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| Open AccessVolcanic Island lightning prebiotic chemistry and the origin of life in the early Hadean eon
The early Hadean eon (>4Ga) may have had a periodically ice-covered global ocean and limited subaerial landmass, and this could have resulted in infrequent lightning occurrence. This infrequency of lightning may have limited the synthesis of prebiotic compounds necessary for life’s origins. Here I present a hypothesis that lightning associated with volcanic island eruptions created focal points for the generation of prebiotic ingredients and ultimately the origin of life.
- Jeffrey L. Bada
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Article
| Open AccessIncreased warm water intrusions could cause mass loss in East Antarctica during the next 200 years
The East Antarctic Ice Sheet is currently surrounded by relatively cool water but changes in ocean dynamics may lead to warmer ocean water on the shelf in the future. This has the potential to dramatically increase its future sea level contribution.
- James R. Jordan
- , B. W. J. Miles
- & C. R. Stokes
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Article
| Open AccessWidespread detection of chlorine oxyacids in the Arctic atmosphere
Observations are reported of HClO3 and HClO4 in the atmosphere and their widespread occurrence over the pan-Arctic during spring, providing further insights into atmospheric chlorine cycling in the polar environment.
- Yee Jun Tham
- , Nina Sarnela
- & Alfonso Saiz-Lopez
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Article
| Open AccessUracil in the carbonaceous asteroid (162173) Ryugu
Uracil was identified in the sample returned from the asteroid Ryugu. Having been provided to the early Earth as a component in such asteroidal materials, these molecules might have played a role for prebiotic chemical evolution on the early Earth
- Yasuhiro Oba
- , Toshiki Koga
- & Yuichi Tsuda
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Article
| Open AccessInsights into the formation and evolution of extraterrestrial amino acids from the asteroid Ryugu
Amino acid concentrations from 2 particles returned from different touchdown sites on the surface of Ryugu are reported. Differences in chemistry suggest different levels of aqueous alteration are recorded at the 2 sampled locations.
- Christian Potiszil
- , Tsutomu Ota
- & Eizo Nakamura
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Article
| Open AccessGenesis of Hawaiian lavas by crystallization of picritic magma in the deep mantle
Here the authors demonstrate that Hawaiian lavas are formed by partial melting of mantle peridotite with subsequent fractionation of clinopyroxene and garnet in the deep magma chamber (90 km) and reequilibration with harzburgite at a shallower depth (<60 km).
- Junlong Yang
- , Chao Wang
- & Zhenmin Jin
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Article
| Open AccessClimate-driven tradeoffs between landscape connectivity and the maintenance of the coastal carbon sink
Coastal connectivity between ecosystems increases with sea level rise but fails to maintain landscape carbon storage and marsh extent at extreme rates of sea level rise.
- Kendall Valentine
- , Ellen R. Herbert
- & Matthew L. Kirwan
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Comment
| Open AccessPlanetary defense with the Double Asteroid Redirection Test (DART) mission and prospects
NASA’s Double Asteroid Redirection Test (DART) mission intentionally impacted the asteroid Dimorphos on September 26, 2022, and this kinetic impact changed Dimorphos’ orbit around its binary companion Didymos. This first planetary defense test explored technological readiness for this method of asteroid deflection.
- Andrew S. Rivkin
- & Andrew F. Cheng
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Article
| Open AccessUntrackable distal ejecta on planetary surfaces
Heterogeneous shock impedances of planetary materials cause abrupt changes of ejection angles, forming non-radial ejecta. Interpretations for provenances of surface deposits and ages derived from crater counts are affected by such untrackable ejecta.
- Rui Xu
- , Zhiyong Xiao
- & Jun Cui
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Article
| Open AccessMagnesium oxide-water compounds at megabar pressure and implications on planetary interiors
Magnesium Oxide and water are abundant in the interior of planets. Here, the authors predict three new MgO-H2O compounds: Mg2O3H2, MgO3H4 and MgO4H6, and they exhibit superionic behavior in planetary interior conditions.
