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The Copernican Revolution: The Birth of...
Web Destinations
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Chapter 1 Web Destinations
No matter how hard we try, and despite the many other online sections and
resources here, there will always be more information available in the world
than can be contained on one server.
Here are our favorites for this chapter. Go ahead and check them out, but be
sure to return back to do more exploring when you're done!
For a good selection of general sites of broad interest and utility that are
related to many chapters of the book, see our collection of General Web Destinations for All
Chapters.
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List of Constellation Facts and Figures
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Includes the stars the constellations contain, and a sky map too. Also at this
site you will find The Constellations and Their Stars Web page, maintained by
Chris Dolan at the University of Wisconson-Madison Department of Astronomy.
Other resources are listed
in our General Web
Destinations For All Chapters.
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Primer on Seasons
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See why the modern explanation of the pattern of the seasons fits important
observable facts and is not "just a theory."
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Astrophysical Coordinates
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All astronomical positions are measured on the sky in spherical
coordinates. That is, we use some form of latitude, longitude measure for
location. Just as on the Earth you can use either the axis of rotation or the
magnetic pole as your reference, on the sky there are a number of alternative
reference systems. The purpose of this document is to provide a brief
background on the definitions used in astronomy, and a starting point for
those who are new to the subject.
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Celestial
Spheres
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A celestial sphere shows directions in a coordinate system analogous to
Earth's latitude and longitude projected up into the heavens.
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Stardial
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Stardial is a stationary weatherproof electronic camera for recording images
of the sky at night. Like a sundial, Stardial is a stationary device placed
outside 24 hours a day. Both depend on and make evident the rotation of the
Earth. A sundial operates with sunlight, while Stardial operates with
starlight. There the similarity ends. Stardial's purpose is to record images
of the night sky and provide them in real time to the World Wide Web. These
images
can be used for a variety of purposes, including visualization of
geosynchronous satellites, monitoring the daily apparent motion of the stars,
looking for dim or variable objects such as variable stars or comets, or just
"looking up."
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What
Time Is It?
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Until recently, when atomic clocks became available, time was reckoned by the
Earth's motions. One rotation on its axis was a "day," one revolution about
the Sun was a "year," an hour was one twenty-fourth of a day, and so on. The
position of the Sun in the sky was used to measure various intervals. Now
there are many methods used to keep time, each having its own special use and
advantage. Learn about the differences between local time, apparent time,
mean time, civil time, universal time, international standard time, sidereal
time,
and ephemeris time from the discussion given at this site.
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Solar System
Live
- Caution, slow link from non-European sites!
An interactive orrery on the Web. You can view the entire solar system or just
the inner planets through the orbit of Mars, using either realistic or compressed scales. The controls allow you to set time and date,
viewpoint, observing location, orbital elements to track an asteroid or comet,
and a variety of other parameters. You can compose a request with custom
settings and save the results in your browser's hotlist or bookmark table,
allowing direct access with all the controls preset to your own preferences.
To use this page,
you need a graphical Web browser which supports forms and the ability to display
GIF images.
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Deep Space
Network
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NASA's Deep Space Network is the largest and most sensitive scientific
telecommunications system and the most precise radio navigation network in the
solar system. Its principal responsibilities are to support interplanetary
spacecraft missions and radio and radar astronomy observations in the
exploration of the solar system and the universe. Find out how this network is
used for modern spacecraft navigation and distance measurement.
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The Moon Phase Page
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This site delivers an image of the current phase of the Moon as viewed from the
central US (mountain time). This page can also be used to view the Moon's
phase for any date that you select. See also the similar and well-done Phase of the Moon page
of Lunar Outreach Services.
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Sundial
Tutorial
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The earliest known sundial, found in Egypt, dates from at least 3500 years
ago, although crude versions must have been in use for even longer. As the
Earth rotates on its axis, the Sun appears to move uniformly across the sky.
If a rod is placed parallel to the Earth's axis, its shadow will naturally
move uniformly around itself. In other words, as the Sun appears to move, due
to the Earth's rotation, through the sky at a rate of about 15 degrees per
hour, so will the shadow move at the same rate. This is the principle on which
most (but
not all) sundials are based. Learn more, including the history of the variable
length of "hours" in a day, via this site.
