had the ability to launch satellites from 1957 to 1965. In subsequent years France, Japan, India, and China launched earth satellites of ever-increasing sophistication, and in May 1984 the 13-member European Space Agency began its own launch program from a space center at Kourou in French Guiana. The United States and the USSR, however, remained the only nations with launch vehicles capable of placing in orbit payloads of many tons-the prerequisite for manned spaceflight.
 
Launching and Reentry
A space vehicle is launched from a specially constructed launchpad, where the space vehicle and the rocket that propels it are set up and carefully inspected before launching. The operation is supervised by engineers and technicians in the nearby control center. When all preparations are complete, the rocket engines are fired and the rocket and spacecraft lift off.

Reentry is the name applied to the problem of slowing down a returning spacecraft so that it lands on earth without being destroyed by the intense heat caused by friction with the earth's atmosphere. The spaceflights of the U.S. Mercury, Gemini, and Apollo programs overcame the problem of reentry by protecting the leading surface of the returning capsule with a specially developed heat shield, made of metals, plastics, and ceramic materials that melt and vaporize during reentry, thereby carrying off or dissipating the heat without damage to the capsule or the astronauts. The heat shield developed to protect the space shuttle during reentry consists of a covering of ceramic tiles individually cemented to the shuttle's hull. Prior to the development of the space shuttle, which lands on a runway, all American manned spacecraft used the ocean to cushion the impact of landing; the astronauts and the capsules were retrieved quickly by helicopter and taken aboard waiting naval vessels. Soviet cosmonauts have landed on solid ground in various sites in Siberia.
 
Orbiting the Earth
The orbit of a spacecraft around the earth can be in the shape of a circle or an ellipse. A satellite in a circular orbit travels at a constant speed. The higher the altitude, however, the lower the speed relative to the surface of the earth. Maintaining an altitude of 35,800 km (22,300 mi) over the equator, a satellite is geostationary. It moves in geosynchronous orbit, at exactly the same speed as the earth, so it remains in a fixed position over some particular spot on the equator. Most communications satellites. are placed in such orbits.


Polar Orbiting Artificial Satellite
Nimbus, an environmental satellite, takes photos as it circles the earth several times in a day in an orbit that passes over the North and South Poles. Because the earth rotates, each pass produces a new set of images and the entire earth can be photographed every day. Information about the earth's atmosphere and oceans is relayed back to the surface.
 


GOES Weather Satellite
Broadcasters use data from meteorological satellites to predict weather and broadcast storm warnings when necessary. Satellites like the GOES (Geostationary Operational Environmental Satellite) collect meteorological and infrared information about the atmosphere and the ocean. A camera on the GOES is continuously pointed at the earth, broadcasting satellite images of cloud patterns both day and night. Here, the GOES-C satellite is being encapsulated inside its payload fairing aboard a Delta rocket.


Solar Maximum Mission Satellite
The Solar Maximum Mission Satellite was a scientific satellite designed to study solar radiation. Launched in early 1980, the craft failed later in the year. It was repaired and relaunched by the space shuttle in 1984, collecting information until 1989, when it was destroyed by a solar flare. Information collected by the satellite indicated that the corona displays an unexpectedly high amount of violent activity related to sunspot cycling. Data also showed that sunspots reduce the amount of solar energy reaching the earth's atmosphere.
 
In an elliptical orbit, the speed varies and is greatest at perigee (minimum altitude) and least at apogee (maximum altitude). Elliptical orbits can lie in any plane that passes through the earth's center. A polar orbit lies in a plane passing through the North and South poles-that is, it passes through the axis of rotation of the earth. An equatorial orbit is one that lies in a plane passing through the equator. The angle between the orbital plane and the equatorial plane is called the inclination of the orbit.
The earth rotates once every 24 hours under a satellite in a polar orbit. A polar-orbit weather satellite, carrying television and infrared cameras, can thus observe meteorological conditions over the entire globe from pole to pole in a single day. An orbit at another inclination covers a smaller portion of the earth, omitting areas around the poles.
As long as the orbit of an object keeps it in the vacuum of space, the object will continue to orbit without propulsive power because no frictional force slows it down. If part or all of the orbit passes through the atmosphere of the earth, however, the body is slowed by aerodynamic friction with the air. This causes the orbit to decay gradually to lower and lower altitudes until the object has fully reentered the atmosphere and burns up, like a meteor.
 
Space Programs-Unmanned
The long history of myths, dreams, fiction, science, and technology culminated in the dramatic launching of the first artificial orbiting earth satellite, Sputnik 1, by the USSR on October 4, 1957. Sputnik Zemli, meaning "traveling companion of the world" is the Russian name for an artificial satellite, a companion of the earth as it travels around the sun. In the United States, this name was abbreviated to Sputnik.