What is the National Virtual Observatory?
The National Virtual Observatory (NVO) is a new research project whose goal is
to make all astronomy data in the world quickly and easily accessible by anyone. The
NVO was created to solve two difficult problems that astronomers currently face in
doing their research. This document describes what the problems are and how the NVO
will solve them.
What happens to old data?
How do scientists get data from all wavelengths of the electromagnetic spectrum?
Solution: the NVO
Problem #1: Getting New Results from Old Data
For thousands of years, astronomers have been studying the sky. They started
looking at the sky with their eyes, creating star charts and maps. In the 1600s,
astronomers began using telescopes, allowing them to see many more stars and galaxies.
Over the past several hundred years, telescopes have gotten more and more powerful,
allowing astronomers to see millions more stars and galaxies. When computers were
invented, astronomers began to use computers to control their telescopes.
Today, telescopes are so powerful that they can see thousands or millions of sky
objects every night. Sophisticated computer programs identify and analyze the objects
seen in the telescope images. These powerful new computer-equipped telescopes are
making observations faster than astronomers can keep up with them.
Today, when an astronomer uses a telescope to make an observation, she studies the
new observation carefully, seeing how it fits with other observations she has made
already. The new observation then goes into a data archive.
Of course, her new observation is useful not only to her; other astronomers could
potentially learn a great deal about the universe by studying her observation, and
comparing them to other observations that they have made. But the other astronomers
are busy with their own research observations – they probably do not even know that
her observation exists. So the observation sits in the data archive, waiting to be
rediscovered and reinterpreted by another astronomer.
In this way, lots of useful astronomy data ends up hidden in data archives, with
the potential to be rediscovered and to answer important questions about the universe.
Astronomers need a way to easily search through archived data, quickly find the data
that they are interested in, and analyze the data in new and exciting ways.
Problem #2: Getting Data from All Wavelengths
Over the past several decades, astronomers have built telescopes to see the sky
in other wavelengths of the electromagnetic spectrum: radio waves, infrared light,
ultraviolet light, x-rays, and gamma rays. Just like visible-light telescopes, these
telescopes in other wavelengths are producing huge volumes of data ready to be
studied by ambitious astronomers.
Although these telescopes look at the sky in many different wavelengths of light,
they are all looking at the same sky. Many sky objects have images taken in nearly
all wavelengths of light. Each image shows different features of the object being
studied, so astronomers would like to combine all the images to get a complete
picture of the object.
But the images were taken by different telescopes at different times, organized
by different groups of astronomers in different places. In the past, combining all
these images into a single picture of the object was time-consuming and required
lots of specific knowledge about how the images were taken. Astronomers need a way
to seamlessly combine images and data from many different wavelengths of light to
form a single coherent picture of a sky object.
Solution: The NVO
The National Virtual Observatory (NVO) was created to give astronomers the tools
they need to do their research, giving them immediate access to all astronomy data
ever taken. With NVO, astronomers will explore data that others have already collected,
finding new uses and new discoveries in existing data. They will easily combine data
from many wavelengths, enabling them to understand objects as seen in all wavelengths
of light. The NVO will enable astronomers to do a new type of research that, combined
with traditional telescope observations, will lead to many new and interesting
discoveries.
The NVO will be like an Internet search engine for astronomy data, available
not only to astronomers, but to the general public. You can use the NVO’s web
interfaces to request data – for example, to display all Hubble space telescope
pictures of the Andromeda galaxy, or to display all bright galaxies that have images
in both visible and ultraviolet light.
For the past three years, NVO scientists have been working to develop the standards
to allow data to be shared across the world. Now that this behind-the-scenes work of
defining standards has been done, NVO scientists are building tools to access data.
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