PROXIMA CENTAURI B: DISCOVERY AND HABITABILITY XIANG ZHANG

Size: px
Start display at page:

Download "PROXIMA CENTAURI B: DISCOVERY AND HABITABILITY XIANG ZHANG"

Transcription

1 PROXIMA CENTAURI B: DISCOVERY AND HABITABILITY XIANG ZHANG

2 Advertisement time

3 Discovery methods of exoplanets Discovery Method Number Astrometry 1 Imaging 44 Radial Velocity 621 Transit 2707 Transit timing variations 15 Eclipse timing variations 8 Microlensing 44 Pulsar timing variations 5 Pulsation timing variations 2 Orbital brightness modulations 6 Total 3453 Data from NASA exoplanet Archive. Updated 22/02/2017.

4 Discovery methods of exoplanets Bennet, Jeffrey, et al. The essential cosmic perspective. Addison-Wesley, 2008.

5 Discovery method: Transit Bennet, Jeffrey, et al. The essential cosmic perspective. Addison-Wesley, 2008.

6 The Kepler Mission Objective: Determining the frequency of Earth-sized planets in and near the habitable zone of Sun-like stars. Observation: Monitoring about 150,000 main sequence stars for several years Confirmed planets: 2330 (up to 16/02/2017) Borucki, William J., et al. "Kepler planet-detection mission: introduction and first results." Science (2010): Koch, David G., et al. "Kepler mission design, realized photometric performance, and early science." The Astrophysical Journal Letters (2010): L79.

7 Discovery method: Radial velocity K is the amplitude of radial variations of a star of mass M_* that are introduced by an orbiting planet of mass M_p. Lissauer, Jack J., and Imke De Pater. Fundamental planetary science: physics, chemistry and habitability. Cambridge University Press, 2013.

8 High Accuracy Radial velocity Planet Searcher (HARPS) A fibre-fed, cross-dispersed echelle spectrograph installed on the ESO's 3.6m telescope at La Silla Observatory in Chile. Precision: 1 m/s Has discovered over 130 exoplanets Mayor, M. et al. "Setting new standards with HARPS." The Messenger 114 (2003): 20.

9 The Alpha Centauri System Closest star system to the Solar system. Distance: 4.37 light years Composed of three stars: Alpha Centauri A Alpha Centauri B Alpha Centauri C (also known as Proxima Centauri)

10 A planet discovered in 2012? Exoplanets down to the size of Earth have been found, but not in the habitable zone. Dumusque, Xavier, et al. "An Earth-mass planet orbiting Alpha Centauri B." Nature (2012):

11 And then there were none The 3.24 d signal observed in the Alpha Cen B data almost certainly arises from the window function of the original data. Rajpaul, Vinesh, Suzanne Aigrain, and S. Roberts. "Ghost in the time series: no planet for Alpha Cen B." Monthly Notices of the Royal Astronomical Society: Letters (2016): L6-L10.

12 Proxima Centauri b discoverd Anglada-Escudé, Guillem, et al. "A terrestrial planet candidate in a temperate orbit around Proxima Centauri." Nature (2016):

13 Proxima Centauri b discoverd Discovery method: Radial velocity Instruments: HARPS and the Ultraviolet and Visual Echelle Spectrograph (UVES), both at ESO Doppler semi-amplitude: 1.4 m/s Signal period: 11.2 day Anglada-Escudé, Guillem, et al. "A terrestrial planet candidate in a temperate orbit around Proxima Centauri." Nature (2016):

14 Some properties of Proxima b Anglada-Escudé, Guillem, et al. "A terrestrial planet candidate in a temperate orbit around Proxima Centauri." Nature (2016):

15 Possible internal structures Possible radius: R_Earth Minimum radius: A Mercury-like planet with 65% core mass fraction Maximum radius: An ocean planet with 50% water in mass Brugger, B., et al. "Possible Internal Structures and Compositions of Proxima Centauri b. The Astrophysical Journal Letters (2016): L16.

