Signal processing in Python for the detection and characterization of extrasolar planets

Size: px
Start display at page:

Download "Signal processing in Python for the detection and characterization of extrasolar planets"

Transcription

1 Signal processing in Python for the detection and characterization of extrasolar planets Institut d astrophysique spatial Université Paris-Sud August 2011

2 1 Personal background

3 1 Personal background

4 Areas of research Science Extrasolar planets Stellar physics

5 Areas of research Science Extrasolar planets Stellar physics Techniques Adaptive optics Doppler spectrometry (radial velocimetry) High-precision photometry Long-baseline stellar interferometry

6 The choice of Python Frustrations with IDL 6.2 (2006) not (or poorly) interactive graphical windows for data inspection only low to moderate-quality graphics for publications failed to make a Fresnel-propagation library work properly costs more than a laptop

7 The choice of Python Frustrations with IDL 6.2 (2006) not (or poorly) interactive graphical windows for data inspection only low to moderate-quality graphics for publications failed to make a Fresnel-propagation library work properly costs more than a laptop Data-processing languages widely used for astronomy proprietay: IDL, Matlab open-source: Java, Python (promoted by the STScI), Scilab, Yorick...

8 1 Personal background

9 Transit of Mercury in front of the Sun Solar Heliospheric Observatory 7 May 2003

10 Transit of an exoplanet F F = ( ) 2 Rp R Jupiter 10 2 Earth 10 4

11 The Corot space mission Cnes mission + European partners + Brazil (165 M ) 27-cm diameter telescope, 3.5 o 2.8 o field of view 4 CCD detectors ( nm) Launched 27 Dec for 3+3 years Polar orbit at an altitude of 900 km Science: asteroseismology + exoplanets

12 Corot-2 light curve 78 transits in 152 days! Alonso et al., A&A 482, L21 (2008)

13 Corot-2b: transit and characteristics Average transit Planet s portrait Radius = ± R J Mass = 3.53 ± 0.24 M J Density = 1.50 ± 0.18 Period = ± d Semi-major axis = AU Host-star = G7 V

14 1 Personal background

15 Light curve prefiltering

16 Detection by matched-filtering

17 Fitting a trapezoid model

18 Individual transit check

19 Handling 10,000 light curves

20 1 Personal background

21 Corot-8b direct model

22 Corot-8b inverse model

23 1 Personal background

24 Recent and future work HTML output replaced by a MySQL database (done) Coding in C the cross-correlation function (future) PDF reports for every light curve using ReportLab (future)

25 Recent and future work HTML output replaced by a MySQL database (done) Coding in C the cross-correlation function (future) PDF reports for every light curve using ReportLab (future) Underway: implementation of a Bayesian approach with MCMC computations (PyMC?)

26 Recent and future work HTML output replaced by a MySQL database (done) Coding in C the cross-correlation function (future) PDF reports for every light curve using ReportLab (future) Underway: implementation of a Bayesian approach with MCMC computations (PyMC?) Notebooks in Python Have tried Sage and TeXmacs as Python interfaces to produce notebooks.

27 Python for teaching? For programming in L3?... C# chosen instead.

28 Python for teaching? For programming in L3?... C# chosen instead. For data display in L3?... Matlab chosen instead.

29 Python for teaching? For programming in L3?... C# chosen instead. For data display in L3?... Matlab chosen instead. For signal processing in M1?... Matlab chosen instead.

30 Python for teaching? For programming in L3?... C# chosen instead. For data display in L3?... Matlab chosen instead. For signal processing in M1?... Matlab chosen instead. Signal processing in M2?... Yes! using Pylab and IPython.

Helioseismology: GONG/BiSON/SoHO

Helioseismology: GONG/BiSON/SoHO Helioseismology: GONG/BiSON/SoHO Asteroseismology: Solar-like oscillations in other stars Study stars of different Masses, Ages and Chemical Composition Stellar Structure and Evolution Solar-like oscillations

More information

Searching for Other Worlds

Searching for Other Worlds Searching for Other Worlds Lecture 32 1 In-Class Question What is the Greenhouse effect? a) Optical light from the Sun is reflected into space while infrared light passes through the atmosphere and heats

More information

Lecture #15: Plan. Telescopes (cont d) Effects of Earth s Atmosphere Extrasolar planets = Exoplanets

Lecture #15: Plan. Telescopes (cont d) Effects of Earth s Atmosphere Extrasolar planets = Exoplanets Lecture #15: Plan Telescopes (cont d) Effects of Earth s Atmosphere Extrasolar planets = Exoplanets Resolving Power (review) The bigger the size of the telescope, the better it is at discerning fine details

More information

II Planet Finding.

