JpGU Meeting 2019
Session outline| Space and Planetary Sciences (P) | ||
|---|---|---|
| Session Sub-category | Planetary Sciences(PS) | |
| Session ID | P-PS06 | |
| Title | Planetary Sciences | |
| Short Title | Planetary Sciences | |
| Main Convener | Name | Kenji Kurosaki |
| Affiliation | Department of Physics, Nagoya University | |
| Co-Convener 1 | Name | Yusuke Nakauchi |
| Affiliation | Japan Aerospace Exploration Agency | |
| Session Language | J | |
| Scope | We call for general interest papers for Planetary Scienses. Planetary Sciences consist of a variety of studies on the past, present, and future of our solar system and exoplanetary systems, Discussions based on various backgrounds are encouraged. | |
| Presentation Format | Oral and Poster presentation | |
| Time | Presentation No | Title | Presenter | Abstract |
|---|---|---|---|---|
| Oral Presentation May 27 AM1 | ||||
| 09:00 - 09:15 | PPS06-01 | Current status of the PLANETS telescope project for planetary and exoplanetary atmospheric monitoring | Takeshi Sakanoi | |
| 09:15 - 09:30 | PPS06-02 | Martian Moon eXploration MMX: science objectives and their promotion | Kiyoshi Kuramoto | |
| 09:30 - 09:45 | PPS06-03 | Implantation of Martian Materials in the Inner Solar System by a Mega Impact on Mars | Ryuki Hyodo | |
| 09:45 - 10:00 | PPS06-04 | Hydrodynamic escape of a reduced proto-atmosphere on early Mars | Tatsuya Yoshida | |
| 10:00 - 10:15 | PPS06-05 | Orbital evolution of Martian moons by rotating Martian proto-atmosphere with low angular momentum | Ryo Matsuoka | |
| 10:15 - 10:30 | PPS06-06 | N-body simulations of Moon formation with cooling evolution of the protolunar disk | Takanori Sasaki | |
| Oral Presentation May 27 AM2 | ||||
| 10:45 - 11:00 | PPS06-07 | Possibility of giant planet formation by pebble accretion in Class 0/I YSOs | Yuki Tanaka | |
| 11:00 - 11:15 | PPS06-08 | The effect of the three-dimensional gas flow around an embedded planet on pebble accretion | Ayumu Kuwahara | |
| 11:15 - 11:30 | PPS06-09 | Icy pebble accretion onto terrestrial planets: the effect of gas flow | Hiroyuki Kurokawa | |
| 11:30 - 11:45 | PPS06-10 | Delivery of ammonia ice to Ceres by pebble accretion | Yuto Nara | |
| 11:45 - 12:00 | PPS06-11 | Volatile-driven cryovolcanic eruption on asteroid Ceres as a probe to its interior | Koki Yumoto | |
| 12:00 - 12:15 | PPS06-12 | Ice sheet formation on synchrnously rotating earth-like planets in M-dwarf abitable zones | Masaki Ishiwatari | |
| Oral Presentation May 27 PM1 | ||||
| 13:45 - 14:00 | PPS06-13 | Three-dimensional linear calculation for non-isothermal type 1 planetary migration | Kohei Okada | |
| 14:00 - 14:15 | PPS06-14 | Dependence of Central star mass on Protoplanetary disk evolution | Ryuunosuke Nakano | |
| 14:15 - 14:30 | PPS06-15 | Radiation Hydrodynamic Simulations of the Formation of Circumplanetary Disks | Yuri Fujii | |
| 14:30 - 14:45 | PPS06-16 | Inefficient Magnetic Accretion Heating in Protoplanetary Disks: Evolution of The Snow Line | Shoji Mori | |
| 14:45 - 15:00 | PPS06-17 | Formation of super-Earths and their atmospheres with N-body simulations | Masahiro Ogihara | |
| 15:00 - 15:15 | PPS06-18 | The orbital stability of planets in resonances: the evolution of mass ratio | Yuji Matsumoto | |
| Oral Presentation May 27 PM2 | ||||
| 15:30 - 15:45 | PPS06-19 | Experimental study on the structure of shock remnant magnetization | Shota Kato | |
| 15:45 - 16:00 | PPS06-20 | Low-dispersion spectra of lunar impact flashes in 2018 Geminids | Masahisa Yanagisawa | |
| 16:00 - 16:15 | PPS06-21 | High velocity cratering experiments on sand-gypsum targets simulating asteroids | Ryo Sugimura | |
| 16:15 - 16:30 | PPS06-22 | Experimental study on collisional processes of highly porous ice balls simulating Saturn’s ring particles | Yukari Toyoda | |
| 16:30 - 16:45 | PPS06-23 | IN-SITU FORMATION OF THE URANIAN SATELLITES FROM WIDE DEBRIS DISK FORMED BY GIANT IMPACT | Ishizawa Yuya | |