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Eclipse Tutorial
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An eclipse occurs when a body cuts off the light from a light source so that
we can no longer see it shining. An eclipse can be due either to a dark body
coming between us and a light emitter, so that we can no longer see the
source, or it can be a body coming between a light source and the body that
the light is illuminating, so that we no longer see the illuminated body.
Learn more from this site, including the conditions for a solar or lunar
eclipse.
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Solar Eclipse Path Predictions
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Includes ASCII text files for all central solar eclipses from now through the
early portion of the next decade, and complete NASA eclipse bulletins
available 18 to 24 months before each eclipse. The full bulletins contain
detailed predictions, maps, and meteorological data for future central solar
eclipses, and the site includes charts and animations of the predicted eclipse
paths.
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Primer on Archaeoastronomy
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One of the fundamental objectives of archaeoastronomy is to find an
alignment at a site. Archaeoastronomers look for pairs of stones or
architectural features, located at some distance from each other. When
they find a pair, the alignment between these features and celestial objects
can be checked.
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Astronomiae Historia / History of Astronomy
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By far the most comprehensive and academically rich source of
information on topics related to the history of astronomy on the Web, this
site is a tour de force. Included are index entries, for example, on the
topics of Archaeoastronomy and Ethnoastronomy, Astrology, Mythology, Religion,
Astrophysics, Calendars, Time and Chronology, Celestial Mechanics,
Constellations, Maps and Atlases, Cosmology, Extragalactic Astronomy,
Instruments, Nebulae and Star Clusters, Space Exploration, Stellar Astronomy, and World Systems. Recommended.
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Celestial
Instruments
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Browse through some of the historical instruments on display
at the University of Bologna. The instruments used by the Bolognese
astronomers from the early 18th century to mid-19th century have been brought
back to their original rooms and photographed in place as they would
originally have been used.
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Scientific
Method FAQ
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Frequently Asked Questions on the scientific method. This useful primer covers
the difference between a fact, a theory, and a hypothesis and explains the
basic ground rules for scientific investigation.
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Nicolaus Copernicus
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Copernicus came from a middle-class background and received a good
standard education, studying first at the university of Krakow (then the
capital of Poland) and then traveling to Italy, where he studied at the
universities of Bologna and Padua. While there, Copernicus visited
Rome, and it seems to have been for friends there that in about 1513 he wrote
a short account of what has since become known as the Copernican theory,
namely that the Sun (not the Earth) is at rest in the center of what we now
know as the solar system.
Learn more from this biography.
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Galileo Galilei
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Galilei was born in Pisa in 1564, the son of Giulia Ammannati and Vincenzo Galilei (well known for
his studies of music). He studied at Pisa, where he later
held the chair in mathematics from 1589 - 1592. He was then appointed to the
chair of mathematics at the University of Padua, where he remained until 1610.
It was at Padua that he made his most famous dicoveries. Read and see more in
this excellent biography from a site based in Florence, Italy.
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Making
A Model Of The Solar
System - This page provides many links to sites that will help
you build and better understand
the scale of our solar system. If you decide to build your own scale
model you will
find that you may need more than a pencil and tape measure. You may also
need to use other
instruments, like the odometer in your car!
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Laws
of Science Abused by Science Fiction
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It is possible to learn a lot about the laws of science by attempting an
informal feasibility study on, for example, a spacecraft from a science-fiction comic book, a sci-fi magazine cover, or a Star Wars or Star Trek
video. This site gives some of the laws of science that are frequently
violated by artists and authors. Descriptive examples of such errors are
given and studied. This page is part of the NASA Multimedia Space Educators'
Handbook.
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Keplerian
Elements Tutorial
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Do you want to go beyond the absolute basics and understand in a bit more
detail how we keep track of the exact locations of the kazillions of
satellites and other objects in orbit around the Earth (and elsewhere)? Then
this tutorial is highly recommended. It gives a straightforward introduction
to the vocabulary and concepts, and even manages to make thinking about such
things in three dimensions seem somewhat easy.
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