II Planet Finding. II Planet Finding http://sgoodwin.staff.shef.ac.uk/phy229.html 1.0 Introduction There are a lot of slides in this lecture. Much of this should be familiar from PHY104 (Introduction to Astrophysics) and

More information

Extrasolar planets. Lecture 23, 4/22/14

Extrasolar planets. Lecture 23, 4/22/14 Extrasolar planets Lecture 23, 4/22/14 Extrasolar planets Extrasolar planets: planets around other stars Also called exoplanets 1783 exoplanets discovered as of 4/21/14 Orbitting 1105 different stars Number

More information

EXOPLANET DISCOVERY. Daniel Steigerwald

EXOPLANET DISCOVERY. Daniel Steigerwald EXOPLANET DISCOVERY Daniel Steigerwald WHAT IS AN EXOPLANET? An exoplanet is a planet outside of our solar system Extrastellar Rogue 1853 Planets 1162 planetary systems 473 Multiple planetary systems HISTORY

More information

EXONEST The Exoplanetary Explorer. Kevin H. Knuth and Ben Placek Department of Physics University at Albany (SUNY) Albany NY

EXONEST The Exoplanetary Explorer. Kevin H. Knuth and Ben Placek Department of Physics University at Albany (SUNY) Albany NY EXONEST The Exoplanetary Explorer Kevin H. Knuth and Ben Placek Department of Physics University at Albany (SUNY) Albany NY Kepler Mission The Kepler mission, launched in 2009, aims to explore the structure

More information

Alternative Pre- Observation Catalogue for Photometric Follow- Up of Transiting Exoplanets

Alternative Pre- Observation Catalogue for Photometric Follow- Up of Transiting Exoplanets Alternative Pre- Observation Catalogue for Photometric Follow- Up of Transiting Exoplanets Terreka S Hart Tennessee State University Advisor: Dr John A Johnson University of Hawai i - Institute for Astronomy

More information

Importance of the study of extrasolar planets. Exoplanets Introduction. Importance of the study of extrasolar planets

Importance of the study of extrasolar planets. Exoplanets Introduction. Importance of the study of extrasolar planets Importance of the study of extrasolar planets Exoplanets Introduction Planets and Astrobiology (2017-2018) G. Vladilo Technological and scientific spin-offs Exoplanet observations are driving huge technological

More information

Lecture #15: Plan. Telescopes (cont d) Effects of Earth s Atmosphere Extrasolar planets = Exoplanets

Lecture #15: Plan. Telescopes (cont d) Effects of Earth s Atmosphere Extrasolar planets = Exoplanets Lecture #15: Plan Telescopes (cont d) Effects of Earth s Atmosphere Extrasolar planets = Exoplanets Collecting Area Light bucket : the bigger the area of the telescope s mirror or lens, the more photons

More information

Chapter 13 Lecture. The Cosmic Perspective. Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc.

Chapter 13 Lecture. The Cosmic Perspective. Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc. Chapter 13 Lecture The Cosmic Perspective Seventh Edition Other Planetary Systems: The New Science of Distant Worlds 13.1 Detecting Planets Around Other Stars Our goals for learning: Why is it so challenging

More information

Astronomy 101 Lab: Hunt for Alien Worlds

Astronomy 101 Lab: Hunt for Alien Worlds Name: Astronomy 101 Lab: Hunt for Alien Worlds Be prepared to make calculations in today s lab. Laptops will also be used for part of the lab, but you aren t required to bring your own. Pre-Lab Assignment:

More information

2010 Pearson Education, Inc.

2010 Pearson Education, Inc. Thought Question Suppose you found a star with the same mass as the Sun moving back and forth with a period of 16 months. What could you conclude? A. It has a planet orbiting at less than 1 AU. B. It has

More information

III The properties of extrasolar planets

III The properties of extrasolar planets III The properties of extrasolar planets (as of early 2016) http://sgoodwin.staff.shef.ac.uk/phy229.html 3.0 Introduction This lecture will discuss what we have found so far. It is important to remember

More information

Pan-Planets with PANSTARRS1. And : CfA, John Hopkins Uni., UK Consortium, Centr. Uni. Taiwan

Pan-Planets with PANSTARRS1. And : CfA, John Hopkins Uni., UK Consortium, Centr. Uni. Taiwan Pan-Planets with PANSTARRS1 And : CfA, John Hopkins Uni., UK Consortium, Centr. Uni. Taiwan Panoramic Survey Telescope and Rapid Response System The renaissance of wide-field imaging Wide-field imaging

More information

Michaël Gillon (Université de Liège, Belgium)

Michaël Gillon (Université de Liège, Belgium) 12th Meeting of the FNRS Contact Group Astronomie & Astrophysique 17 May 2011 Planetarium, Brussels Michaël Gillon (Université de Liège, Belgium) michael.gillon@ulg.ac.be ~1% pour Soleil + Jupiter Brown

More information

The Search for Habitable Worlds Lecture 3: The role of TESS

The Search for Habitable Worlds Lecture 3: The role of TESS The Search for Habitable Worlds Lecture 3: The role of TESS David W. Latham Lucchin PhD School, Asiago, 26 June 2013 A aaaaaaaa Dave Latham, Science Director, CfA AAAAAAAAAAAA Selected for launch in 2017

