Planet2014
ÏÇÀ±¥»¥ß¥Ê¡¼2014 †
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Schedule & History †
ÆüÄø | astro-ph | ȯɽ |
Á°´ü Âè1²ó 4/8 | ¾®µ×ÊݱѰìϺ (2/24-28) ÀÐÄž°´î (3/17-21) ²¡ÌîæÆ°ì (3/24-28) ÏÆÅÄÌÐ (3/31-4/4) | |
Á°´ü Âè2²ó 4/15 | ¼ÆÅÄͺ (4/7-11) | |
Á°´ü Âè3²ó 5/13 | ÀÐÄž°´î (4/14-18) ¾®µ×ÊݱѰìϺ (4/21-25) | ĹëÀɧ ¡Ö¸¶»ÏÏÇÀ±·Ï±ßÈפˤª¤±¤ë¥À¥¹¥È¤ÎÀ®Ä¹¤ÈÄÀŤª¤è¤ÓshearÉÔ°ÂÄê¤Î²ÄǽÀ¡× |
Á°´ü Âè4²ó 5/20 | ²¡ÌîæÆ°ì (4/28-5/2) ÏÆÅÄÌÐ (5/5-9) | ¹õß·¹Ì²ð(ÀéÍÕ¹©¶ÈÂç³Ø) ¡Öð¨ÀнÅÇú·â´ü¤Ë¤ª¤±¤ë¶âÀ±¡¢Ãϵ塢²ÐÀ±¤ÎÂ絤¿Ê²½¡× |
Á°´ü Âè5²ó 5/30 | ¾¾ËÜÐһΠ(5/12-16) ĹëÀɧ (5/19-23) | ¾¾ËÜÐһΠ¡Ö¸¶»ÏÏÇÀ±¤Î¾×ÆÍ¤Ëȼ¤¦Î¥¿´Î¨¤Î¿Ê²½¤Ë¤Ä¤¤¤Æ¡× |
Á°´ü Âè6²ó 6/13 | ¼ÆÅÄͺ (5/26-30) ÀÐÄž°´î (6/2-6) | ¾®µ×ÊݱѰìϺ¡ÖFormation of Close-in Super-Earths by Giant Impacts¡× |
Á°´ü Âè7²ó 6/20 | ¾®µ×ÊݱѰìϺ (6/9-13) | |
Á°´ü Âè8²ó 6/27 | ÏÆÅÄÌÐ (6/16-20) | ÀÐÄž°´î ¡Ö¥À¥¹¥ÈÄÀÅÂÀ®Ä¹²áÄø¤Ë¤ª¤±¤ë Rayleigh-Taylor ÉÔ°ÂÄêÀ¡× |
Á°´ü Âè9²ó 7/4 | ²¡ÌîæÆ°ì (6/23-27) | |
Á°´ü Âè10²ó 7/18 | ¾¾ËÜÐһΠ(6/30-7/4) ĹëÀɧ (7/7-11) | |
¸å´ü Âè1²ó 9/5 | ¼ÆÅÄͺ (7/14-18) ¾®µ×ÊݱѰìϺ (7/28-8/1) ²¡ÌîæÆ°ì (8/4-8) ÏÆÅÄÌÐ (8/11-15) ¾¾ËÜÐһΠ(8/18-22) ĹëÀɧ (8/25-29) | |
¸å´ü Âè2²ó 9/19 | ÀÐÄž°´î (7/21-25) ¼ÆÅÄͺ (9/1-5) | |
¸å´ü Âè3²ó 10/3 | ÀÐÄž°´î (9/8-12) ¾®µ×ÊݱѰìϺ (9/15-19) ²¡ÌîæÆ°ì (9/22-26) | ÏÆÅÄÌÐ ¡ÖEarly Solar System Chronology¡× |
¸å´ü Âè4²ó 10/10 | ÏÆÅÄÌÐ (9/29-10/3) | |
¸å´ü Âè5²ó 10/17 | ¾¾ËÜÐһΠ(10/6-10) | ²¡ÌîæÆ°ì ¡ÖN-body simulation with UPC¡× |
¸å´ü Âè6²ó 11/7 | ĹëÀɧ (10/13-17) °ë¹¾ËãΤ (10/20-24) | ¼ÆÅÄͺ ¡Ö¸¶»ÏÏÇÀ±¤Î¼«Å¾ÆÃÀ¡× |
¸å´ü Âè7²ó 11/14 | ĹëÀîÌ÷¹É (10/27-31) ÀÐÄž°´î (11/3-7) | |
¸å´ü Âè8²ó 11/28 | ¼ÆÅÄͺ (11/10-14) ¾®µ×ÊݱѰìϺ (11/17-21) | |
¸å´ü Âè9²ó 12/5 | ²¡ÌîæÆ°ì (11/24-28) | ĹëÀɧ ¡Ö¥À¥¹¥È¤Î¾×ÆÍÇ˲õ¤ò¹Íθ¤·¤¿±ßÈפνÅÎÏÉÔ°ÂÄê¤Î²ÄǽÀ¤Î¸¦µæ¤Ë¸þ¤±¤Æ¡× |
¸å´ü Âè10²ó 12/12 | ÏÆÅÄÌÐ (12/1-5) | |
¸å´ü Âè11²ó 12/19 | ¾¾ËÜÐһΠ(12/8-12) | |
¸å´ü Âè12²ó 1/9 | ĹëÀɧ (12/15-19) °ë¹¾ ËãΤ (12/22-26) | |
¸å´ü Âè13²ó 1/16 | ĹëÀîÌ÷¹É (12/29-1/2) ÀÐÄž°´î (1/5-9) | |
¸å´ü Âè14²ó 1/23 | ÂçµÜÀµ»Î (NAOJ) ¡Ö¶áÀÖ³°¥É¥Ã¥×¥é¡¼Ë¡¤Ë¤è¤ëÄã¼ÁÎÌÀ±¼þ¤ê¤Î¥Ï¥Ó¥¿¥Ö¥ëÃϵ巿ÏÇÀ±Ãµº÷¡× | |
¸å´ü Âè15²ó 1/30 | ¼ÆÅÄͺ (1/12-16) | ĹëÀîÌ÷¹É ¡ÖPopulation synthesis calculations: The effect of gas accretion¡× |
¸å´ü Âè16²ó 2/6 | ²¡ÌîæÆ°ì (1/26-30) | |
