Gemini North Under a Blanket of Airglow

The Milky Way shares the stage with a luminous bubble of green and orange airglow in this panoramic image of Gemini North, one half of the International Gemini Observatory, supported in part by the U.S. National Science Foundation (NSF) and operated by NSF NOIRLab. Gemini North (right) is accompanied here by the Canada-France-Hawai‘i Telescope (CFHT) (left). In this image, you could remove all of the stars, the brilliant stripe of the Milky Way, and the nearby city lights of Hilo, Hawai‘i (far left), and you would still be left with a picture that isn’t completely dark. This is thanks to the persistent light of airglow.

Airglow is primarily caused by sunlight interacting with atoms and molecules in Earth’s upper atmosphere, which allows them to gain excess energy. This excess energy is then released as a particle of light called a photon. The frequencies of the photons determine the captivating colors of airglow. While it’s often difficult to see this light with the naked eye, a camera can capture it, as seen in the photo above. Intersecting the Milky Way is another lucent phenomenon known as zodiacal light with the gegenschein to the right.

This photo was taken as part of the NOIRLab 2022 Photo Expedition to all the NOIRLab sites. Petr Horálek, the photographer, is a NOIRLab Audiovisual Ambassador. Fulldome and extended view versions of this photo also are available.