Astronomical Archive Produced by 2MASS Telescope Project
UMass astronomers headed the 10-year, $40-million effort
AMHERST, Mass. – The vast archive of images and data resulting from the Two
Micron All-Sky Survey (2Mass), the most thorough, high-resolution survey of
the sky, has been completed. The archive, which features some five million
images, is now available online for scientists and sky watchers. The project,
which relied on twin infrared telescopes, was led by astronomers at the
University of Massachusetts Amherst.
“The aim of the 2Mass science team was to produce a comprehensive map of the
sky that could be shared with the rest of the science community,” said Martin
Weinberg, a UMass astronomer who has been closely involved in the project. “We
as scientists were motivated to do the project by the promise of the science
that will result from it in coming years. This is a major astronomical archive
that will have context and worth for decades.”
“The sky has been surveyed by astronomers before, but by looking at infrared
light 2MASS was able to detect some objects that were invisible at optical
wavelengths,” said Stephen Schneider, another UMass astronomer closely
involved in the project. “Even known astronomical sources reveal many new
things about themselves in infrared light. There are hundreds of discoveries
waiting to be made in this immense database.”
“This survey was an old human activity, but with a modern twist,” said project
manager Rae Stiening at UMass. “Just as English admiralty sent Captain Cook
and others to map the world, this new survey has mapped the nearby universe.”
The survey was conducted using infrared light to peer through the dust within
and beyond our Milky Way galaxy, enabling astronomers to detect and identify
more than 500 million objects, primarily stars, but including galaxies,
asteroids, and comets. The project used two dedicated 1.3-meter telescopes,
one at Mount Hopkins, Ariz., the other at the Cerro Tololo Inter-American
Observatory in Chile. Observations began in 1997 and concluded in early 2001.
Scientists have spent the past year completing an analysis of the entire sky.
The survey produced two major catalogs detailing nearly half a billion objects.
“This survey will change the way astronomy is conducted and the types of
experiments that can be carried out, because astronomers can now sit at their
desk and have data for any spot on the sky literally at their fingertips,
without going to a telescope,” said Roc Cutri, the survey’s project scientist
at the Infrared Processing and Analysis Center of the California Institute of
Technology and NASA’s Jet Propulsion Laboratory, Pasadena, Calif. “It also
makes astronomy more open to the public, providing beautiful pictures and
serving as a powerful educational tool.”
The survey’s findings include:
a. Confirmation of a new class of stars, known as brown dwarfs, which are
very red, and too cool to be seen by previous methods;
b. a more complete understanding of our Milky Way’s structure;
c. a new view of the “nearby” universe, and the way that galaxies cluster
together over distances of hundreds of millions of light years;
d. the most detailed database ever of location, brightness, color and
position of asteroids in the nearby universe.
The findings are now available to scientists and sky watchers through two
catalogs that are essentially final inventories of stars and galaxies
throughout our sky. The first identifies “point sources,” throughout the sky;
that is, all discernable sources of light, from the very brightest stars to
sources that are tens of thousands of times fainter, Weinberg explained. The
second catalog of extended sources includes over a million galaxies and
nebulae, some at a distance of billions of light years.
The galaxy catalog can be downloaded into an existing PC. The point-source
catalog, which is on six DVD Roms, requires a specialized server, but building
the server is well within the financial means of research universities,
Weinberg said.
“The public will ‘ooooh and aaaah’ at the pictures, while scientists will mine
the data for decades, learning more about our Milky Way galaxy and hundreds of
millions of its stars, and about the millions of galaxies in the nearby
universe,” said Michael Skrutskie, principal investigator for 2Mass.
Skrutskie, with the University of Virginia, Charlottesville, was formerly with
UMass.
2Mass is a collaboration between the University of Massachusetts Amherst and
the Infrared Processing and Analysis Center. The University was responsible
for design, construction and operation of the survey cameras and telescopes,
as well as the observations and acquisition of images. The Center developed
the software system that converted the nearly 25 terabytes of raw digital data
into images and catalogues. The survey is primarily funded by NASA’s Office of
Space Science, with additional funding from the National Science Foundation.
Note: Martin Weinberg can be reached at 413/545-3821
or weinberg@owl.astro.umass.edu
Steve Schneider can be reached at 413/545-2076
or schneider@astro.umass.edu
A sampling of additional 2MASS images is at
http://pegasus.astro.umass.edu/ and at http://www.ipac.caltech.edu/2mass/gallery
