The following links provide plenty of information on the past of the Isaac Newton Telescope (INT):
The born-again INT at La Palma,
differs significantly in its mechanics, electronics and optics from the
earlier incarnation at Herstmonceux:
The change in latitude from 50 degrees 51 minutes 58 seconds to 28 degrees
45 minutes 43.4 seconds resulted in a large change of angle to the polar disc which
stands almost on edge. A segment was removed from the disc in order to
allow operation to a declination of -30 degrees. New encoders and drive
electronics were fitted and a new computer control system was written.
The primary mirror was replaced with a slightly larger one (from 98 inches
to 100 inches) of considerably higher optical quality made of low-expansion
material. The old prime-focus assembly, which required a caged observer,
was replaced with one operated entirely by remote control; similarly, the
Acquisition and Guidance Box at the Cassegrain focus is completely new.
The telescope is housed in a new dome, the old one being left as a landmark
for channel shipping. Finally, there is a suite of new instruments and
a computer system to control them.
- Lee T. Macdonald, 2012, "'A Large Chunk of Glass': The 98-inch mirror of the Isaac Newton Telescope, 1945-1959", The Antiquarian Astronomer
(Journal of the Society for the History of Astronomy), 6, 4.
- Lee T. Macdonald, 2010, "The origins and construction of the Isaac Newton Telescope, Herstmonceux, 1944-1967", J. Br. Astron. Assoc., 120, 2.
- Article "Castle in the sky – the story of the Royal Greenwich Observatory at Herstmonceux" by Chas Parker.
- BBC reporting on the new Isaac Newton Telescope at Herstmonceux
- BBC reporting on the visit of the Duke of Edinburgh to RGO in Herstmonceux
- Book "The Isaac Newton Telescope at Herstmonceux and on La Palma", Anthony Wilson, ISBN 978-0-9512394-2-1.
The mechanical structure of the
INT was shipped to La Palma in 1981 and was re-erected into the bare frame
of its building in 1982. The mirror arrived on the island on December 10,
1982; the building was handed over by the contractors to the RGO on January
17, 1983 and work began on preparing the laboratories and workshops for
the commissioning of the telescope. The first of three direct air shipments
of machinery, instruments and computers arrived on La Palma on January
25. By September the building was in full operation and the telescope was
fully assembled, with a freshly aluminised mirror, by the end of the year.
On the first night of February 1984 stars were first seen in the telescope,
at the prime focus. The telescope commissioning programme had been targeted
towards the completion of the Cassegrain spectrograph since this would
be the most widely demanded instrument; it was also tolerant to telescope
pointing and tracking.
In the spring of 1984 there was
a concentrated effort to commission the Cassegrain instrumentation, including
acquisition TV cameras, Intermediate Dispersion Spectrograph (IDS), IPCS
and CCD detectors and ADAM, the software environment which brings together
this complex of instruments into one working station. This programme was
completed in May.
On May 29 1984, the telescope
welcomed its first scheduled astronomer. It operated for astronomers for
47% of the time in the first six-month period (Semester F), 50% in semester
G, 62% in Semester H and 73% in Semester I. The rest of the time was used
for engineering work.
The optical telescope assembly weighs
51,361 kg and including the mounting 85,361 kg.