Planet2017

Last-modified: 2018-05-11 (¶â) 13:23:11 (73d)

Planet

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Schedule & History †

2016ǯÅÙ 2015ǯÅÙ 2014ǯÅÙ

astro-ph ¥ê¥ó¥¯ †

4/4

ÅÄÃæͤ´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

4/11

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)

• The cool and distant formation of Mars

4/25

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)

• Testing the chondrule-rich accretion model for planetary embryos using calcium isotopes

5/9

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

5/16

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

6/13

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

7/4

ÏÆÅÄÌÐ(6/12-16)

• Radially resolved simulations of collapsing pebble clouds in protoplanetary discs

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

7/18

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

7/27

²¡ÌîæÆ°ì(7/17-21)

• On the Impact Origin of Phobos and Deimos I: Thermodynamic and Physical Aspects

9/5

¼ÆÅÄͺ(7/24-28)

• Seasonal Mass Transfer on the Nucleus of Comet 67P/Chuyumov-Gerasimenko

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)

• What pebbles are made of: Interpretation of the V883 Ori disk

9/19

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)~

• Dust-driven viscous ring-instability in protoplanetary disks

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