- Shuning Pan
- , Tianheng Huang
- & Jian Sun
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Article
| Open AccessThermodynamics of diamond formation from hydrocarbon mixtures in planets
This study combines computational chemistry and machine learning to provide insight on whether diamonds can form inside ice giants. This can help explain the dichotomy of Uranus and Neptune.
- Bingqing Cheng
- , Sebastien Hamel
- & Mandy Bethkenhagen
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Comment
| Open AccessLife on Mars, can we detect it?
Searching for evidence of life on Mars is a major impetus for exploration. A new study published in Nature Communications finds that current Mars mission instruments lack the essential sensitivity to identify life traces in Chilean desert samples that strongly resemble the martian area currently under study by NASA’s Perseverance rover.
- Carol R. Stoker
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Article
| Open AccessDark microbiome and extremely low organics in Atacama fossil delta unveil Mars life detection limits
Unique microorganisms of a fossil river delta in the Atacama Desert unveil the current limits of life detection on Mars.
- Armando Azua-Bustos
- , Alberto G. Fairén
- & Elizabeth Rampe
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Article
| Open AccessChondrule-like objects and Ca-Al-rich inclusions in Ryugu may potentially be the oldest Solar System materials
Chondrule-like objects and CAIs in the Ryugu samples are early generations of chondrules and possibly oldest solids in the Solar System. They were transported from the inner solar nebula to the formation location of the Ryugu original parent body.
- Daisuke Nakashima
- , Tomoki Nakamura
- & Yuichi Tsuda
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Article
| Open AccessEvidence for a rosiaite-structured high-pressure silica phase and its relation to lamellar amorphization in quartz
Rapid compression experiments on quartz provide evidence for a metastable high-pressure phase with rosiaite structure. The phase forms as lamellae and breaks down to glass during decompression. These discoveries may solve the enigma of lamellar amorphization of quartz during impact events.
- Christoph Otzen
- , Hanns-Peter Liermann
- & Falko Langenhorst
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Article
| Open AccessUnveiling the spectrum of electrohydrodynamic turbulence in dust storms
Electrohydrodynamic features of dust storm turbulence have puzzled scientists for over a hundred years. Here, the authors reveal the characteristics of the multifield spectra in dust storms using a combined observational and theoretical approach.
- Huan Zhang
- & You-He Zhou
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Article
| Open AccessThe rocky road to organics needs drying
How complex organics form in a prebiotic world remains a missing key to establish where life emerged. The authors present a road to abiotic organic synthesis and diversification in hydrothermal contexts involving magmatism and rock hydration.
- Muriel Andreani
- , Gilles Montagnac
- & Bénédicte Ménez
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Article
| Open AccessConstraints on the martian crust away from the InSight landing site
The authors show that the Martian crust, ~4300 km from the InSight landing site, has a subsurface interface similar to that beneath the lander, suggesting it is a regional or global feature that may be related to the closure of pore spaces at depth.
- Jiaqi Li
- , Caroline Beghein
- & W. Bruce Banerdt
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Article
| Open AccessBepiColombo mission confirms stagnation region of Venus and reveals its large extent
BepiColombo mission had two Venus flybys on its way to Mercury. Here, the authors show that during its second flyby of Venus BepiColombo has crossed the stagnation region, which was predicted by the models.
- M. Persson
- , S. Aizawa
- & G. Murakami
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Article
| Open AccessThe sound of a Martian dust devil
Dust devils are common on Mars and understanding their dynamics is important to gain insights about the meteorology of the planet. Here, the authors show characteristics of a Martian dust devil and its sound from Perseverance rover multi-sensor data combined with modelling.
