2008 APS April Meeting and HEDP/HEDLA Meeting
Volume 53, Number 5
Friday–Tuesday, April 11–15, 2008;
St. Louis, Missouri
Session B6: Triumphs of 20th Century Astrophysics I: Observatories and Telescopes
10:45 AM–12:33 PM,
Saturday, April 12, 2008
Hyatt Regency St. Louis Riverfront (formerly Adam's Mark Hotel),
Room: Promenade D
Sponsoring
Units:
FHP DAP
Chair: Ramanath Cowsik, Washington University
Abstract ID: BAPS.2008.APR.B6.1
Abstract: B6.00001 : Lick Observatory, California, and 20th Century Leadership in Optical Astronomy
10:45 AM–11:21 AM
Preview Abstract
Abstract
Author:
Joseph Miller
(Lick Observatory)
With the establishment of the Lick Observatory on Mt. Hamilton in
California
in 1888 it was immediately established that an observatory
located on a
relatively high site far from city lights was a far superior
location for
optical astronomy than the previously common city locations. A
few years
after its beginning, astronomers at Lick convincingly
demonstrated the clear
advantage of the reflecting telescope for astrophysical research.
Not only
was a reflector achromatic over all wavelengths, but it could be
made with a
small focal ratio that provided high photographic speed.
Furthermore, since
light did not pass through the optic and it could be supported
from behind,
it could easily be made in large sizes. Over the first half of
the 20$^{th}$
century the establishment of the Mt. Wilson and Palomar
Observatories
expanded California's dominance in optical astronomy. Also with
the new
larger telescopes came major progress in the in design of focal
plane
instrumentation that allowed these telescopes to be superb tools for
astrophysical research.
The California observatories of the 20th century were largely
independent of
Federal funding for operations. Their facilities were were
maintained and
mostly used by their permanent staffs. This led to a style of doing
forefront research that was highly effective, as both long-term
survey-type
programs and more speculative investigations with less-clear
payoffs at the
outset could be supported. Also the, the close connection of the
scientists
doing the research to the development of the telescopes and
instruments they
used for their research conferred advantages. At present, this
style of
doing astronomical observational research is a relatively small
fraction of
all this kind of research.
At the end of the 20$^{th}$ century the California pioneering
advancement in
ground-based optical astronomy was repeated with the creation of
the Keck
Observatory. A joint project of the University of California and the
California Institute of Technology, this observatory features two
10-m
telescopes, current the largest general-purpose optical/infrared
telescopes
in the world. However, California skies were abandoned in favor
of a much
superior site in Hawaii.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2008.APR.B6.1