Measuring Lightscapes

An NPS scientist stands in silhouette against a dusk sky and conducts an equipment check with a CCD Camera prior to a night of data collection; Great Basin National Park. NPS / Kate Magargal.
An NPS scientist stands in silhouette against a dusk sky and conducts an equipment check with a CCD Camera prior to a night of data collection—Great Basin National Park.

NPS / Kate Magargal

National parks are preserves of biotic diversity and natural processes, as well as the "crown jewels" of America's most scenic lands. Humans have gazed awe-struck into the universe for millennia, and ecosystems have adapted to the natural rhythms of the moon and stars. In recent years light pollution has encroached upon lands that were once remote from large cities, such as national parks. Keeping such treasures unimpaired for future generations relies on science, reliable data, and sound judgment.

Efforts to protect naturally dark environments in our national parks are driven by NPS management policies. But before any action can be taken, park planners and managers need reliable data about a park's existing lightscape. Resource inventories tell park managers and concerned citizens of the existing night sky quality and the departure from natural conditions and identify what is causing any degradation. Such baseline assessments become the foundation for monitoring programs to detect long-term changes and provide feedback for those who join the NPS in stewardship of natural lightscapes.

An oil rig drilling site emits bright lights into the atmosphere.
An oil rig drilling site emits bright lights into the atmosphere.


Components of Sky Brightness

The night sky as we see it is a combination of both natural and human-caused sources of light. Natural light sources include moonlight, starlight from individual stars and planets, the Milky Way (also called galactic light or integrated starlight), the zodiacal light (sunlight reflected off dust particles in the solar system), and airglow. Airglow is similar to a faint aurora (e.g., northern lights) and is caused by radiation striking air molecules in the upper atmosphere.

Airglow is somewhat unpredictable, while the other sources of natural light can be predicted and modeled. Other intermittent sources of natural light include fire, lightning, and meteors.

The largest human-caused source of light is outdoor electrical lighting, but this can also include gas flares and other minor sources such as aircraft, automobiles, and satellites. While most natural light sources are emitted from great distances away, human-caused sources are relatively close. Light pollution includes both direct glare and skyglow (human-caused light scattered through the atmosphere).

In the highest quality skies, human-caused sources of light are less luminous than natural sources, and natural features of the night sky predominate. In a degraded natural lightscape condition, human-caused light is greater than that produced by natural sources. In some cases, many tens of times brighter.
Panorama of the night sky and silhouetted horizon at Rocky Mountain National Park, Colorado.
Panorama of the night sky and silhouetted horizon at Rocky Mountain National Park, Colorado.

NPS / Jeremy M. White

Different Approaches

The opportunity to enjoy and appreciate natural lightscapes and starry night skies are dependent on the weather, the clarity of the air, and the amount of light pollution present. There is a range of methods for measuring the amount of light pollution:

  • The visibility of certain celestial features can be used to make simple qualitative appraisals of the night sky. For example, the ability to see the Milky Way in the night sky (our own galaxy seen edge-on) indicates a moderate level of sky quality. These estimates can be done quickly by a dark-adapted observer but tend to be biased from one person to another. The most popular qualitative assessment is the Bortle Dark Sky Scale.
  • Another simple method is using "star counts." A defined area of the sky, such as the constellation Orion, is examined and the number of stars are either counted or the constellation is compared to a series of images. Each image shows an increasing number of stars;the more light pollution, the less contrast is afforded the observer and the less stars are seen. This estimate can be made by a dark-adapted observer with a basic understanding of the night sky in about 20 or 30 minutes. Star counts can also be biased from one individual to another and depend on the visual awareness and patience of the observer. Worldwide star counts allow the public to participate;one popular count is the Globe at Night program. You can try this yourself in your own neighborhood or park by exploring How Dark Is Your Night Sky.
  • A more sophisticated solution is to use a light sensor that measures illuminance (the light falling upon a surface) or luminance (the brightness of a surface). These are typically photodiodes, but even a simple solar panel can be adapted to measure the relatively faint nighttime light striking it. These can be readily filtered and calibrated to estimate brightness as the human eye sees it, or can be tuned to what a specific wildlife species "sees." A recent innovation of this type is inexpensive sky quality meters. These are similar to a photographer's light meter but are tuned for measuring the luminance of the night sky as seen by human night vision. These provide a single quantitative measure of the night sky, typically pointed straight up at the zenith. The most common device is the Unihedron Sky Quality Meter.
  • Another approach entirely is to put the camera in space onboard a satellite and look downward upon Earth's surface. This method has been used to look at the global span of light pollution, trace the development of cities, and reconstruct the growth of light pollution over time.
Fog shrouds this view of a rising moon over Healy Ridge in Denali National Park and Preserve.
Fog shrouds this view of a rising moon over Healy Ridge in Denali National Park and Preserve.

NPS / Shan Burson

Effects of Air Quality

The brightness and appearance of skyglow depends on atmospheric factors—chiefly moisture, air pollution, and dust particles. Clean, dry air scatters light pollution less, resulting in darker skies for observers close to the light source. However light travels farther through the air, so under good air quality conditions observers far from the light source may experience somewhat more light pollution. Poor air quality has the opposite effect, increasing light pollution close to the source and decreasing it at longer distance. However, poor air quality is seldom an advantage as it will also dim the natural features of the night sky.

Naturally occurring moisture in the air, such as clouds, fog, and haze, increase the scattering and reflectance of human-caused light sources at night. While cloudy conditions may naturally render the stars invisible, the interaction between clouds and light pollution should not be dismissed, as such conditions impact nocturnal habitats. As bright as light pollution on a clear night sometimes appears, the majority of stray light scatters freely into space. When clouds cover cities and towns, the bulk of stray light is reflected back down toward Earth's surface. This results in ground illumination sometimes being several times brighter under a cloudy sky than a clear sky.
NPS scientist prepares cameras to measure sky glow conditions in the desert at night.

NPS Methods

NPS has pioneered portable instrumentation and techniques for measuring sky glow conditions in parks

Bright areas on this map show sky glow from artificial light scattering into the atmosphere.

Night Sky Monitoring Database

Metrics captured in national parks across the USA express observed and estimated artificial sky brightness

Data mosaic shows

Night Sky Monitoring Report

The report provides metrics data and visual indicators of sky quality.