- N. Murdoch
- , A. E. Stott
- & D. Mimoun
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Article
| Open AccessPotassium isotope heterogeneity in the early Solar System controlled by extensive evaporation and partial recondensation
This study reports strikingly light K isotopic compositions for the extremely K-depleted angrite meteorites, thereby providing the first observation of isotope fractionation likely controlled by partial recondensation at a planetary scale.
- Yan Hu
- , Frédéric Moynier
- & Martin Bizzarro
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Article
| Open AccessVenus’ light slab hinders its development of planetary-scale subduction
The simulation of slab buoyancy in 2-D models shows that Venus’ light slabs, due to a less eclogitized crust, experience more resistance to subduction. Thus, plate tectonics might have been more difficult to develop on Venus than on Earth.
- Junxing Chen
- , Hehe Jiang
- & Xu Chu
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Article
| Open AccessA changing thermal regime revealed from shallow to deep basalt source melting in the Moon
Ancient (~3.9 Ga) KREEP-free basalts were sourced from a relatively cool and shallow pyroxene-rich mantle distinct from later-erupted (<3.8 Ga) KREEP-bearing basalts, indicating a fundamental change in melting regimes in the Moon.
- Yash Srivastava
- , Amit Basu Sarbadhikari
- & Atsushi Takenouchi
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| Open AccessInsights into magma ocean dynamics from the transport properties of basaltic melt
The viscosity of magma plays a crucial role in the dynamics of planet Earth. In this study, the authors show how transport properties of basaltic melt can give us insights into magma ocean dynamics.
- Suraj K. Bajgain
- , Aaron Wolfgang Ashley
- & Bijaya B. Karki
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Article
| Open AccessRossby wave second harmonic generation observed in the middle atmosphere
Rossby waves occur in rotating fluids. Here, the authors show observation of a Rossby wave second harmonic generation event in the middle atmosphere and confirm theoretically anticipated Rossby wave nonlinearity.
- Maosheng He
- & Jeffrey M. Forbes
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Article
| Open AccessLiquid water on cold exo-Earths via basal melting of ice sheets
Liquid water is key for life as we know it. Here, the authors show even with a modest geothermal heat flow, subglacial oceans of liquid water can form at the base of and within the ice sheets on exo-Earths, which may provide habitable conditions for an extended period.
- Lujendra Ojha
- , Bryce Troncone
- & George McDonald
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Article
| Open AccessConstraining surface properties of asteroid (162173) Ryugu from numerical simulations of Hayabusa2 mission impact experiment
Hayabusa2 mission impact experiment on asteroid Ryugu formed a crater larger than expected. Here, the authors show numerical impact simulations and find that the target cohesion may be very low, indicating the Hayabusa2 impact experiment probably occurred in the transitional cratering regime.
- Martin Jutzi
- , Sabina D. Raducan
- & Masahiko Arakawa
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Article
| Open AccessInner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission
BepiColombo mission had already two flybys of Mercury, over the total of six, as planned before entering the planet’s orbit in 2025. Here, the authors show the first ion measurements of Mercury’s inner southern magnetosphere during BepiColombo mission’s first Mercury flyby.
- S. Orsini
- , A. Milillo
- & A. Vorburger
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Article
| Open AccessSub-microscopic magnetite and metallic iron particles formed by eutectic reaction in Chang’E-5 lunar soil
Magnetite is rarely present on the Moon. Here the authors report the magnetite formed by eutectic reaction during the impact process in Chang’E-5 lunar soil, and the potential contribution of this magnetite formation to magnetic anomalies on the Moon.
- Zhuang Guo
- , Chen Li
- & Ziyuan Ouyang
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Article
| Open AccessA distinct ripple-formation regime on Mars revealed by the morphometrics of barchan dunes
Dust storms on Mars drive water escape to space. Here, the authors show the impact Martian dust storms have on the abundance of atmospheric hydrogen and oxygen, and how this helps to overall oxidize the Martian atmosphere.
