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posted by takyon on Wednesday June 06 2018, @04:18AM   Printer-friendly
from the the-Fermi-GAP dept.

The Moons of Some Giant Alien Planets Could Host Life

Researchers have identified more than 100 giant exoplanets that may have potentially life-hosting moons. The new analysis could change the way scientists search for life in the cosmos, study team members said. That search has generally focused on places more or less like Earth — rocky planets in the "habitable zone" of their host star, that just-right range of distances where liquid water could exist on a world's surface. Jupiter-like planets don't seem like good candidates in this regard, because they have no discernible surface. But the rocky moons of such gas giants may be a different story, study team members said.

Also at University of California, Riverside.

Exploring Kepler Giant Planets in the Habitable Zone (arXiv:1805.03370)


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  • (Score: 2) by Immerman on Wednesday June 06 2018, @02:19PM

    by Immerman (3985) on Wednesday June 06 2018, @02:19PM (#689307)

    Amino acids are an important step, but *only* a step. Once you have acids raining down from above, you need an environment for them to arrange into more complex structures. Doesn't have to be water, but liquids offer a nice blend of stability and constant molecular jostling to promote the formation of more complex structures. Water vapor wouldn't cut it. And even the idea of "primordial soup" has it's detractors, with many thinking the additional density, stability, and 2-D simplification of a film on a solid surface substrate may have been necessary (i.e. life first formed as thin slime on the surface of submerged rocks)

    On Jupiter in contrast that amino acid rain would fall, and fall, and fall... until it reached a depth where the temperatures and pressures were to great for amino acids to exist, or at least where they exists as a gas, without any surface tension to help molecules bind together. And that's a big one - our best guess for how cells first formed was as lipid rings around RNA-water solutions. Without surface tension such a thing would never form in the first place.

    Of course, with a big enough laboratory even those difficulties might be overcome by time and the sheer size of the experiment. And Jupiter's upper atmosphere is phenomenally huge. The next problem is it's almost entirely hydrogen. Plenty of other things exist, but as diffuse gasses in a hydrogen atmosphere - almost all molecular interactions will be with hydrogen - even if two amino acids bond together in a productive manner, they will have to survive being bombarded by thousands, maybe millions of hydrogen molecules before they encounter another amino acid. And they'll probably have to collide with thousands of amino acids before they hit one at just the right angle and speed to allow a new bond to form.

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