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* ߥʡ2017 [#zbb5ecca]


// ߥʡȯɽ
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** Schedule & History [#vfafd1d8]


|[[ 1 4/4>#planet0404]]|ͤ (3/20-24)|ͤ &br;ּήȶưΥμС|
|[[ 2 4/11>#planet0411]]|ư(3/27-31) &br;ͺ(4/3-7)|Steven Rieder(AICS, RIKEN)&br;J1407b: a Super-Saturn or something else?|
|[[ 3 4/12>#planet0412]]||Ĺչ&br;֥ȥꥲȤξͥߥ졼ĹǤΤǤʤΡ|
|[[ 4 4/25>#planet0425]]|ݱѰϺ(4/10-14)&br;(4/17-21)|&br;Asteroids and their compositions|
|[[ 5 5/9>#planet0509]]|(4/24-28) &br;ä̤(5/1-5)||
|[[ 6 5/16>#planet0516]]|ůϯ(5/8-12)|ư&br;High-Resolution N-body Simulations of Planet Formation|
|[[ 7 6/13>#planet0613]]|ͻ(5/15-19)&br; ư(5/22-26)&br; ͺ(5/29-6/2)&br; ݱѰϺ(6/5-9)|ͺ&br;Spin of Protoplanets by Planetesimal accretion|

** astro-ph  [#gd4ae1b1]


ͤ (3/20-24)~

- [[Reassessment of the Null Result of the HST Search for Planets in 47 Tucanae:https://arxiv.org/abs/1703.06136]]
- [[Assessing the Habitability of the TRAPPIST-1 System Using a 3D Climate Model:https://arxiv.org/abs/1703.05815]]
- [[The GTC exoplanet transit spectroscopy survey. VII. Detection of sodium in WASP-52b's cloudy atmosphere:https://arxiv.org/abs/1703.06716]]
- [[Formation of TRAPPIST-1 and other compact systems:https://arxiv.org/abs/1703.06924]]
- [[Testing the existence of optical linear polarization in young brown dwarfs:https://arxiv.org/abs/1703.07341]]
- [[The effect of the stellar absorption line centre-to-limb variation on exoplanet transmission spectrum observations:https://arxiv.org/abs/1703.07585]]
- [[Planetesimal formation by the streaming instability in a photoevaporating disk:https://arxiv.org/abs/1703.07895]]



- [[The stability of tightly-packed, evenly-spaced systems of Earth-mass planets orbiting a Sun-like star:https://arxiv.org/abs/1703.08426]]
- [[Water transport to circumprimary habitable zones from icy planetesimal disks in binary star systems:https://arxiv.org/abs/1703.09000]]
- [[Size and density sorting of dust grains in SPH simulations of protoplanetary discs:https://arxiv.org/abs/1703.10385]]


- [[The cool and distant formation of Mars:https://arxiv.org/abs/1704.00184]]



- [[Plausible Compositions of the Seven TRAPPIST-1 Planets Using Long-term Dynamical Simulations:https://arxiv.org/abs/1704.02261]]
- [[The curiously warped mean plane of the Kuiper belt:https://arxiv.org/abs/1704.02444]]
- [[Limits on the Stability of TRAPPIST-1:https://arxiv.org/abs/1704.02957]]
- [[A Minimum Mass Nebula for M Dwarfs:https://arxiv.org/abs/1704.03265]]
- [[The Destruction of an Oort Cloud in a rich stellar cluster:https://arxiv.org/abs/1704.03341]]


- [[Testing the chondrule-rich accretion model for planetary embryos using calcium isotopes:https://arxiv.org/abs/1704.05726]]



- [[Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets:https://arxiv.org/abs/1704.06459]]
- [[Acceleration of Cooling of Ice Giants by Condensation in Early Atmospheres:https://arxiv.org/abs/1704.07558]]
- [[Titan brighter at twilight than in daylight:https://arxiv.org/abs/1704.07460]]
- [[Avoiding resonance capture in multi-planet extrasolar systems:https://arxiv.org/abs/1704.07836]]


- [[3D radiative transfer of intrinsically polarized dust emission based on aligned aspherical grains:https://arxiv.org/abs/1705.01047]]
- [[Survey of cold water lines in protoplanetary disks: indications of systematic volatile depletion:https://arxiv.org/abs/1705.00799]]
- [[A likely detection of a local interplanetary dust cloud passing near the Earth in the AKARI mid-infrared all-sky map:https://arxiv.org/abs/1705.01541]]



- [[Composition of Early Planetary Atmospheres II: Coupled Dust and Chemical Evolution in Protoplanetary Disks:https://arxiv.org/abs/1705.02381]]
- [[Chemical enrichment of giant planets and discs due to pebble drift:https://arxiv.org/abs/1705.03305]]
- [[Evidence for universality in the initial planetesimal mass function:https://arxiv.org/abs/1705.03889]]
- [[N-body simulations of planet formation via pebble accretion I: First Results:https://arxiv.org/abs/1705.04264]]



- [[Dynamics of Porous Dust Aggregates and Gravitational Instability of Their Disk:https://arxiv.org/abs/1705.04520]]
- [[Detection of the Yarkovsky effect for C-type asteroids in the Veritas family:https://arxiv.org/abs/1705.04333]]
- [[Shape models and physical properties of asteroids:https://arxiv.org/abs/1705.05710]]
- [[Driven by Excess? Climatic Implications of New Global Mapping of Near-Surface Water-Equivalent Hydrogen on Mars:https://arxiv.org/abs/1705.05556]]
- [[The compositional diversity of non-Vesta basaltic asteroids:https://arxiv.org/abs/1705.06304]]


- [[Formation of Close-in Super-Earths by Giant Impacts: Effects of Initial Eccentricities and Inclinations of Protoplanets:https://arxiv.org/abs/1705.07810]]
- [[In situ accretion of gaseous envelopes on to planetary cores embedded in evolving protoplanetary discs:https://arxiv.org/abs/1705.08147]]


- [[Internal Structure of Giant and Icy Planets: Importance of Heavy Elements and Mixing:https://arxiv.org/abs/1705.09320]]
- [[Capture of free-floating planets by stellar systems:https://arxiv.org/abs/1705.10332]]


- [[Cladistical analysis of the Jovian and Saturnian satellite systems:https://arxiv.org/abs/1706.01423]]
- [[Dynamics and Collisional Evolution of Closely Packed Planetary Systems:https://arxiv.org/abs/1706.01975]]

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