Abstract

The persistent increase of artificial light emissions is causing a progressive brightening of the night sky in most regions of the world. This process is a threat for the long-term sustainability of the scientific and educational activity of ground-based astronomical observatories operating in the optical range. Huge investments in building, scientific and technical workforce, equipment and maintenance can be at risk if the increasing light pollution levels hinder the capability of carrying out the top-level scientific observations for which these key scientific infrastructures were built. Light pollution has other negative consequences, as e.g. biodiversity endangering and the loss of the starry sky for recreational, touristic and preservation of cultural heritage. The traditional light pollution mitigation approach is based on imposing conditions on the photometry of individual sources, but the aggregated effects of all sources in the territory surrounding the observatories are seldom addressed in the regulations. We propose that this approach shall be complemented with a top-down, ambient artificial skyglow immission limits strategy, whereby clear limits are established to the admissible deterioration of the night sky above the observatories. We describe the general form of the indicators that can be employed to this end, and develop linear models relating their values to the artificial emissions across the territory. This approach can be easily applied to other protection needs, like e.g. to protect nocturnal ecosystems, and it is expected to be useful for making informed decisions on public lighting, in the context of wider spatial planning projects.

Highlights

  • The persistent increase in the emissions of artificial light [1] is giving rise to a progressive deterioration of the natural night, royalsocietypublishing.org/journal/rsos R

  • One of the most visible effects of light pollution is the loss of the darkness of the night sky, due to the atmospheric scattering of the light emitted by artificial sources [11,12,13,14]

  • The practical application of this approach requires addressing three main issues: (i) choosing the appropriate indicators of the quality of the night sky, and establishing their acceptable limiting values, (ii) developing a quantitative model relating the values of these indicators to the artificial light sources existing in the region around the observatory, and (iii) allocating among the surrounding municipalities and other local administrative bodies the possible quota of new light emissions or distributing the burden of reducing the emissions

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Summary

Introduction

The persistent increase in the emissions of artificial light [1] is giving rise to a progressive deterioration of the natural night, royalsocietypublishing.org/journal/rsos R. The practical application of this approach requires addressing three main issues: (i) choosing the appropriate indicators of the quality of the night sky, and establishing their acceptable limiting values, (ii) developing a quantitative model relating the values of these indicators to the artificial light sources existing in the region around the observatory, and (iii) allocating among the surrounding municipalities and other local administrative bodies the possible quota of new light emissions (in case the present value of the indicators still did not reach the limiting values, and it could be accepted to increase the emissions in spite of its detrimental consequences) or distributing the burden of reducing the emissions (in case the critical values of the indicators have been surpassed).

Sky quality indicators and the point spread function of artificial lights
Calculating the indicators with geographical information system
Emission quota allocation
Long-term planning
Conclusion
Spectral radiance and night sky brightness measurements
The point spread function of light pollution
Findings
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Full Text
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