- Lior Rubanenko
- , Mathieu G. A. Lapôtre
- & Andrew Gunn
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Article
| Open AccessUnraveling sulfur chemistry in interstellar carbon oxide ices
The authors report photolytic H atom transfer reactions of HOSO• in astronomical CO & CO2 ices, forming reactive acyl radicals & molecular complexes with SO & SO2. Connecting the photochemistry of S oxides & C oxides in cold molecular clouds in the interstellar medium.
- Xiaolong Li
- , Bo Lu
- & Xiaoqing Zeng
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Article
| Open AccessEconomy-wide evaluation of CO2 and air quality impacts of electrification in the United States
Electrification is a decarbonization strategy that has the potential to reduce pollutant emissions and improve air quality. Here the authors evaluate CO2 and air quality co-benefits of electrification scenarios in the United States and find that electrification can substantially lower CO2 and improve ozone and fine particulate matter regionally.
- John E. T. Bistline
- , Geoffrey Blanford
- & Greg Yarwood
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Article
| Open AccessAlternate oscillations of Martian hydrogen and oxygen upper atmospheres during a major dust storm
Dust storms on Mars drive water escape to space. Here, the authors show the impact Martian dust storms have on the abundance of atmospheric hydrogen and oxygen, and how this helps to overall oxidize the Martian atmosphere.
- Kei Masunaga
- , Naoki Terada
- & Ichiro Yoshikawa
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Article
| Open AccessVolcanically hosted venting with indications of ultramafic influence at Aurora hydrothermal field on Gakkel Ridge
The Aurora hydrothermal field (Arctic Ocean) is hosted in volcanic rocks but also shows evidence of mantle rock influence in the shallow sub-surface. Our discovery is pertinent to disciplines from marine mining to the search for life beyond Earth.
- Christopher R. German
- , Eoghan P. Reeves
- & Antje Boetius
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Article
| Open AccessEthylene industrial emitters seen from space
Combining 13 years of satellite measurements led to the discovery of 300 global hotspots of atmospheric ethylene (C2H4). They are found to be linked to heavy industries and megacities, and are currently misrepresented in emission inventories.
- Bruno Franco
- , Lieven Clarisse
- & Pierre-François Coheur
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Article
| Open AccessSpectral interpretation of late-stage mare basalt mineralogy unveiled by Chang’E-5 samples
Laboratory spectroscopic and X-ray diffraction analyses on the Chang’E-5 lunar soil samples have demonstrated that the spectral features of lunar late-stage mare basalts are representative of iron-rich high-Ca pyroxene rather than olivine.
- Dawei Liu
- , Xing Wang
- & Chunlai Li
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Article
| Open AccessLow 13C-13C abundances in abiotic ethane
Distinguishing biotic compounds from abiotic ones is critical to the search for life in the universe. Here, the authors demonstrate that the abiotic ethane has distinctively low 13C-13C abundances compared to biotic ethane.
- Koudai Taguchi
- , Alexis Gilbert
- & Yuichiro Ueno
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Article
| Open AccessUsing MARSIS signal attenuation to assess the presence of South Polar Layered Deposit subglacial brines
MARSIS attenuation and thermal data confirm that liquid brines are the most plausible source for the bright reflections at the base of the South Polar Layered Deposits. Such results also justify why SHARAD does not penetrate to the base of the ice.
- Sebastian E. Lauro
- , Elena Pettinelli
- & Roberto Orosei
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Article
| Open AccessChang’E-5 samples reveal high water content in lunar minerals
Lunar soils returned by China’s Chang’E−5 (CE5) mission record the unique information of solar wind essential to understanding the preservation and distribution of lunar surficial water. Here the authors report abundant water formed by solar wind implantation in minerals of CE5 lunar soils; the water content in CE5 lunar soils is estimated to be ~ 170 ppm.