More information

Astrometric Detection of Exoplanets

Astrometric Detection of Exoplanets Astrometric Detection of Exoplanets Angles & Coordinates: 1 full circle = 360 degrees 1 degree = 60 arcminutes 1 arcminute = 60 arcseconds ~ 1 inch @ 100 yards (2.908 cm at 100 meters) 1 milliarcsec (mas)

More information

Credit: NASA/Kepler Mission/Dana Berry. Exoplanets

Credit: NASA/Kepler Mission/Dana Berry. Exoplanets Credit: NASA/Kepler Mission/Dana Berry Exoplanets Outline What is an exoplanet? Why are they interesting? How can we find them? Exolife?? The future... Jon Thaler Exoplanets 2 What is an Exoplanet? Most

More information

Detection of Exoplanets Using the Transit Method

Detection of Exoplanets Using the Transit Method Detection of Exoplanets Using the Transit Method De nnis A fanase v, T h e Geo rg e W a s h i n g t o n Un i vers i t y, Washington, DC 20052 dennisafa@gwu.edu Abstract I conducted differential photometry

More information

EXOPLANETS. Aurélien CRIDA

EXOPLANETS. Aurélien CRIDA EXOPLANETS Aurélien CRIDA EXOPLANETS Giordano Bruno said that the many stars are like our Sun, with planets like our Earth, inhabited as well (in de l'infinito universo e mondi (1574) ). He was burnt alive

More information

Gravitational microlensing. Exoplanets Microlensing and Transit methods

Gravitational microlensing. Exoplanets Microlensing and Transit methods Gravitational microlensing Exoplanets Microlensing and s Planets and Astrobiology (2016-2017) G. Vladilo May take place when a star-planet system crosses the visual of a background star, as a result of

More information

Kepler s Multiple Planet Systems

Kepler s Multiple Planet Systems Kepler s Multiple Planet Systems TITech & Kobe Univ. February 2018 Jack J. Lissauer NASA Ames Outline Solar System & Exoplanets Kepler Mission Kepler planets and planetery systems Principal Kepler findings

More information

Planets in other Star Systems

Planets in other Star Systems Planets in other Star Systems test out how planets are formed with more examples first extrasolar planet observed in 1995. In Jan 2000, 28 observed and now >3700 confirmed (10/2017). Many systems with

More information

Planet Detection! Estimating f p!

Planet Detection! Estimating f p! Planet Detection! Estimating f p! Can We See Them?! Not easily! Best cases were reported in late 2008! Will see these later! Problem is separating planet light from star light! Star is 10 9 times brighter

More information

Detecting Other Worlds with a Backyard Telescope! Dennis M. Conti Chair, AAVSO Exoplanet Section

Detecting Other Worlds with a Backyard Telescope! Dennis M. Conti Chair, AAVSO Exoplanet Section Detecting Other Worlds with a Backyard Telescope! Dennis M. Conti Chair, AAVSO Exoplanet Section www.astrodennis.com The Night Sky Q: Which stars have one or more planets (exoplanets) around them? A: Most

More information

Doppler Technique Measuring a star's Doppler shift can tell us its motion toward and away from us.

Doppler Technique Measuring a star's Doppler shift can tell us its motion toward and away from us. Doppler Technique Measuring a star's Doppler shift can tell us its motion toward and away from us. Current techniques can measure motions as small as 1 m/s (walking speed!). Sun motion due to: Jupiter:

More information

Astronomy 330 HW 2. Outline. Presentations. ! Kira Bonk ascension.html

Astronomy 330 HW 2. Outline. Presentations. ! Kira Bonk  ascension.html Astronomy 330 This class (Lecture 11): What is f p? Eric Gobst Suharsh Sivakumar Next Class: Life in the Solar System HW 2 Kira Bonk http://www.ufodigest.com/news/0308/ ascension.html Matthew Tenpas http://morphman.hubpages.com/hub/alien-

More information

Interferometry & Asteroseismology of Solar-like Stars

Interferometry & Asteroseismology of Solar-like Stars Interferometry & Asteroseismology of Solar-like Stars (+ their Connection to Exoplanets) Daniel Huber NASA Ames Research Center Feb 11 2014 Supergiants Giants Hot Dwarfs White Dwarfs Cool Dwarfs Griffith

More information

PLAnetary Transits and Oscillations of stars

PLAnetary Transits and Oscillations of stars PLATO: Contribución n española PLAnetary Transits and Oscillations of stars J. Miguel Mas-Hesse Centro de Astrobiología (CSIC-INTA) 29 de junio 2011 Introduction PLATO: PLAnetary Transits and Oscillations

More information

Lecture 12: Extrasolar planets. Astronomy 111 Monday October 9, 2017

Lecture 12: Extrasolar planets. Astronomy 111 Monday October 9, 2017 Lecture 12: Extrasolar planets Astronomy 111 Monday October 9, 2017 Reminders Star party Thursday night! Homework #6 due Monday The search for extrasolar planets The nature of life on earth and the quest

More information

Can We See Them?! Planet Detection! Planet is Much Fainter than Star!

