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* ߥʡ2015 [#zbb5ecca]


// ߥʡȯɽ
// ä->->->->빾->Ĺë->->->ƻ

** Schedule & History [#vfafd1d8]


|[[ 1 4/3>#planet0403]]|ݱѰϺ (3/23-27)||
|[[ 2 4/10>#planet0410]]|ͺ (3/16-20)&br;ư (3/30-4/3)||
|[[ 3 4/17>#planet0417]]| (4/6-10)|ä̤&br;HiCIAOѤֳи¬ˤIM Lupפδ¬|
|[[ 4 4/24>#planet0424]]|һ (4/13-17)||
|[[ 5 5/1>#planet0501]]|Ĺëɧ (4/20-24)||
|[[ 6 5/8>#planet0508]]|Ĺë (4/27-5/1)||
|[[ 7 5/15>#planet0515]]|빾Τ (5/4-8)||
|[[ 8 5/22>#planet0522]]|ͺ (5/11-15)|&br;Oxygen isotopes in the solar nebula|
|[[ 9 5/29>#planet0529]]|ƻ۽ (5/18-22)|ư&br;Formation and evolution of Pluto's small satellites|
|[[ 10 6/5>#planet0605]]|ݱѰϺ (5/25-29)||
|[[ 11 6/11>#planet0611]]||Wladimir Lyra (Caltech/JPL)|
|[[ 12 6/19>#planet0619]]|ư (6/1-5)&br;  (6/8-12)|Ĺëɧ&br;ֹ-θϱפǷΥ|
|[[ 13 6/26>#planet0626]]|һ (6/15-19)||
|[[ 14 7/10>#planet0710]]|Ĺëɧ (6/22-26)&br; 빾Τ (6/29-7/3)|Ĺë&br;Chondrule Formation|
|[[ 15 7/17>#planet0717]]|ͺ (7/6-10)||
|[[ 16 7/24>#planet0724]]|ƻ۽ (7/13-17)||
|[[ 1 9/18>#planet0918]]|ư (7/27-31)&br;  빾Τ (8/24-28)&br;  ͺ (8/31-9/4)&br;  ƻ۽ (9/7-11)||
|[[ 2 9/25>#planet0925]]| (8/3-7)&br;  Ĺëɧ (8/17-21)|ͺ&br;Planet formation: statistics of spin rates and obliquities of extrasolar planets|
|[[ 3 10/2>#planet1002]]|һ (8/10-14)&br;  ݱѰϺ (9/14-18)|빾Τ&br;֡The Mass Distribution Function of Planets (Renu Malhotra, 2015)|
|[[ 4 10/9>#planet1009]]|ư (9/21-25)|һ&br;εƻΥ®ٰ¸|
|[[ 5 10/30>#planet1030]]|һ (10/5-9)&br;  빾Τ (10/19-23) ||
|[[ 6 11/6>#planet1106]]| (9/28-10/2)&br;  Ĺëɧ (10/12-16)&br;  ͺ (10/26-10/30)||
|[[ 7 11/13>#planet1113]]|ƻ۽ (11/2-6)|ƻ۽&br;ֹ̩󥰤νǴ|
|[[ 8 11/20>#planet1120]]|ݱѰϺ (11/9-13)|&br;Grains in the early Solar System|
|[[ 9 12/11>#planet1211]]|ư (11/16-20)&br;   (11/23-27)&br;  һ (11/30-12/5)|ư&br;VOLATILE DELIVERY TO PLANETS FROM WATER-RICH PLANETESIMALS AROUND LOW-MASS STARS|
|[[ 10 12/18>#planet1218]]|Ĺëɧ (12/7-11) ||
|[[ 11 12/25>#planet1225]]|빾Τ (12/14-18) ||
|[[ 12 1/8>#planet0108]]|ͺ (12/21-25)&br;  ƻ۽ (12/28-1/1)  |Ĺëɧ&br;Critical Dust-to-Gas Ratio Revisited for Gravitational Instability|
|[[ 13 2/12>#planet0212]]|ݱѰϺ (1/4-8)&br; ư (1/11-15)&br;  һ (1/25-29)|ݱѰϺ&br;Formation of Close-in Terrestrial Planets by Giant Impacts: The Basic Scaling Laws|
|[[ 14 2/19>#planet0219]]||Marc Fouchard&br;The Oort cloud: shape and dynamics|
|[[ 15 2/26>#planet0226]]| (1/18-22)&br;  Ĺëɧ (2/1-5)&br;  ƻ۽ (2/15-19) ||
|[[ 16 3/4>#planet0304]]|ݱѰϺ (2/22-26) ||
|[[ 17 3/11>#planet0311]]|ͺ (2/8-12)&br;  ư (2/29-3/4)  |ͺ&br;Ѥˤ븶μž|
|[[ 18 3/18>#planet0318]]| (3/7-11) ||