| 16:45 - 17:00 | PPS06-24 | Effect on the obliquity due to a giant impact on a rotating ice giant | Kenji Kurosaki | |
| Oral Presentation May 28 AM1 | ||||
| 09:00 - 09:15 | PPS06-25 | Tensile Strength of Porous Dust Aggregates Measured with Dust N-body Simulations | Misako Tatsuuma | |
| 09:15 - 09:30 | PPS06-26 | Filling factor dependence of the thermal conductivity understood from the graph structure of dust aggregates | Sota ARAKAWA | |
| 09:30 - 09:45 | PPS06-27 | Collisional disruption of planetesimals: dependence of material strength | Ryo Suetsugu | |
| 09:45 - 10:00 | PPS06-28 | Size and cooling rate of chondrules formed thorough collision between planetesimals containing volatile materials | Sin-iti Sirono | |
| 10:00 - 10:15 | PPS06-29 | From Dust to Planet via collisional growth | Hiroshi Kobayashi | |
| 10:15 - 10:30 | PPS06-30 | Impact Conditions for the Formation of the Extremely Elongated Shape of 1I/’Oumuamua | Keisuke Sugiura | |
| Presentation No | Title | Presenter | Abstract |
|---|---|---|---|
| Poster Presentation May 28 PM2 | |||
| PPS06-P01 | The Study of Using SLR and GPS Observation Data to Estimate Geocenter Motion. | Yih Jack Cheng | |
| PPS06-P02 | Evolution of Pluto's surface albedo due to sublimation and condensation of ice | Hisashi Matsui | |
| PPS06-P03 | Origin of the moon, Reason why Moon is always facing to Earth, Origin of Moon Sea, reasons why there is no Ocean behind Moon | Akira Taneko | |
| PPS06-P04 | Proposed the Good model to verifyOrigins of Solar System (Planet, Asteroid belt, Earth, Moon) with "Multi Impact Hypothesis ",from 16' results of one time Evolution by | Akira Taneko | |
| PPS06-P05 | Quantitative evaluation of the cumulus convection schemes for the implementation into the Paleo Martian Global Climate Model | Katsushige Toriumi | |
| PPS06-P06 | Forced libration of Ganymede including the visco-elastic tidal deformation | shinichiro kojima | |
| PPS06-P07 | Experimental study on collision destruction simulating the primitive meteorite parent body | Horikawa Kazuhiro | |
| PPS06-P08 | Evolution of atmospheric composition in the early Martian atmosphere | Ryosuke Yagi | |
| PPS06-P09 | Observation of catastrophic destruction of two different targets using X Ray photography | Takumi Nagano | |
| PPS06-P10 | Charge transport between granular particles in an ejecta curtain produced by hypervelocity impacts | Kosuke Kurosawa | |
| PPS06-P11 | Nonlinear outcome of gravitational instability in irradiated protoplanetary disks | Shigenobu Hirose | |
| PPS06-P12 | Rheology of clay paste and application to the investigation of formation process of surface topography on the Mars | Chihiro Uemura | |
| PPS06-P13 | An Explanation for Physical Mechanism of the Streaming Instability | Hiroaki Kaneko | |
| PPS06-P14 | Spatial motion of the Earth-Moon system and Earth pole oscillatory process | Alexandra Sergeevna Filippova | |
| PPS06-P15 | Chondrule formation model by lightning in high dust density regions | Chihiro Ikeda | |
| PPS06-P16 | The transition to superrotation in stratospheric atmospheres | Motoki Sumi | |
| PPS06-P17 | ExPRES: a Tool to Simulate Exoplanetary and Planetary Radio Emissions | Corentin LOUIS | |
| PPS06-P18 | Crustal structures of major mercurian basins | Qingyun Deng | |
| PPS06-P19 | Application of LiDAR Technique for the 3D Digital Documentation of Cultural Heritage Sites | Sachchidanand - | |
| PPS06-P20 | Tidal Interaction in the Earth-Moon System Treated as a Double Planet | Aleksandr Aphanasievich Zlenko | |
| PPS06-P21 | The consequences of Saturn’s “ring rain” | James O Donoghue | |
| PPS06-P22 | Calculation of kinetic rate constants using high-level ab initio quantum chemical methods for planetary sciences and astrochemistry | Shiblee Ratan Barua | |
| PPS06-P23 | How many conditions must be satisfied to produce a habitable planet? | Shigenori Maruyama | |
| PPS06-P24 | Quantitative Evaluations for Meteorite Impact Tsunami | Naotaka YAMAMOTO CHIKASADA | |