The Grand Tour of Exoplanets The New Worlds around Other Stars The Grand Tour of Exoplanets The New Worlds around Other Stars Dániel Apai Space Telescope.

Slides:



Advertisements
Similar presentations
PLAnetary Transits and Oscillations of stars H. Rauer 1, C. Catala 2, D. Pollacco 3, S. Udry 4 and the PLATO Team 1: Institut für Planetenforschung, DLR.
Advertisements

Ge/Ay133 What can transit observations tell us about (exo)-planetary science? Part II – “Spectroscopy” & Atmospheric Composition/Dynamics Kudos to Heather.
Destination: A Planet like Earth Caty Pilachowski IU Astronomy Mini-University, June 2011 Caty Pilachowski Mini-University 2011.
Overview on Extra Solar Planets Rahul I. Patel PHY 599 – Grad Seminar Oct. 18 th 2010.
Exoplanet Atmospheres: Insights via the Hubble Space Telescope Nicolas Crouzet 1, Drake Deming 2, Peter R. McCullough 1 1 Space Telescope Science Institute.
Lecture 1: Introduction & Methods 1.Introduction 2.Techniques for discovery & study 3.The NASA Kepler mission Planetary Systems Orbiting Diverse Stars.
Tim Healy Tony Perry Planet Survey Mission. Introduction Finding Planets Pulsar Timing Astrometry Polarimetry Direct Imaging Transit Method Radial Velocity.
Exploring a Nearby Habitable World …. Orbiting an M-dwarf star Drake Deming NASA’s Goddard Space Flight Center.
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.
Ge/Ay133 What have radial velocity surveys told us about (exo)-planetary science?
DEPARTMENT OF PHYSICS AND ASTRONOMY Extra-solar planets Dr. Matt Burleigh.
Habitable Planets Astronomy 315 Professor Lee Carkner Special Topic.
All About Exoplanets Dimitar D. Sasselov Harvard-Smithsonian Center for Astrophysics.
The Search for Earth-sized Planets Around Other Stars The Kepler Mission (2009)
From Brown Dwarfs to Giant Planets Stan Metchev (Stony Brook Astronomy Group) Stan Metchev (Stony Brook Astronomy Group) Artist’s rendition of a brown.
Extrasolar Planets.I. 1.What do we know and how do we know it. 2.Basic planetary atmospheres 3.Successful observations and future plans.
Lecture 11: The Discovery of the World of Exoplanets
First direct image of extrasolar planets billion miles.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
Lecture 16: Searching for Habitable Planets: Remote Sensing Methods and parameters we can measure Mean density measurements: internal structure Measurements.
PX437 EXOPLANETS Solar wobble Displacement of the Sun over 45-year period, as observed from 33 light-years away. NASA JPL.
Extrasolar planets. Finding planets Finding planets around other stars is hard!  need to look for something very faint very close to something that is.
3677 Life in the Universe: Extra-solar planets
HOW TO DETECT EXOPLANETS EAAE General Assembly ESO HQ, Garching bei München, Germany March 4, 2005 March 4, 2005 Anders Västerberg European Association.
6.5 Other Planetary Systems Our goals for learning: How do we detect planets around other stars? How do extrasolar planets compare with those in our own.
PTYS 214 – Spring 2011  Review Guide has been uploaded to class website  Review Session – Monday May 2 nd ? Thursday May 6 th ? – time??  Class website:
Norio Narita (NAOJ Fellow) Special Thanks to IRD Transit Team Members
Lecture 34. Extrasolar Planets. reading: Chapter 9.
(Institute for Advanced Study)
Chapter 12.  Extrasolar Systems
Further Science of IRD: Synergy with Transiting Planets
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ The First Images of Exoplanets New images show planets orbiting bright young nearby.
Transits of exoplanets – Detection & Characeterization
The Search for Extrasolar Planets Since it appears the conditions for planet formation are common, we’d like to know how many solar systems there are,
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.
Are We Alone? Chris De Pree RARE CATS June The Questions Are there other planetary systems? How do we detect other planetary systems? What is Life?

