Memorandum from Mr Gerald White, The Norman
Lockyer Observatory
LIGHT POLLUTION AND ASTRONOMY
The Norman Lockyer Observatory is one of the
larger working optical observatories in the United Kingdom and
enjoys a relatively dark sky site in mainland Britain. A more
detailed report on the Observatory and the effect of light pollution
is enclosed (see Annex), but in this letter I offer my personal
opinion on the specific questions to be addressed by the Select
Committee.
1. The United Kingdom affords inefficient
sites for astronomical observation compared with those funded
elsewhere because:
The latitude limits view of the sky,
whereas observatories near the equator can observe both hemispheres.
Britain's oceanic climate limits
opportunities for observation.
Light pollution coupled with other
forms of pollution rarely permit a truly clear sky.
2. Current rules do not allow authorities
to rectify errors made in the past. The Observatory was not used
for astronomical research between 1963 and 1989, during which
period local light pollution increased considerably. Responsible
authorities do not seem to apply existing guidelines equally.
3. I am aware of instances where retrospective
consent has been granted after the installation of lanterns that
do not conform to the best standards. In some instances the supplier
and/or installer gave advice on selection of lanterns; perhaps,
there was a conflict of interest as suppliers have a natural concern
to sell as many lanterns as possible. It is difficult for planning
committees to contradict or challenge the advice of such "experts".
4. As light pollution affects photographic
and spectral work of observatories, it should be measurable. However,
the back scattering of polluting light from the sky depends on
particles present in the atmosphere. Ice crystals form in the
upper atmosphere and mist or haze at lower altitudes. Atmospheric
particles derive from industrial, traffic and aircraft exhausts,
smoke from domestic and accidental fires, pollen, salt, soil and
dust from industrial and natural sources. Fortunately, the Observatory
enjoys a relatively clean westerly air stream from the Atlantic.
While the upwards emission of light from a city is roughly constant
or increases only slowly, the amount of wasted light energy scattered
back by the sky varies with the weather, season, wind direction
and other factors. Measurements of sky clarity need to be conducted
over a sustained period.
5. New explicit guidelines and controls
seem necessary to ensure that non-polluting fittings are easily
available, particularly for outdoor domestic use. A large local
DIY store was recently noticed to carry stocks of nine different
patterns of outdoor lanterns of which only one approached the
desired standard or gave instructions on correct fitting.
I have enclosed a more detailed paper with photographic
evidence (not printed). However, the Observatory believes that
the most pressing reason for improvement and regulation of outdoor
lighting is the benefit to the saving in energy.
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