Planet2014

Last-modified: 2015-03-30 (·î) 16:27:03 (1827d)

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Schedule & History †

astro-ph ¥ê¥ó¥¯ †

5/13

ÀÐÄž°´î (4/14-18)

• Protoplanetary dust porosity and FU Orionis Outbursts: Solving the mystery of Earth's missing volatiles
• The ballistic transport instability in Saturn's rings II: nonlinear wave dynamics
• The ballistic transport instability in Saturn's rings III: numerical simulations
  

¾®µ×ÊݱѰìϺ (4/21-25)

• The Formation of Uranus & Neptune: Challenges and Implications For Intermediate-Mass Exoplanets
• On the Abundance of Circumbinary Planets

5/20

²¡ÌîæÆ°ì (4/28-5/2)

• Dancing with the Stars: Formation of the Fomalhaut triple system and its effect on the debris disks
• On the Spin-axis Dynamics of a Moonless Earth

ÏÆÅÄÌÐ (5/5-9)

• Density, porosity, mineralogy, and internal structure of cosmic dust and alteration of its properties during high velocity atmospheric entry
• Diversity of planetary systems in low-mass disks: Terrestrial-type planet formation and water delivery

5/30

¾¾ËÜÐһΠ(5/12-16)

• Secular Effects of Tidal Damping in Compact Planetary Systems
• Chemistry in an Evolving Protoplanetary Disk: Effects on Terrestrial Planet Composition

ĹëÀɧ (5/19-23)

• Disc-protoplanet interaction Influence of circumprimary radiative discs on self-gravitating protoplanetary bodies in binary star systems

6/13

¼ÆÅÄͺ (5/26-30)

• Impact inducted surface heating by planetesimals on early Mars
• Planet formation in stellar binaries I: planetesimal dynamics in massive protoplanetary disks

ÀÐÄž°´î (6/2-6)

• Modeling dust growth in protoplanetary disks: The breakthrough case
• Formation of Isothermal Disks around Protoplanets. I. Introductory Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets

6/20

¾®µ×ÊݱѰìϺ (6/9-13)

• Earthshine on a Young Moon: Explaining the Lunar Farside Highlands

6/27

ÏÆÅÄÌÐ (6/16-20)

• Water Ice and Dust in the Innermost Coma of Comet 103P/Hartley 2
• The Opposition Effect of the Asteroid 4 Vesta

7/4

²¡ÌîæÆ°ì (6/23-27)

• Global Models of Planet Formation and Evolution
• A Statistical Reconstruction of the Planet Population Around Kepler Solar-Type Stars

7/18

¾¾ËÜÐһΠ(6/30-7/4)

• A stellar-mass-dependent drop in planet occurrence rates
• Explaining Mercury's Density through Magnetic Erosion

ĹëÀɧ (7/7-11)

• Turbulence-Induced Relative Velocity of Dust Particles III: The Probability Distribution

9/5

¼ÆÅÄͺ (7/14-18)

• Water Delivery and Giant Impacts in the 'Grand Tack' Scenario
• Influence of Stellar Multiplicity On Planet Formation. II. Planets Are Less Common in Multiple-Star Systems with Separations Smaller than 1500 AU

¾®µ×ÊݱѰìϺ (7/28-8/1)

• Overcoming the Meter Barrier and The Formation of Systems with Tightly-packed Inner Planets (STIPs)

²¡ÌîæÆ°ì (8/4-8)

• Dynamical Stability of Terrestrial Planets in the Binary ¦Á Centauri System
• Terrestrial Planet Formation in the Presence of Migrating Super-earths

ÏÆÅÄÌÐ (8/11-15)

• Formation of pebble-pile planetesimals
• The role of impact and radiogenic heating in the early thermal evolution of Mars

¾¾ËÜÐһΠ(8/18-22)

• Towards Chemical Constraints on Hot Jupiter Migration
• How to reach the orbital configuration of the inner three planets in HD 40307 Planet System ?

ĹëÀɧ (8/25-29)

• Separating gas-giant and ice-giant planets by halting pebble accretion

9/19

ÀÐÄž°´î (7/21-25)

• On the Feeding Zone of Planetesimal Formation by the Streaming Instability
• A six-part collisional model of the main asteroid belt

¼ÆÅÄͺ (9/1-5)

• Stability of the Kepler-11 System and its Origin
• Understanding the assembly of Kepler's compact planetary systems

10/3

ÀÐÄž°´î (9/8-12)

• Spherically Symmetric Gravitational Collapse of a Clump of Solids in a Gas
• How Rocky Are They? The Composition Distribution of Kepler's Sub-Neptune Planet Candidates within 0.15 AU

¾®µ×ÊݱѰìϺ (9/15-19)

• Make Super-Earths, Not Jupiters: Accreting Nebular Gas onto Solid Cores at 0.1 AU and Beyond
• Challenges in Forming the Solar System's Giant Planet Cores via Pebble Accretion

²¡ÌîæÆ°ì (9/22-26)

