|
The Future of Space Travel
The Hubble Space Telescope
The Hubble Space Telescope is a wonder of engineering and ingenuity. The idea for building a telescope in space that could see far beyond our own solar system was conceived in 1962 by the National Academy of Sciences in the United States. It wasn't until 1977 that the Congress of the United States finally voted to actually fund the project.
The Hubble telescope is named for Edwin P. Hubble. Hubble was a trailblazing astronomer who was born in 1889 and died in 1953.
The Hubble telescope has given astronomers unprecedented access to views of deep space. It has actually revolutionized the science of astronomy in many ways. The Hubble Telescope can "see" far beyond our own solar system and beyond our own galaxy into deep space, where fledgling galaxies are only just beginning to form.
The Hubble telescope wasn't launched until 1990 even though it was originally scheduled to launch in 1983. The launch experienced many delays, the most notable of which was the space shuttle Challenger disaster in 1986. The Hubble telescope was launched into space on April 25, 1990, and was sending pictures back to earth in a matter of days -- but the pictures were out of focus. The problem was found to be a flaw in the giant mirror -- it was too flat on one edge by 1/50th the width of a single human hair.
In 1993, the problem with the Hubble was resolved when the space shuttle Endeavor captured the Hubble Space Telescope and added a camera to correct problems with the telescope's primary mirror.
There have been other problems with the Hubble over the years, but it is still one of the wonders of the world and is providing astronomers with information that they could never have gained access to without it.
See Also:
Short focal Length Lense and Deep Sky Objects?
The Moon Shot
The Planet Uranus
William Herschel accidentally discovered the planet Uranus in 1781. Uranus had been seen many times before, but it had always been dismissed as a star.
Uranus is made up mostly of hydrogen and helium like Jupiter and Saturn, but it has higher concentrations of heavy elements. Our closest look at Uranus was given to us by Voyager 2 in 1986.
Uranus is one of the four "Giant Gas Planets" (the other three are Jupiter, Saturn, and Neptune). The rings around Uranus are made up of rock, rather than ice like those of Saturn. We do know that there are five large moons and at least 10 smaller moons. The rotational period of Uranus is a little over 17 hours, and its orbital period is 84 years.
Uranus appears to be a giant blue featureless ball. Voyager 2 got relatively close to Uranus and could not pick up any distinguishable features. It is believed that the upper atmosphere of Uranus has a high-level petrochemical haze that probably obscures features lower in the atmosphere. The blue color is caused by methane gas in the atmosphere. Methane gas absorbs red and orange light, which leaves more blue light.
Voyager 2 confirmed that Uranus has a magnetic field. The field is more than 50 times stronger than that of Earth and is tilted about 60 degrees.
The latest scientific data suggests that Uranus is surrounded by at least five rings. The brightest ring is called the Epsilon ring. Voyager 2 located two small shepherd moons for it, one just inside and one just outside. These two shepherd moons have been named Ophelia and Cordelia.
The most interesting moon that circles Uranus is Miranda. Miranda isn't very big, but it has some very interesting geological features. |
|
More articles:
February 21 in Russian history. Amateur astronomy.
Curious About Astronomy? Careers in Astronomy
Humor About Astronomy and Space
The Planet Jupiter
327)Comprehensive quotes of Aga Khan IV and others relating to ...
Astronomy Clubs
Sir Christopher Wren
Sir Christopher Wren once said, "In things to be seen at once, much variety makes confusion, another vice of beauty. In things that are not seen at once, and have no respect one to another, great variety is commendable, provided this variety transgress not the rules of optics and
geometry." For those of you who do not know, Christopher Wren was an English architect and mathematician who became Savilian Professor of Astronomy at Oxford in 1661. He is most famous for the buildings that he designed after the Great Fire of London.
Wren was interested in many things, and over his lifetime, he made many contributions to scientific knowledge and in many different ways. For example, he constructed a transparent beehive for the purpose of scientific observation; he studied the moon and experimented on terrestrial magnetism; and he also performed the first successful injection of a substance into a dog's bloodstream.
Along with Sir Paul Neile, Wren constructed a 35-foot telescope. During this timeframe, Wren also studied and improved the microscope and the telescope.
Wren was fascinated by the planet, Saturn. He began his observations of Saturn about 1652 with the intention of explaining the rings. Wren developed a hypothesis which he wrote in De Corpore Saturni. Before his work could be published however, Christian Huygens (a Dutch astronomer) presented his theory of the rings of Saturn. Wren immediately recognized the fact that Huygens' was a better hypothesis than his own, so De Corpore Saturni was never published.
Wren constructed a beautifully detailed model of the moon and gave it to the king. Although Sir Christopher Wren eventually turned his attention to architecture, he remained fascinated by astronomy all of his life.
Related Topics: Binoculars for Astronomy,
Galileo Galilei, The Moon Shot
|