Can We See Them?! Planet Detection! Planet is Much Fainter than Star! Can We See Them?! Planet Detection! Estimating f p! Not easily! Best cases were reported in late 2008! Will see these later! Problem is separating planet light from star light! Star is 10 9 times brighter

More information

Lecture 8. October 25, 2017 Lab 5

Lecture 8. October 25, 2017 Lab 5 Lecture 8 October 25, 2017 Lab 5 News Lab 2 & 3 Handed back next week (I hope). Lab 4 Due today Lab 5 (Transiting Exoplanets) Handed out and observing will start Friday. Due November 8 (or later) Stellar

More information

Observations of Extrasolar Planets

Observations of Extrasolar Planets Observations of Extrasolar Planets Hamilton 2005 Shay Zucker Observations of Extrasolar Planets Spectroscopic detection of exoplanets Emerging properties of the sample Transiting planets Future prospects

More information

The Doppler Method, or Radial Velocity Detection of Planets: I. Technique

The Doppler Method, or Radial Velocity Detection of Planets: I. Technique ASTs309L The Doppler Method, or Radial Velocity Detection of Planets: I. Technique 1. Keplerian Orbits 2. Spectrographs/Doppler shifts 3. Precise Radial Velocity measurements ASTs309L The Doppler Effect:

More information

The Physics of Exoplanets

The Physics of Exoplanets The Physics of Exoplanets Heike Rauer Institut für Planetenforschung, DLR, Berlin-Adlershof, Zentrum für Astronomie und Astrophysik, TU Berlin Formation in protoplanetary disk, migration Loss of primary,

More information

Detection and characterization of exoplanets from space

Detection and characterization of exoplanets from space Detection and characterization of exoplanets from space Heike Rauer 1,2, 1:Institute for Planetary Research, DLR, Berlin 2:Center for Astronomy and Astrophysics, TU Berlin Exoplanet Space Missions and

More information

Indirect Methods: gravitational perturbation of the stellar motion. Exoplanets Doppler method

Indirect Methods: gravitational perturbation of the stellar motion. Exoplanets Doppler method Indirect Methods: gravitational perturbation of the stellar motion Exoplanets The reflex motion of the star is proportional to M p /M * This introduces an observational bias that favours the detection

More information

Plato, Euclid and the New Hard X-Ray mission

Plato, Euclid and the New Hard X-Ray mission Schiaparelli and his Legacy Meeting on Future planetary, scientific and robotic space missions Biblioteca Nazionale Universitaria, Torino, 21/10/2010 Template reference : 100181670S-EN Plato, Euclid and

More information

Chapter 13 Other Planetary Systems. The New Science of Distant Worlds

Chapter 13 Other Planetary Systems. The New Science of Distant Worlds Chapter 13 Other Planetary Systems The New Science of Distant Worlds 13.1 Detecting Extrasolar Planets Our goals for learning Why is it so difficult to detect planets around other stars? How do we detect

More information

Actuality of Exoplanets Search. François Bouchy OHP - IAP

Actuality of Exoplanets Search. François Bouchy OHP - IAP Actuality of Exoplanets Search François Bouchy OHP - IAP How detect extrasolar planets? Two main difficulties : 1 A tiny angular separation 0.75 arcsec Sun Jupiter at 4 light years 4 Sun Jupiter at 100

More information

The Transit Method: Results from the Ground

The Transit Method: Results from the Ground The Transit Method: Results from the Ground Results from individual transit search programs The Mass-Radius relationships (internal structure) Global Properties The Rossiter-McClaughlin Effect There are

More information

Planets in other Star Systems

Planets in other Star Systems Planets in other Star Systems test out how planets are formed with more examples first extrasolar planet observed in 1995. In Jan 2000, 28 observed and now >3700 confirmed (3/2018). Many systems with 2

More information

Science Olympiad Astronomy C Division Event National Exam

Science Olympiad Astronomy C Division Event National Exam Science Olympiad Astronomy C Division Event National Exam University of Nebraska-Lincoln May 15-16, 2015 Team Number: Team Name: Instructions: 1) Please turn in all materials at the end of the event. 2)

More information

Habitability Outside the Solar System. A discussion of Bennett & Shostak Chapter 11 HNRS 228 Dr. H. Geller

Habitability Outside the Solar System. A discussion of Bennett & Shostak Chapter 11 HNRS 228 Dr. H. Geller Habitability Outside the Solar System A discussion of Bennett & Shostak Chapter 11 HNRS 228 Dr. H. Geller 1 Chapter Overview Distant Suns (11.1) Life cycle of stars and their habitability zones Extrasolar

More information

Detection of Exoplanets by Amateur Astronomers

Detection of Exoplanets by Amateur Astronomers Detection of Exoplanets by Amateur Astronomers September 17, 2015 by Dennis M. Conti email: dennis_conti@hotmail.com 1 Background Exoplanet (Extrasolar Planet) a planet orbiting a distant host star First

