Visibility of stars in the night sky declines faster than previously thought

This is shown by a study in Science based on a worldwide Citizen Science project on light pollution that has collected data over the last eleven years.


People around the world are seeing fewer and fewer stars in the night sky. The change in star visibility can be explained by an increase in the sky brightness of 7-10 percent per year. The rate of change is faster than satellite measurements of artificial light emissions on Earth would at first suggest. This is the finding of a study published in the journal Science, conducted by a research group led by Christopher Kyba of the GFZ German Research Centre for Geosciences and the Ruhr-Universität Bochum with colleagues from the GFZ and the US National Science Foundation’s NOIRLab. They analysed more than 50,000 naked-eye observations by citizen scientists around the world from 2011 to 2022 as part of the “Globe at Night” Citizen Science Project. The results show that citizen science data are an important supplement to previous measurement methods.

Light pollution background

Over a large part of the Earth's land surface, the sky continues to glow with an artificial twilight long after sunset. This “skyglow” is a form of light pollution that has serious effects on the environment and should therefore be the focus of research, as Constance Walker, co-author of the study and head of the Globe at Night project of NSF's NOIRLab since its inception, emphasizes. After all, many behaviours and physiological processes of living creatures are determined by daily and seasonal cycles – and thus influenced by light. “Skyglow affects both diurnal and nocturnal animals and also destroys an important part of our cultural heritage,” says Walker. The appearance of the night sky is changing, with negative effects on stargazing and astronomy.

Need for suitable measurement methods

The change in skyglow over time has not previously been measured globally. While it could in principle be measured by satellites, the only current sensors that monitor the entire Earth do not have sufficient accuracy or sensitivity.

A promising approach is therefore to use the observational power of people using the human eye as a sensor, and in doing so – within the framework of Citizen Science experiments – to rely on the power of the crowd. The “Globe at Night" project, initiated by the US National Science Foundation’s NOIRLab, has been running since 2006. People all over the world can participate in this project.

With Citizen Science...

Participants look at their night sky, and then report which of a set of eight star charts best matches what they see using an online form. Each chart shows the sky under different levels of light pollution.

“The contributions of individual people work together as if they were a global sensor network, making new science possible,” says Christopher Kyba from the GFZ German Research Centre for Geosciences in Potsdam and the Ruhr University Bochum. Together with his GFZ colleague Yigit Öner Altıntas and Constance E. Walker and Mark Newhouse from NOIRLab, he has analyzed data from 51,351 participants around the world taken on cloud- and moon-free nights between 2011 and 2022. They were obtained from 19,262 locations worldwide, including 3,699 locations in Europe and 9,488 locations in North America.

In order to calculate a rate of change in sky brightness from this data and to take into account that the observers were also at different locations over the years, they made use of a global model for sky brightness based on satellite data from 2014. surprising findings

“The rate at which stars are becoming invisible to people in urban environments is dramatic,” sums up Christopher Kyba, lead author of the study. The researchers found that the change in the number of visible stars can be explained by increases in night sky brightness. In Europe, they found a 6.5 per cent increase in brightness per year matched the data; in North America, it's 10.4 per cent.

To put these numbers into a more understandable context, Kyba explains the consequences for seeing stars in a place with a 9.6 per cent per year increase, which was the average over all locations worldwide. “If the development were to continue at that rate, a child born in a place where 250 stars are visible will only be able to see 100 stars there on his 18th birthday.”

Based on the slower growth in upward emissions seen in satellite data, the researchers were surprised by the speed of this development in skyglow. In fact, for the locations of the observers, the artificial brightness measured by satellite had slightly decreased (by 0.3 percent per year in Europe, by 0.8 percent in North America).

Causes for the difference between measurements from Earth and from space

Christopher Kyba believes that the difference between human observation and satellite measurements is probably due to changes in lighting practices: "Satellites are most sensitive to light that is directed upwards towards the sky. But it is horizontally emitted light that accounts for most of the skyglow," Kyba explains. “So, if advertisements and facade lighting become more frequent, bigger or brighter, they could have a big impact on skyglow without making much of a difference on satellite imagery.”

Another factor the authors cite is the widespread switch from orange sodium vapor lamps to white LEDs, which emit much more blue light. “Our eyes are more sensitive to blue light at night, and blue light is more likely to be scattered in the atmosphere, so contributes more to skyglow,” Kyba says. “But the only satellites that can image the whole Earth at night are not sensitive in the wavelength range of blue light.”

