Planet2015
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Schedule & History †
ÆüÄø | astro-ph | ȯɽ |
Á°´ü Âè1²ó 4/3 | ¾®µ×ÊݱѰìϺ (3/23-27) | |
Á°´ü Âè2²ó 4/10 | ¼ÆÅÄͺ (3/16-20) ²¡ÌîæÆ°ì (3/30-4/3) | |
Á°´ü Âè3²ó 4/17 | ÏÆÅÄÌÐ (4/6-10) | äÇÏ̤º»»Ò ¡ÖHiCIAO¤òÍѤ¤¤¿ÀÖ³°ÀþÊи÷´Ñ¬¤Ë¤è¤ëIM Lup¤ÎÀ±¼þ±ßÈפδѬ¡× |
Á°´ü Âè4²ó 4/24 | ¾¾ËÜÐһΠ(4/13-17) | |
Á°´ü Âè5²ó 5/1 | ĹëÀɧ (4/20-24) | |
Á°´ü Âè6²ó 5/8 | ĹëÀîÌ÷¹É (4/27-5/1) | |
Á°´ü Âè7²ó 5/15 | °ë¹¾ËãΤ (5/4-8) | |
Á°´ü Âè8²ó 5/22 | ¼ÆÅÄͺ (5/11-15) | ÏÆÅÄÌÐ ¡ÖOxygen isotopes in the solar nebula¡× |
Á°´ü Âè9²ó 5/29 | Æ»±Û½¨¸ã (5/18-22) | ²¡ÌîæÆ°ì ¡ÖFormation and evolution of Pluto's small satellites¡× |
Á°´ü Âè10²ó 6/5 | ¾®µ×ÊݱѰìϺ (5/25-29) | |
Á°´ü Âè11²ó 6/11 | Wladimir Lyra (Caltech/JPL) | |
Á°´ü Âè12²ó 6/19 | ²¡ÌîæÆ°ì (6/1-5) ÏÆÅÄÌÐ (6/8-12) | ĹëÀɧ ¡Ö¹â¥À¥¹¥È-¥¬¥¹Èæ¤Î¸¶»ÏÏÇÀ±·Ï±ßÈפǷÁÀ®¤µ¤ì¤ëÈùÏÇÀ±¤Î¥µ¥¤¥º¡× |
Á°´ü Âè13²ó 6/26 | ¾¾ËÜÐһΠ(6/15-19) | |
Á°´ü Âè14²ó 7/10 | ĹëÀɧ (6/22-26) °ë¹¾ËãΤ (6/29-7/3) | ĹëÀîÌ÷¹É ¡ÖChondrule Formation¡× |
Á°´ü Âè15²ó 7/17 | ¼ÆÅÄͺ (7/6-10) | |
Á°´ü Âè16²ó 7/24 | Æ»±Û½¨¸ã (7/13-17) | |
Á°´ü Âè17²ó 7/31 | ¾®µ×ÊݱѰìϺ (7/20-24) | ¾®µ×ÊݱѰìϺ ¡ÖSPACING OF KEPLER PLANETS: SCULPTING BY DYNAMICAL INSTABILITY¡× |
¸å´ü Âè1²ó 9/18 | ²¡ÌîæÆ°ì (7/27-31) °ë¹¾ËãΤ (8/24-28) ¼ÆÅÄͺ (8/31-9/4) Æ»±Û½¨¸ã (9/7-11)¡¡ | |
¸å´ü Âè2²ó 9/25 | ÏÆÅÄÌÐ (8/3-7) ĹëÀɧ (8/17-21) | ¼ÆÅÄͺ ¡ÖPlanet formation: statistics of spin rates and obliquities of extrasolar planets¡× |
¸å´ü Âè3²ó 10/2 | ¾¾ËÜÐһΠ(8/10-14) ¾®µ×ÊݱѰìϺ (9/14-18) | °ë¹¾ËãΤ ¡Ö¡ÈThe Mass Distribution Function of Planets¡É (Renu Malhotra, 2015)¡× |
¸å´ü Âè4²ó 10/9 | ²¡ÌîæÆ°ì (9/21-25) | ¾¾ËÜÐһΠ¡ÖÏÇÀ±¤Îµ°Æ»°ÂÄêÀ¤Î¥é¥ó¥À¥à®Åٰ͸À¡× |
¸å´ü Âè5²ó 10/30 | ¾¾ËÜÐһΠ(10/5-9) °ë¹¾ËãΤ (10/19-23) | |
¸å´ü Âè6²ó 11/6 | ÏÆÅÄÌÐ (9/28-10/2) ĹëÀɧ (10/12-16) ¼ÆÅÄͺ (10/26-10/30) | |
¸å´ü Âè7²ó 11/13 | Æ»±Û½¨¸ã (11/2-6) | Æ»±Û½¨¸ã ¡Ö¹âÌ©ÅÙÏÇÀ±¥ê¥ó¥°¤Î½ÅÎÏÇ´À¡× |
¸å´ü Âè8²ó 11/20 | ¾®µ×ÊݱѰìϺ (11/9-13) | ÏÆÅÄÌÐ ¡ÖGrains in the early Solar System¡× |
¸å´ü Âè9²ó 12/11 | ²¡ÌîæÆ°ì (11/16-20) ÏÆÅÄÌÐ (11/23-27) ¾¾ËÜÐһΠ(11/30-12/5) | ²¡ÌîæÆ°ì ¡ÖVOLATILE DELIVERY TO PLANETS FROM WATER-RICH PLANETESIMALS AROUND LOW-MASS STARS¡× |
¸å´ü Âè10²ó 12/18 | ĹëÀɧ (12/7-11) | |
¸å´ü Âè11²ó 12/25 | °ë¹¾ËãΤ (12/14-18) | |
¸å´ü Âè12²ó 1/8 | ¼ÆÅÄͺ (12/21-25) Æ»±Û½¨¸ã (12/28-1/1) | ĹëÀɧ ¡ÖCritical Dust-to-Gas Ratio Revisited for Gravitational Instability¡× |