More information

The light curve of the exoplanet transit of GJ 436 b

The light curve of the exoplanet transit of GJ 436 b The light curve of the exoplanet transit of GJ 436 b Dana Simard 06179344 Phys 315 Term Project Lab Partner: Natasha Urbancic April 5th, 2013 Abstract The transit of the exoplanet GJ 436 b was observed

More information

The Problem. Until 1995, we only knew of one Solar System - our own

The Problem. Until 1995, we only knew of one Solar System - our own Extrasolar Planets Until 1995, we only knew of one Solar System - our own The Problem We had suspected for hundreds of years, and had confirmed as long ago as the 1800s that the stars were extremely distant

More information

Exoplanet Search Techniques: Overview. PHY 688, Lecture 28 April 3, 2009

Exoplanet Search Techniques: Overview. PHY 688, Lecture 28 April 3, 2009 Exoplanet Search Techniques: Overview PHY 688, Lecture 28 April 3, 2009 Course administration final presentations Outline see me for paper recommendations 2 3 weeks before talk see me with draft of presentation

More information

Finding Extra-Solar Earths with Kepler. William Cochran McDonald Observatory

Finding Extra-Solar Earths with Kepler. William Cochran McDonald Observatory Finding Extra-Solar Earths with Kepler William Cochran McDonald Observatory Who is Bill Cochran? Senior Research Scien;st McDonald Observatory Originally interested in outer planet atmospheres Started

More information

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

Search for Transiting Planets around Nearby M Dwarfs. Norio Narita (NAOJ) Search for Transiting Planets around Nearby M Dwarfs Norio Narita (NAOJ) Outline Introduction of Current Status of Exoplanet Studies Motivation for Transiting Planets around Nearby M Dwarfs Roadmap and

More information

Exomoons around transiting exoplanets

Exomoons around transiting exoplanets UNIVERSITY OF SZEGED THE FACULTY OF SCIENCE AND INFORMATICS DEPARTMENT OF EXPERIMENTAL PHYSICS DOCTORAL SCHOOL IN PHYSICS Exomoons around transiting exoplanets PhD thesis Author: Supervisors: Attila Simon,

More information

Lab 5: Searching for Extra-Solar Planets

Lab 5: Searching for Extra-Solar Planets Lab 5: Searching for Extra-Solar Planets Until 1996, astronomers only knew about planets orbiting our sun. Though other planetary systems were suspected to exist, none had been found. Now, thirteen years

More information

Chapter 13 Other Planetary Systems. Why is it so difficult to detect planets around other stars? Brightness Difference

Chapter 13 Other Planetary Systems. Why is it so difficult to detect planets around other stars? Brightness Difference Chapter 13 Other Planetary Systems The New Science of Distant Worlds 13.1 Detecting Extrasolar Planets Our goals for learning:! Why is it so difficult to detect planets around other stars?! How do we detect

More information

cheops Assemble your own planet watcher cheops Paper Model Scale 1:15

cheops Assemble your own planet watcher cheops Paper Model Scale 1:15 cheops cheops Assemble your own planet watcher Paper Model Scale 1:15 About CHEOPS The CHaracterising ExOPlanet Satellite, or CHEOPS, is a space science mission dedicated to the study of known exoplanets

More information

There are 4 x stars in the Galaxy

There are 4 x stars in the Galaxy ExtraSolar Planets Our solar system consists of 1 Star 4 Jovian planets (+ icy moons) 4 Terrestrial planets The asteroid belt (minor planets) The Kuiper belt (dwarf planets, plutinos and TNOs) The Oort

More information

Lab #5. Searching for Extrasolar Planets

Lab #5. Searching for Extrasolar Planets Lab #5 Searching for Extrasolar Planets Introduction Since the beginning of recorded history, humans have wondered whether we are alone in the Universe. Recently, Astronomers have begun to make significant

More information

Extrasolar Planets. Properties Pearson Education Inc., publishing as Pearson Addison-Wesley

Extrasolar Planets. Properties Pearson Education Inc., publishing as Pearson Addison-Wesley Extrasolar Planets Properties 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Finding extrasolar planets is hard quick recap Planet Detection Direct: pictures or spectra of the planets

More information

Extrasolar Planets. Methods of detection Characterization Theoretical ideas Future prospects

Extrasolar Planets. Methods of detection Characterization Theoretical ideas Future prospects Extrasolar Planets Methods of detection Characterization Theoretical ideas Future prospects Methods of detection Methods of detection Methods of detection Pulsar timing Planetary motion around pulsar

More information

Extrasolar Planets. Materials Light source to mimic star Ball to mimic planet Light meter Interface

Extrasolar Planets. Materials Light source to mimic star Ball to mimic planet Light meter Interface Name: Date: Extrasolar Planets Objectives: Learn about Extrasolar planets planets orbiting other stars Explain how astronomers detect and characterize Extrasolar planets Materials Light source to mimic

More information

The peculiar transit signature of CoRoT-29b

The peculiar transit signature of CoRoT-29b The peculiar transit signature of J. Cabrera and the CoRoT Exoplanet Science Team Extrasolar Planets and Atmospheres Institute of Planetology German Aerospace Center (DLR) Berlin, Germany 07.07.2014 Folie

More information

Chapter 13 Lecture. The Cosmic Perspective Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc.

