Subaru Measurements of the Rossiter-McLaughlin Effect and Direct Imaging Observations for Transiting Planetary Systems Norio Narita (NAOJ) and SEEDS/HiCIAO/AO188.

Slides:

Advertisements

Similar presentations

Origin & Evolution of Habitable Planets: Astronomical Prospective D.N.C. Lin University of California, Santa Cruz, KIAA, Peking University, with Pathways.

Advertisements

Spin-Orbit Misalignment in Planetary Systems and Magnetic Star -- Disk Interaction IAU Astrophysics of Planetary Systems, Torino, Italy, Oct.14, 2010 Dong.

Open Clusters: At The Interface of Stellar Evolution and Stellar Dynamics Robert D. Mathieu University of Wisconsin - Madison.

Kozai Migration Yanqin Wu Mike Ramsahai. The distribution of orbital periods P(T) increases from 120 to 2000 days Incomplete for longer periods Clear.

Tidal Dynamics of Transiting Exoplanets Dan Fabrycky UC Santa Cruz 13 Oct 2010 Photo: Stefen Seip, apod/ap At: The Astrophysics of Planetary Systems:

Norio Narita National Astronomical Observatory of Japan

Planet Characterization by Transit Observations Norio Narita National Astronomical Observatory of Japan.

1. Global Properties 2. The Rossiter-McClaughlin Effect II. Results from Transiting Planets.

Mapping the Realm of Hot Jupiters Bun’ei Sato, Shigeru Ida （ Titech ）, Eri Toyota （ Kobe Univ. ）, Masashi Omiya （ Tokai Univ. ）, Debra Fischer （ SFSU ）,

Introduction of the RV subcategory of the SEEDS project 1.57 Yasuhiro H. Takahashi GUAS/NAOJ and the RV subcategory member.

Status of RV Sub-Catelogy Norio Narita (NAOJ) Yasuhiro H. Takahashi (Univ. of Tokyo) Bun’ei Sato (Titech) Ryuji Suzuki (NAOJ) and SEEDS/HiCIAO/AO188 teams.

1 Determining the internal structure of extrasolar planets, and the phenomenon of retrograde planetary orbits Rosemary Mardling School of Mathematical.

Tidal Influence on Orbital Dynamics Dan Fabrycky 4 Feb, 2010 Collaborators: Scott Tremaine Eric Johnson Jeremy Goodman Josh.

Extrasolar Planets More that 500 extrasolar planets have been discovered In 46 planetary systems through radial velocity surveys, transit observations,

Transits and Starspots Jeremy Tregloan-Reed Ph.D. Research Student Supervisor: John Southworth.

Transit Timing Variations Szilárd CsizmadiaJena University Institut for Planetary Research, German Aerospace Center Berlin, Germany

Effects of Kozai Migration on Formation of Close-in Planets Soko Matsumura (University of Maryland) Douglas P. Hamilton (University of Maryland)

Stellar obliquities in exoplanetary systems

PX437 EXOPLANETS Outline 1.Before Exoplanets 2.Detecting exoplanets 1.Direct imaging 2.Reflex Motion of Star 3.Transiting exoplanets 3.Planet Formation.

PX437 EXOPLANETS Outline 1.Before Exoplanets 2.Detecting exoplanets 1.Direct imaging 2.Reflex Motion of Star 3.Transiting exoplanets 3.Planet Formation.

Reflected Light From Extra Solar Planets Modeling light curves of planets with highly elliptical orbits Daniel Bayliss, Summer Student, RSAA, ANU Ulyana.

Norio Narita (NAOJ Fellow) Special Thanks to IRD Transit Team Members

Chaotic Case Studies: Sensitive dependence on initial conditions in star/planet formation Fred C. Adams Physics Department University of Michigan With:

1 29 August 2012IAU SS13, Beijing Stellar Physics Revealed by Planetary Transits Willie Torres Harvard-Smithsonian Center for Astrophysics IAU General.

Further Science of IRD: Synergy with Transiting Planets

Discriminating Migration Mechanisms of Tilted or Eccentric Planetary Systems Norio Narita (NAOJ/University of Hawaii)

Subaru HDS Transmission Spectroscopy of the Transiting Extrasolar Planet HD b The University of Tokyo Norio Narita collaborators Yasushi Suto, Joshua.

Observational Studies for Understanding Planetary Migration Norio Narita National Astronomical Observatory of Japan.

Jean-Pierre needs to be brought up to date on what’s really going on in astronomy these days!

Simultaneous Subaru/MAGNUM Observations of Extrasolar Planetary Transits Norio Narita (U. Tokyo, JSPS Fellow, Japan) Collaborators Y. Ohta, A. Taruya,

Search for Transiting Planets around Nearby M Dwarfs Norio Narita (NAOJ)

Aligned, Tilted, Retrograde Exoplanets and their Migration Mechanisms Norio Narita (JSPS Fellow) National Astronomical Observatory of Japan.