¸å´ü Âè13²ó 2/12 | ¾®µ×ÊݱѰìϺ (1/4-8) ²¡ÌîæÆ°ì (1/11-15) ¾¾ËÜÐһΠ(1/25-29) | ¾®µ×ÊݱѰìϺ ¡ÖFormation of Close-in Terrestrial Planets by Giant Impacts: The Basic Scaling Laws¡× |
¸å´ü Âè14²ó 2/19 | Marc Fouchard ¡ÖThe Oort cloud: shape and dynamics¡× | |
¸å´ü Âè15²ó 2/26 | ÏÆÅÄÌÐ (1/18-22) ĹëÀɧ (2/1-5) Æ»±Û½¨¸ã (2/15-19) | |
¸å´ü Âè16²ó 3/4 | ¾®µ×ÊݱѰìϺ (2/22-26) | |
¸å´ü Âè17²ó 3/11 | ¼ÆÅÄͺ (2/8-12) ²¡ÌîæÆ°ì (2/29-3/4) | ¼ÆÅÄͺ ¡ÖÈùÏÇÀ±½¸ÀѤˤè¤ë¸¶»ÏÏÇÀ±¤Î¼«Å¾¡× |
¸å´ü Âè18²ó 3/18 | ÏÆÅÄÌÐ (3/7-11) |
astro-ph ¥ê¥ó¥¯ †
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
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
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
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
ĹëÀɧ (4/20-24)
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
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
Æ»±Û½¨¸ã (5/18-22)
¾®µ×ÊݱѰìϺ (5/25-29)
²¡ÌîæÆ°ì (6/1-5)
ÏÆÅÄÌÐ (6/8-12)
- Sequential planet formation in the HD 100546 protoplanetary disk?
- Internal Structure of Asteroids Having Surface Shedding due to Rotational Instability
¾¾ËÜÐһΠ(6/15-19)
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)
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
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
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)
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?
ÏÆÅÄÌÐ (8/3-7)
ĹëÀɧ (8/17-21)
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?
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
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)
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)
¼ÆÅÄͺ (10/26-10/30)
- A population-based Habitable Zone perspective
- The Pluto system: Initial results from its exploration by New Horizons
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
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
²¡ÌîæÆ°ì (11/16-20)
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)
°ë¹¾ËãΤ (12/14-18)
¼ÆÅÄͺ (12/21-25)
Æ»±Û½¨¸ã (12/28-1/1)
¾®µ×ÊݱѰìϺ (1/4-8)
²¡ÌîæÆ°ì (1/11-15)
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
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)
Æ»±Û½¨¸ã (2/15-19)
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
¼ÆÅÄͺ (2/8-12)
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
ÏÆÅÄÌÐ (3/7-11)