- Chuanjiao Zhou
- , Hong Tang
- & Yuanyun Wen
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Article
| Open AccessMarine phosphate availability and the chemical origins of life on Earth
Phosphate is critical for all life on Earth but its origins have remained enigmatic. Experiments indicate that phosphate may have been abundant in ancient Fe-rich seawater, providing a crucial ingredient for the origins of life on Earth.
- Matthew P. Brady
- , Rosalie Tostevin
- & Nicholas J. Tosca
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Article
| Open AccessJuno spacecraft gravity measurements provide evidence for normal modes of Jupiter
Juno spacecraft experienced unknown accelerations near the closest approach to Jupiter. Here, the authors show that Jupiter’s axially symmetric, north-south asymmetric gravity field measured by Juno is perturbed by a time-variable component, associated to internal oscillations.
- Daniele Durante
- , Tristan Guillot
- & Scott J. Bolton
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Article
| Open AccessGeoelectrochemistry-driven alteration of amino acids to derivative organics in carbonaceous chondrite parent bodies
Researchers at Earth-Life Science Institute (ELSI) discovered a chemical process that can explain the very low amino acid abundances in aqueously altered carbonaceous chondrites, deepening our understanding on the Solar System chemical evolution.
- Yamei Li
- , Norio Kitadai
- & Kristin Johnson-Finn
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Article
| Open AccessWidespread impact-generated porosity in early planetary crusts
Large impacts can create deep lying porosity far away from the crater. This result explains GRAIL’s findings and suggests impacts could support widespread fluid circulation, which has implications for habitable environments on early Earth and Mars.
- Sean E. Wiggins
- , Brandon C. Johnson
- & Simone Marchi
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Article
| Open AccessNitrogen isotope evidence for Earth’s heterogeneous accretion of volatiles
How and when Earth acquired its major volatiles N-C-H-S remains unclear. Here the authors show that Earth may have acquired its major volatiles from both reduced and oxidized impactors before and during the Moon-forming giant impact.
- Lanlan Shi
- , Wenhua Lu
- & Yuan Li
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Article
| Open AccessEndogenically sourced volatiles on Charon and other Kuiper belt objects
We show cryovolcanic eruptions released sufficient methane to source volatile products on Charon. Irradiated methane products are found on other Kuiper belt objects, so endogenically sourced volatiles could be important across the Kuiper belt.
- Stephanie M. Menten
- , Michael M. Sori
- & Ali M. Bramson
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Article
| Open AccessInferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu
Asteroid interiors are key to understand their formation and evolution. Here, the authors show that numerically simulated low-cohesion and low-friction structures with several high-cohesion internal zones can explain asteroid Bennu’s geophysical characteristics and the absence of the moons.
- Yun Zhang
- , Patrick Michel
- & Dante S. Lauretta
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Article
| Open AccessPhotochemical and thermochemical pathways to S2 and polysulfur formation in the atmosphere of Venus
Polysulfur compounds have been ascribed as the unknown near-UV absorbers in Venusian atmosphere and play a key role in the sulfur chemical cycle of this planet. Here, authors establish their production from (SO)2 on the grounds of quantifications of photochemical and thermal pathways involved in the sulfur chemical cycle of the planet.
- Antonio Francés-Monerris
- , Javier Carmona-García
- & Daniel Roca-Sanjuán
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Article
| Open AccessInverse altitude effect disputes the theoretical foundation of stable isotope paleoaltimetry
The “inverse altitude effect” (IEA) directly contradicts the basic theory of stable isotope paleoaltimetry. This study explores the causes of the IAE from an atmospheric circulation perspective using δD in water vapor on the global scale.
- Zhaowei Jing
- , Wusheng Yu
- & Rong Guo
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Article
| Open AccessEarly crustal processes revealed by the ejection site of the oldest martian meteorite
A new study pinpoints the ejection site of the 4.5-Ga-old Martian breccia NWA 7034 and paired stones to an area northeast of the Terra 679 Cimmeria–Sirenium province.
- A. Lagain
- , S. Bouley
- & P. A. Bland
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