16 Orbital resonance

17 Orbit of Proxima b -- 1:1 or 3:2? Proxima b s obliquity is likely null and its spin is either synchronous or in a 3:2 spin-orbit resonance, depending on the planet s eccentricity and level of triaxiality. Ribas, Ignasi, et al. "The habitability of Proxima Centauri b-i. Irradiation, rotation and volatile inventory from formation to the present." Astronomy & Astrophysics 596 (2016): A111.

18 Temperature Turbet, Martin, et al. "The habitability of Proxima Centauri b-ii. Possible climates and observability." Astronomy & Astrophysics 596 (2016): A112.

19 Turbet, Martin, et al. "The habitability of Proxima Centauri b-ii. Possible climates and observability." Astronomy & Astrophysics 596 (2016): A112.

20 Turbet, Martin, et al. "The habitability of Proxima Centauri b-ii. Possible climates and observability." Astronomy & Astrophysics 596 (2016): A112.

21 Proxima Centauri: a star with flares Davenport, James RA, et al. MOST Observations of our Nearest Neighbor: Flares on Proxima Centauri. The Astrophysical Journal Letters (2016): L31.

22 Proxima Centauri: a star with flares Observational instrument: microsatellite Microvariability and Oscillations of STars (MOST) Flare occurrence rate: 63 flares per day Superflares with energies 10^33 erg occur about 8 times per year Davenport, James RA, et al. MOST Observations of our Nearest Neighbor: Flares on Proxima Centauri. The Astrophysical Journal Letters (2016): L31.

23 Stellar wind from Proxima Centauri Garraffo, Cecilia, Jeremy J. Drake, and Ofer Cohen. The Space Weather of Proxima Centauri b. The Astrophysical Journal Letters (2016): L4.

24 High-energy irradiation Ribas, Ignasi, et al. "The habitability of Proxima Centauri b-i. Irradiation, rotation and volatile inventory from formation to the present." Astronomy & Astrophysics 596 (2016): A111.

25 Proxima Centauri, a history Barnes, Rory, et al. "The Habitability of Proxima Centauri b I: Evolutionary Scenarios." arxiv preprint arxiv: (2016).

26 The evolution of its habitable zone The habitable zone moved inwards, while the planet Barnes, Rory, et al. "The Habitability of Proxima Centauri b I: Evolutionary Scenarios." arxiv preprint arxiv: (2016).

27 XUV flux evolution for Proxima Ribas, Ignasi, et al. "The habitability of Proxima Centauri b-i. Irradiation, rotation and volatile inventory from formation to the present." Astronomy & Astrophysics 596 (2016): A111.

28 Any water left for Proxima b? Barnes, Rory, et al. "The Habitability of Proxima Centauri b I: Evolutionary Scenarios." arxiv preprint arxiv: (2016).

29 Conclusions: is Proxima b habitable? Aspects Internal structure Orbital resonance Stellar flare Space weather Evolution history Habitability Possible Possible Maybe not Maybe not Possible

30 The Trappist-1 system Gillon, Michaël, et al. "Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1." Nature 542 (2017),

31 The Trappist-1 system Gillon, Michaël, et al. "Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1." Nature 542 (2017),

Red dwarfs and the nearest terrestrial planets

Red dwarfs and the nearest terrestrial planets Red dwarfs and the nearest terrestrial planets Guillem Anglada-Escudé Queen Mary University of London Abel Mendez/PHL Alexandre Santerne/ESO Alexandre Santerne/ESO Fantastic planet$ And where to find them

More information

Signs of planet detected around sun s nearest neighbor star

Signs of planet detected around sun s nearest neighbor star News Astronomy, Exoplanets Signs of planet detected around sun s nearest neighbor star Proxima Centauri companion orbits in habitable zone By Christopher Crockett 1:00pm, August 24, 2016 A WORLD NEXT DOOR

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

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

The Role of Precision Spectroscopy in the Search for Earth 2.0. Jacob Bean University of Chicago

The Role of Precision Spectroscopy in the Search for Earth 2.0. Jacob Bean University of Chicago The Role of Precision Spectroscopy in the Search for Earth 2.0 Jacob Bean University of Chicago Known exoplanets N 5000 radial velocity transit direct imaging microlensing The role of precision spectroscopy