• Terrestrial planet formation in low-mass disks: dependence with initial conditions
• Planetesimal fragmentation and giant planet formation: the role of planet migration

10/10

ÏÆÅÄÌÐ (9/29-10/3)

• Water Vapour Absorption in the Clear Atmosphere of an exo-Neptune
• Outward migration of Jupiter and Saturn in 3:2 or 2:1 resonance in radiative disks: implications for the Grand Tack and Nice models

10/17

¾¾ËÜÐһΠ(10/6-10)

• Formation of close in Super-Earths & Mini-Neptunes: Required Disk Masses & Their Implications
• Thermal structure of an exoplanet atmosphere from phase-resolved emission spectroscopy

11/7

ĹëÀɧ (10/13-17)

• Can dust coagulation trigger streaming instability?
• Effects of dust feedback on vortices in protoplanetary disks

°ë¹¾ËãΤ (10/20-24)

• Spin-orbit angle in compact planetary systems perturbed by an inclined companion. Application to the 55 Cancri system
• Gas and dust structures in protoplanetary disks hosting multiple planets

11/14

ĹëÀîÌ÷¹É (10/27-31)

• Embryo impacts and gas giant mergers II: Diversity of Hot Jupiters' internal structure
• The stickiness of micrometer-sized water-ice particles
• Migration and Growth of Protoplanetary Embryos II: Emergence of Proto-Gas-Giants Cores versus Super Earths' Progenitor
• Radiation-Driven Warping of Circumbinary Disks Around Eccentric Young Star Binaries
• CO gas inside the protoplanetary disk cavity in HD 142527: disk structure from ALMA

ÀÐÄž°´î (11/3-7)

• Collisions of small ice particles under microgravity conditions
• 1D accretion discs around eccentric planets: observable near-infrared variability

11/28

¼ÆÅÄͺ (11/10-14)

• Reassessing the formation of the Inner Oort cloud in an embedded star cluster II: Probing the inner edge
• Migration of massive planets in accreting disks

¾®µ×ÊݱѰìϺ (11/17-21)

• Late Accretion and the Late Veneer
• Chaotic Disintegration of the Inner Solar System

12/5

²¡ÌîæÆ°ì (11/24-28)

• Detectable close-in planets around white dwarfs through late unpacking
• Dynamical Interactions Make Hot Jupiters in Open Star Clusters

12/12

ÏÆÅÄÌÐ (12/1-5)

• Photophoresis in protoplanetary disks: a numerical approach
• New insight into the Solar System's transition disk phase provided by the unusual meteorite Isheyevo

12/19

¾¾ËÜÐһΠ(12/8-12)

• Spiral arms in scattered light images of protoplanetary discs: Are they the signposts of planets?
• Erosion and the limits to planetesimal growth

1/9

ĹëÀɧ (12/15-19)

• Near-Infrared Image of the Debris Disk around HD 15115
• Minimum Core Masses for Giant Planet Formation With Realistic Equations of State and Opacities

°ë¹¾ ËãΤ (12/22-26)

• Ammonia, Water Clouds and Methane Abundances of Giant Exoplanets and Opportunities for Super-Earth Exoplanets

1/16

ĹëÀîÌ÷¹É (12/29-1/2)

• Accretion of the Moon from non-canonical disks
• Halting Migration: Numerical Calculations of Corotation Torques in the Weakly Nonlinear Regime

ÀÐÄž°´î (1/5-9)

• Collisions of small ice particles under microgravity conditions (II): Does the chemical composition of the ice change the collisional properties?
• Sulfurization of Iron in the Dynamic Solar Nebula and Implications for Planetary Compositions

1/30

¼ÆÅÄͺ (1/12-16)

• The formation of the solar system
• Circumbinary planets - why they are so likely to transit

2/6

²¡ÌîæÆ°ì (1/26-30)

• Gas giant planets as dynamical barriers to inward-migrating super-Earths
• The Dynamical Evolution of the Asteroid Belt

2/13

¾®µ×ÊݱѰìϺ (1/19-23)

• The Feeding Zones of Terrestrial Planets and Insights into Moon Formation
• Giant Planets

ÏÆÅÄÌÐ (2/2-6)

• Compound Chondrules fused Cold
• Micron-scale D/H heterogeneity in chondrite matrices: a signature of the pristine solar system water?

2/20

¾¾ËÜÐһΠ(2/9-13)

• Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)
• Planetary Systems and the Formation of Habitable Planets

3/6

ĹëÀɧ (2/16-20)

• Near-IR imaging of T Cha: evidence for scattered-light disk structures at solar system scales

3/27

°ë¹¾ËãΤ (2/23-27)

• The destruction of inner planetary systems during high-eccentricity migration of gas giants

ĹëÀîÌ÷¹É (3/2-6)

• Combining high-dispersion spectroscopy (HDS) with high contrast imaging (HCI): Probing rocky planets around our nearest neighbors
• Stellar Multiplicity and Debris Disks: An Unbiased Sample

ÀÐÄž°´î (3/9-13)

• Time evolution of snow regions and planet traps in an evolving protoplanetary disk

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