Chapter 13 Lecture. The Cosmic Perspective Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc. Chapter 13 Lecture The Cosmic Perspective Seventh Edition Other Planetary Systems: The New Science of Distant Worlds 13.1 Detecting Planets Around Other Stars Our goals for learning: Why is it so challenging

More information

Planets Around Other Stars Extrasolar Planet Detection Methods. February, 2006

Planets Around Other Stars Extrasolar Planet Detection Methods. February, 2006 Planets Around Other Stars Extrasolar Planet Detection Methods February, 2006 Distribution of this File Extrasolar_planet_detection.ppt This Powerpoint presentation was put together for the purpose of

More information

GJ 436. Michaël Gillon (Geneva)

GJ 436. Michaël Gillon (Geneva) Michaël Gillon (Geneva) Michelson Summer Workshop - July 25, 2007 2004: first hot Neptunes detected by radial velocity Among them: b (Butler et al. 2004, Maness et al. 2007) M * ~ 0.44 M Sun (M2.5V) R

More information

Eric L. Nielsen, Steward Observatory Michelson Fellow

Eric L. Nielsen, Steward Observatory Michelson Fellow A Uniform Analysis of 118 Stars with High- Contrast Imaging: Long Period Extrasolar Giant Planets are Rare around Sun-like Stars (re-submitted to ApJ, Nielsen and Close 2009) Eric L. Nielsen, Steward Observatory

More information

Journal of Astrobiology and Outreach Dr. Jean Schneider Editorial Board member

Journal of Astrobiology and Outreach Dr. Jean Schneider Editorial Board member Journal of Astrobiology and Outreach Dr. Jean Schneider Editorial Board member Senior Researcher in Astronomy Univers et Théorie Paris Observatory Meudon France Biography Dr. Jean Schneider He is a Promoter

More information

Exoplanets. Saturday Physics for Everyone. Jon Thaler October 27, Credit: NASA/Kepler Mission/Dana Berry

Exoplanets. Saturday Physics for Everyone. Jon Thaler October 27, Credit: NASA/Kepler Mission/Dana Berry Exoplanets Saturday Physics for Everyone Jon Thaler October 27, 2012 Credit: NASA/Kepler Mission/Dana Berry Outline What is an exoplanet? Why are they intereskng? How can we find them? Exolife?? The future...

More information

Chapter 13 Other Planetary Systems. Why is it so difficult to detect planets around other stars? Size Difference. Brightness Difference

Chapter 13 Other Planetary Systems. Why is it so difficult to detect planets around other stars? Size Difference. Brightness Difference Chapter 13 Other Planetary Systems Why is it so difficult to detect planets around other stars? Size Difference Planets are small compared to interstellar distances 10 billion to 1 scale Sun is size of

More information

Why Search for Extrasolar Planets?

Why Search for Extrasolar Planets? Why Search for Extrasolar Planets? What is the diversity of habitats for life in the universe? Are Earth-like planets common or rare in our region of the galaxy? We have an elaborate and self-consistent

More information

Astronomy 141 Life in the Universe Professor Gaudi Homework #4 Solutions

Astronomy 141 Life in the Universe Professor Gaudi Homework #4 Solutions Astronomy 141 Life in the Universe Autumn Quarter 008 Prof Gaudi Homework #4 Solutions These questions concern the concept of targets for searches for extrasolar planets specifically (a) the number of

More information

Properties of the Solar System

Properties of the Solar System Properties of the Solar System Dynamics of asteroids Telescopic surveys, especially those searching for near-earth asteroids and comets (collectively called near-earth objects or NEOs) have discovered

More information

Planets and Brown Dwarfs

Planets and Brown Dwarfs Extra Solar Planets Extra Solar Planets We have estimated there may be 10 20 billion stars in Milky Way with Earth like planets, hospitable for life. But what evidence do we have that such planets even

More information

Searching for Extra-Solar Planets

Searching for Extra-Solar Planets Searching for Extra-Solar Planets Until 1996, astronomers only knew about planets orbiting our sun. Though other planetary systems were suspected to exist, none had been found. Now, thirteen years later,

More information

The Direct Study of Exoplanet Atmospheres

The Direct Study of Exoplanet Atmospheres The Direct Study of Exoplanet Atmospheres David Charbonneau (Harvard-Smithsonian Center for Astrophysics) Symposium in Honor of Giovanni Fazio 27 May 2008 Statement about the Astronomy & Astrophysics 2010

More information

PEGASE: a DARWIN/TPF pathfinder

PEGASE: a DARWIN/TPF pathfinder Direct Imaging of Exoplanets: Science & Techniques Proceedings IAU Colloquium No. 200, 2005 C. Aime and F. Vakili, eds. c 2006 International Astronomical Union doi:10.1017/s1743921306009380 PEGASE: a DARWIN/TPF

More information

Lecture 12: Distances to stars. Astronomy 111

Lecture 12: Distances to stars. Astronomy 111 Lecture 12: Distances to stars Astronomy 111 Why are distances important? Distances are necessary for estimating: Total energy released by an object (Luminosity) Masses of objects from orbital motions

More information

10/16/ Detecting Planets Around Other Stars. Chapter 10: Other Planetary Systems The New Science of Distant Worlds

10/16/ Detecting Planets Around Other Stars. Chapter 10: Other Planetary Systems The New Science of Distant Worlds 10/16/17 Lecture Outline 10.1 Detecting Planets Around Other Stars Chapter 10: Other Planetary Systems The New Science of Distant Worlds Our goals for learning: How do we detect planets around other stars?

