Monday, August 12, 2019

1:30 PM–1:40 PM Welcoming Remarks

1:40 PM–2:00 PM Poster Presenters

2:00 PM–2:40 PM Douglas P. Hamilton (Univ. of Maryland, USA)†

1. Circumplanetary dust: Spokes in Saturn’s B ring ➤
   

2:40 PM–3:00 PM Srama Ralf (Univ. Stuttgart, Germany)

1. The 2014 and 2016 dust occultations observed by Cassini CDA ➤
   

3:00 PM–4:00 PM Poster Session/Coffee Break

4:00 PM–4:40 PM Takafumi Ootsubo (ISAS/JAXA)†

1. Cometary dust: A perspective from mid-infrared spectroscopy ➤
   

4:40 PM–5:00 PM Hiroshi Kimura (PERC/Chitech, Japan)

1. The morphological, elastic, and electric properties of dust aggregates in comets: A close look at COSIMA/Rosetta’s data on dust in comet 67P/Churyumov-Gerasimenko ➤
   

6:00 PM-8:00 PM Optional Dinner@Sakanadonya Uoichishouten

Tuesday, August 13, 2019

9:00 AM–9:40 AM John H. Debes (STScI, USA)†

1. Challenges for understanding dust in planetary systems 
   

9:40 AM–10:00 AM Aoi Takahashi (NINS Astrobiology Center, Japan)

1. Mineralogy of interplanetary dust investigated from mid-infrared spectroscopic observations with AKARI ➤
   

10:00 AM–11:00 AM Poster Session/Coffee Break

11:00 AM–11:20 AM Ludmilla Kolokolova (Univ. of Maryland, USA)

1. New techniques for computer modeling of light scattering by the dust layers on cosmic bodies ➤
   

11:20 AM–11:40 AM Yuna G. Kwon (Seoul National Univ., Korea)

1. Rotationally resolved infrared (3.0–4.0 μm) spectra of Jupiter Trojans ➤
   

11:40 AM–12:00 PM A Tour of PERC

12:00 PM–2:00 PM Lunch

2:00 PM–2:40 PM Christine H. Chen (STScI, USA)†

1. Characterizing dusty debris with the Gemini Planet Imager ➤
   

2:40 PM–3:00 PM Maximilian Sommer (Univ. of Stuttgart, Germany)

1. The effects of neighbouring planets on the formation of circumsolar resonant dust rings in the inner Solar System ➤
   

3:00 PM–4:00 PM Poster Session/Coffee Break

4:00 PM–4:40 PM Eric Pantin (Univ. of Florida, USA & CE Saclay, France)†

1. Infrared light polarization as a tool to study circumstellar disks dust properties ➤
   

4:40 PM–5:00 PM Ryo Tazaki (Tohoku Univ., Japan)

1. Probing dust aggregate structure in protoplanetary disks by millimeter-wave polarization ➤
   

6:00 PM-8:00 PM Optional Dinner@Arigatou

Wednesday, August 14, 2019

9:00 AM–9:20 AM François Ménard (Univ. Grenoble Alpes, France)

1. A micro-wave analogy experiment to measure the scattering properties of dust aggregates: Experimental set-up and first results for protoplanetary disks ➤
   

9:20 AM–9:40 AM Misako Tatsuuma (Univ. of Tokyo, Japan)

1. Tensile strength of porous dust aggregates in protoplanetary disks ➤
   

9:40 AM–10:00 AM Hiroshi Kobayashi (Nagoya Univ., Japan)

1. Collisional growth from dust to planets in a protoplanetary disk ➤
   

10:00 AM–11:00 AM Poster Session/Coffee Break

11:00 AM–11:40 AM Hiroshi Hidaka (ILTS/Hokkaido Univ., Japan)†

1. Reactive desorption of methanol from amorphous solid water at 10K 
   

11:40 AM–12:00 PM Jacek Krełowski (Center for Astronomy, Poland)

1. Dust particles interactions with interstellar molecules ➤
   

12:00 PM–1:30 PM Lunch

1:30 PM–5:30 PM Excursion@Naritasan

6:00 PM-9:00 PM Banquet@Chiba Beer Garden

Thursday, August 15, 2019

9:00 AM–9:40 AM Sebastian F. Hoenig (Univ. of Southampton, UK)†

1. Tori, disks, and winds: the infrared emission in active galactic nuclei ➤
   

9:40 AM–10:00 AM Takuro Tsuchikawa (Nagoya Univ., Japan)

1. An infrared spectroscopic study of silicate dust in heavily obscured AGNs with AKARI and Spitzer ➤
   

10:00 AM–11:00 AM Poster Session/Coffee Break

11:00 AM–11:20 AM Hiroyuki Hirashita (ASIAA, Taiwan)

1. Radiation-pressure-driven dust transport to galaxy halos at high redshift ➤
   

11:20 AM–11:40 AM Aleksandra Leśniewska (Adam Mickiewicz Univ., Poland)

1. Dust production in galaxies at z > 6 ➤
   

11:40 AM–12:00 PM Tsutomu T. Takeuchi (Nagoya Univ., Japan)

1. Far-infrared metal and dust emission in a galaxy at redshift ~ 8 ➤
   

12:00 PM–2:00 PM Lunch

2:00 PM–2:40 PM Julie Brisset (Univ. of Central Florida, USA)†

1. Levitating dust clouds on orbital platforms: Pathways to support the experimental calibration of interstellar dust models ➤
   

