JpGU Meeting 2024
セッション概要| 宇宙惑星科学(P) | |||
|---|---|---|---|
| セッション小記号 | 宇宙惑星科学複合領域・一般(CG) | ||
| セッションID | P-CG19 | ||
| タイトル | 和文 | 系外惑星 | |
| 英文 | Exoplanet | ||
| タイトル短縮名 | 和文 | 系外惑星 | |
| 英文 | Exoplanet | ||
| 代表コンビーナ | 氏名 | 和文 | 小玉 貴則 |
| 英文 | Takanori Kodama | ||
| 所属 | 和文 | 地球生命研究所、東京工業大学 | |
| 英文 | Earth-Life Science Institute, Tokyo Institute of Technology | ||
| 共同コンビーナ 1 | 氏名 | 和文 | 野津 翔太 |
| 英文 | Shota Notsu | ||
| 所属 | 和文 | 東京大学 大学院理学系研究科 地球惑星科学専攻 地球惑星システム科学講座 | |
| 英文 | Earth and Planetary System Science Group, Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo | ||
| 共同コンビーナ 2 | 氏名 | 和文 | 川島 由依 |
| 英文 | Yui Kawashima | ||
| 所属 | 和文 | 東北大学 | |
| 英文 | Tohoku University | ||
| 共同コンビーナ 3 | 氏名 | 和文 | 森 万由子 |
| 英文 | Mayuko Mori | ||
| 所属 | 和文 | 東京大学 | |
| 英文 | The University of Tokyo | ||
| 発表言語 | E | ||
| スコープ | 和文 |
The number of exoplanets discovered until now is increasing thanks to space telescopes, such as Kepler and TESS. So far, we have learned of the diversity of exoplanets, which include Hot-Jupiters and Super-Earths. Among them, some exoplanets are thought to be rocky planets within the so-called habitable zone. James Webb Space Telescope, JWST, has brought fantastic results, and exoplanetary science is standing on a new era of characterization of exoplanetary atmosphere. Various next projects are underway, like Ariel and JASMINE space telescopes and TMT. A new generation of exoplanetary science will be not only a field of astronomy but also Earth-Planetary Science. Thus, we must have a comprehensive discussion based on various science backgrounds, such as stellar physics, disk evolution, planetary formation, and planetary climate. This session aims to share their knowledge and research results, inform the current status of each project of exoplanets, and to engage in lively discussions based on physics and chemistry. We welcome participants from various fields of science. |
|
| 英文 |
The number of exoplanets discovered until now is increasing thanks to space telescopes, such as Kepler and TESS. So far, we have learned of the diversity of exoplanets, which include Hot-Jupiters and Super-Earths. Among them, some exoplanets are thought to be rocky planets within the so-called habitable zone. James Webb Space Telescope, JWST, has brought fantastic results, and exoplanetary science is standing on a new era of characterization of exoplanetary atmosphere. Various next projects are underway, like Ariel and JASMINE space telescopes and TMT. A new generation of exoplanetary science will be not only a field of astronomy but also Earth-Planetary Science. Thus, we must have a comprehensive discussion based on various science backgrounds, such as stellar physics, disk evolution, planetary formation, and planetary climate. This session aims to share their knowledge and research results, inform the current status of each project of exoplanets, and to engage in lively discussions based on physics and chemistry. We welcome participants from various fields of science. |
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| 発表方法 | 口頭および（または）ポスターセッション | ||
| 招待講演 |
Rafael Luque Lorenzo Pino (INAF - Osservatorio Astrofisico di Arcetri) Antonio Garcia Munoz (CEA Paris-Saclay) Anastasia Kokori (University College London) |
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| 時間 | 講演番号 | タイトル | 発表者 |
|---|---|---|---|
| 口頭発表 5月28日 AM1 | |||
| 09:00 - 09:15 | PCG19-01 | The ExoClock Project: An open integrated and interactive platform to continuous monitor the targets of the Ariel space mission | Anastasia Kokori |
| 09:15 - 09:30 | PCG19-02 | The new finding for the planetary system TOI-1883 revealed by radial velocity follow-up observations | 福田 生鵬 |
| 09:30 - 09:45 | PCG19-03 | Low densities, eccentricities, and entropies in the young, compact multi-planet system V1298 Tau | John Livingston |
| 09:45 - 10:00 | PCG19-04 | マイクロレンズ惑星頻度の主星質量依存性に対する初の有効な制限 | 布田 寛介 |
