Planet2017
Last-modified: 2018-05-11 (¶â) 13:23:11 (1031d)
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ÏÇÀ±¥»¥ß¥Ê¡¼2017 †
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Schedule & History †
ÆüÄø | astro-ph | ȯɽ |
Á°´ü Âè1²ó 4/4 | ÅÄÃæÍ¤´õ (3/20-24) | ÅÄÃæÍ¤´õ ¡Ö¼§µ¤Î®ÂÎÇÈ¶îÆ°¤Î¥¬¥¹ÏÇÀ±¤«¤é¤Î¼ÁÎÌÊü½Ð¡× |
Á°´ü Âè2²ó 4/11 | ²¡ÌîæÆ°ì(3/27-31) ¼ÆÅÄͺ(4/3-7) | Steven Rieder(AICS, RIKEN) ¡ÖJ1407b: a Super-Saturn or something else?¡× |
Á°´ü Âè3²ó 4/12 | ÏÂÅĹÀÆó¡ÊÀéÍÕ¹©Âç¡Ë ¡Ö¥À¥¹¥È¥¢¥°¥ê¥²¥¤¥È¤Î¾×ÆÍ¥·¥ß¥å¥ì¡¼¥·¥ç¥ó¡§À®Ä¹¤Ç¤¤ë¤Î¤Ç¤¤Ê¤¤¤Î¡©¡× | |
Á°´ü Âè4²ó 4/25 | ¾®µ×ÊݱѰìϺ(4/10-14)¡¡ ÏÆÅÄÌÐ(4/17-21) | ÏÆÅÄÌÐ ¡ÖAsteroids and their compositions¡× |
Á°´ü Âè5²ó 5/9 | ²®¸¶ÀµÇî(4/24-28) äÇÏ̤º»»Ò(5/1-5) | |
Á°´ü Âè6²ó 5/16 | Âíůϯ(5/8-12) | ²¡ÌîæÆ°ì ¡ÖHigh-Resolution N-body Simulations of Planet Formation¡× |
Á°´ü Âè7²ó 6/13 | ²¡¾å¾Í»Ò(5/15-19) ²¡ÌîæÆ°ì(5/22-26) ¼ÆÅÄͺ(5/29-6/2) ¾®µ×ÊݱѰìϺ(6/5-9) | ¼ÆÅÄͺ ¡ÖSpin of Protoplanets by Planetesimal accretion¡× |
Á°´ü Âè8²ó 7/4 | ÏÆÅÄÌÐ(6/12-16) ²®¸¶ÀµÇî(6/19-23) äÇÏ̤º»»Ò(6/26-30) | |
Á°´ü Âè9²ó 7/18 | Âíůϯ(7/3-7) ²¡¾å¾Í»Ò(7/10-14) | Ramon Brasser (ELSI) ¡ÖThe Cool and Distant Formation of Mars¡× |
Á°´ü Âè10²ó 7/27 | ²¡ÌîæÆ°ì(7/17-21) | äÇÏ̤º»»Ò ¡ÖGravitational Instability of a Porous Silicate Dust Disk¡× |
Á°´ü Âè11²ó 8/3 | Maxwell Cai (Leiden Observatory) ¡ÖDynamical Evolution of Multiplanetary Systems in Star Clusters¡× | |
¸å´ü Âè1²ó 9/5 | ¼ÆÅÄͺ(7/24-28) ¾®µ×ÊݱѰìϺ(7/31-8/4) ÏÆÅÄÌÐ(8/7-8/11) ²®¸¶ÀµÇî(8/14-8/18) | |
¸å´ü Âè2²ó 9/19 | Âíůϯ(8/28-9/1) ²¡ÌîæÆ°ì(9/4-8) | ¾®µ×ÊݱѰìϺ ¡ÖThe Final Stage of Terrestrial Planet Formation¡× |
¸å´ü Âè3²ó 10/10 | ¼ÆÅÄͺ(9/11-15) ¾®µ×ÊݱѰìϺ(9/18-22) ÏÆÅÄÌÐ(9/25-29) ²®¸¶ÀµÇî(10/2-6) | |
¸å´ü Âè4²ó 10/31 | ²®¸¶ÀµÇî | |
¸å´ü Âè5²ó 11/21 | Âíůϯ | |
¸å´ü Âè6²ó 12/5 | ÏÆÅÄÌÐ | |
¸å´ü Âè7²ó 12/19 | ²¡ÌîæÆ°ì | |
¸å´ü Âè8²ó 1/9 | ¼ÆÅÄͺ | |
¸å´ü Âè9²ó 1/23 | ¾®µ×ÊݱѰìϺ |
astro-ph ¥ê¥ó¥¯ †
ÅÄÃæÍ¤´õ (3/20-24)
- Reassessment of the Null Result of the HST Search for Planets in 47 Tucanae
- Assessing the Habitability of the TRAPPIST-1 System Using a 3D Climate Model
- The GTC exoplanet transit spectroscopy survey. VII. Detection of sodium in WASP-52b's cloudy atmosphere
- Formation of TRAPPIST-1 and other compact systems
- Testing the existence of optical linear polarization in young brown dwarfs
- The effect of the stellar absorption line centre-to-limb variation on exoplanet transmission spectrum observations
- Planetesimal formation by the streaming instability in a photoevaporating disk
²¡ÌîæÆ°ì(3/27-31)
- The stability of tightly-packed, evenly-spaced systems of Earth-mass planets orbiting a Sun-like star
- Water transport to circumprimary habitable zones from icy planetesimal disks in binary star systems
- Size and density sorting of dust grains in SPH simulations of protoplanetary discs
¼ÆÅÄͺ(4/3-7)
¾®µ×ÊݱѰìϺ(4/10-14)
- Plausible Compositions of the Seven TRAPPIST-1 Planets Using Long-term Dynamical Simulations
- The curiously warped mean plane of the Kuiper belt
- Limits on the Stability of TRAPPIST-1
- A Minimum Mass Nebula for M Dwarfs
- The Destruction of an Oort Cloud in a rich stellar cluster
ÏÆÅÄÌÐ(4/17-21)
²®¸¶ÀµÇî(4/24-28)
- Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets
- Acceleration of Cooling of Ice Giants by Condensation in Early Atmospheres
- Titan brighter at twilight than in daylight
- Avoiding resonance capture in multi-planet extrasolar systems
äÇÏ̤º»»Ò(5/1-5)
- 3D radiative transfer of intrinsically polarized dust emission based on aligned aspherical grains
- Survey of cold water lines in protoplanetary disks: indications of systematic volatile depletion
