geology Archives - Page 19 of 34 - Astrobiology

ID: ESP_042572_2640 date: 26 August 2015 altitude: 318 km Larger image -- NASA/JPL-Caltech/University of Arizona

Analog Studies, Arctic / Antarctic / Alpine, Astrogeology, Icy Worlds, Imaging & Spectroscopy, Mapping, Geodesy, Cartography, Bathymetry, Mars, Status Report

Orbital View Of A Polar Avalanche On Mars

by Keith CowingOctober 20, 2024

This scarp at the edge of the North Polar layered deposits of Mars is the site of the most frequent frost avalanches seen by HiRISE.

The plume from Hunga Tonga-Hunga Ha‘apai behaved like a mega-thunderstorm that rose 58 kilometers (38 miles) into the atmosphere. NASA Earth Observatory images and video by Joshua Stevens, using data courtesy of Kristopher Bedka and Konstantin Khlopenkov/NASA Langley Research Center, and GOES-17 imagery courtesy of NOAA and the National Environmental Satellite, Data, and Information Service (NESDIS). Story by Sofie Bates, NASA’s Earth Science News Team, with Mike Carlowicz. Larger image

Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Caves, Craters, Mountains, Subsurface, Lava Tubes, Extinction events, Gaia - Planetary Perspectives, Habitable Zones, Imaging & Spectroscopy, Impact events, Lava / magma ocean / Volcanic Worlds, Status Report, Terraforming & Geoengineering, Water/Hycean Worlds & Oceanography

X-Raying Neutral Density Disturbances in the Mesosphere and Lower Thermosphere induced by the 2022 Hunga-Tonga Volcano Eruption-Explosion

by Keith CowingOctober 16, 2024October 16, 2024

We present X-ray observations of the upper atmospheric density disturbance caused by the explosive eruption of the Hunga Tonga-Hunga Ha’apai (HTHH) volcano on 15 January 2022.

Panel A: crust age and thickness for 15 different zones of Loki Patera. Panel B: location of the zones chosen for the analysis. The color of the zones is coded according to the age of the crust, as indicated by the color bar to the right. The reference time for the crust age is set to the final observation epoch: April 9, 2024. -- astro-ph.EP

Astrogeology, Atmospheres, Climate, Weather, Imaging & Spectroscopy, Io, Jupiter, Lava / magma ocean / Volcanic Worlds, Mapping, Geodesy, Cartography, Bathymetry, Missions & Hardware, Status Report

Volcano World Survey: Observations Of Loki Patera By Juno During Close Flybys

by Keith CowingOctober 15, 2024October 15, 2024

We used data from the Juno spacecraft to investigate both the spatial and temporal properties of Loki Patera on Io, acquired in two infrared bands between December 2022 and April […]

Nanoscale molecular information of the CCM. (A) TOF-SIMS mapping showing association of C-H (purple) and CN (blue) in CCM -- PNAS

Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Biophysics, Biosignatures & Paleobiology, Origin & Evolution of Life, Status Report

Unraveling Abiotic Organic Synthesis Pathways In The Mafic Crust Of Mid-ocean Ridges

by Keith CowingOctober 14, 2024October 14, 2024

The aqueous alteration of the oceanic lithosphere provides significant energy that impacts the synthesis and diversity of organic compounds, which are crucial for the deep carbon cycle and may have […]

Overview of our models for gas disk and particles evolution in different disk regions. The blue and yellow particles represent silicates with and without refractory carbon. The light blue particles represent icy pebbles. The pink particles show the oxygen atoms which are formed by the destruction of oxygen molecules because of the FUV radiation which is described as red arrows. The light blue dashed line is the snow line. Icy pebbles enclosing many small silicates drift to the snow line (blue dashed line) from the outer region. Orange upper and lower layers are FUV-exposed regions, where oxygen atoms exist. -- astro-ph.EP

Astrochemistry, Astrogeology, Biochemistry & Organic Chemistry, Biosignatures & Paleobiology, Habitable Zones, Imaging & Spectroscopy, Interstellar, Status Report

Effect of Different Stickiness Between Icy and Silicate Particles on Carbon Depletion in Protoplanetary Disks

by Keith CowingOctober 12, 2024October 12, 2024

Earth and other rocky bodies in the inner Solar System are significantly depleted in carbon compared to the Sun and interstellar medium (ISM) dust.

