Featured
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A fundamental role of carbonate–sulfate melts in the formation of iron oxide–apatite deposits
Iron-rich carbonate–sulfate melts are fundamental to the formation of iron oxide–apatite ore deposits, according to a detailed fluid-inclusion study that characterized the mineralizing fluids for two mineralizing systems in the United States.
- Wyatt M. Bain
- , Matthew Steele-MacInnis
- & Erin E. Marsh
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Post-impact cryo-hydrologic formation of small mounds and hills in Ceres’s Occator crater
Mounds within Ceres’s Occator crater may have formed by freezing of water-rich impact-induced melt, by a process analogous to that of pingo formation on Earth, according to an analysis of data from NASA’s Dawn mission.
- B. E. Schmidt
- , H. G. Sizemore
- & C. T. Russell
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Article |
Valley formation on early Mars by subglacial and fluvial erosion
Some valleys in the southern highlands of Mars may have formed by subglacial erosion, consistent with a cold and icy early Mars, according to a statistical analysis of valley morphometry.
- Anna Grau Galofre
- , A. Mark Jellinek
- & Gordon R. Osinski
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Heavy iron isotope composition of iron meteorites explained by core crystallization
Experiments show that the iron isotopic composition of iron meteorites can be explained by core crystallization, and suggest the presence of sulfur-rich core material that remains unsampled by meteorite collections.
- Peng Ni
- , Nancy L. Chabot
- & Anat Shahar
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Review Article |
Materials and pathways of the organic carbon cycle through time
A review of the organic carbon cycle explores the interactions between the Earth’s surface and deeper reservoirs, the expanding inorganic controls on the organic carbon cycle, and how these links have strengthened through geological time.
- Matthieu E. Galvez
- , Woodward W. Fischer
- & Timothy I. Eglinton
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News & Views |
Redrawing the early sulfur cycle
The Archaean atmosphere may have been well oxygenated, according to a reconsideration of sulfur cycling at that time. This challenges the view that sedimentary sulfur records oxygen-poor conditions during Earth’s first two billion years.
- Desiree Roerdink
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Article |
Corona structures driven by plume–lithosphere interactions and evidence for ongoing plume activity on Venus
Thermomechanical modelling shows that the formation and diverse morphologies of coronae on Venus can be explained by interactions between the lithosphere and impinging mantle plumes. Some corona structures are consistent with ongoing plume activity.
- Anna J. P. Gülcher
- , Taras V. Gerya
- & Jessica Munch
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Geomorphological evidence for a dry dust avalanche origin of slope streaks on Mars
Patterns of erosion and deposition by some slope streaks on Mars are consistent with a dry dust avalanche origin, according to an analysis of orbital images before and after new streaks formed.
- Colin M. Dundas
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Article |
Evidence for a hot start and early ocean formation on Pluto
Pluto’s subsurface ocean may have formed early due to accretionary heating, a comparison of thermal evolution modelling with observed tectonic structures suggests.
- Carver J. Bierson
- , Francis Nimmo
- & S. Alan Stern
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Article |
Experimental evidence for lava-like mud flows under Martian surface conditions
Experimental mudflows under Martian surface conditions propagate similarly to terrestrial pahoehoe lava flows, suggesting mud (rather than igneous) volcanism can explain some flow morphologies on Mars.
- Petr Brož
- , Ondřej Krýza
- & Manish R. Patel
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Article |
The Earth’s core as a reservoir of water
The Earth’s core may host most of the planet’s water inventory, according to calculations of the partitioning behaviour of water at conditions of core formation.
- Yunguo Li
- , Lidunka Vočadlo
- & John P. Brodholt
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News & Views |
Clues to late accretion from Venus’s atmosphere
Whether Earth’s water was delivered early or late in its formation is debated. The composition of Venus’s atmosphere may indicate that late accretion, the final stage of planet formation, delivered little water to the terrestrial planets.
- Ramon Brasser
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Article |
Dry late accretion inferred from Venus’s coupled atmosphere and internal evolution
Venus’s atmospheric composition suggests limited water delivery to the terrestrial planets by late accretion, according to numerical simulations of the interior and atmospheric evolution of Venus under various late accretion scenarios.
- C. Gillmann
- , G. J. Golabek
- & V. Debaille
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Early crust building enhanced on the Moon’s nearside by mantle melting-point depression
Early magmatism on the Moon’s nearside may have been enhanced by a geochemical anomaly lowering the melting point of the mantle source region, according to high-temperature experiments and thermal numerical modelling.
- Stephen M. Elardo
- , Matthieu Laneuville
- & Charles K. Shearer
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Article |
Multiple early-formed water reservoirs in the interior of Mars
Mars’s mantle is chemically heterogeneous and contains multiple primordial water reservoirs, according to an analysis of the hydrogen isotopic composition of minerals in Martian meteorites.