More information

ASTRO Fall 2012 LAB #6: Extrasolar Planets

ASTRO Fall 2012 LAB #6: Extrasolar Planets ASTRO 1050 - Fall 2012 LAB #6: Extrasolar Planets ABSTRACT This is an exciting time in astronomy. Over the past two decades we have begun to indirectly detect planets that orbit stars other than our sun.

More information

Feasible Mission Designs for Solar Probe Plus to Launch in 2015, 2016, 2017, or November 19, 2008

Feasible Mission Designs for Solar Probe Plus to Launch in 2015, 2016, 2017, or November 19, 2008 Feasible Mission Designs for Solar Probe Plus to Launch in 2015, 2016, 2017, or 2018 2007 Solar Probe Study & Mission Requirements Trajectory study and mission design trades were conducted in the fall

More information

Exoplanet Transits: Light Curve Photometry

Exoplanet Transits: Light Curve Photometry > REPLACE THIS LINE WITH YOUR PAPER IDENTIFICATION NUMBER (DOUBLE-CLICK HERE TO EDIT) < 1 Exoplanet Transits: Light Curve Photometry Lydia Shannon Center for Astrophysics, Space Physics and Engineering

More information

AST 101 Intro to Astronomy: Stars & Galaxies

AST 101 Intro to Astronomy: Stars & Galaxies AST 101 Intro to Astronomy: Stars & Galaxies Telescopes Mauna Kea Observatories, Big Island, HI Imaging with our Eyes pupil allows light to enter the eye lens focuses light to create an image retina detects

More information

Searching for planets around other stars. Searching for planets around other stars. Searching for other planetary systems this is a hard problem!

Searching for planets around other stars. Searching for planets around other stars. Searching for other planetary systems this is a hard problem! Reading: Chap. 21, Sect.21.4-21.6 Final Exam: Tuesday, December 12; 4:30-6:30PM Homework 10: Due in recitation Dec. 1,4 1 Brief review of last time: Formation of Planetary Systems Observational Clues:

More information

Other Solar Systems. Week 15 (Chapter 13): Other Planetary Systems

Other Solar Systems. Week 15 (Chapter 13): Other Planetary Systems Week 15 (Chapter 13): Other Planetary Systems Nov. 30 Please pickup your grade sheet at front. We ll discuss at end of class. Other Solar Systems First one (51 Pegasi) discovered in 1995 Currently 268

More information

The New Worlds Observer:

The New Worlds Observer: ASTR 1: Stars & Galaxies April 3, 8 Next class: Review for Final & Wrap-up. Final Exam: May 5, 4:3 7: pm; Chapters: 1.1-1., 4.1-4.4, 5, 13, 14, 15, 16, 17, 18, 19,, 1,, 3. The New Worlds Observer: Looking

More information

International Symposium on Planetary Science (IAPS2013)

International Symposium on Planetary Science (IAPS2013) International Symposium on Planetary Science (IAPS2013) Venue: 3 rd floor of Astronomical Building Shanghai Astronomical Observatory, Chinese Academy of Sciences The follow-up observations of several exoplanet

More information

Gregg Hallinan National Radio Astronomy Observatory & University of California Berkeley

Gregg Hallinan National Radio Astronomy Observatory & University of California Berkeley Donati et al. 2006 Hallinan et al. 2007 Clarke et al. 1998 Gregg Hallinan National Radio Astronomy Observatory & University of California Berkeley Southern Cross Astrophysics Conference Series Kiama 10

More information

ASTRO Fall Lecture 18. Thursday October 28, 2010

ASTRO Fall Lecture 18. Thursday October 28, 2010 ASTRO 2233 Fall 2010 Planet Detec4on Issues Lecture 18 Thursday October 28, 2010 Astrometry: Advantages: Direct measurement of mass of the planet assumes we know star s mass from stellar type i.e. spectral

More information

Yes, inner planets tend to be and outer planets tend to be.