** astro-ph  [#gd4ae1b1]


ݱѰϺ (3/23-27)~

- [[Jupiter's Decisive Role in the Inner Solar System's Early Evolution:http://arxiv.org/abs/1503.06945]]
- [[Growth of asteroids, planetary embryos and Kuiper belt objects by chondrule accretion:http://arxiv.org/abs/1503.07347]]


ͺ (3/16-20)~

- [[Planet formation around binary stars: Tatooine made easy:http://arxiv.org/abs/1503.03876]]
- [[Habitability of waterworlds: runaway greenhouses, atmospheric expansion and multiple climate states of pure water atmospheres:http://arxiv.org/abs/1503.04835]]

ư (3/30-4/3)~

- [[Dynamical Evolution of Multi-Resonant Systems: the Case of GJ876:http://arxiv.org/abs/1504.00051]]
- [[Birth Locations of the Kepler Circumbinary Planets:http://arxiv.org/abs/1504.00460]]



- [[A ∼32-70 K formation temperature range for the ice grains agglomerated by comet 67P/Churyumov-Gerasimenko:http://arxiv.org/abs/1504.01678]]
- [[A Search for Subkilometer-sized Ordinary Chondrite Like Asteroids in the Main-Belt:http://arxiv.org/abs/1504.01543]]


һ (4/13-17)~

- [[A reassessment of the in situ formation of close-in super-Earths:http://arxiv.org/abs/1504.03237]]
- [[Gas density drops inside dust cavities of transitional disks around young stars observed with ALMA:http://arxiv.org/abs/1504.03927]]


Ĺëɧ (4/20-24)~

- [[Millimeter-wave polarization of protoplanetary disks due to dust scattering:http://arxiv.org/abs/1504.04812]]


Ĺë (4/27-5/1)~

- [[How to form planetesimals from mm-sized chondrules and chondrule aggregates:http://arxiv.org/abs/1501.05314]]
- [[UV driven evaporation of close-in planets: energy-limited; recombination-limited and photon-limited flows:http://arxiv.org/abs/1504.07170]]


ͺ (5/11-15)~

- [[The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis:http://arxiv.org/abs/1505.01845]]
- [[The orbital evolution of asteroids, pebbles and planets from giant branch stellar radiation and winds:http://arxiv.org/abs/1505.01851]]


ƻ۽ (5/18-22)~

- [[No circumbinary planets transiting the tightest Kepler binaries - a fingerprint of a third star:http://arxiv.org/abs/1505.05749]]


ݱѰϺ (5/25-29)~

- [[Orbits of Potential Pluto Satellites and Rings Between Charon and Hydra:http://arxiv.org/abs/1505.05933]]


ư (6/1-5)~

- [[Mercury's resonant rotation from secular orbital elements:http://arxiv.org/abs/1506.00008]]
- [[The Complex History of Trojan Asteroids:http://arxiv.org/abs/1506.01658]]


- [[Sequential planet formation in the HD 100546 protoplanetary disk?:http://arxiv.org/abs/1506.02383]]
- [[Internal Structure of Asteroids Having Surface Shedding due to Rotational Instability:http://arxiv.org/abs/1506.03354]]


һ (6/15-19)~

- [[Numerically Predicted Indirect Signatures of Terrestrial Planet Formation:http://arxiv.org/abs/1506.05233]]


Ĺëɧ (6/22-26)~

- [[Outwards migration for planets in stellar irradiated 3D discs:http://arxiv.org/abs/1506.07348]]
- [[Bimodality of circumstellar disk evolution induced by Hall current:http://arxiv.org/abs/1506.07242]]

빾Τ (6/29-7/3)~

- [[On the probability of the collision of a Mars-sized planet with the Earth to form the Moon:http://arxiv.org/abs/1506.09043]]


ƻ۽ (7/13-17)~

- [[The Structure of Spiral Shocks Excited by Planetary-mass Companions:http://arxiv.org/abs/1507.03599]]
- [[Observational Signatures of Planets in Protoplanetary Disks: Spiral Arms Observed in Scattered Light Imaging Can be Induced by Planets:http://arxiv.org/abs/1507.03596]]