- Jessica J. Barnes
- , Francis M. McCubbin
- & Carl B. Agee
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Article |
Supply of phosphate to early Earth by photogeochemistry after meteoritic weathering
Reduced phosphorus species delivered by meteorites can be oxidized in reactions with hydrogen sulfide under ultraviolet light to provide a ready supply of phosphate to support prebiotic chemistry, as demonstrated by experiments.
- Dougal J. Ritson
- , Stephen J. Mojzsis
- & John. D. Sutherland
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Article |
Distinct oxygen isotope compositions of the Earth and Moon
High-precision measurements suggest that the Earth and Moon have distinct oxygen isotope compositions. This implies distinct oxygen isotopic compositions of the proto-Earth and its impactor that were not fully homogenized by the Moon-forming impact.
- Erick J. Cano
- , Zachary D. Sharp
- & Charles K. Shearer
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Editorial |
Mars gets geophysical
The first marsquakes detected by NASA’s InSight mission mark just the start of seismology on Mars. Both Earth and planetary scientists alike should embrace this new frontier of geophysics.
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Article |
Limited Archaean continental emergence reflected in an early Archaean 18O-enriched ocean
The water cycle was in two different steady states, before and after continental emergence, as recorded in the decreasing oxygen isotope values of seawater since the Archaean, according to an inverse geochemical model of the oceanic crustal record.
- Benjamin W. Johnson
- & Boswell A. Wing
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News & Views |
InSight searches high to see below
Mars’s newest seismometer needed to separate marsquakes from meteorology. Continuous weather observations to keep it honest are revealing new facets of Mars’s churning atmosphere.
- Nicholas Heavens
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Comment |
Rebirth of extraterrestrial seismology
The InSight mission on Mars is currently providing us with the first seismic data from a planetary body other than our own Earth since the 1970s. Past efforts will inform this next chapter in planetary seismology.
- Yosio Nakamura
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Perspective |
Initial results from the InSight mission on Mars
Geophysical and meteorological measurements by NASA’s InSight lander on Mars reveal a planet that is seismically active and provide information about the interior, surface and atmospheric workings of Mars.
- W. Bruce Banerdt
- , Suzanne E. Smrekar
- & Mark Wieczorek
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Article |
Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data
The crust beneath the InSight lander on Mars is altered or fractured to 8–11 km depth and may bear volatiles, according to an analysis of seismic noise and wave scattering recorded by InSight’s seismometer.
- P. Lognonné
- , W. B. Banerdt
- & P. Zweifel
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Crustal and time-varying magnetic fields at the InSight landing site on Mars
The magnetic field measured by the InSight lander on Mars varies daily and is ten times stronger than expected. The field is inferred to originate from components of basement rocks magnetized by an ancient dynamo of Earth-like strength.
- Catherine L. Johnson
- , Anna Mittelholz
- & William B. Banerdt
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The seismicity of Mars
Mars is seismically active: 24 subcrustal magnitude 3–4 marsquakes and 150 smaller events have been identified up to 30 September 2019, by an analysis of seismometer data from the InSight lander.
- D. Giardini
- , P. Lognonné
- & C. Yana
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The atmosphere of Mars as observed by InSight
The InSight lander has expanded our knowledge of the atmosphere of Mars by observing various phenomena, including airglow, bores, infrasound and Earth-like turbulence.
- Don Banfield
- , Aymeric Spiga
- & W. Bruce Banerdt
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A thick crustal block revealed by reconstructions of early Mars highlands
A discrete block of thick ancient crust revealed by a crustal reconstruction suggests a complex geologic history for the southern highlands of Mars.
- Sylvain Bouley
- , James Tuttle Keane
- & Brigitte Zanda
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Matters Arising |
Reply to: Penitente formation is unlikely on Europa
- Daniel E. J. Hobley
- , Jeffrey M. Moore
- & Orkan M. Umurhan
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Article |
A tenfold slowdown in river meander migration driven by plant life
River meanders migrate much faster in barren than in vegetated landscapes, according to global analyses of active meander migration of both unvegetated and vegetated rivers. The difference in migration rates suggests that the rise of land plants had a significant influence on landscapes.
- Alessandro Ielpi
- & Mathieu G. A. Lapôtre
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An interval of high salinity in ancient Gale crater lake on Mars
Brines from evaporation of a lake in Gale crater on Mars are inferred from bulk enrichments of Ca- and Mg-sulfates in Hesperian sedimentary rocks, identified by geochemical analyses and observations by NASA’s rover Curiosity.
- W. Rapin
- , B. L. Ehlmann
- & A. R. Vasavada
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Editorial |
The familiarity of icy worlds
The geological similarities between icy and rocky worlds invite comparison and cross-fertilization of knowledge.
