ESA Catches Glowing Venus
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 that 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 because 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 can give us a lot of information,” says Antonio GarcÃƒa MuÃƒ±oz, who was at the Australian National University when the research was carried out; he is now located at the Instituto de AstrofÃƒsica de Canarias, Tenerife, Spain. “It can provide details about the temperature, wind direction, composition and chemistry of an 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.
But 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. “Luckily for us, Venus has a temperamental atmosphere,” says GarcÃƒa MuÃƒ±oz, “Packets of oxygen and nitrogen atoms are blown around.” Sometimes these become dense enough to boost the brightness of the nightglow, making it visible to VIRTIS.
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. “Perhaps when we have more observations, we will understand the correlation between them,” says GarcÃƒa MuÃƒ±oz.
In order to do that, the VIRTIS team plans to continue monitoring the planet, building up a database of this fascinating phenomenon.
It also highlights a new mystery. “These results show that there could be at least twice as much hydrogen in the upper atmosphere of Venus than we thought,” says Delva. The detected hydrogen ions could exist in atmospheric regions high above the surface of the planet; but the source of these regions is unknown.
So like a true lady, Venus still retains some of her mystery.
* “ËœThe near-infrared nitric oxide nightglow in the upper atmosphere of Venus’ by A. GarcÃƒa MuÃƒ±oz, F. P. Mills, G. Piccioni, and P. Drossart is published in the Proceedings of the National Academy of Science Journal, on 27 January 2009.
Image 1: This artist’s impression shows Venus Express focusing on studying the peculiar atmosphere of Venus, with a precision never achieved before. In doing so, the mission is making the first ever use of the so called ‘infrared windows’ present in Venus’ atmosphere; they are narrow bands in the atmospheric spectrum, discovered in the 1980s thanks to ground observations. Looking through these ‘windows’ Venus Express is able to gather precious information about the lower layers of the atmosphere and even the surface. Credits: ESA – AOES Medialab
Image 2: This false-color composite image of Venus’s atmosphere was obtained by the Visible and Infrared Thermal Imaging Spectrometer (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
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