THERMAL ESCAPE FROM SUPER EARTH ATMOSPHERES IN THE HABITABLE ZONES OF M STARS by Tian, Feng

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Observing Atmospheric Escape in Sub-Jovian Worlds with JWST by Leonardo A. Dos Santos, Munazza K. Alam, Néstor Espinoza, Shreyas Vissapragada

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The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System

“…In contrast to some other low-mass stars that host Earth-sized planets in their habitable zones, TOI-700 exhibits low levels of stellar activity, presenting a valuable opportunity to study potentially rocky planets over a wide range of conditions affecting atmospheric escape. …”
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The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System by Burke, Christopher J., Daylan, Tansu, Ricker, George R, Vanderspek, Roland K, Seager, Sara, Essack, Zahra

“…In contrast to some other low-mass stars that host Earth-sized planets in their habitable zones, TOI-700 exhibits low levels of stellar activity, presenting a valuable opportunity to study potentially rocky planets over a wide range of conditions affecting atmospheric escape. …”
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The Distribution of Impactor Core Material During Large Impacts on Earth-like Planets by Jonathan P. Itcovitz, Auriol S. P. Rae, Thomas M. Davison, Gareth S. Collins, Oliver Shorttle

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Future missions related to the determination of the elemental and isotopic composition of Earth, Moon and the terrestrial planets by Dandouras, I, Blanc, M, Fossati, L, Gerasimov, M, Guenther, EW, Kislyakova, KG, Lammer, H, Lin, Y, Marty, B, Mazelle, C, Rugheimer, S, Scherf, M, Sotin, C, Sproß, L, Tachibana, S, Wurz, P, Yamauchi, M

“…These missions are expected to trace the evolutionary paths of these two noble gas atmospheres, with a special emphasis on understanding the effect of atmospheric escape on the fate of water. Future missions to these planets will be key to help us establishing a comparative view of the evolution of climates and habitability at Earth, Venus and Mars, one of the most important and challenging open questions of planetary science. …”

Evolution of a Water-rich Atmosphere Formed by a Giant Impact on an Earth-sized Planet by Kenji Kurosaki, Yasunori Hori, Masahiro Ogihara, Masanobu Kunitomo

“…We investigate the X-ray- and UV-driven mass loss from an Earth-mass planet with an impact-induced multicomponent H _2 –He–H _2 O atmosphere for Gyr. …”
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Escaping Outflows from Disintegrating Exoplanets: Day-side versus Night-side Escape by Kang, Wanying, Ding, Feng, Wordsworth, Robin, Seager, Sara

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Origin-of-life Molecules in the Atmosphere after Big Impacts on the Early Earth by Nicholas F. Wogan, David C. Catling, Kevin J. Zahnle, Roxana Lupu

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Enhanced Hydrogen Escape on Mars during the 2018 Global Dust Storm: Impact of Horizontal Wind Field by Mingyang Sun, Hao Gu, Jun Cui, Xiaoshu Wu, Xu Huang, Yangxin Ni, Zhaopeng Wu, Lei Li

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Will 3552 Don Quixote Escape from the Solar System? by Suryadi Siregar

“…Investigation of its orbital evolution is conducted by using the SWIFT subroutine package, where the gravitational perturbations of eight major planets in the Solar System are considered. Over very short time scales (ï¾220 kyr) relative to the Solar System life time (ï¾10 Gyr), the asteroid 3552 Don Quixote gave an example of chaotic motion that can cause asteroid to move outward and may be followed by escaping from the Solar System. …”
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Detection of Atmospheric Escape from Four Young Mini-Neptunes by Michael Zhang, Heather A. Knutson, Fei Dai, Lile Wang, George R. Ricker, Richard P. Schwarz, Christopher Mann, Karen Collins

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Narrow Loophole for H2-Dominated Atmospheres on Habitable Rocky Planets around M Dwarfs by Renyu Hu, Fabrice Gaillard, Edwin S. Kite

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Earth atmospheric loss through the plasma mantle and its dependence on solar wind parameters by Audrey Schillings, Rikard Slapak, Hans Nilsson, Masatoshi Yamauchi, Iannis Dandouras, Lars-Göran Westerberg

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THE HYPOTHESIS OF “THE ESCAPE FROM THE MALTHUSIAN TRAP” THROUGH THE “FASTER TECHNOLOGICAL GROWTH”: THE CRITICAL ANALYSIS by A. A. Romanchuk

“…The key thesis of cliodynamics is a conclusion that starting from the certain moment of human history the technologies began to grow faster than the growth of population of the planet. …”
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CARBON SEQUESTRATION IN THE OCEAN-AN ESCAPE ROUTE by Wilson Uzochukwu Eze, Mekidani Aaron Musa, Virginia Ngozi Okolo, Amos Dindul Kalip, Pascalina Paulleo, Bernard Egwu Igiri, Abba John, David Ibeabuchi Onyemachi

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Indexing Exoplanets with Physical Conditions Potentially Suitable for Rock-Dependent Extremophiles by Madhu Kashyap Jagadeesh, Sagarika Rao Valluri, Vani Kari, Katarzyna Kubska, Łukasz Kaczmarek

“…Currently, according to the NASA Exoplanet Archive database, 3876 exoplanets have been discovered. The Earth Similarity Index (ESI) is defined as the geometric mean of radius, density, escape velocity, and surface temperature and ranges from 0 (dissimilar to Earth) to 1 (similar to Earth). …”
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Atmospheric mass loss during planet formation: The importance of planetesimal impacts by Sari, Re’em, Yalinewich, Almog, Schlichting, Hilke E

“…Despite being bombarded by the same planetesimal population, we find that the current differences in Earth’s and Venus’ atmospheric masses can be explained by modest differences in their initial atmospheric masses and that the current atmosphere of the Earth could have resulted from an equilibrium between atmospheric erosion and volatile delivery to the atmosphere from planetesimal impacts. …”
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A New Database of Giant Impacts over a Wide Range of Masses and with Material Strength: A First Analysis of Outcomes by Alexandre Emsenhuber, Erik Asphaug, Saverio Cambioni, Travis S. J. Gabriel, Stephen R. Schwartz, Robert E. Melikyan, C. Adeene Denton

“…Here, we present a high-resolution database of giant impacts for differentiated colliding bodies of iron–silicate composition, with target masses ranging from 1 × 10 ^−4 M _⊕ up to super-Earths (5 M _⊕ ). …”
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An Integrated Approach of Multi-Criteria Decision Making to Determine the Most Habitable Planet by Gizem Gunaydin, Gamze Duvan, Eren Ozceylan

“…According to the VIKOR method, Earth is ranked first, Mars is ranked second, and Mercury is ranked third in the order of the most habitable planets. …”
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