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Detection of Phosphates Originating from Enceladus's Ocean

Frank Postberg · Yasuhito Sekine · Fabian Klenner · Christopher R. Glein · Zenghui Zou · Bernd Abel · Nozair Khawaja · Jon K. Hillier · Juergen Fiebig · Kelly E. Miller · Ralf Srama · Sascha Kempf · Nathalie Cabrol · Hunter Waite

Nature · 2023

Cassini mass spectra of Enceladus ice grains confirm sodium phosphates in the moon's subsurface ocean at concentrations at least 100 times higher than Earth's oceans, completing the CHNOPS biogenic-element inventory and strengthening the habitability case.

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Brief

Using archived data from the Cosmic Dust Analyser (CDA) aboard NASA's Cassini spacecraft, Postberg et al. identified sodium phosphates in ice grains ejected from Enceladus's subsurface ocean into Saturn's E ring, the first detection of phosphorus in any extraterrestrial ocean. Geochemical modeling supports water-rock interaction in Enceladus's porous rocky core as the source mechanism, consistent with serpentinization under alkaline, silica-rich conditions. The inferred ocean phosphate concentration is at least 1 mmol/kg, roughly two to three orders of magnitude above typical Earth surface-ocean levels (~0.001–0.003 mmol/kg). The finding adds phosphorus to the carbon, hydrogen, nitrogen, oxygen, and sulfur already confirmed at Enceladus, satisfying the full CHNOPS checklist for life-as-we-know-it.

Metadata

Category
Search
Venue
Nature
Type
Peer-reviewed
Year
2023
Authors
Frank Postberg, Yasuhito Sekine, Fabian Klenner, Christopher R. Glein, Zenghui Zou, Bernd Abel, Nozair Khawaja, Jon K. Hillier, Juergen Fiebig, Kelly E. Miller, Ralf Srama, Sascha Kempf, Nathalie Cabrol, Hunter Waite
Access
Paywalled
Programs
Cassini-Huygens
Instruments
Cassini Cosmic Dust Analyser (CDA)
Data sources
Cassini CDA mass spectra, Saturn E-ring ice grain data, Enceladus plume particle archive
Tags
astrobiology, biosignature, ocean worlds, habitability, phosphorus detection, CHNOPS, icy moons

Key points

  • Sodium phosphates detected in Enceladus ice grains via Cassini Cosmic Dust Analyser mass spectra, first confirmed phosphorus in an extraterrestrial ocean.p.2
  • Inferred ocean phosphate concentration is ≥1 mmol/kg, at least 100× the phosphate level in Earth's surface ocean, making Enceladus's ocean unusually phosphorus-rich.p.3
  • Geochemical modeling attributes the high phosphate abundance to dissolution of phosphate-bearing minerals in the rocky core under the moon's alkaline, carbonate- and silica-rich ocean chemistry.p.4
  • Detection completes the CHNOPS inventory for Enceladus: carbon, hydrogen, nitrogen, oxygen, and sulfur had been confirmed previously by Cassini; phosphorus was the final missing element.p.1
  • Both orthophosphates and polyphosphates were identified in the CDA spectral signatures, indicating multiple phosphate species present in the ocean source material.p.3
  • Phosphorus on Earth is typically a limiting nutrient for biological productivity; Enceladus's multi-millimolar concentrations would not be limiting, removing a key habitability barrier.p.5
  • The Cassini Grand Finale data archive, collected before the spacecraft's 2017 controlled impact into Saturn, provides the primary dataset; no future mission to Enceladus is currently operational.p.2

Most interesting

  • Phosphorus is considered the scarcest biogenic element in the solar system's icy moon environments, yet Enceladus appears to harbor it at concentrations that dwarf Earth's open ocean, an inversion of the expected gradient.
  • The detection was made from data collected by a spacecraft that no longer exists: Cassini was deliberately destroyed in Saturn's atmosphere on 15 September 2017, making the CDA archive a non-renewable scientific resource.
  • The high phosphate abundance is thought to be self-sustaining: Enceladus's alkaline, carbonate-rich ocean chemistry thermodynamically suppresses phosphate mineral precipitation, keeping phosphate dissolved rather than sequestered in rock.
  • Enceladus is now the only body beyond Earth where all six CHNOPS elements, the complete molecular alphabet of terrestrial biochemistry, have been directly detected in a liquid water environment.
  • Saturn's E ring, the broad diffuse ring in which Enceladus orbits, is largely composed of the same ice grains analyzed in this study, meaning the habitability fingerprint of Enceladus's ocean is physically embedded in the ring system visible from Earth.
  • The 14-author team spans planetary science, geochemistry, mass spectrometry, and astrobiology across institutions in Germany, Japan, France, and the United States, reflecting the breadth of expertise required to interpret a single instrument's spectral output.

Cross-references