How to conduct a night sky quality survey
A thorough night sky quality survey is essential to a successful application to the International Dark Sky Places program.
There are a variety of ways to approach making a survey. These include:
Sky quality meter survey
The Unihedron Sky Quality Meter-Lens (SQM-L) is the most widely used device for taking scientific-quality measurements of sky brightness. This small, battery-powered device is available directly from the manufacturer.
The SQM-L is easy to use: Simply hold the device above your head, point the photometer at the zenith (straight up), and push the button. The screen will then display the sky brightness at that point in astronomer units (magnitudes per square arcsecond, or mpsas). This unit is somewhat counterintuitive in that the higher the number, the darker the sky is. Take at least six measurements per location per visit, discarding the first measurement. Report all of the measurements.
Never take a measurement directly underneath a light source or anything that might block the clear sky. Always take measurements with a clear, open sky without cloud cover, to prevent any sky glow measurements that will deter the accuracy of the device. Also, always take measurements when the moon is below the horizon. Measurements taken while the moon is visible will not accurately reflect the natural darkness of your location.
Similarly, keep in mind the impact of twilight on your measurements. Only take readings under conditions of astronomical darkness, meaning that the sun is at least 18º below the local horizon. Good sources of information for the times of the beginning and end of astronomical twilight at your location on any given night can be found here. (Note that for these calculators you may need to know your latitude, longitude, and local time zone offset from GMT.)
It is essential to include areas in the survey that represent the darkest, brightest, and most accessible areas to visitors to achieve a comprehensive survey. This data can then be organized into a map and corresponding table showing approximate locations and readings of measurements. An example map and table are provided below. Advocates are encouraged to use DarkSky’s standardized spreadsheet when taking measurements out in the field or compiling measurements taken throughout the course of a year. Directions for access and edits are provided at the top of each spreadsheet.
If you are able, upload your data to community science programs like Globe at Night to further help scientists track night sky quality across the world. Data from dark sites, and especially communities, are essential in monitoring this natural resource and the presence and intensity of light pollution globally. When reporting data to this application, you can indicate that this is a measurement made in support of DarkSky advocacy by adding the string “IDA” to the ‘Location comments’ section on the Globe At Night form. For measurements made in support of International Dark Sky Places Program nominations, add the string “IDSP” to the same section.
Bortle scale interpretation
The Bortle scale provides an estimate of sky brightness and helps in interpreting how light pollution is affecting one’s view of night sky phenomena. The lower the number is, the better the sky quality. The easiest way to interpret the Bortle scale is to follow a descriptive flow chart; follow the questions to reveal what Bortle class your skies fall under. This may need to be done at different locations across an area if sky brightness varies between Bortle classes.
Steve Owens, past Dark Sky Places Committee member, is credited with the flow chart below. Learn more about it on his Dark Sky Diary.
Have little to no experience stargazing? No problem! Visit Sky and Telescope’s Beginner’s Guide to learn more about picking up amateur astronomy skills.
We also recommend looking for advice and help from amateur astronomers and local astronomy clubs near you. You may also search for local DarkSky Chapters or Delegates to assist in night sky monitoring efforts.
Documenting nighttime phenomena with photography provides verification that the quantitative SQM-L measurements are accurate. Photographs also help document whether light domes are visible along the horizon, which the SQM-L device may not detect.
When providing images to DarkSky, include a breakdown of the camera details used to take it, such as exposure time, focal length, and ISO speed. (See the example below.)
|Location:||Cerro Pachón, near SOAR Telescope in Chile (GPS location if available)|
|Phenomenon Shown:||Milky Way, Large Magellanic Cloud|
|Exposure:||17.5 sec (1/0)|
|Focal Length:||18 mm|
These methods in unison have proven successful in providing quantitative data and qualitative assessments of the night sky. If you have additional questions, please contact the Director of Conservation.