Extrasolar Planet Search OGLE-2005-BLG-390Lb The Age of Miniaturization: Smaller is Better OGLE-2005-BLG-390Lb is believed to be the smallest exoplanet.
Lecture 14: The Discovery of the World of Exoplanets Indirect methods for planet detection The Astrometric method The Doppler shift method The Transit.
Extra-Solar Planet Populations Stephen Eikenberry 4 November 2010 AST
Extra Solar Planets ASTR 1420 Lecture 17 Sections 11.2.
Gliese 581b Gliese 581gGliese 581eEarth Gliese 581f Gliese 581c Gliese 581d.
Extrasolar Planets Exo planets are planets outside the Solar System. They orbit another star. 861 confirmed…18,000 identified, but likely billions exist.
CHARA Collaboration Year-Eight Science Review Host stars investigations with VEGA/CHARA R. Ligi, D. Mourard, A.-M. Lagrange, K. Perraut Observatoire de.
Life in the Milky Way: Panel Discussion Wesley A. Traub Chief Scientist, NASA’s Exoplanet Exploration Program Jet Propulsion Laboratory, California Institute.
Detection of Extrasolar Giant Planets Hwihyun Kim 03/30/06.
Homework 8 Due: Monday, Nov. 28, 9:00 pm, Exam 2: Weds., Nov. 30.
Lecture 34 ExoPlanets Astronomy 1143 – Spring 2014.
Transiting Exoplanet Search and Characterization with Subaru's New Infrared Doppler Instrument (IRD) Norio Narita (NAOJ) On behalf of IRD Transit Group.
Eva Meyer MPIA-Student-Workshop, Italy Various information from different detection methods.
Exoplanet Characterization with JWST
How Other Projects Will Enable JWST Transiting Planet Science David Charbonneau (Harvard) 18 November 2015.
NASA’s Kepler and K2 Missions:
Discoveries in Planetary Sciencehttp://dps.aas.org/education/dpsdisc/ First Rocky Exoplanet Detected Most known exoplanets are large and have low densities.
Extra-Solar Planet Populations George Lebo 10 April 2012 AST
2003 UB313: The 10th Planet?. Extra-Solar or Exoplanets Planets around stars other than the Sun Difficult to observe Hundreds discovered (> 2000 so far)
2003 UB313: The 10th Planet?. Extra-Solar or Exoplanets Planets around stars other than the Sun Difficult to observe Hundreds discovered (> 2000 so far)
How many of these ? Out there. At least One in Six stars has an Earth-size planet Francois Fressin, G. Torres, D. Charbonneau & the team.
Spitzer Space Telescope Mww-1 Warm Spitzer and Astrobiology Presented to NASA Astrobiology Institute Planetary System Formation Focus Group Michael Werner.
Characterisation of hot Jupiters by secondary transits observed with IRIS2 Lucyna Kedziora-Chudczer (UNSW) George Zhou (Harvard-Smithsonian CfA) Jeremy.
PX437 EXOPLANETS Solar wobble Displacement of the Sun over 45-year period, as observed from 33 light-years away. NASA JPL.
Chapitre 1- Introduction
Nature of Exoplanets 26 October 2016.
3677 Life in the Universe: Extra-solar planets
Past and Future Studies of Transiting Extrasolar Planets
NASA discovery (22th February 2017):
New Worlds: Detection of Exoplanet systems
Extra Solar Planets - Worlds around Other Stars
Presentation transcript:

The Grand Tour of Exoplanets The New Worlds around Other Stars The Grand Tour of Exoplanets The New Worlds around Other Stars Dániel Apai Space Telescope Science Institute Dániel Apai Space Telescope Science Institute

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Fictional Planets Tatooine / Star Wars B612, Dune, Terminus, Tatooine Hundreds more listed on Wikipedia page

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Age of Planets

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 R Jup ≈ 11 R Earth R sun ≈ 10 R jup M sun ≈ 1000 M jup M Jup ≈ 320 M Earth

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 The Planet Zoo No Fancy Names - just plain old lowercase alphabet, excluding a What is a planet anyway? HR8799d - 3rd planet discovered around the star HR8799 Poor Pluto isn’t.

