Experimental weathering of rocks and minerals at Venus conditions in the Glenn Extreme Environments Rig (GEER)
AR Santos, MS Gilmore, JP Greenwood… - Journal of …, 2023 - Wiley Online Library
We report two experiments using 13 mineral and rock samples exposed to a complex
synthetic Venus atmosphere composed of nine gases for durations of 30 and 11 days …
synthetic Venus atmosphere composed of nine gases for durations of 30 and 11 days …
Exploring Venus: Next generation missions beyond those currently planned
SS Limaye, JB Garvin - Frontiers in Astronomy and Space Sciences, 2023 - frontiersin.org
As of mid-2023 at least ten missions are in development or being planned to explore Venus
in the next 2 decades. Most of these emphasize atmospheric chemistry and surface/interior …
in the next 2 decades. Most of these emphasize atmospheric chemistry and surface/interior …
[HTML][HTML] Geological history of Theia Mons, Beta Regio plume, Venus: Recognition of two main magmatic centers for flows, radiating dyke swarms and triple junction …
AS Shimolina, RE Ernst, H El Bilali… - Planetary and Space …, 2025 - Elsevier
ABSTRACT Theia Mons (centered at 23.4 º N, 79.4 º W) is the main volcanic center for the
Beta Regio plume, of the Beta-Atla-Themis (BAT) region, Venus. Synthetic aperture radar …
Beta Regio plume, of the Beta-Atla-Themis (BAT) region, Venus. Synthetic aperture radar …
Estimated seismicity of Venusian wrinkle ridges based on fault scaling relationships
L Sabbeth, SE Smrekar, JM Stock - Earth and Planetary Science Letters, 2023 - Elsevier
Venus' young surface age implies significant geologic activity. Several lines of evidence
suggest current volcanism, but there is no data to directly constrain current tectonism …
suggest current volcanism, but there is no data to directly constrain current tectonism …
Ground-assisted position navigation and timing (pnt) for moon and mars
KM Cheung, WW Jun, S Bhamidipati… - 2024 IEEE Aerospace …, 2024 - ieeexplore.ieee.org
The recent exploration initiatives for robotic and human missions to the Moon and Mars
require long-term communications and navigation infrastructures that provide accurate and …
require long-term communications and navigation infrastructures that provide accurate and …
Constraints on the effusive volcanic eruptions that formed Kallistos Vallis, Venus
DA Berman, DW Leverington - Geomorphology, 2023 - Elsevier
Abstract Kallistos Vallis is a Venusian channel system that extends> 1200 km downslope
from a source region marked by a graben-like feature and chaotic terrain, terminating at …
from a source region marked by a graben-like feature and chaotic terrain, terminating at …
The VenSpec-U spectrometer onboard EnVision: sensitivity studies
L Conan, E Marcq, B Lustrement… - Infrared Remote …, 2024 - spiedigitallibrary.org
The dual-channel UV spectrometer VenSpec-U onboard ESA's next mission to Venus,
EnVision, will study the upper layer of the atmosphere located above the clouds. It aims to …
EnVision, will study the upper layer of the atmosphere located above the clouds. It aims to …
Venus Interferometric Synthetic Aperture Radar Instrument Performance and Options
The Venus Interferometric Synthetic Aperture Radar (VISAR) is one of two instruments
carried by the VERITAS Discovery Mission to Venus that was selected by NASA in 2021 …
carried by the VERITAS Discovery Mission to Venus that was selected by NASA in 2021 …
[引用][C] Detailed Mapping of Large Shield Volcanoes on Venus-Challenges and Perspectives Based on the Study OF Atira Mons, Bat Region, Venus
CHG Braga, RE Ernst, H El Bilali, JW Head… - The Thirteenth Moscow …, 2022 - elibrary.ru