ESA’s Venus Express spacecraft has observed an eerie glow in the night-time atmosphere of Venus.
This infrared light comes from nitric oxide and is showing scientists the atmosphere of Earth’s nearest neighbor is a temperamental place of high winds and turbulence. Unfortunately, the glow on Venus cannot be seen with the naked eye as it occurs at the invisible wavelengths of infrared. ESA’s Venus Express, however, is equipped with the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) instrument, which can see these wavelengths. VIRTIS has made two unambiguous detections of the so-called nightglow for nitric oxide at Venus. This is the first time such infrared detections have been made for any planet and provide a new insight into Venus’s atmosphere.
The nightglow is ultimately caused by the Sun’s ultraviolet light, which streams into a planet’s atmosphere and breaks the molecules up into atoms and other simpler molecules. The free atoms may recombine again and, in specific cases, the resulting molecule is endowed with some extra energy that is subsequently lost in the form of light. On the day-side of the planet, any atoms that do find their way back together are outshone by the sunlight falling into the atmosphere. However, on the night-side where atoms are transported by a vigorous diurnal circulation, the glow can be seen with appropriate instruments, such as VIRTIS. A nitric oxide nightglow in the infrared has never been observed in the atmospheres of Mars or Earth, although we know that the necessary nitric oxide molecules are present because they have been observed in ultraviolet.
The nightglow on Venus has been seen at infrared wavelengths before, betraying oxygen molecules and the hydroxyl radical, but this is the first detection of nitric oxide at those wavelengths. It offers data about the atmosphere of Venus that lies above the cloud tops at around 70 km. The oxygen and hydroxyl emissions come from 90-100 km, whereas the nitric oxide comes from 110-120 km altitude. Yet, even VIRTIS cannot see the nitric oxide nightglow all the time because it is often just too faint. Venus Express can observe the three nightglow emissions simultaneously, and this gives rise to a mystery. The nightglows from the different molecules do not necessarily happen together. The VIRTIS team plans to continue monitoring the planet, building up a database of this fascinating phenomenon.
(Source: ESA – top image, Venus Express — the bottom image, a false-color composite image of Venus’s atmosphere, was obtained by VIRTIS on board ESA’s Venus Express, from a limb (or profile) perspective. The top panel shows the oxygen nightglow of Venus at an altitude of approximately 96 km over the surface of the planet, seen at a wavelength of 1.27 microns. The bottom panel shows the same portion of the atmosphere observed at the same time, but at a different wavelength (around 1.22 microns). Here it is possible to see the nightglow of nitric oxide, which is much weaker than that of oxygen and comes from an higher altitude — around 110 km above the surface. In red is the thermal emission of Venus at 1.74 microns; one of the atmospheric windows of Venus exploited by VIRTIS. Credits: ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA)