¸å´ü Âè17²ó 2/13 | ¾®µ×ÊݱѰìϺ (1/19-23) ÏÆÅÄÌÐ (2/2-6) | ¾®µ×ÊݱѰìϺ ¡ÖFormation of Close-in Super-Earths by Giant Impacts¡× |
¸å´ü Âè18²ó 2/20 | ¾¾ËÜÐһΠ(2/9-13) | ¾¾ËÜÐһΠ¡Ö½é´ü¥é¥ó¥À¥à®Å٤εðÂç¾×ÆÍÃʳ¬¤ÎÏÇÀ±½¸ÀѤؤαƶÁ¡× |
¸å´ü Âè19²ó 2/27 | ÀÐÄž°´î ¡Ö¥À¥¹¥ÈÁؽÅÎÏÉÔ°ÂÄêÀ¤Î¿ôÃÍ¥·¥ß¥å¥ì¡¼¥·¥ç¥ó¡× | |
¸å´ü Âè20²ó 3/6 | ĹëÀɧ (2/16-20) | |
¸å´ü Âè21²ó 3/13 (ÍýÏÀ¥³¥í¥¥¦¥à¤È¹çƱ) | ÉðÆ£¶³Ç·(¹©³Ø±¡Âç) ¡Ö¸¶»ÏÏÇÀ±·Ï±ßÈפξܺٹ½Â¤¤È¿ÇÈĹ´Ñ¬¡× Man Hoi Lee(The University of Hong Kong) ¡ÖThe Puzzle of the Pluto Satellite System¡× | |
¸å´ü Âè22²ó 3/27 | °ë¹¾ËãΤ (2/23-27) ĹëÀîÌ÷¹É (3/2-6) ÀÐÄž°´î (3/9-13) |
astro-ph ¥ê¥ó¥¯ †
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
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
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)
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
¾®µ×ÊݱѰìϺ (6/9-13)
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
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
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)
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)
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)
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
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
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
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
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
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
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)
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
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
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
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)
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
¼ÆÅÄͺ (1/12-16)
²¡ÌîæÆ°ì (1/26-30)
- Gas giant planets as dynamical barriers to inward-migrating super-Earths
- The Dynamical Evolution of the Asteroid Belt
¾®µ×ÊݱѰìϺ (1/19-23)
ÏÆÅÄÌÐ (2/2-6)
- Compound Chondrules fused Cold
- Micron-scale D/H heterogeneity in chondrite matrices: a signature of the pristine solar system water?
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
ĹëÀɧ (2/16-20)
°ë¹¾ËãΤ (2/23-27)
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)