Curiosities of Science, Past and Present: A Book for Old and YoungTimbs, John
Science
Curiosities of Science, Past and Present: A Book for Old and Young
Timbs, John
Science
The first telescope “the starry Galileo” constructed with a leaden
tube a few inches long, with a spectacle-glass, one convex and one
concave, at each of its extremities. It magnified three times.
Telescopes were made in London in February 1610, a year after
Galileo had completed his own (Rigaud, _On Harriot’s Papers_,
1833). They were at first called _cylinders_. The telescopes which
Galileo constructed, and others of which he made use for observing
Jupiter’s satellites, the phases of Venus, and the solar spots,
possessed the gradually-increasing powers of magnifying four,
seven, and thirty-two linear diameters; but they never had a higher
power.--Arago, in the _Annuaire_ for 1842.
Clock-work is now applied to the equatorial telescope, so as to
allow the observer to follow the course of any star, comet, or
planet he may wish to observe continuously, without using his hands
for the mechanical motion of the instrument.
ANTIQUITY OF TELESCOPES.
Long tubes were certainly employed by Arabian astronomers, and very
probably also by the Greeks and Romans; the exactness of their
observations being in some degree attributable to their causing the
object to be seen through diopters or slits. Abul Hassan speaks very
distinctly of tubes, to the extremities of which ocular and object
diopters were attached; and instruments so constructed were used in
the observatory founded by Hulagu at Meragha. If stars be more easily
discovered during twilight by means of tubes, and if a star be sooner
revealed to the naked eye through a tube than without it, the reason
lies, as Arago has truly observed, in the circumstance that the tube
conceals a great portion of the disturbing light diffused in the
atmospheric strata between the star and the eye applied to the tube.
In like manner, the tube prevents the lateral impression of the faint
light which the particles of air receive at night from all the other
stars in the firmament. The intensity of the image and the size of the
star are apparently augmented.--_Humboldt’s Cosmos_, vol. iii. p. 53.
NEWTON’S FIRST REFLECTING TELESCOPE.
The year 1668 may be regarded as the date of the invention of
Newton’s Reflecting Telescope. Five years previously, James Gregory
had described the manner of constructing a reflecting telescope with
two concave specula; but Newton perceived the disadvantages to be so
great, that, according to his statement, he “found it necessary, before
attempting any thing in the practice, to alter the design, and place
the eye-glass at the side of the tube rather than at the middle.” On
this improved principle Newton constructed his telescope, which was
examined by Charles II.; it was presented to the Royal Society near the
end of 1671, and is carefully preserved by that distinguished body,
with the inscription:
“THE FIRST REFLECTING TELESCOPE; INVENTED BY SIR ISAAC NEWTON, AND
MADE WITH HIS OWN HANDS.”
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account