Anna Pakhomova, scientist at the ESRF, has been awarded the ERC Consolidator Grant for her project OCEAN, which aims to study the effect of high pressure on organic chemistry in large ocean worlds. The grant also acknowledges the new capabilities of high-pressure ESRF beamlines like ID27, which went through the Extremely Brilliant Source upgrade.
The presence of water in its liquid state is thought to have driven Earth’s prebiotic chemistry and is considered an essential element for the emergence of life. This is why icy moons harboring subsurface oceans are the most promising objects for extraterrestrial habitability.
There are several current and future space missions that will remotely probe intriguing Jupiter and Saturn’s icy moons. The ESA’s JUICE mission will arrive in 2031, the NASA’s Europa Clipper in 2030 and DragonFly will be launched in 2028.
“Until today, however, the question of the existence of life has always been looked at from the Earth’s perspective, while in fact, the pressure in the oceans of the Earth and those in icy moons is very different”, explains Pakhomova. “We know of some volatile organics in those large oceans that could be biological precursors, but we do not have information on their chemical evolution at the right pressure-temperature-composition conditions in water”, she adds. “This is what we want to find out with OCEAN”, she adds.
Read more on the ESRF website
Image: Anna Pakhomova on beamline ID27
Credit: S. Candé
