Planet2015

Last-modified: 2016-03-21 (·î) 19:04:59 (1650d)

Planet

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Schedule & History †

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astro-ph ¥ê¥ó¥¯ †

4/3

¾®µ×ÊݱѰìϺ (3/23-27)

• Jupiter's Decisive Role in the Inner Solar System's Early Evolution
• Growth of asteroids, planetary embryos and Kuiper belt objects by chondrule accretion

4/10

¼ÆÅÄͺ (3/16-20)

• Planet formation around binary stars: Tatooine made easy
• Habitability of waterworlds: runaway greenhouses, atmospheric expansion and multiple climate states of pure water atmospheres

²¡ÌîæÆ°ì (3/30-4/3)

• Dynamical Evolution of Multi-Resonant Systems: the Case of GJ876
• Birth Locations of the Kepler Circumbinary Planets

4/17

ÏÆÅÄÌÐ (4/6-10)

• A ∼32-70 K formation temperature range for the ice grains agglomerated by comet 67P/Churyumov-Gerasimenko
• A Search for Subkilometer-sized Ordinary Chondrite Like Asteroids in the Main-Belt

4/24

¾¾ËÜÐһΠ(4/13-17)

• A reassessment of the in situ formation of close-in super-Earths
• Gas density drops inside dust cavities of transitional disks around young stars observed with ALMA

5/1

ĹëÀɧ (4/20-24)

• Millimeter-wave polarization of protoplanetary disks due to dust scattering

5/8

ĹëÀîÌ÷¹É (4/27-5/1)

• How to form planetesimals from mm-sized chondrules and chondrule aggregates
• UV driven evaporation of close-in planets: energy-limited; recombination-limited and photon-limited flows

5/22

¼ÆÅÄͺ (5/11-15)

• The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis
• The orbital evolution of asteroids, pebbles and planets from giant branch stellar radiation and winds

5/29

Æ»±Û½¨¸ã (5/18-22)

• No circumbinary planets transiting the tightest Kepler binaries - a fingerprint of a third star

6/5

¾®µ×ÊݱѰìϺ (5/25-29)

• Orbits of Potential Pluto Satellites and Rings Between Charon and Hydra

6/19

²¡ÌîæÆ°ì (6/1-5)

• Mercury's resonant rotation from secular orbital elements
• The Complex History of Trojan Asteroids

ÏÆÅÄÌÐ (6/8-12)

• Sequential planet formation in the HD 100546 protoplanetary disk?
• Internal Structure of Asteroids Having Surface Shedding due to Rotational Instability

6/26

¾¾ËÜÐһΠ(6/15-19)

• Numerically Predicted Indirect Signatures of Terrestrial Planet Formation

7/10

ĹëÀɧ (6/22-26)

• Outwards migration for planets in stellar irradiated 3D discs
• Bimodality of circumstellar disk evolution induced by Hall current

°ë¹¾ËãΤ (6/29-7/3)

• On the probability of the collision of a Mars-sized planet with the Earth to form the Moon

7/24

Æ»±Û½¨¸ã (7/13-17)

• The Structure of Spiral Shocks Excited by Planetary-mass Companions
• Observational Signatures of Planets in Protoplanetary Disks: Spiral Arms Observed in Scattered Light Imaging Can be Induced by Planets

7/31

¾®µ×ÊݱѰìϺ (7/20-24)

• Evolution of the protolunar disk: dynamics, cooling timescale and implantation of volatiles onto the Earth
• A Quantitative Criterion for Defining Planets

9/18

²¡ÌîæÆ°ì (7/27-31)

• On planet formation in HL Tau
• [[Building massive compact planetesimal disks from the accretion of pebbles:Building massive compact planetesimal disks from the accretion of pebbles]]

°ë¹¾ËãΤ (8/24-28)

• Resolution Dependence of Disruptive Collisions between Planetesimals in the Gravity Regime

¼ÆÅÄͺ (8/31-9/4)

• Dynamical Heating Induced by Dwarf Planets on Cold Kuiper Belt-like Debris Disks
• A particle-based hybrid code for planet formation

Æ»±Û½¨¸ã (9/7-11)

• Titania may produce abiotic oxygen atmospheres on habitable exoplanets
• Which type of planets do we expect to observe in the Habitable Zone?

9/25

ÏÆÅÄÌÐ (8/3-7)

• Nebular dead zone effects on the D/H ratio in chondrites and comets

ĹëÀɧ (8/17-21)

• Scattered light images of spiral arms in marginally gravitationally unstable discs with an embedded planet

10/2

¾¾ËÜÐһΠ(8/10-14)

• The dynamical fate of planetary systems in young star clusters
• Inside-Out Planet Formation. III. Planet-disk interaction at the dead zone inner boundary

¾®µ×ÊݱѰìϺ (9/14-18)

• The Resonance Overlap and Hill Stability Criteria Revisited
• Dynamics of Self-Gravity Wakes in Dense Planetary Rings I. Pitch Angle
• Could Jupiter or Saturn Have Ejected a Fifth Giant Planet?

