News on Minor Planets
- Dawn reveals asteroid Vesta’s role in solar system history
- Analysis of Vesta's chemistry
- Mountain on Vesta produces terrestial meteorites
- Comlpex molecules on Plutos surface
- Is Vesta really a small Earthlike planet?
- Dawn spirals to lovest orbity around Vesta
- Pluto's minor-planetary twin Eris
- Giant mountain on Vesta
- New images and video of Vesta
- Discovery of ice and possibly methane on distant dwarf-planet
- New moon discovered around Pluto
- Neptune celebrates its 1-year anniversary
- A day on a giant gas-planet
- Astronomers observe rare occultation of planet and its moon
- SOFIA observes challenging Pluto occultation
- First sights of asteroid Vesta
- The dwarf planet Haumea
- First glimpse of Vesta
- Pluto extensive atmosphere
- Scientists suggests a large planet may be hiding in our solar outskirts
- Minor-planet Eris has more atmosphere than Pluto
- Tritons summersky full of CO and Methane
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Tritons summersky full of CO and Methane
Wednesday, 07 April 2010 14:32
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| Solar system - Minor planets |
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"We have found real evidence that the Sun still makes its presence felt on Triton, even from so far away. This icy moon actually has seasons just as we do on Earth, but they change far more slowly," says Emmanuel Lellouch, the lead author of the paper reporting these results in Astronomy & Astrophysics. On Triton, where the average surface temperature is -235'C, it is currently summer in the southern hemisphere and winter in the northern. As Triton's southern hemisphere warms up, a thin layer of frozen nitrogen, methane, and carbon monoxide on Triton's surface sublimates into gas, thickening the icy atmosphere as the season progresses during Neptune's 165-year orbit around the Sun. A season on Triton lasts a little over 40 years, and Triton passed the southern summer solstice in 2000. Based on the amount of gas measured, Lellouch and his colleagues estimate that Triton's atmospheric pressure may have risen by a factor of four compared to the measurements made by Voyager 2 in 1989, when it was still spring on the giant moon. The atmospheric pressure on Triton is now between 40 and 65 microbars — 20 000 times less than on Earth. Carbon monoxide was known to be present as ice on the surface, but Lellouch and his team discovered that Triton's upper surface layer is enriched with carbon monoxide ice by about a factor of ten compared to the deeper layers, and that it is this upper "film" that feeds the atmosphere. While the majority of Triton’s atmosphere is nitrogen (much like on Earth), the methane in the atmosphere, first detected by Voyager 2 , and only now confirmed in this study from Earth, plays an important role as well. "Climate and atmospheric models of Triton have to be revisited now, now that we have found carbon monoxide and re-measured the methane," says co-author Catherine de Bergh. Of Neptune's 13 moons, Triton is by far the largest, and, at 2700km in diameter (or three quarters the Earth’s Moon), is the seventh largest moon in the whole Solar System. Since its discovery in 1846, Triton has fascinated astronomers thanks to its geologic activity, the many different types of surface ices, such as frozen nitrogen as well as water and dry ice (frozen carbon dioxide), and its unique retrograde motion. Observing the atmosphere of Triton, which is roughly 30x further from the Sun than Earth, is not easy. In the 1980s, astronomers theorised that the atmosphere on Neptune's moon might be as thick as that of Mars (7 millibars).
It wasn't until Voyager 2 passed the planet in 1989 (See image right) that the atmosphere of nitrogen and methane, at an actual pressure of 14 microbars was measured. Since then, ground-based observations have been limited. Observations of stellar occultations (a phenomenon that occurs when a Solar System body passes in front of a star and blocks its light) indicated that Triton’s surface pressure was increasing in the 1990's. It took the development of the Cryogenic High-Resolution Infrared Echelle Spectrograph (CRIRES) at the Very Large Telescope (VLT) to provide the team the chance to perform a far more detailed study of Triton’s atmosphere. "We needed the sensitivity and capability of CRIRES to take very detailed spectra to look at the very tenuous atmosphere," says co-author Ulli Käufl. The observations are part of a campaign that also includes a study of Pluto Pluto, often considered a cousin of Triton and with similar conditions, is receiving renewed interest in the light of the carbon monoxide discovery, and astronomers are racing to find this chemical on the even more distant dwarf planet. This is only the first step for astronomers using CRIRES to understand the physics of distant bodies in the Solar System. "We can now start monitoring the atmosphere and learn a lot about the seasonal evolution of Triton over decades," Lellouch says. Source: ESO |




According to the first ever infrared analysis of the atmosphere of Neptune's moon Triton, where it presently is summer in its southern hemisphere. The analysis discovered CO and Methane in Triton's thin atmosphere, and revealed that it varies seasonally, thickening when warmed.