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, Kaj Strand: Nearby triple star system 61 Cygni has a companion 16 M Jup Indirect detection is a possibility; tiny signals are easily misinterpreted. The First “Detections” Peter van de Kamp, Sproul Observatory, Perturbations in Barnard’s Star track ⇒ 1.6 M Jup planet Never confirmed... many other claims followed

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 PSR bcd Alex Wolszczan PSR (Becker et al. 1992) Rocky planets can be at odd places and may form easily. Wolszczan et al b: 0.02 M earth at 0.19 AU with P=25d c: 4.1 M earth at 0.36 AU with P=67d d: 3.8 M earth at 0.46 AU with P=98d Pulsar, timing variations

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, Peg Mayor & Queloz 1995 Nature Sun-like star + Jupiter-mass Planet! 4.2 day orbital period! Lessons: 1) Planets can be very close to their host stars 2) Planets migrate 3) Expect the Unexpected G2 sun-like star, V=5.5 mag - Radial Velocity

GJ 876

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 GJ 876 System Delfosse et al Marcy et al Correia et al GJ876b: 2.6 M J planet at 0.2 AU with 61 day period (1998) GJ876c: 0.83 M J planet at 0.13 AU with 30 day period (1998) GJ876d: 0.02 M J =6.3 M E planet at AU with 1.9 day period (2005) M4 red dwarf, V=10.2 mag - Radial Velocity

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 GJ 876 System What we learned: 1) Planets can form around cool red dwarfs 2) Giant planets in resonant orbit (2:1) 2) Multiple planets with very different masses Jupiter-sized planets are rare around low-mass stars Delfosse et al Marcy et al Correia et al GJ876b: 2.6 M J planet at 0.2 AU with 61 day period (1998) GJ876c: 0.83 M J planet at 0.13 AU with 30 day period (1998) GJ876d: 0.02 M J =6.3 M E planet at AU with 1.9 day period (2005) M4 red dwarf, V=10.2 mag - Radial Velocity

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Gl581 - The Second Habitable world? GJ581b: 16 M E planet at 0.04 AU with 5.4 day period Bonfils et al. (2005) GJ581c: 5 M E planet at 0.07 AU with 13 day period Udry et al. (2007) GJ581d: 8 M E planet at 0.22 AU with 67 day period Udry et al. (2007) GJ581e: 2 M E planet at 0.03 AU with 3.1 day period Mayor et al. (2009) M3 red dwarf, V=10.6 mag - Radial Velocity

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Gl581 - The Second Habitable world? M3 red dwarf, V=10.6 mag - Radial Velocity

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Gl581 - The Second Habitable world? GJ581b: 16 M E planet at 0.04 AU with 5.4 day period Bonfils et al. (2005) GJ581c: 5 M E planet at 0.07 AU with 13 day period Udry et al. (2007) GJ581d: 8 M E planet at 0.22 AU with 67 day period Udry et al. (2007) GJ581e: 2 M E planet at 0.03 AU with 3.1 day period Mayor et al. (2009) M3 red dwarf, V=10.6 mag - Radial Velocity

ESO

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Gl581 - The Second Habitable world? Habitable planets around cool red dwarfs? GJ581b: 16 M E planet at 0.04 AU with 5.4 day period Bonfils et al. (2005) GJ581c: 5 M E planet at 0.07 AU with 13 day period Udry et al. (2007) GJ581d: 8 M E planet at 0.22 AU with 67 day period Udry et al. (2007) GJ581e: 2 M E planet at 0.03 AU with 3.1 day period Mayor et al. (2009) M3 red dwarf, V=10.6 mag - Radial Velocity The habitability of the GJ581 system remains debated.