ݱѰϺ (7/20-24)~

- [[Evolution of the protolunar disk: dynamics, cooling timescale and implantation of volatiles onto the Earth:http://arxiv.org/abs/1507.05658]]
- [[A Quantitative Criterion for Defining Planets:http://arxiv.org/abs/1507.06300]]


ư (7/27-31)~

- [[On planet formation in HL Tau:http://arxiv.org/abs/1507.06719]]
- [[Building massive compact planetesimal disks from the accretion of pebbles:Building massive compact planetesimal disks from the accretion of pebbles]]

빾Τ (8/24-28)~

- [[Resolution Dependence of Disruptive Collisions between Planetesimals in the Gravity Regime:http://arxiv.org/abs/1508.05473]]

ͺ (8/31-9/4)~

- [[Dynamical Heating Induced by Dwarf Planets on Cold Kuiper Belt-like Debris Disks:http://arxiv.org/abs/1508.06990]]
- [[A particle-based hybrid code for planet formation:http://arxiv.org/abs/1508.07377]]

ƻ۽ (9/7-11)~

- [[Titania may produce abiotic oxygen atmospheres on habitable exoplanets:http://arxiv.org/abs/1509.03123]]
- [[Which type of planets do we expect to observe in the Habitable Zone?:http://arxiv.org/abs/1509.02429]]



- [[Nebular dead zone effects on the D/H ratio in chondrites and comets:http://arxiv.org/abs/1508.00263]]

Ĺëɧ (8/17-21)~

- [[Scattered light images of spiral arms in marginally gravitationally unstable discs with an embedded planet:http://arxiv.org/abs/1508.04443]]


һ (8/10-14)~

- [[The dynamical fate of planetary systems in young star clusters:http://arxiv.org/abs/1508.01593]]
- [[Inside-Out Planet Formation. III. Planet-disk interaction at the dead zone inner boundary:http://arxiv.org/abs/1508.02791]]

ݱѰϺ (9/14-18)~

- [[The Resonance Overlap and Hill Stability Criteria Revisited:http://arxiv.org/abs/1509.03607]]
- [[Dynamics of Self-Gravity Wakes in Dense Planetary Rings I. Pitch Angle:http://arxiv.org/abs/1509.03933]]
- [[Could Jupiter or Saturn Have Ejected a Fifth Giant Planet?:http://arxiv.org/abs/1509.05397]]


ư (9/21-25)~

- [[Giant Impact: An Efficient Mechanism for Devolatilization of Super-Earths:http://arxiv.org/abs/1509.05772]]
- [[Terrestrial-type planet formation: Comparing different types of initial conditions:http://arxiv.org/abs/1509.07217]]


һ (10/5-9)~

- [[Photo-dynamical mass determination of the multi-planetary system K2-19:http://arxiv.org/abs/1510.01047]]
- [[Characterization of the K2-19 Multiple-Transiting Planetary System via High-Dispersion Spectroscopy, AO Imaging, and Transit Timing Variations:http://arxiv.org/abs/1510.01060]]

빾Τ (10/19-23)~

- [[A disintegrating minor planet transiting a white dwarf:http://arxiv.org/abs/1510.06387]]



- [[Tatooine Nurseries: Structure and Evolution of Circumbinary Protoplanetary Disks:http://arxiv.org/abs/1509.07524]]
- [[Compositional evolution during rocky protoplanet accretion:http://arxiv.org/abs/1509.07504]]

Ĺëɧ (10/12-16)~

- [[Photophoresis in a Dilute, Optically Thick Medium and Dust Motion in Protoplanetary Disks:http://arxiv.org/abs/1510.03427]]

ͺ (10/26-10/30)~

- [[A population-based Habitable Zone perspective:http://arxiv.org/abs/1510.06885]]
- [[The Pluto system: Initial results from its exploration by New Horizons:http://arxiv.org/abs/1510.07704]]


ƻ۽ (11/2-6)~

- [[The Role of the Cooling Prescription for Disk Fragmentation: Numerical Convergence & Critical Cooling Parameter in Self-Gravitating Disks:http://arxiv.org/abs/1511.00303]]
- [[The Possible Orbital Decay and Transit Timing Variations of the Planet WASP-43b:http://arxiv.org/abs/1511.00768]]
- [[A semi-analytical model for exploring Galilean satellites formation from a massive disk:http://arxiv.org/abs/1511.01867]]


