Posted on 06/30/2018 4:43:05 PM PDT by Simon Green
Complex organic molecules have been discovered for the first time coming from the depths of Saturn's moon Enceladus, a new study reported.
Spacecraft scheduled to launch soon could explore what this new discovery says about the chances of life within icy moons like Enceladus, the study's researchers said.
The sixth largest of Saturn's moons, Enceladus is only about 314 miles (505 kilometers) in diameter. This makes the moon small enough to fit inside the borders of Arizona.
In 2005, NASA's Cassini spacecraft detected plumes of water vapor and icy particles erupting from Enceladus, revealing the existence of a giant ocean hidden under the moon's frozen shell. Because there is life virtually wherever there is water on Earth, these findings suggested that life might also exist on Enceladus.
Previously, scientists had detected only simple organic (carbon-based) compounds, each less than about five carbon atoms in size, in the plumes of Enceladus. Now, researchers have detected complex organic molecules from the moon, including some at least 15 carbon atoms in size.
"This is the first-ever detection of complex organics coming from an extraterrestrial water world," study lead author Frank Postberg, a planetary scientist at the University of Heidelberg in Germany, told Space.com.
The scientists analyzed data that Cassini gathered when it flew within a plume from Enceladus, as well as from when the probe passed through Saturn's E ring, which is made up of ice grains spewed from Enceladus. The investigators detected ice grains loaded with complex organic material in both the plume and the E ring.
The researchers conjectured that these organic materials were cooked up inside the hot, rocky and fragmented core of Enceladus, which prior work suggested had water seeping through its pores.
"The organics are then injected, together with the hot water, into the overlying cooler ocean by hydrothermal vents," Postberg said. "Then, they can be transported upwards to the ocean surface on the walls of rising bubbles of gas."
Postberg noted that most of the organic-loaded ice grains the researchers saw were in Saturn's E ring. This might suggest that these complex organic molecules were not produced within Enceladus, but instead resulted from sunlight-triggered chemical reactions in space.
"However, we observe the highest proportion of these complex organics in the young, inner E ring close to Enceladus, as compared to the old, outer E ring far away from Enceladus," Postberg said. "Furthermore, we also see the complex organics directly in the plume."
The researchers cautioned that these new findings are not solid evidence for life, as biological reactions are not the only potential sources of complex organic molecules. The next logical step is to go back to Enceladus soon "and see if there is extraterrestrial life," Postberg said. "Nowhere else can a potentially habitable extraterrestrial ocean habitat be so easily probed by a space mission as in the case of Enceladus."
Postberg added that NASA and the European Space Agency already have missions, Europa Clipper and JUICE, respectively, scheduled to launch in 2022 that will visit Europa and Ganymede, the icy moons of Jupiter that have subsurface oceans. These missions will check for habitability on those worlds.
The scientists detailed their findings online June 27 in the journal Nature.
Supposedly. But I’m not a NASA scientist. I don’t even play one on TV.
Also of interest is that Earth is actually rather dry, taken in total:
http://www.businessinsider.com/water-space-volume-planets-moons-2016-10
...
Cool article that presents data that conflicts with intuition.
Who could imagine that Pluto has almost as much liquid water as Earth?
Thanks again for a post that contrasts with many of the ignorant comments on the thread.
“Pretty amazing that we can detect something 5 carbon atoms
in size, around another planet.”
https://en.wikipedia.org/wiki/List_of_interstellar_and_circumstellar_molecules
The molecules listed below were detected by spectroscopy. Their spectral features are generated by transitions of component electrons between different energy levels, or by rotational or vibrational spectra. Detection usually occurs in radio, microwave, or infrared portions of the spectrum.[1]
Interstellar molecules are formed by chemical reactions within very sparse interstellar or circumstellar clouds of dust and gas. Usually this occurs when a molecule becomes ionized, often as the result of an interaction with a cosmic ray. This positively charged molecule then draws in a nearby reactant by electrostatic attraction of the neutral molecule’s electrons. Molecules can also be generated by reactions between neutral atoms and molecules, although this process is generally slower.[2] The dust plays a critical role of shielding the molecules from the ionizing effect of ultraviolet radiation emitted by stars.[3]
+1
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