Team D: Kaniesha Stern Charles Ammon Jowers III Tracy Diggs.

Toward Detections and Characterization of Habitable Transiting Exoplanets Norio Narita (NAOJ)

Diversity of Data in the Search for Exoplanets Rachel Akeson NASA Exoplanet Science Institute California Institute of Technology.

Testing Planet Migration Theories by Observations of Transiting Exoplanetary Systems 1/39 University of Tokyo Norio Narita.

Discriminating Planetary Migration Mechanisms by Direct Imaging Norio Narita National Astronomical Observatory of Japan on behalf of SEEDS/HiCIAO/AO188.

December 7, 1631December 9, 1874 December 4, 1639December 6, 1882 June 6, 1761June 8, 2004 June 3, 1769June 6, 2012 Transits of Venus across the disk of.

The Transit Method: Results from the Ground

Characterization of Planets: Mass and Radius (Transits Results Part I) I. Results from individual transit search programs II. Interesting cases III. Global.

Spectroscopic Transits

Spin-Orbit Alignment Angles and Planetary Migration of Jovian Exoplanets Norio Narita National Astronomical Observatory of Japan.

Poster 67. A PHOTOMETRIC TRANSIT SEARCH FOR PLANETS AROUND COOL STARS FROM THE ITALIAN ALPS: RESULTS FROM A FEASIBILITY STUDY A. Bernagozzi (1), E. Bertolini.

Detection of Extrasolar Giant Planets Hwihyun Kim 03/30/06.

The University of Tokyo Norio Narita

Transiting Exoplanet Search and Characterization with Subaru's New Infrared Doppler Instrument (IRD) Norio Narita (NAOJ) On behalf of IRD Transit Group.

Exoplanet Discovery Joshua Pepper Vanderbilt University Keivan Stassun, Rob Siverd, Leslie Hebb, Phil Cargile - Vanderbilt University Rudi Kuhn – The University.

Sarah, Ellie, Adan and Sruthy. The Transit Method.

Newton’s Law of Universal Gravitation && Kepler’s Laws of Planetary Motion.

Observation vs. Inferences The Local Environment.

Companion Candidates around Transiting Planetary Systems: SEEDS First/Second Year Results Norio Narita (NAOJ) Yasuhiro H. Takahashi (Univ. of Tokyo) and.

SEEDS プロジェクトによるトランジット惑星系の直接撮像観測成田憲保 ( 国立天文台 ) 、高橋安大 ( 東大 ) 、佐藤文衛 ( 東工大 ) 、鈴木竜二、神鳥亮、田村元秀 ( 国立天文台 ) 、ほか SEEDS/HiCIAO/AO188 チーム.

Lectures 2 and 3 1. Kepler’s three laws 2. Use parallax, spectroscopic parallax, and the distance modulus to calculate distances to planetary systems 3.

Results of HARPS-N observations of the transiting system Qatar-1 in GAPS E. Covino M. Esposito, M. Barbieri, S. Desidera, L. Mancini, V. Nascimbeni, J.

Презентацию подготовила Хайруллина Ч.А. Муслюмовская гимназия Подготовка к части С ЕГЭ.

Measuring the Spin-Orbit Alignments of Transiting Exoplanetary Systems: The Case for TrES-1 Norio Narita, Keigo Enya, Bun'ei Sato, Yasuhiro Ohta, Joshua.

IAU253 Transiting Planets: May

1 / 12 Simultaneous Spectroscopic & Photometric Observations of a Transit of TrES-1b Norio Narita (UT, JSPS Fellow) Collaborators K. Enya (JAXA), B. Sato.

Pre-Cursor Data Needed for JWST Transit and Eclipse Observations

Past and Future Studies of Transiting Extrasolar Planets

Subaru Measurements of the Rossiter-McLaughlin Effect

RM 2 7 +RM 2 4 RM 7 3 +RM 1 6 RM 5 2 +RM 2 4 RM 1 3 +RM5 2.

Citing your sources.

News from the McDonald Observatory Planet Search

Norio Narita National Astronomical Observatory of Japan

The University of Tokyo Norio Narita

Оюутны эрдэм шинжилгээний хурлын зорилго:

Subaru HDS Ground-based Transmission Spectroscopy

Presentation transcript:

Subaru Measurements of the Rossiter-McLaughlin Effect and Direct Imaging Observations for Transiting Planetary Systems Norio Narita (NAOJ) and SEEDS/HiCIAO/AO188 teams

How to discriminate migration models Disk-Planet interaction Planet-Planet scattering Kozai migration orbital eccentricity by radial velocity spin-orbit alignment angle by the RM effect

Can we discriminate two models? Planet-Planet scattering Kozai migration Additional information from direct imaging! We introduce a procedure to discriminate two planetary migration models by direct imaging.

HAT-P-7 (Kepler-2) Result Come to Poster 3.9! N E NN et al. (2010)