Airglow of the Earth The Earth's night sky is illuminated by diffuse light, called
airglow, that is produced by radiative transitions of atoms and molecules. Among the most intense such features observed in the Earth's night sky is a group of infrared transitions at wavelengths between 700 nanometers and 900 nanometers. In 1950,
Aden Meinel showed that these were transitions of the hydroxyl molecule, OH.
NASA also reported in 2009 that the
LCROSS probe revealed an
ultraviolet emission spectrum consistent with hydroxyl presence. On 26 October 2020,
NASA reported definitive evidence of water on the sunlit surface of the Moon, in the vicinity of the crater
Clavius (crater), obtained by the
Stratospheric Observatory for Infrared Astronomy (SOFIA). The SOFIA Faint Object infrared Camera for the SOFIA Telescope (FORCAST) detected emission bands at a wavelength of 6.1 micrometers that are present in water but not in hydroxyl. The abundance of water on the Moon's surface was inferred to be equivalent to the contents of a 12-ounce bottle of water per cubic meter of lunar soil. The
Chang'e 5 probe, which landed on the Moon on 1 December 2020, carried a mineralogical spectrometer that could measure infrared reflectance spectra of lunar rock and regolith. The reflectance spectrum of a rock sample at a wavelength of 2.85 micrometers indicated localized water/hydroxyl concentrations as high as 180 parts per million.
Atmosphere of Venus The
Venus Express orbiter collected
Venus science data from April 2006 until December 2014. In 2008, Piccioni,
et al. reported measurements of night-side airglow emission in the atmosphere of Venus made with the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on Venus Express. They attributed emission bands in wavelength ranges of 1.40–1.49 micrometers and 2.6–3.14 micrometers to vibrational transitions of OH. This was the first evidence for OH in the atmosphere of any planet other than Earth.
Exoplanets In 2021, evidence for OH in the dayside atmosphere of the exoplanet
WASP-33b was found in its emission spectrum at wavelengths between 1 and 2 micrometers. Evidence for OH in the atmosphere of exoplanet
WASP-76b was subsequently found. Both
WASP-33b and
WASP-76b are
ultra-hot Jupiters and it is likely that any water in their atmospheres is present as dissociated ions. == See also ==