More information

What will the future bring? Scientific discoveries expected from the E-ELT

What will the future bring? Scientific discoveries expected from the E-ELT What will the future bring? Scientific discoveries expected from the E-ELT Planets & Stars Stars & Galaxies Galaxies & Cosmology Eline Tolstoy Kapteyn Astronomical Institute, University of Groningen E-ELT

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

Climate and radiative properties of a tidally-locked planet around Proxima Centauri

Climate and radiative properties of a tidally-locked planet around Proxima Centauri Climate and radiative properties of a tidally-locked planet around Proxima Centauri D. Galuzzo 1,2 F. Berrilli 1 C. Cagnazzo 2 L. Giovannelli 1 F. Fierli 2 1 Department of Physics, University of Rome Tor

More information

Design Reference Mission. DRM approach

Design Reference Mission. DRM approach Design Reference Mission The Design Reference Mission (DRM) is a set of observing programs which together provide a tool to assist with tradeoff decisions in the design of the E-ELT (examples of observing

More information

Terrestrial Planet (and Life) Finder. AST 309 part 2: Extraterrestrial Life

Terrestrial Planet (and Life) Finder. AST 309 part 2: Extraterrestrial Life Terrestrial Planet (and Life) Finder AST 309 part 2: Extraterrestrial Life The Drake Equation: N = N * f pl n hab f L f C f T L/T Stars? Planets? Habitable Origin Complex Intelligence, Lifetime planets?

More information

Extrasolar Planets. Today. Dwarf Planets. Extrasolar Planets. Next week. Review Tuesday. Exam Thursday. also, Homework 6 Due

Extrasolar Planets. Today. Dwarf Planets. Extrasolar Planets. Next week. Review Tuesday. Exam Thursday. also, Homework 6 Due Extrasolar Planets Today Dwarf Planets Extrasolar Planets Next week Review Tuesday Exam Thursday also, Homework 6 Due will count best 5 of 6 homeworks 2007 Pearson Education Inc., publishing as Pearson

More information

Colors of a second earth: from exoplanets to astrobiology

Colors of a second earth: from exoplanets to astrobiology Colors of a second earth: from exoplanets to astrobiology Yasushi Suto Department of Physics and Research Center for the Early Universe, the University of Tokyo Introductory astronomy class @ Sejong University,

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

Addressing stellar activity at every step in the RV follow-up of small planets. Raphaëlle D. Haywood. Stellar activity or Earth-mass planet?

Addressing stellar activity at every step in the RV follow-up of small planets. Raphaëlle D. Haywood. Stellar activity or Earth-mass planet? Addressing stellar activity at every step in the RV follow-up of small planets Stellar activity or Earth-mass planet? Raphaëlle D. Haywood and the GTO Science Team NASA Sagan Fellow, Harvard College Observatory

More information

Scientists discover 7 Earthlike planets orbiting a nearby star

Scientists discover 7 Earthlike planets orbiting a nearby star Scientists discover 7 Earthlike planets orbiting a nearby star By Sarah Kaplan February 22 at 1:00 PM 5 things to know about the newly discovered solar system Play Video1:55 Astronomers found a new solar

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

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

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

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

Finding terrestrial planets in the habitable zones of nearby stars

Finding terrestrial planets in the habitable zones of nearby stars Finding terrestrial planets in the habitable zones of nearby stars Part II Astrophysics Essay Simon Hodgkin & Mark Wyatt (on sabbatical) Terrestrial? 15 Exoplanets Solar system 5 4.5 g cm 3 Winn et al.

More information

Future Opportunities for Collaborations: Exoplanet Astronomers & Statisticians

Future Opportunities for Collaborations: Exoplanet Astronomers & Statisticians Future Opportunities for Collaborations: Exoplanet Astronomers & Statisticians Eric B. Ford Penn State Astronomy & Astrophysics Center for Astrostatistics Center for Exoplanets & Habitable Worlds Institute

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

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

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

[25] Exoplanet Characterization (11/30/17)

[25] Exoplanet Characterization (11/30/17) 1 [25] Exoplanet Characterization (11/30/17) Upcoming Items APOD 12/2/16 1. Read chapters 24.1-24.3 for Tuesday 2. We will have a final exam review in the last discussion section (Friday, Dec 8) and also

