2022年度の論文紹介と輪読

2023 1.12 & 19 山口

Cordier, D. and Carrasco, N. (2019)
The floatability of aerosols and wave damping on Titan’s seas
Nature Geoscience 12, 315-320

2022 12.15 & 19 米津

Kamata, S. et al. (2019)
Pluto’s ocean is capped and insulated by gas hydrates
Nature Geoscience 12, 407-410

2022 12. 1 & 8 櫻井

Huang, Y. H. et al. (2022)
Bombardment history of the Moon constrained by crustal porosity
Nature Geoscience 15, 531-535

2022 11.17 & 24 松原

Nicklas, R. W. et al. (2022)
Early silicic magmatism on a differentiated asteroid
Nature Geoscience 15, 696-699

2022 10.27 & 11.7 野間

Park, R. S. et al. (2016)
A partially differentiated interior for (1) Ceres deduced from its gravity field and shape
Nature 537, 515-517

2022 10.13 & 20 山下

Faulk, S. P. et al. (2017)
Regional patterns of extreme precipitation on Titan consistent with observed alluvial fan distribution
Nature Geoscience 10, 827-831

2022 9.26 & 10. 6 池谷

Moores, J. E., et al. (2017)
Penitentes as the origin of the bladed terrain of Tartarus Dorsa on Pluto
Nature 15, 171-176

2022 7.7 & 14 池谷

Ding, L., et al. (2022)
Surface characteristics of the Zhurong Mars rover traverse at Utopia Planitia
Nature Geoscience 15, 171-176

2022 6.30 & 7. 7 山下

Nakajima, M., et al. (2022)
Large planets may not form fractionally large moons
Nature Communications 13, 568

2022 6.16 & 23 松原

Rubanenko, L., et al. (2019)
Thick ice deposits in shallow simple craters on the Moon and Mercury
Nature Geoscience 12, 597-601

2022 6. 2 & 9 野間

Wakita, S., et al. (2021)
Impactor material records the ancient lunar magnetic field in antipodal anomalies
Nature communications 12, 6543

2022 5.12 & 19 櫻井

Sharkey, B. N., et al. (2021)
Lunar-like silicate material forms the Earth quasi-satellite (469219)2016 HO3 Kamo'oalewa
Communications Earth & Environment 2, 231.

2022 4.21 & 28 山口

Tachibana, S. et al. (2022)
Pebbles and sand on asteroid (162173) Ryugu: In situ observation and particles returned to Earth
Science 375, 1011-1016.

2022 4. 7 & 14 米津

Cox, M.A. et al. (2022)
Impact and habitability scenarios for early Mars revisited based
on a 4.45-Ga shocked zircon in regolith breccia
Science advances 8, eabl7497.