Observatories
Enhancement

| Carnegie
astronomy is now on the verge of what promises to be its most
important era as astronomers begin realizing the remarkable
opporunities created by the Magellan Project telescopes. |
Carnegie
Observatories:
Fulfilling the Promise of the New Millennium
For nearly a century, the Carnegie Observatories have made extraordinary
contributions to our understanding of the universe. Observations
carried out at Carnegie’s Mount Wilson Observatory in the
early decades of the twentieth century transformed astronomy
and laid the foundation for modern cosmology. Using what were
then the world’s largest telescopes, Carnegie astronomers
unraveled the mysteries of stellar evolution and the structure
of the Milky Way Galaxy while Edwin Hubble captured the attention
of the world with his discovery that the universe is expanding.
Two bold decisions by Carnegie’s trustees later in the century
ensured the continuation of Carnegie leadership in astronomy: first,
the establishment in 1965 of an observatory in the southern hemisphere
and, second, the construction there in the late 1990s of the twin
6.5-meter telescopes of the Magellan Project. The Magellan telescopes
at Carnegie’s Las Campanas Observatory, high in the Chilean
Andes, are providing American astronomers with extraordinary access
to the southern sky, with its unique view of the center of the Milky
Way and neighboring galaxies.
Carnegie astronomy is now entering its most important era as the
institution’s astronomers begin realizing the remarkable opportunities
created by the Magellan Project, and as they lay the groundwork for
a larger and even more ambitious effort, the Giant Magellan Telescope.
Researchers at the Carnegie Observatories are leaders in the study
of stellar populations and the evolution of galaxies, while astronomers
at Carnegie’s Department of Terrestrial Magnetism lead the
way in investigating how planets form and in detecting extra-solar
system planets. The Carnegie Institution will augment these specialties
and enlarge the scope of its astronomy research by recruiting a group
of theoretical astrophysicists. Cooperation between observers and
theorists is essential to meeting the challenges posed by the increasingly
complex data arriving from new telescopes, and by the need to design
observation projects optimized for high-impact science. Our campaign
goal is to raise $5 million, which will cover much of the costs incurred
in instituting a 10-year program to bring two senior theorists, two
postdoctoral fellows, and a rotation of visiting theorists to the
Observatories.
While the Magellan telescopes push the boundaries of current research,
Carnegie astronomers are also planning a next generation telescope
that will enable the institution to remain at the leading edge of
astronomy well into the 21st century. In conjunction with a range
of respected partners, Carnegie is in the midst of designing a 24.5-meter
telescope that will answer many of the questions at the forefront
of astronomy today and will pose new and unanticipated riddles for
future generations. The campaign’s goal is to contribute $6.8
million, by December 2006, to the design phase of the Giant Magellan
Telescope, a critical early step in the development of this new tool.
As of January 2006, $2.75 million is still needed to reach this goal.
Building telescopes is only part of the success story at the Observatories.
Instruments are the workhorses that enable astronomers to record
and analyze light. In order to take advantage of the increased light-gathering
power of the new telescopes, the Observatories must intensify its
program for the design and construction of instruments for imaging
and spectroscopy. To that end, the campaign has set a total goal
of $2.775 million for instrumentation. This amount includes a goal
of $2.1 million for the high-powered Four-Star near-infrared camera,
of which $1.5 is still needed. It also includes a target of $475,000
for research into the burgeoning field of adaptive optics, of which
$250,000 remains to be raised.
Finally, as an important fixture in the history of astronomy, the
Carnegie Observatories have an obligation to preserve their heritage.
To that end, a campaign goal of $200,000 was established to fund
much-needed repairs to the Observatories’ historic 1912 headquarters
building in Pasadena, and a separate goal $225,000 was set to preserve
and catalog the Institution’s irreplaceable collection of hundreds
of thousands of astronomical glass plates ($60,000 remaining). These
plates constitute a unique and fragile record of both the Sun and
the night sky for much of the 20th century.
Thus, of the total $15 million goal for the Carnegie Observatories,
generous contributors have already given $5.75 million. We are actively
seeking the remaining $9.25 million to fully fund these projects
and priorities, which will impact the future success of Carnegie
astronomy.
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