| 10:00 - 10:15 | PCG19-05 | Probing the Occurrence Rate of Exoplanets as a Function of Stellar Age | 宮崎 翔太 |
| 10:15 - 10:30 | PCG19-06 | Towards a holistic understanding of sub-Neptunes | Rafael Luque |
| 口頭発表 5月28日 AM2 | |||
| 10:45 - 11:00 | PCG19-07 | High dispersion optical phase curves of ultra-hot Jupiters with SHINE ON. | Lorenzo Pino |
| 11:00 - 11:15 | PCG19-08 | Revealing the Ultra-Hot Jupiterʼs Dayside Emission Spectrum Using Ground-Based Telescopes | 林 優哉 |
| 11:15 - 11:30 | PCG19-09 | Characterizing the nearest brown dwarfs with ExoJAX | 山 響 |
| 11:30 - 11:45 | PCG19-10 | Unveiling Atmospheric Features of HR 7672B Observed by REACH/Subaru | 笠木 結 |
| 11:45 - 12:00 | PCG19-11 | Spectral Line Profile Measurement of Methane for Investigating the Atmospheres Rich in H2 and He in Substellar Objects | 細川 晃 |
| 口頭発表 5月28日 PM1 | |||
| 13:45 - 14:15 | PCG19-12 | On the Physics of Atmospheric Escape | Antonio Garcia Munoz |
| 14:15 - 14:30 | PCG19-13 | Reduced water loss by photochemical reactions on terrestrial planets in runaway greenhouse conditions around pre-main-sequence M dwarfs | 川村 陽 |
| 14:30 - 14:45 | PCG19-14 | 恒星XUV放射のフォワードモデリング：太陽から若い太陽型星、前主系列段階へ | 庄田 宗人 |
| 14:45 - 15:00 | PCG19-15 | Silane: Magma-derived gas of super-Earth with reduced rocky core and hydrogen-rich atmosphere | 伊藤 祐一 |
| 15:00 - 15:15 | PCG19-16 | On the origin of reflective aerosols in close-in giant exoplanets: Haze composition evolution | 大野 和正 |
| 口頭発表 5月28日 PM2 | |||
| 15:30 - 15:45 | PCG19-17 | A possible correlation between the metal pollution of white dwarfs and the "dirtiness" of their dust disks | 奥谷 彩香 |
| 15:45 - 16:00 | PCG19-18 | Orbital Distribution of Gas Giants from Dust-to-Planet Simulations. | 小林 浩 |
| 16:00 - 16:15 | PCG19-19 | A Novel Method to Constrain Tidal Quality Factor from Non-synchronized Exoplanetary System | 徳野 鷹人 |
| 16:15 - 16:30 | PCG19-20 | Climate system on snowball planets revealed by MIROC4m | 小長谷 貴志 |
| 16:30 - 16:45 | PCG19-21 | Astrobiology x Exoplanetery science: what are the next steps for creating new synergy? | 藤島 皓介 |
| 講演番号 | タイトル | 発表者 |
|---|---|---|
| ポスター発表 5月28日 PM3 | ||
| PCG19-P01 | Development of the MuSCAT series and their latest scientific results | 成田 憲保 |
| PCG19-P02 | Proof of concept for probing Na absorption in hot Jupiters’ atmospheres using the narrow-band filters of MuSCAT3/4 | 川内 紀代恵 |
| PCG19-P03 | Low-resolution transmission spectrum of a Sub-Neptune around a young K-dwarf K2-136 c | 森 万由子 |
| PCG19-P04 | 温帯地球型惑星の大気の特徴付けに対して理想的な惑星の発見 | 葛原 昌幸 |
| PCG19-P05 | Revisiting the effects of rings on the reflected light curves of exoplanets | 菅沼 斗偲 |
| PCG19-P06 | 系外惑星大気のトランジット分光観測に向けた外気圏大気シミュレーション | 加藤 龍雅 |
| PCG19-P07 | Detectability of oxygen exosphere of Earth-like exoplanet by 1.7-m UV space telescope | 亀田 真吾 |
| PCG19-P08 | Climate of a tidally locked terrestrial planet with a global cloud-resolving model | 小玉 貴則 |
| PCG19-P09 | Resolved Clouds on Snowball Planets | 高須賀 大輔 |
| PCG19-P10 | Day-night water cycle dynamics on TRAPPIST-1e using an integrated global climate, hydrological, and glaciological model | 鎌田 有紘 |
| PCG19-P11 | 暴走温室状態の地球型惑星における水蒸気主体大気の流体力学的散逸 | 吉田 辰哉 |
| PCG19-P12 | Atmospheric H-C-O ratio for super-Earth/sub-Neptune with rocky core | Chanoul Seo |
| PCG19-P13 | Development of Magnetosphere-Ionosphere Coupling Model Generalized for Exoplanetary Auroral Radio Emission | Asa Satyagraha |
| PCG19-P14 | 恒星高エネルギー粒子のフルエンスを考慮した系外惑星への影響評価 | 山敷 庸亮 |
| PCG19-P15 | Detectability of the coolest Y-type brown dwarfs by a next-generation infrared satellite | 川島 由依 |
| PCG19-P16 | Differentiable Planetary Spectrum Model as a Foundation Software for Exoplanet Atmosphere Characterization | 河原 創 |
| PCG19-P17 | Planetary sciences expected by the next-generation infrared astronomical satellite GREX-PLUS | 野津 翔太 |
| PCG19-P18 | Semi-analytical model for close-in planet formation via giant collisions | 木村 真博 |