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 HD189733b HD209458b K1 star, V=7.7 mag - Radial Velocity G0 sun-like star, V=7.7 mag - Radial Velocity HD b: 0.6 M J planet at AU with 3.5 day period (1999) HD b: 1.1 M J at 0.03 AU with 2.2 day period Planetary Transits and Eclipses provide Information on Atmospheric Composition!

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 HD189733b HD209458b CO Swain et al. (2009) CH 4, Water Swain et al. (2009) Water Tinetti et al. (2007) Spitzer Space Telescope HST Water, methane, CO Multiple teams, HST, Spitzer

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Corot-1b G0 star, V=14 mag - Transit Rogers et al Too bright! 1 M Jup planet at AU with 1.5 day period

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 WASP-18 F9 sun-like star, V=9.3 mag - Transit Survey WASP-18b: 10.4 M J at 0.02 AU with 0.94 day period Hellier et al Tidal interactions - planets swallowed in less than a million year?

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 GJ 436 From Sasselov 2008

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 GJ 1214b GJ1214b: 6.55 M E planet at AU with 1.6 day period Red dwarf, 13 pc, 0.16M ⊙ - Transit Survey Charbonneau et al Transit Depth: 1.3%

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Charbonneau et al. 2009

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 GJ 1214b GJ1214b: 6.55 M E planet at AU with 1.6 day period Charbonneau et al Transit Depth: 1.3% Planet Radius = 12% of R star (R pl / R star ) 2 =1.3% R star = 0.2 R sun = 0.2 Rsun × 109 R earth [R sun = 109 R earth ] R GJ1214b = 12% of 20% of 109 R earth = 2.6 R earth Volume? (2.6) 3 = 17.6 Earth Volume Density: 6.55 M earth / 17.8 V Earth = 37% of Earth’s Density! Red dwarf, 13 pc, 0.16M ⊙ - Transit Survey

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 GJ 1214b - The Ocean World GJ1214b: 5.7 M E planet at AU with 1.6 day period Nature Mass: 6.55 Earth Mass Density: 37% of Earth Density Stellar Luminosity: 0.3% of Sun Semi-major axis: AU Insolation: 15× that of Earth Equilibrium Temperature: A B = 0 T eq = 555 K = 539 F A B = 0.75 T eq = 393 K = 247 F Red dwarf, 13 pc, 0.16M ⊙ - Transit Survey

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Chauvin et al MASS1207b - The Little Brown Dwarf and the Big Planet 2MASS1207b ~8 M Jup Brown dwarf, 62 pc, 0.025M ⊙ - Direct Imaging Planetary-mass Objects may form in Different Ways Temperature - Brightness - Radius Inconsistency

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Fomalhaut A3 star, 7 pc, 2.1 M ⊙ - Direct Imaging Mass < 3 M Jup Proj. separation: 115 AU Kalas et al Contribution from Scattered Light Unknown nature

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Golimowski et al. Kalas & Jewitt

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Beta Pic Lagrange et al Beta Pictoris A6 star, 19 pc, 1.8 M ⊙ - Direct Imaging Mass ~ 8 M Jup Proj. separation: 8 AU To be confirmed

Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 HR 8799 bcd Marois et al VLT/NACO A5 star, 39 pc, 1.5M ⊙ - Direct Imaging Marois et al HR8799b: 5-11 M J planet 68 AU (P~460yr) HR8799c: 7-13 M J planet at 38 AU (P~190yr) HR8799d: 7-13 M J planet at 24 AU (P~100yr) Perplexing System - Very High Relative Planet mass at very large separations!

Chauvin et al Marois et al MASS1207 Beta Pic Lagrange et al Kalas et al Grand Tour of Exoplanets Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010 Daniel Apai / Space Telescope Science Institute Hubble Science Briefings - March 11, 2010

The Grand Tour of Exoplanets - Vast Diversity Observed Dániel Apai Space Telescope Science Institute Dániel Apai Space Telescope Science Institute Summary - Super-Jupiters, Neptunes, Super-Earths Earths, - Planets close to the Habitable Zone - Earth-sized Planets - Atmospheric Properties and Composition Exciting Times for Planets! - Keep an Eye on NASA’s Kepler Mission!