Gizmodo57%
Europa's Hidden Ocean May Be Even Harder to Reach Than We Thought 5%
By Gayoung Lee22%
7/24/2026, 1:45:01 PM
Keywords: Europa, Planetary Science
BS Summary: This article contains 2 faulty reasoning types, including False Dilemma, with Negativity Bias as the most egregious example at 16.6% saturation with 79 hits. Analysis detected 103 faulty-reasoning hits from 476 analyzed words, generating a BS Score of 19.1% and a BS Rank of 5% (20,969 of 21,887 articles). This article is better (less manipulative) than 95.80% of the article peer group.
Earlier this year, researchers warned against the dangers of “fluffy ice” on Europa’s surface.
If unaccounted for, missions headed to Jupiter’s moon could drown themselves in its deep, icy oceans.
A new study suggests that this won’t happen—but for reasons that won’t make our Europa trips any easier.
A paper published yesterday in Nature Astronomy challenges the assumption that the shallow pools of water on Europa’s surface represent a direct access route to the moon’s deep, icy oceans.
In theory, this supposed access route could make it easier for a probe to explore how liquid water from Europa’s deep oceans traveled through cracks in the ice to the surface.
Unfortunately, we’re not sure if this even happens.
“This is exactly what we wanted to test,” Lujendra Ojha, the study’s first author and an earth scientist at Rutgers University, told Gizmodo.
“In particular, we asked whether the water could travel this distance before losing enough heat to freeze and whether the fractures could remain open long enough to transport a meaningful amount of water.”
Prospects real icy
For the study, Ojha and colleagues simulated the movement and cooling of water inside the fractures of Europa’s icy shell.
In a Rutgers statement, Ojha explained that earlier models “often treated water rising through Europa’s ice as if it moved in a relatively orderly way.”
They also draw an analogy between volcanoes and icy volcanoes, although there are “fundamental” differences between ice, liquid water, lava, and volcanoes, he added.
The latest approach, on the other hand, takes a more realistic approach by accommodating for numerous factors, such as water velocity, the size of the crack, turbulence, and supercooling.
The simulations arrived at a simple—perhaps discouraging—conclusion.
All things considered, there are too many obstacles for deep ocean water to reliably arrive at the surface.
For instance, if the water rises turbulently, it would “lose heat rapidly to the surrounding ice and form small ice crystals that could eventually clog the fracture,” Ojha told Gizmodo.
For the Europa fans
So the small pools of water we’ve observed at the surface probably come from melted sections of the icy crust, rather than from deep down below.
Having said that, Ojha told Gizmodo that the findings don’t necessarily warrant drastic shifts in our missions to Europa.
But if spacecraft detect shallow liquid-water reservoirs on Europa, we’d be smart not to “automatically assume that the water came from Europa’s deep ocean,” he said.
“In that case, the chemical, physical, maybe biological constraints we are able to derive from studying the shallow liquid water layer may not at all reflect the chemistry of the underlying ocean,” Ojha concluded.
“Future missions should, therefore, focus not only on finding shallow water but also on determining its origin and whether it is connected to the deeper ocean.”
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0%flagged-word coverageLujendra Ojha
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