10/9

²¡ÌîæÆ°ì (9/21-25)

• Giant Impact: An Efficient Mechanism for Devolatilization of Super-Earths
• Terrestrial-type planet formation: Comparing different types of initial conditions

10/30

¾¾ËÜÐһΠ(10/5-9)

• Photo-dynamical mass determination of the multi-planetary system K2-19
• Characterization of the K2-19 Multiple-Transiting Planetary System via High-Dispersion Spectroscopy, AO Imaging, and Transit Timing Variations

°ë¹¾ËãΤ (10/19-23)

• A disintegrating minor planet transiting a white dwarf

11/6

ÏÆÅÄÌÐ (9/28-10/2)

• Tatooine Nurseries: Structure and Evolution of Circumbinary Protoplanetary Disks
• Compositional evolution during rocky protoplanet accretion

ĹëÀɧ (10/12-16)

• Photophoresis in a Dilute, Optically Thick Medium and Dust Motion in Protoplanetary Disks

¼ÆÅÄͺ (10/26-10/30)

• A population-based Habitable Zone perspective
• The Pluto system: Initial results from its exploration by New Horizons

11/13

Æ»±Û½¨¸ã (11/2-6)

• The Role of the Cooling Prescription for Disk Fragmentation: Numerical Convergence & Critical Cooling Parameter in Self-Gravitating Disks
• The Possible Orbital Decay and Transit Timing Variations of the Planet WASP-43b
• A semi-analytical model for exploring Galilean satellites formation from a massive disk

11/20

¾®µ×ÊݱѰìϺ (11/9-13)

• Viscous Instability Triggered by Layered Accretion in Protoplanetary Disks
• On the Fate of Unstable Circumbinary Planets: Tatooine's Close Encounters with a Death Star
• A rocky planet transiting a nearby low-mass star
• Giant Impacts on Earth-like Worlds
• On the growth of pebble-accreting planetesimals

12/11

²¡ÌîæÆ°ì (11/16-20)

• Planetary System Formation in Protoplanetary Disk around HL Tauri

ÏÆÅÄÌÐ (11/23-27)

• Resolved gas cavities in transitional disks inferred from CO isotopologues with ALMA
• Direct imaging of the water snow line at the time of planet formation using two ALMA continuum bands

¾¾ËÜÐһΠ(11/30-12/5)

• In Situ Formation and Dynamical Evolution of Hot Jupiter Systems

12/25

°ë¹¾ËãΤ (12/14-18)

• Dynamical Constraints on Outer Planets in Super-Earth Systems

1/8

¼ÆÅÄͺ (12/21-25)

• From Planetesimals to Planets in Turbulent Protoplanetary Disks I. Onset of Runaway Growth

Æ»±Û½¨¸ã (12/28-1/1)

• Effects of Dynamical Evolution of Giant Planets on the Delivery of Atmophile Elements During Terrestrial Planet Formation

2/12

¾®µ×ÊݱѰìϺ (1/4-8)

• Near-Infrared Imaging Polarimetry of LkCa 15: A Possible Warped Inner Disk

²¡ÌîæÆ°ì (1/11-15)

• On the formation of compact planetary systems via concurrent core accretion and migration

¾¾ËÜÐһΠ(1/25-29)

• Comprehensive tests of artificial viscosities, their switches and derivative operators used in Smoothed Particle Hydrodynamics
• A Neptune-sized Exoplanet Consistent with a Pure Rock Composition

2/26

ÏÆÅÄÌÐ (1/18-22)

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

ĹëÀɧ (2/1-5)

• The Giant Impact Simulations with Density Independent Smoothed Particle Hydrodynamics

Æ»±Û½¨¸ã (2/15-19)

• The effect of orbital damping during planet migration on the Inclination and Eccentricity Distributions of Neptune Trojans

3/4

¾®µ×ÊݱѰìϺ (2/22-26)

• Constraints on the location of a possible 9th planet derived from the Cassini data
• Neptune's Orbital Migration Was Grainy, Not Smooth
• Evolution and Magnitudes of Candidate Planet Nine

3/11

¼ÆÅÄͺ (2/8-12)

• Origin of the chaotic motion of the Saturnian satellite Atlas

²¡ÌîæÆ°ì (2/29-3/4)

• Interaction Cross Sections and Survival Rates for Proposed Solar System Member Planet Nine
• Mean radius and shape of Pluto and Charon from New Horizons images

3/18

ÏÆÅÄÌÐ (3/7-11)

• Mercury (Hg) in meteorites: variations in abundance, thermal release profile, mass-dependent and mass-independent isotopic fractionation
• Dust diffusion and settling in the presence of collisions: Trapping (sub)micron grains in the midplane

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