Yes, inner planets tend to be and outer planets tend to be. 1. Planet Density Make some general comments about inner and outer planets density Inner Planets Density Outer Planets Density Is there a pattern or a trend in planet density? Yes, inner planets tend to

More information

The Kepler Exoplanet Survey: Instrumentation, Performance and Results

The Kepler Exoplanet Survey: Instrumentation, Performance and Results The Kepler Exoplanet Survey: Instrumentation, Performance and Results Thomas N. Gautier, Kepler Project Scientist Jet Propulsion Laboratory California Institute of Technology 3 July 2012 SAO STScI 2012

More information

The exploration of the solar system and the search for water. Thérèse Encrenaz LESIA, Observatoire de Paris

The exploration of the solar system and the search for water. Thérèse Encrenaz LESIA, Observatoire de Paris The exploration of the solar system and the search for water Thérèse Encrenaz LESIA, Observatoire de Paris The exploration of the solar system and the search for water The exploration of solar system:

More information

ASTB01 Exoplanets Lab

ASTB01 Exoplanets Lab ASTB01 Exoplanets Lab Author: Anders Johansen Revision date: $Date: 2015/08/28 14:55:59 $ Planets orbiting stars other than the Sun are called exoplanets. Stellar light reflected off

More information

» How vast those Orbs must be, and how inconsiderable this Earth, the Theatre upon which all our mighty Designs, all our Navigations, and all our

» How vast those Orbs must be, and how inconsiderable this Earth, the Theatre upon which all our mighty Designs, all our Navigations, and all our » How vast those Orbs must be, and how inconsiderable this Earth, the Theatre upon which all our mighty Designs, all our Navigations, and all our Wars are transacted, is when compared to them. A very fit

More information

Observational Astronomy (PHYS-380) Fall 2008 Course Information

Observational Astronomy (PHYS-380) Fall 2008 Course Information Observational Astronomy (PHYS-380) Fall 2008 Course Information Observational astronomy has come a long way since the time of the Babylonians, 2000 BCE, mostly due to advancements in equipment. However,

More information

Stellar Observations Network Group

Stellar Observations Network Group Stellar Observations Network Group Frank Grundahl, Jørgen Christensen Dalsgaard, Uffe Gråe Jørgensen, Hans Kjeldsen, Søren Frandsen, Per Kjærgaard Rasmussen + participation from IAC (Pere Pallé, Orlagh

More information

LAST RESULTS ON THE CHARACTERIZATION OF EXOPLANETS AND THEIR STELLAR HOSTS with VEGA/CHARA Ligi et al. 2016, A&A, 586, A94

LAST RESULTS ON THE CHARACTERIZATION OF EXOPLANETS AND THEIR STELLAR HOSTS with VEGA/CHARA Ligi et al. 2016, A&A, 586, A94 LAST RESULTS ON THE CHARACTERIZATION OF EXOPLANETS AND THEIR STELLAR HOSTS with VEGA/CHARA Ligi et al. 2016, A&A, 586, A94 ROXANNE LIGI CNES POST-DOCTORAL FELLOW LABORATOIRE D ASTROPHYSIQUE DE MARSEILLE

More information

Chapter 13 Lecture. The Cosmic Perspective Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc.

Chapter 13 Lecture. The Cosmic Perspective Seventh Edition. Other Planetary Systems: The New Science of Distant Worlds Pearson Education, Inc. Chapter 13 Lecture The Cosmic Perspective Seventh Edition Other Planetary Systems: The New Science of Distant Worlds 13.1 Detecting Planets Around Other Stars Our goals for learning: Why is it so challenging

More information

Observations of extrasolar planets

Observations of extrasolar planets Observations of extrasolar planets 1 Mercury 2 Venus radar image from Magellan (vertical scale exaggerated 10 X) 3 Mars 4 Jupiter 5 Saturn 6 Saturn 7 Uranus and Neptune 8 we need to look out about 10 parsecs

More information

Exoplanets Atmospheres. Characterization of planetary atmospheres. Photometry of planetary atmospheres from direct imaging

Exoplanets Atmospheres. Characterization of planetary atmospheres. Photometry of planetary atmospheres from direct imaging Photometry of planetary atmospheres from direct imaging Exoplanets Atmospheres Planets and Astrobiology (2016-2017) G. Vladilo Example: planetary system detected with direct imaging HR 8799 b, c, d (Marois

More information

4. Direct imaging of extrasolar planets. 4.1 Expected properties of extrasolar planets. Sizes of gas giants, brown dwarfs & low-mass stars

4. Direct imaging of extrasolar planets. 4.1 Expected properties of extrasolar planets. Sizes of gas giants, brown dwarfs & low-mass stars 4. Direct imaging of extrasolar planets Reminder: Direct imaging is challenging: The proximity to its host star: 1 AU at 1 for alpha Cen 0.15 for the 10th most nearby solar-type star The low ratio of planet

More information

HD Transits HST/STIS First Transiting Exo-Planet. Exoplanet Discovery Methods. Paper Due Tue, Feb 23. (4) Transits. Transits.

HD Transits HST/STIS First Transiting Exo-Planet. Exoplanet Discovery Methods. Paper Due Tue, Feb 23. (4) Transits. Transits. Paper Due Tue, Feb 23 Exoplanet Discovery Methods (1) Direct imaging (2) Astrometry position (3) Radial velocity velocity Seager & Mallen-Ornelas 2003 ApJ 585, 1038. "A Unique Solution of Planet and Star

More information