PPT-Potential for Characterization of Transiting Planets with JWST

Nick Cowan Northwestern Study Analysis Group 10 SAGX What is the full diversity of planet properties needed to characterize and understand the climate of shortperiod exoplanets Which measurement suites and how much observing time are needed to characterize the climate of transiting planets . Nick Cowan . (Northwestern). Study Analysis Group 10 (SAG-X). What is the full diversity of planet properties needed to characterize and understand the climate of short-period exoplanets? . Which measurement suites and how much observing time are needed to characterize the climate of transiting planets? . To Be A Planet, Or Not To Be?. Physical Characteristics . 5 - Recognized Dwarf Planets. Ceres, Pluto, . Haumea. , . Makemake. , Eris. Classification Criteria. Directly orbits the Sun (not a satellite). Lecture 7. By reading this chapter, you will . learn. 4-1. How ancient astronomers attempted to explain the motions of the planets. 4-2 . What led Copernicus to a Sun-centered model of planetary motion. The outer planets are called Jovian or Jupiter-like.. These planets are made of gas and are several times more massive than the Earth.. The Jovian planets grew to present size in about 10 million years.. R. epeatability. WFC3 – spatial . s. can mode analysis – . work in progress. Mark Swain, Pieter . Deroo. , . Kiri. . Wagstaff. IPAC . JWST workshop . 3/11/14. Jet Propulsion Laboratory, California Institute of Technology. Transits and SONG. Angelle . Tanner. . The Transit Method. Venus. Transiting the Sun. Information from Transits. Transit Frequency gives us . ORBIT SIZE. Orbit Size with Star Temperature tells us if planet is in . Studies for Transiting . Exoplanets. Norio Narita. National Astronomical Observatory of Japan. Outline. Introduction of Science of Transiting . Exoplanets. What’s New and What’s Going on Now?. Near Future Prospects. Exoplanets. Norio Narita (NAOJ). Transit of Venus on June 5, 2012 at Hawaii. Outline. Introduction of Transit. Current Status of Studies. . of Transiting . Exoplanets. Further . Studies of Transiting . JWST Community Lecture. Jay Anderson, STScI. Nov 29, 2016. Astrometric Calibration. What is Distortion?. Any “non-conformal” mapping . . (shift, scale, rotation). Linear terms (“skew”). Non-linear terms. Goddard Space Flight Center, Greenbelt MD. Joint Base Andrews, MD. Johnson Space . Center,. Houston TX. Northrop-Grumman, Los Angeles CA. Panama Canal. ESA Kourou, French Guiana. L2. JWST. Road to. The stars. Studies for Transiting . Exoplanets. Norio Narita. National Astronomical Observatory of Japan. Outline. Introduction of Science of Transiting . Exoplanets. What’s New and What’s Going on Now?. Near Future Prospects. NIRCam. Grism Mode for Transit Observations. C. Beichman, Dimitra . Touli. ,. Gautam . Vasisht. , Roger Smith. Tom Greene. 4 March 2014. JWST grism simulator. 1. Caltech Detector Testbed. Caltech testbed (Roger Smith) projects simulated spectra and other images onto HgCdTe array to assess precision photometry for transits, weak lensing, etc. for Explorer concepts, JWST, WFIRST, EUCLID. . 2013 NASA Annual IV&V Workshop . Chris Lescinsky IV&V Analyst, TASC. Rick Hess, IV&V Analyst, TASC. 9/10/2013. Agenda. JWST Overview (ORBIT and ISIM). JWST Key Elements. ISIM Layout. JIST Test Bed. 40 Balmer jump and slopes 4000 age Very young population x0000- emission lines UV slopes Old star populations in high-z objects eg Egami et al 2005 Eyles et al 2005 Richard et al 2011 Zeng e