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News & Views |
Building mountains on Ceres
The large domes found on the dwarf planet Ceres may not result from cryovolcanism, but from solid-state flow analogous to salt doming on Earth, according to numerical simulations of gravitational loading.
- Michael Küppers
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Article |
Dome formation on Ceres by solid-state flow analogous to terrestrial salt tectonics
Domes on the dwarf planet Ceres could form by solid-state flow of low-density, ice-rich parts of its crust—a process analogous to salt doming on Earth—according to numerical simulations.
- M. T. Bland
- , D. L. Buczkowski
- & C. T. Russell
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Sharp 660-km discontinuity controlled by extremely narrow binary post-spinel transition
The post-spinel transition in mantle composition, which occurs at 660-km depth in Earth’s mantle, takes place over a pressure range equivalent to 250 m in depth, according to multi-anvil experiments for realistic mantle compositions and temperatures.
- Takayuki Ishii
- , Rong Huang
- & Tomoo Katsura
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Possible explosion crater origin of small lake basins with raised rims on Titan
Some lake basins in the polar regions of Titan may be craters from nitrogen vapour explosions due to past warming, according to analysis of their morphology in comparison to terrestrial explosion craters from magma–water interaction.
- Giuseppe Mitri
- , Jonathan I. Lunine
- & Valerio Poggiali
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Tin isotopes indicative of liquid–vapour equilibration and separation in the Moon-forming disk
Vigorous mixing between the protolunar disk and Earth followed by processes in the cooling disk may explain the enrichment in light isotopes of tin on the Moon relative to Earth, as found by analysis of lunar rocks and geochemical calculations.
- Xueying Wang
- , Caroline Fitoussi
- & Sébastien Charnoz
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News & Views |
A silicon memory of subduction
Subduction processes may have operated very early in Earth’s history according to the heavy silicon isotope compositions of Archaean igneous rocks. The silicon that precipitated out of the Archaean oceans as chert was subducted and melted to yield seawater-like heavy isotope signatures in early granitic rocks.
- Franck Poitrasson
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Article |
Early continental crust generated by reworking of basalts variably silicified by seawater
Granitic continental crust in the Archaean formed from a basaltic source that was enriched in silica due to interaction with the early oceans before melting, according to silicon isotope analyses on rocks from the Kaapvaal craton.
- Luc André
- , Kathrin Abraham
- & Stephen Foley
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News & Views |
The Earth–Moon late-accretion conundrum
The distribution of iron-loving elements between the mantles of the Moon and Earth may differ from established belief, suggest two studies that determine the hafnium–tungsten ratio and sulfide–silicate melt partitioning of elements in the lunar mantle.
- Philipp Gleißner
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Article |
Abundance of highly siderophile elements in lunar basalts controlled by iron sulfide melt
The abundance of iron-loving elements in Moon rocks cannot indicate the amount of late accretion onto the Moon, according to experiments and thermodynamic calculations constraining the behaviour of these elements under lunar mantle conditions.
- James M. Brenan
- , James E. Mungall
- & Neil R. Bennett
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Selenium isotopes as tracers of a late volatile contribution to Earth from the outer Solar System
Material that accreted to Earth after its core formed largely comprised carbonaceous, volatile-rich meteorites, according to analysis of the selenium isotopic composition of terrestrial mantle rocks.
- María Isabel Varas-Reus
- , Stephan König
- & Ronny Schoenberg
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Early Moon formation inferred from hafnium–tungsten systematics
The Moon formed around 50 Myr after the Solar System, suggests a lunar silicate Hf/W ratio higher than that of Earth, from high-precision compositional analysis of lunar rock samples.
- Maxwell M. Thiemens
- , Peter Sprung
- & Carsten Münker
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Arc magmas oxidized by water dissociation and hydrogen incorporation in orthopyroxene
Oxidation of arc magmas may be a secondary feature, acquired as hydrogen from magmatic water is incorporated into anhydrous minerals in the mantle wedge, according to analyses of orthopyroxenes in mantle xenoliths from an arc setting.
- Peter Tollan
- & Jörg Hermann
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Thick ice deposits in shallow simple craters on the Moon and Mercury
Ice deposits up to around 50 m thick infill some craters near the Moon’s south pole and Mercury’s north pole, as inferred from the poleward shallowing of simple craters.
- Lior Rubanenko
- , Jaahnavee Venkatraman
- & David A. Paige
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News & Views |
Plateaus from seafloor spreading
Ocean-floor plateaus are not voluminous lava flows from central volcanoes as thought, but anomalously thick oceanic crust, suggest magnetic anomaly patterns from the Shatsky Rise, in the northwestern Pacific Ocean.
- Joanne M. Whittaker
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