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

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

DETECTING TRANSITING PLANETS WITH COROT. Stefania Carpano ESAC (25th of November 2009)

DETECTING TRANSITING PLANETS WITH COROT. Stefania Carpano ESAC (25th of November 2009) DETECTING TRANSITING PLANETS WITH COROT Stefania Carpano ESAC (25th of November 2009) Outline 1) Introduction: Exoplanet science and detection methods Detection of exoplanets using the transit method The

More information

Lecture 16 The Measuring the Stars 3/26/2018

Lecture 16 The Measuring the Stars 3/26/2018 Lecture 16 The Measuring the Stars 3/26/2018 Test 2 Results D C B A Questions that I thought were unfair: 13, 18, 25, 76, 77, 80 Curved from 85 to 79 Measuring stars How far away are they? How bright are

More information

Planet Detection. AST 105 Intro Astronomy The Solar System

Planet Detection. AST 105 Intro Astronomy The Solar System Review AST 105 Intro Astronomy The Solar System MIDTERM III this THURSDAY 04/8 covering LECT. 17 through We ve talked about the Terrestrial Planets and the Jovian Planets - What about planets around other

More information

Welcome back! from one version of the Olympics

Welcome back! from one version of the Olympics Welcome back! from one version of the Olympics Welcome back! from one version of the Olympics Welcome back! from one version of the Olympics Passing the torch Welcome back! Welcome back! Olympic flame

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 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

Lecture Outlines. Chapter 17. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 17. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 17 Astronomy Today 8th Edition Chaisson/McMillan Chapter 17 Measuring the Stars Units of Chapter 17 17.1 The Solar Neighborhood 17.2 Luminosity and Apparent Brightness 17.3 Stellar

More information

Scientists say they found an Earth-like planet

Scientists say they found an Earth-like planet Scientists say they found an Earth-like planet By Scientific American, adapted by Newsela staff on 08.30.16 Word Count 971 The two bright stars are (left) Alpha Centauri and (right) Beta Centauri. The faint

More information

Measuring Radial Velocities of Low Mass Eclipsing Binaries

Measuring Radial Velocities of Low Mass Eclipsing Binaries Measuring Radial Velocities of Low Mass Eclipsing Binaries Rebecca Rattray, Leslie Hebb, Keivan G. Stassun College of Arts and Science, Vanderbilt University Due to the complex nature of the spectra of

More information

Science of extrasolar Planets A focused update

Science of extrasolar Planets A focused update Science of extrasolar Planets A focused update Raffaele Gratton, INAF Osservatorio Astronomico di Padova Extrasolar planets: a rapidly growing field of astronomy Top Tenz: Top 10 most important discoveries

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

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

Key Ideas: The Search for New Planets. Scientific Questions. Are we alone in the Universe? Direct Imaging. Searches for Extrasolar Planets

Key Ideas: The Search for New Planets. Scientific Questions. Are we alone in the Universe? Direct Imaging. Searches for Extrasolar Planets The Search for New Planets Key Ideas: Search for planets around other stars. Successful Search Techniques: Astrometric Wobble Doppler Wobble major discovery method Planetary Transits planets we can study

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

Radiation conditions near exoplanets оf G- M stars Alexei Struminsky, Andrei Sadovski

Radiation conditions near exoplanets оf G- M stars Alexei Struminsky, Andrei Sadovski Radiation conditions near exoplanets оf G- M stars Alexei Struminsky, Andrei Sadovski Space Research Institute, Moscow, Russia The goal is to estimate fluxes of galactic and stellar CR near exoplanets

More information

Other planetary systems

Other planetary systems Exoplanets are faint! Other planetary systems Planets are seen only by reflected light at optical wavelengths At the distance of another star the faint light of a planet is lost in the glare of the star

More information

arxiv: v1 [astro-ph.sr] 22 Aug 2014

arxiv: v1 [astro-ph.sr] 22 Aug 2014 18th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun Proceedings of Lowell Observatory (9-13 June 2014) Edited by G. van Belle & H. Harris Using Transiting Planets to Model Starspot Evolution

More information

Professional / Amateur collaborations in exoplanetary science

Professional / Amateur collaborations in exoplanetary science Professional / Amateur collaborations in exoplanetary science Alexandre Santerne Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto alexandre.santerne@astro.up.pt Outline Exoplanets:

More information

Finding bio-signatures on extrasolar planets, how close are we?

