e to royalty is
manifestly intended to give a British tone to the narrative),
'subscribed his name for a contribution of L10,000, with a promise that
he would zealously submit the proposed instrument as a fit object for
the patronage of the privy purse. He did so without delay; and his
Majesty, on being informed that the estimated expense was L70,000,
naively enquired if the costly instrument would conduce to any
improvement in _navigation_. On being informed that it undoubtly would,
the sailor king promised a _carte blanche_ for any amount which might be
required.'
All this is very clever. The 'sailor king' comes in as effectively to
give _vraisemblance_ to the narrative as 'Crabtree's little bronze
Shakspeare that stood over the fireplace,' and the 'postman just come to
the door with a double letter from Northamptonshire.'
Then comes a description of the construction of the object-glass,
twenty-four feet in diameter, 'just six times the size of the elder
Herschel's;' who, by the way, never made a telescope with an
object-glass. The account of Sir John Herschel's journey from England,
and even some details of the construction of the observatory, were based
on facts, indeed, so many persons in America as well as in England were
acquainted with some of these circumstances, that it was essential to
follow the facts as closely as possible. Of course, also, some
explanation had to be given of the circumstance that nothing had before
been heard respecting the gigantic instrument taken out by Sir John
Herschel. 'Whether,' says the story, 'the British Government were
sceptical concerning the promised splendour of the discoveries, or
wished them to be scrupulously veiled until they had accumulated a
full-orbed glory for the nation and reign in which they originated, is a
question which we can only conjecturally solve. But certain it is that
the astronomer's royal patrons enjoined a masonic taciturnity upon him
and his friends until he should have officially communicated the results
of his great experiment.'
It was not till the night of January 10, 1835, that the mighty telescope
was at length directed towards our satellite. The part of the moon
selected was on the eastern part of her disc. 'The whole immense power
of the telescope was applied, and to its focal image about one half of
the power of the microscope. On removing the screen of the latter, the
field of view was covered throughout its entire area with a beautiful
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