In It For Life

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The crater was formed when a large object hit the area.

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That could have created an environment that would have all the necessary elements for life. The Dragonfly team hopes to learn whether combining organic material with liquid water and energy in the form of heat could have caused complex molecules to develop — or even life itself. If life is, or has been on Titan, Dragonfly should be able to find it. Its instruments will be searching for is a class of molecules called amino acids, which are found in all life on Earth. Dragonfly is expected to launch in and arrive at Titan in The science and engineering teams are designing and building the spacecraft.

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  • Embed share The code has been copied to your clipboard. The URL has been copied to your clipboard. No media source currently available. Scientists think geologic activity, like warmer ice rising from below, could be erasing the craters over time.

    We’re in it for life.

    Europa's bright, icy surface is a landscape unlike anything seen on Earth. To start with, in an overall sense, it's quite smooth, with no towering mountains, and no deep basins or chasms.

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    Myriad ridges and grooves crisscross the surface, breaking up the landscape. Many of these features coincide with long, curving streaks that are dark and reddish in color — some stretching across the surface in great arcs over miles kilometers long. Elsewhere, domes, pits and chaotic jumbles of icy blocks hint that warm ice may be rising from deep below.

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    Models suggest that Europa's icy shell is relatively thin. The icy moon gets stretched and released by the tug of Jupiter's gravity, in an endless cycle, as Europa orbits the giant planet. This squeezing in and out is a process called tidal flexing, which may be creating heat inside Europa; the warmed ice from this heat may be pushing the surface upward to create the ridges. The tidal flexing also may be creating enough heat inside Europa to maintain a liquid ocean beneath the moon's icy surface.

    Most of the heat would be focused at the boundary between the ocean and the icy crust. For Europa to be potentially habitable, it would need to have the essential chemical ingredients for the chemistry of life.

    These include carbon, hydrogen, nitrogen, oxygen, phosphorus and sulfur, which are common elements, and scientists think it's likely they were present on Europa as it formed. Later on, asteroids and comets impacted the moon and would have deposited even more organic, or carbon containing, materials. The chemical elements for life might be found within Europa's icy shell, as well as its ocean. Tidal heating could be powering a system that cycles water and nutrients between the moon's rocky interior, ice shell and ocean, creating a watery environment rich with chemistry conducive to life.

    This is why studying Europa's chemistry — on the surface and within the suspected ocean — is important for understanding its habitability, because living things extract energy from their environments by chemical reactions. All lifeforms need energy to survive. Where would life on an icy world far from the Sun get energy?

    The type of life that might inhabit Europa likely would not be powered by photosynthesis — but by chemical reactions. Europa's surface is blasted by radiation from Jupiter.

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    • That's a bad thing for life on the surface — it couldn't survive.