Cryptic terrain in Australe Scopuli on Mars (Larger image) -- ESA

Astrogeology, Icy Worlds, Imaging & Spectroscopy, Mapping, Geodesy, Cartography, Bathymetry, Mars, Press Release

Mars Is A World Shaped By Ice

by Keith CowingOctober 9, 2024October 9, 2024

ESA’s Mars Express has captured an astonishing array of landforms emerging from a thick winter blanket of frost as spring arrives in the south polar region of Mars. Some of […]

This picture shows many tiny cells in which DNA is abundantly included inside the cells. First, the microbial cells were detected in fractures in the rock sample using an infrared imaging technique called O-PTIR spectroscopy. After that, they were stained with a green solution and analyzed using both a scanning electron microscope and then fluorescent microscopy. The combination of readings from these three imaging techniques enabled the researchers to confirm the indigenous and living microbial cells in the 2-billion-year-old rock fissure. -- University of Tokyo

Astrogeology, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Caves, Craters, Mountains, Subsurface, Lava Tubes, Fossils & Paleontology, Imaging & Spectroscopy, Microbiology & Virology, Press Release

A 2-billion-year-old Rock Is Home To Living Microbes

by Keith CowingOctober 4, 2024October 4, 2024

Pockets of microbes have been found living within a sealed fracture in 2-billion-year-old rock. The rock was excavated from the Bushveld Igneous Complex in South Africa, an area known for […]

This simulation was run in a uniformly 90% ice crust (Fig. 1a) at the equator and shows total vertical displacement after 1 Gyr of relaxation. The black lines are the initial state of the simulation, and the solid colour shows the final state of the simulation. In this case, the crater has only shallowed by ~70 m from an initial depth of 2,400 m (seen as the solid colour at the centre of the crater slightly offset from the black line), for a relaxation percentage of

Astrogeology, Biogeochemical Cycles & Geobiology, Caves, Craters, Mountains, Subsurface, Lava Tubes, Ceres, Comets and Asteroids, Cryobiology, Icy Worlds, Imaging & Spectroscopy, Impact events, Status Report, Water/Hycean Worlds & Oceanography

An Ancient And Impure Frozen Ocean On Ceres Implied By Its Ice-rich Crust

by Keith CowingSeptember 30, 2024September 29, 2024

Ceres is a key object in understanding the evolution of small bodies and is the only dwarf planet to have been orbited by a spacecraft, NASA’s Dawn mission.

Sampling site PE01 from Cueva Paso Esqueleto (PE) -- Nature

Analog Studies, Astrogeology, Away Teams & Field Reports, Biochemistry & Organic Chemistry, Biosignatures & Paleobiology, Caves, Craters, Mountains, Subsurface, Lava Tubes, Exploration Gear & Tech, Fossils & Paleontology, Habitable Zones, Imaging & Spectroscopy, Mapping, Geodesy, Cartography, Bathymetry, Mars, Microbiology & Virology, Status Report

Decoding Organic Compounds In Lava Tube Sulfates To Understand Potential Biomarkers In The Martian Subsurface

by Keith CowingSeptember 30, 2024September 29, 2024

Exploring molecular biomarkers in lava tube speleothems offers insights into environmental dynamics, biogeochemical processes, and subsurface life, with implications for astrobiology, particularly in Martian analog environments.

a–c Raman measurement of the HV wall near a fluid channel. a Overlay of the Raman map with the corresponding SEM image. The Raman map is a superimposed image of three specific peaks. The Raman map shows that the brucite and Mg-carbonate crystals are discretely located in the wall, while carbonate ions were present in all regions, indicating the adsorption of carbonate ions by the brucite. b Raman spectra of surface crystals (blue) and HV wall (red) at the positions shown in (a, c). c Map of three specific Raman peaks, red: 442.6 cm−1 (brucite lattice vibration, A1g, width 47.5 cm−1), blue: 1109.7 cm−1 (carbonate, width 73.4 cm−1), and green: 3420.7 cm−1 (interlayered water, width 98.8 cm−1). The corresponding peaks are shown in the spectra in (b). -- Nature Communications

Analog Studies, Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Biophysics, Biosignatures & Paleobiology, Caves, Craters, Mountains, Subsurface, Lava Tubes, Exploration Gear & Tech, Extremeophiles and Extreme Environments, Fossils & Paleontology, Imaging & Spectroscopy, Mapping, Geodesy, Cartography, Bathymetry, Microbiology & Virology, Nanotechnology & SynBio, Origin & Evolution of Life, Press Release, ROVs/Submersibles/Diving

Nanostructures In The Deep Ocean Floor Hint At Life’s Origin

by Keith CowingSeptember 27, 2024September 27, 2024

Researchers led by Ryuhei Nakamura at the RIKEN Center for Sustainable Resource Science (CSRS) in Japan and The Earth-Life Science Institute (ELSI) of Tokyo Institute of Technology have discovered inorganic […]