ݱѰϺ (11/9-13)~

- [[Viscous Instability Triggered by Layered Accretion in Protoplanetary Disks:http://arxiv.org/abs/1511.02813]]
- [[On the Fate of Unstable Circumbinary Planets: Tatooine's Close Encounters with a Death Star:http://arxiv.org/abs/1511.03274]]
- [[A rocky planet transiting a nearby low-mass star:http://arxiv.org/abs/1511.03550]]
- [[Giant Impacts on Earth-like Worlds:http://arxiv.org/abs/1511.03663]]
- [[On the growth of pebble-accreting planetesimals:http://arxiv.org/abs/1511.03903]]


ư (11/16-20)~

- [[Planetary System Formation in Protoplanetary Disk around HL Tauri:http://arxiv.org/abs/1511.04822]]


- [[Resolved gas cavities in transitional disks inferred from CO isotopologues with ALMA:http://arxiv.org/abs/1511.07149]]
- [[Direct imaging of the water snow line at the time of planet formation using two ALMA continuum bands:http://arxiv.org/abs/1511.06762]]

һ (11/30-12/5)~

- [[In Situ Formation and Dynamical Evolution of Hot Jupiter Systems:http://arxiv.org/abs/1511.09157]]


빾Τ (12/14-18)~

- [[Dynamical Constraints on Outer Planets in Super-Earth Systems:http://arxiv.org/abs/1512.05710]]


ͺ (12/21-25)~

- [[From Planetesimals to Planets in Turbulent Protoplanetary Disks I. Onset of Runaway Growth:http://arxiv.org/abs/1512.06968]]

ƻ۽ (12/28-1/1)~

- [[Effects of Dynamical Evolution of Giant Planets on the Delivery of Atmophile Elements During Terrestrial Planet Formation:http://arxiv.org/abs/1512.08182]]


ݱѰϺ (1/4-8)~

- [[Near-Infrared Imaging Polarimetry of LkCa 15: A Possible Warped Inner Disk:http://arxiv.org/abs/1601.00742]]

ư (1/11-15)~

- [[On the formation of compact planetary systems via concurrent core accretion and migration:http://arxiv.org/abs/1601.03608]]

һ (1/25-29)~

- [[Comprehensive tests of artificial viscosities, their switches and derivative operators used in Smoothed Particle Hydrodynamics:http://arxiv.org/abs/1601.05903]]
- [[A Neptune-sized Exoplanet Consistent with a Pure Rock Composition:http://arxiv.org/abs/1601.07608]]



- [[Spectral variability on primitive asteroids of the Themis and Beagle families: space weathering effects or parent body heterogeneity?:http://arxiv.org/abs/1601.05277]]
- [[Comet formation in collapsing pebble clouds. What cometary bulk density implies for the cloud mass and dust-to-ice ratio:http://arxiv.org/abs/1601.05726]]

Ĺëɧ (2/1-5)~

- [[The Giant Impact Simulations with Density Independent Smoothed Particle Hydrodynamics:http://arxiv.org/abs/1602.00843]]

ƻ۽ (2/15-19)~

- [[The effect of orbital damping during planet migration on the Inclination and Eccentricity Distributions of Neptune Trojans:http://arxiv.org/abs/1602.04303]]


ݱѰϺ (2/22-26)~

- [[Constraints on the location of a possible 9th planet derived from the Cassini data:http://arxiv.org/abs/1602.06116]]
- [[Neptune's Orbital Migration Was Grainy, Not Smooth:http://arxiv.org/abs/1602.06988]]
- [[Evolution and Magnitudes of Candidate Planet Nine:http://arxiv.org/abs/1602.07465]]


ͺ (2/8-12)~

- [[Origin of the chaotic motion of the Saturnian satellite Atlas:http://arxiv.org/abs/1602.01967]]

ư (2/29-3/4)~

- [[Interaction Cross Sections and Survival Rates for Proposed Solar System Member Planet Nine:http://arxiv.org/abs/1602.08496]]
- [[Mean radius and shape of Pluto and Charon from New Horizons images:http://arxiv.org/abs/1603.00821]]



- [[Mercury (Hg) in meteorites: variations in abundance, thermal release profile, mass-dependent and mass-independent isotopic fractionation:http://arxiv.org/abs/1603.01968]]
- [[Dust diffusion and settling in the presence of collisions: Trapping (sub)micron grains in the midplane:http://arxiv.org/abs/1603.02630]]

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