Limits of the study and further potential

However, the Citizen Science approach also has its limitations. For example, the number of participants from different regions of the world determines the significance of spatial and temporal trends. So far people from North America and Europe have had the largest participation in the experiment, and half of the Asian contributions come from a single country: Japan. “The most data comes from the regions of Earth where skyglow is currently most prevalent. That’s useful, but it means that we can’t say much about skyglow change in regions with few observations,” Kyba emphasizes. Especially in developing countries, rapid changes in artificial skyglow are suspected, but there have been few observations so far.

Two conclusions: Lighting policy and Citizen Science

The researchers draw two main conclusions from their findings: On the one hand, they show that current lighting policies, such as the use of LEDs, have not yet brought about any improvement, at least on a continental level, despite growing awareness of light pollution.

“And on the other hand, we were able to demonstrate that the Citizen Science data represent an important supplement to the previous measurement methods,” Kyba emphasizes.

Constance Walker adds, “If we had broader participation, we could identify trends for other continents, and possibly even for individual states and cities. The project is ongoing, so feel free to take a look tonight and let us know what you see!”

Further information on “Globe at Night” can be found here.

Original publication: Christopher C. M. Kyba, Yigit Öner Altıntas, Constance E. Walker, Mark Newhouse, Citizen scientists report global rapid reductions in the visibility of stars from 2011 to 2022, Science (2023), DOI: 10.1126/science.abq7781


Scientific contact

Media contact

Additional News

Portrait Lars Bernard, green background

The Board of Trustees appoints Prof. Lars Bernard to the Scientific Advisory Board of the…

Portrait photo of Harald Schuh, background: green

AGU Award for Harald Schuh

The glass building with flagging "IASS" at Helmholtzstraße 5.

An ideal addition to the Helmholtz Association

SLR Station, Laser

New DFG Research Unit “Clock Metrology: A Novel Approach to TIME in Geodesy” with GFZ…

Niels Hovius portrait

Niels Hovius appointed to the renowned "National Academy of Science and Engineering –…

[Translate to English:] GFZ-Logo

GFZ's position on the Leopoldina paper “Earth System Science”

Kimberella fossile

Feeding strategies of the oldest known animals (Ediacara)

Portraits of the five young researchers

EGU OSPP Awards 2022 to five GFZ researchers

[Translate to English:] Lila Flagge wehend über einem Dachgiebel

Interviews on the occasion of the Purple Light Up 2022

Obituary picture of Dr. Kemâl Erbas.

Obituary Dr. Kemâl Erbas

Two profile photos and in between the logo of BMWK and a symbol image for a text document.

Important signal for the expansion of deep geothermal energy

German map with quality-checked data points, shown as columns

A new heat-flow analysis shows higher values for Germany

P. Martinez-Garzon in a forest next to a giant split rock

Dr. Patricia Martinez-Garzon wins ERC Starting Grant for her project QUAKE-HUNTER

Map of Türkiye with the marked epicentre of the earthquake in the northwestern part of the country

Background on today's earthquake in northwest Türkiye

Topography map of the alps.

What is driving the Alps upwards?

Groupp picture ICDP/IODP Kolloquiums

Joint IODP/ICDP-Colloquium at GFZ

Teachers in lecture hall during lecture

"Extreme Events in the Earth System" - 20th "System Earth" Autumn School

Two young researchers stand in front of trees holding their certificates, next to them stands Ludwig Stroink, who awarded the certificates.

“GFZ Friends” honours Theresa Hennig and Lei Wang with the “Friedrich-Robert-Helmert Prize…

Satellite image of a desert area: Colorful spots show different minerals.

German environmental satellite EnMAP: start into regular operation

On the left, a measuring tower in a low overgrown tundra landscape.

More methane from Siberia in summer

[Translate to English:] Profilfoto mit schwarzem Rahmen von Henning Francke

Obituary: Henning Francke

Group photo with projekt responsible

Making geodata interoperable and suited for curiosity driven research: GEO-INQUIRE project…

Schema Energiebereitstellung durch Geothermie

European Geothermal Congress from 17 to 21 October 2022 in Berlin

Gruppenfoto PAM

International Conference on Polar and Alpine Microbiology

Leni Scheck Wenderoth

“AWG Professional Excellence Award” for Magdalena Scheck-Wenderoth

Ausbildung am GFZ

Berufsausbildung und duales Studium am GFZ

Dr. Ute Weckmann during the opening speech of the workshop

Dr. Ute Weckmann takes over the chairmanship of IAGA Division VI

Anke Neumann aon a boat during a research trip

Dr Anke Neumann is a Senior Humboldt Research Fellow

Earth Model

New DFG priority programme on deep Earth evolution over geologic time

Logo of the Helmholtz Innovation Labs: written words only

Successful interim evaluation of the two Helmholtz Innovation Labs at the GFZ

back to top of main content