2:40 PM–3:00 PM Yanxia Xie (KIAA-PKU, China) — CANCELED

1. The widespread presence of nanometer-size dust grains in the interstellar medium of galaxies
   

3:00 PM–4:00 PM Poster Session/Coffee Break

4:00 PM–4:20 PM Thiem Hoang (KASI, Korea)

1. Rotational disruption as a new mechanism of dust destruction and implications ➤
   

4:20 PM–4:40 PM Joonas Herranen (Univ. of Helsinki, Finland)

1. Ensemble study on the efficient radiative alignment fraction of interstellar grains ➤
   

4:40 PM–5:00 PM Mitsuru Kokubo (Tohoku University, Japan)

1. Rapid luminosity decline and subsequent reformation of the innermost dust distribution in the changing-look AGN Mrk 590 ➤
   

6:00 PM-8:00 PM Optional Dinner@Kuimonoya Wan

Friday, August 16, 2019

9:00 AM–9:40 AM Cesare Cecchi Pestellini (INAF-OAPa, Italy)†

1. Amazing grains - The nature of interstellar dust as revealed by light scattering ➤
   

9:40 AM–10:00 AM Haibo Yuan (Beijing Normal Univ., China)

1. Dust studies in the era of precision Galactic astronomy ➤
   

10:00 AM–11:00 AM Poster Session/Coffee Break

11:00 AM–11:20 AM Ruining Zhao (NAOC, China)

1. The circumstellar dust shell around the likely progenitor star of SN 2017eaw ➤
   

11:20 AM–11:40 AM Kazuki Y. Nishida (Nagoya Univ., Japan)

1. Construction of a new galaxy spectral energy distribution model consistent with the evolution of dust ➤
   

11:40 AM–12:00 PM Sayaka K. Nagasaki (Nagoya Univ., Japan)

1. A new dust evolution model in galaxies with gas infall ➤
   

12:00 PM–2:00 PM Lunch

2:00 PM–2:40 PM Lía Corrales (Univ. of Michigan, USA)†

1. Mineralogy of interstellar dust with high resolution X-ray spectroscopy ➤
   

2:40 PM–3:00 PM Joshua M. Young (Univ. of North Texas, USA)

1. Evolution of crystalline phases and diffusion of elements in ion beam irradiation synthesized cosmic dust analogues ➤
   

3:00 PM–4:00 PM Poster Session/Coffee Break

4:00 PM–4:20 PM Norio Ota (Univ. of Tsukuba, Japan)

1. Graphene-molecule compared with fullerene-C60 in carbon-rich planetary nebula by quantum-chemical analysis ➤
   

4:20 PM–4:40 PM Aigen Li (Univ. of Missouri, USA)

1. Graphene and carbon nanotubes in the interstellar medium ➤
   

4:40 PM–4:50 PM Adjourning Remarks

Poster Presenters:

Tomomi Omura (Nagoya Univ., Japan)

1. Experimental study on compaction property of constituent material of primitive body ➤
   

Takayuki Hirai (PERC/Chitech, Japan)

1. In-situ measurement of the circumsolar dust ring around Earth’s orbit by IKAROS-ALADDIN ➤
   

Carsten Henselowsky (DLR, Germany)

1. German space science programme and international collaborations as Destiny+ Dust Analyzer ➤
   

Young-Dae Jung (Hanyang Univ., Korea)

1. Ion-driven instabilities of surface dust ion-acoustic waves in a dusty space plasma layer ➤
   

Yuto Nara (Tokyo Tech, Japan)

1. Delivery of ammonia ice to Ceres by pebble accretion ➤
   

Anna Di Palma (Japan Atomic Energy Agency, Japan)

1. Mosses as biomonitors of airborne dusts and their potential application for monitoring cosmic dusts ➤
   

Yuuya Nagaashi (Kobe Univ., Japan)

1. Measurements of the density of dust clusters forming in a granular stream using flash X-ray ➤
   

Takayuki Matsuura (Tokyo Tech, Japan)

1. Dust evolution in the protoplanetary disk around TW Hya ➤
   

Zhibo Jiang (PMO, China)

1. Gas-to-dust ratio influenced by massive star formation ➤
   

Hiroki Chihara (Osaka Sangyo Univ., Japan)

1. Synthesizing of amorphous silicate with mechanochemical method ➤
   

Gwenaelle Dufour (NASA GSFC, USA)

1. Astrochemical bistability 
   

Omima Osman (Univ. of Western Australia, Australia)

1. Variations in the dust destruction efficiency and dust sticking coefficient ➤
   

Mridusmita Buragohain (Univ. of Tokyo, Japan)

1. Investigation of interstellar polycyclic aromatic hydrocarbon molecules as carriers for mid-infrared emission bands: Combined approach ➤
   

N.B.

1. •Every speaker is assumed to welcome questions whenever arise.
   

2. •Poster presenters are given 1 minute each for oral presentations.
   

3. •The first 10 min. of each poster session is a core time for poster presentations.
   

4. •Invited speakers are marked with a dagger (†).
   

5. •Best poster awardees are marked with a ribbon ().
   

6. •A compilation of abstracts is available for download.
   

7. •Click on arrowheads (➤) to download associated presentations [authorized persons only].