Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
In the southern hemisphere the 24-inch Bruce telescope of Harvard
College Observatory has obtained many very remarkable photographs of
nebulæ, particularly in the vicinity of Eta Carinæ. But the great
reflectors of the Mount Wilson Observatory, on account of their
exceptional location and extraordinary power, have surpassed all others
in the photographic portrayal of these objects, especially of the spiral
nebulæ which appear to show all stages in transition from nebula to
star. No less remarkable are the photographs of such wonderful clusters
as Omega Centauri, a perfect visual representation of which is wholly
impossible. Intercomparison of the photographs of clusters has afforded
Bailey of Harvard, Shapley of Mount Wilson and others the opportunity of
discovery that hundreds of the component stars are variable.
What is the longest photographic exposure ever made? At the Cape of Good
Hope, under the direction of the late Sir David Gill, exposures on
nebulæ were made, utilizing the best part of several nights, and
totaling as high as seventeen, or even twenty-three hours. But the Mount
Wilson observers have far surpassed this duration. To study the rotation
and radial velocity of the central part of the nebula of Andromeda, an
exposure of no less than 79 hours' total duration was made on the
exceedingly faint spectrum, and even that record has since been
exceeded. The eye cannot be removed from the guiding star for a moment
while the exposure is in progress, and this tedious piece of work was
rewarded by determining the velocity of the center of the nucleus as a
motion of approach at the rate of 316 kilometers per second.
But when the stars, their magnitudes and their special peculiarities are
to be investigated _en masse_, photography provides the facile means for
researches that would scarcely have been dreamed of without it. The
international photographic chart of the entire heavens, in progress at
twenty observatories since 1887, the photographic charts of the northern
heavens at Harvard and of the southern sky at Cape Town, the manifold
investigations that have led up to the Harvard photometry, and the
unparalleled photographic researches of the Henry Draper Memorial,
enabling the spectra of many hundred thousand stars to be examined and
classified--all this is but a part of the astronomical work in stellar
fields that photography has rendered possible.
Public-domain text, read in full here on John Shaqi.
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