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Planet2017 ѹ

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* ߥʡ2017 [#zbb5ecca]


// ߥʡȯɽ
// ->->->->->ä->

** 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|
|[[ 8 7/4>#planet0704]]|(6/12-16) &br;(6/19-23) &br;ä̤(6/26-30)||
|[[ 9 7/18>#planet0718]]|ůϯ(7/3-7) &br;ͻ(7/10-14)|Ramon Brasser (ELSI)&br;The Cool and Distant Formation of Mars|
|[[ 10 7/27>#planet0727]]|ư(7/17-21)|ä̤&br;Gravitational Instability of a Porous Silicate Dust Disk|
|[[ 11 8/3>#planet0803]]||Maxwell Cai (Leiden Observatory)&br;Dynamical Evolution of Multiplanetary Systems in Star Clusters|
|[[ 1 9/5>#planet0905]]|ͺ(7/24-28) &br;ݱѰϺ(7/31-8/4) &br;(8/7-8/11) &br;(8/14-8/18)||
|[[ 2 9/19>#planet0919]]|ůϯ(8/28-9/1)&br; ư(9/4-8) |ݱѰϺ&br;The Final Stage of Terrestrial Planet Formation|
|[[ 3 10/10>#planet1010]]|ͺ(9/11-15)&br; ݱѰϺ(9/18-22)&br; (9/25-29)&br; (10/2-6)||
|[[ 4 10/31>#planet1031]]|||
|[[ 5 11/21>#planet1121]]||ůϯ|
|[[ 6 12/5>#planet1205]]|||
|[[ 7 12/19>#planet1031]]||ư|
|[[ 8 1/9>#planet0109]]||ͺ|
|[[ 9 1/23>#planet1031]]||ݱѰϺ|

** 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]]



- [[Radially resolved simulations of collapsing pebble clouds in protoplanetary discs:https://arxiv.org/abs/1706.03655]]


- [[Stable habitable zones of single Jovian planet systems:https://arxiv.org/abs/1706.05805]]
- [[Exoplanets as probes of the winds of host stars: the case of the M dwarf GJ 436:https://arxiv.org/abs/1706.05894]]
- [[Eccentricity excitation and merging of planetary embryos heated by pebble accretion:https://arxiv.org/abs/1706.06329]]
- [[The California-Kepler Survey V. Peas in a Pod: Planets in a Kepler Multi-planet System are Similar in Size and Regularly Spaced:https://arxiv.org/abs/1706.06204]]
- [[A giant planet undergoing extreme ultraviolet irradiation by its hot massive-star host:https://arxiv.org/abs/1706.06723]]
- [[Cloud formation in metal-rich atmospheres of hot super-Earths like 55 Cnc e and CoRot7b:https://arxiv.org/abs/1706.07219]]
- [[Gap and rings carved by vortices in protoplanetary dust:https://arxiv.org/abs/1706.07131]]


- [[Low-velocity collision behaviour of clusters composed of sub-mm sized dust aggregates:https://arxiv.org/abs/1706.07512]]
- [[Submillimetre-sized dust aggregate collision and growth properties:https://arxiv.org/abs/1706.07492]]
- [[NanoRocks: Design and Performance of an Experiment Studying Planet Formation on the International Space Station:https://arxiv.org/abs/1706.08625]]



- [[Generation of inclined protoplanetary discs and misaligned planets through mass accretion I: Coplanar secondary discs:https://arxiv.org/abs/1706.09905]]
- [[Energy Options for Future Humans on Titan:https://arxiv.org/abs/1707.00365]]
- [[Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics:https://arxiv.org/abs/1707.00729]]
- [[Centrifugally driven winds from protostellar accretion discs. I - Formulation and initial results:https://arxiv.org/abs/1707.01088]]
- [[Changes in orientation and shape of protoplanetary discs moving through an ambient medium:https://arxiv.org/abs/1707.01096]]


- [[Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core:https://arxiv.org/abs/1707.01997]]
- [[The highly active Anhur-Bes regions in the 67P/Churyumov - Gerasimenko comet: results from OSIRIS/ROSETTA observations:https://arxiv.org/abs/1707.02945]]
- [[The size distribution of Near Earth Objects larger than 10 meters:https://arxiv.org/abs/1707.04066]]



- [[On the Impact Origin of Phobos and Deimos I: Thermodynamic and Physical Aspects:https://arxiv.org/abs/1707.06282]]



- [[Seasonal Mass Transfer on the Nucleus of Comet 67P/Chuyumov-Gerasimenko:https://arxiv.org/abs/1707.06812]]


- [[Reduced gas accretion on super-Earths and ice giants:https://arxiv.org/abs/1708.00767]]
- [[The Formation of Uranus and Neptune: Fine Tuning in Core Accretion:https://arxiv.org/abs/1708.00862]]
- [[Simulations of Small Solid Accretion onto Planetesimals in the Presence of Gas:https://arxiv.org/abs/1708.00450]]


- [[Ejection of Chondrules from Fluffy Matrices:https://arxiv.org/abs/1708.02326]]
- [[Early formation of planetary building blocks inferred from Pb isotopic ages of chondrules:https://arxiv.org/abs/1708.02631]]


- [[What pebbles are made of: Interpretation of the V883 Ori disk:https://arxiv.org/abs/1708.03328]]



- [[Probing the cold dust emission in the AB Aur disk: a dust trap in a decaying vortex?:https://arxiv.org/abs/1708.08795]]
- [[Gas vs dust radial extent in disks: the importance of their thermal interplay:https://arxiv.org/abs/1708.09345]]


- [[Dust-driven viscous ring-instability in protoplanetary disks:https://arxiv.org/abs/1709.00246]]

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