- A likely detection of a local interplanetary dust cloud passing near the Earth in the AKARI mid-infrared all-sky map
Âíůϯ(5/8-12)
- Composition of Early Planetary Atmospheres II: Coupled Dust and Chemical Evolution in Protoplanetary Disks
- Chemical enrichment of giant planets and discs due to pebble drift
- Evidence for universality in the initial planetesimal mass function
- N-body simulations of planet formation via pebble accretion I: First Results
²¡¾å¾Í»Ò(5/15-19)
- Dynamics of Porous Dust Aggregates and Gravitational Instability of Their Disk
- Detection of the Yarkovsky effect for C-type asteroids in the Veritas family
- Shape models and physical properties of asteroids
- Driven by Excess? Climatic Implications of New Global Mapping of Near-Surface Water-Equivalent Hydrogen on Mars
- The compositional diversity of non-Vesta basaltic asteroids
²¡ÌîæÆ°ì(5/22-26)
- Formation of Close-in Super-Earths by Giant Impacts: Effects of Initial Eccentricities and Inclinations of Protoplanets
- In situ accretion of gaseous envelopes on to planetary cores embedded in evolving protoplanetary discs
¼ÆÅÄͺ(5/29-6/2)
- Internal Structure of Giant and Icy Planets: Importance of Heavy Elements and Mixing
- Capture of free-floating planets by stellar systems
¾®µ×ÊݱѰìϺ(6/5-9)
- Cladistical analysis of the Jovian and Saturnian satellite systems
- Dynamics and Collisional Evolution of Closely Packed Planetary Systems
ÏÆÅÄÌÐ(6/12-16)
²®¸¶ÀµÇî(6/19-23)
- Stable habitable zones of single Jovian planet systems
- Exoplanets as probes of the winds of host stars: the case of the M dwarf GJ 436
- Eccentricity excitation and merging of planetary embryos heated by pebble accretion
- The California-Kepler Survey V. Peas in a Pod: Planets in a Kepler Multi-planet System are Similar in Size and Regularly Spaced
- A giant planet undergoing extreme ultraviolet irradiation by its hot massive-star host
- Cloud formation in metal-rich atmospheres of hot super-Earths like 55 Cnc e and CoRot7b
- Gap and rings carved by vortices in protoplanetary dust
äÇÏ̤º»»Ò(6/26-30)
- Low-velocity collision behaviour of clusters composed of sub-mm sized dust aggregates
- Submillimetre-sized dust aggregate collision and growth properties
- NanoRocks: Design and Performance of an Experiment Studying Planet Formation on the International Space Station
Âíůϯ(7/3-7)
- Generation of inclined protoplanetary discs and misaligned planets through mass accretion I: Coplanar secondary discs
- Energy Options for Future Humans on Titan
- Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics
- Centrifugally driven winds from protostellar accretion discs. I - Formulation and initial results
- Changes in orientation and shape of protoplanetary discs moving through an ambient medium
²¡¾å¾Í»Ò(7/10-14)
- Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core
- The highly active Anhur-Bes regions in the 67P/Churyumov - Gerasimenko comet: results from OSIRIS/ROSETTA observations
- The size distribution of Near Earth Objects larger than 10 meters
²¡ÌîæÆ°ì(7/17-21)
¼ÆÅÄͺ(7/24-28)
¾®µ×ÊݱѰìϺ(7/31-8/4)
- Reduced gas accretion on super-Earths and ice giants
- The Formation of Uranus and Neptune: Fine Tuning in Core Accretion
- Simulations of Small Solid Accretion onto Planetesimals in the Presence of Gas
ÏÆÅÄÌÐ(8/7-8/11)
- Ejection of Chondrules from Fluffy Matrices
- Early formation of planetary building blocks inferred from Pb isotopic ages of chondrules
²®¸¶ÀµÇî(8/14-8/18)
Âíůϯ(8/28-9/1)
- Probing the cold dust emission in the AB Aur disk: a dust trap in a decaying vortex?
- Gas vs dust radial extent in disks: the importance of their thermal interplay
²¡ÌîæÆ°ì(9/4-8)~