Finding bio-signatures on extrasolar planets, how close are we? Finding bio-signatures on extrasolar planets, how close are we? Enric Palle Instituto de Astrofisica de Canarias TMT Forum 2017, Mysore Exoplanet discoveries 3703 planets 2773 system 621 multiple Exoplanets:

More information

Architecture and demographics of planetary systems

Architecture and demographics of planetary systems Architecture and demographics of planetary systems Struve (1952) The demography of the planets that we detect is strongly affected by detection methods psychology of the observer Understanding planet demography

More information

PLANETARY SYSTEM: FROM GALILEO TO EXOPLANETS

PLANETARY SYSTEM: FROM GALILEO TO EXOPLANETS PLANETARY SYSTEM: FROM GALILEO TO EXOPLANETS Rosa M. Ros Technical University of Catalonia, Barcelona (Spain) Abstract When in 1610 Galileo Galilei looked at Jupiter with the use of his telescope, he saw

More information

Scientists are getting closer to discovering Earth-like planets close to Earth

Scientists are getting closer to discovering Earth-like planets close to Earth 1 of 6 22-10-2012 10:36 Content Home Projects LabNotes Press Releases In the News Outreach Media Library Software Tools Data Opportunities Calendars Centers About Press Releases > A Planetary System Around

More information

The Kepler Mission. NASA Discovery Mission # 10: Are there other planets, orbiting other stars, with characteristics similar to Earth?

The Kepler Mission. NASA Discovery Mission # 10: Are there other planets, orbiting other stars, with characteristics similar to Earth? Kepler Update: 2016 http://www.nasa.gov/sites/default/files/styles/side_image/public/thumbnails/imag e/286257main_07-3348d1-kepler-4x3_226-170.jpg?itok=hvzfdmjc The Kepler Mission NASA Discovery Mission

More information

Exoplanets: the quest for Earth twins

Exoplanets: the quest for Earth twins 369, 572 581 doi:1.198/rsta.21.245 Exoplanets: the quest for Earth twins BY MICHEL MAYOR*, STEPHANE UDRY, FRANCESCO PEPE AND CHRISTOPHE LOVIS Observatoire de Genève, Université de Genève, Geneva, Switzerland

More information

GLOBAL CLIMATE MODELS AND EXTREME HABITABILITY

GLOBAL CLIMATE MODELS AND EXTREME HABITABILITY GLOBAL CLIMATE MODELS AND EXTREME HABITABILITY François Forget, Martin Turbet, Jérémy Leconte, Ehouarn Millour, Maxence Lefèvre & the LMD team Laboratoire de Météorologie Dynamique, Paris Modelled surface

More information

EART164: PLANETARY ATMOSPHERES

EART164: PLANETARY ATMOSPHERES EART164: PLANETARY ATMOSPHERES Francis Nimmo Last Week - Dynamics Reynolds number, turbulent vs. laminar flow Velocity fluctuations, Kolmogorov cascade Brunt-Vaisala frequency, gravity waves Rossby waves,

More information

Searching For Habitable Exoplanets

Searching For Habitable Exoplanets Searching For Habitable Exoplanets Gongjie Li, Harvard -> Georgia Tech Life in the Cosmos, Georgia Tech Credit: ESO Are we alone? How common are we in the Universe? Search for alien civilization. Credit:

More information

Proxima Cen b: theoretical spectral signatures for different atmospheric scenarios

Proxima Cen b: theoretical spectral signatures for different atmospheric scenarios Proxima Cen b: theoretical spectral signatures for different atmospheric scenarios A. Léger(1), D. Defrère(2), J.L. Grenfell(3), M. Godolt(3), A Garcia Munoz(3), H. Rauer(3), and F. Tian(4) (1) University

More information

Why Should We Expect to Find Other Planets? Planetary system formation is a natural by-product of star formation

Why Should We Expect to Find Other Planets? Planetary system formation is a natural by-product of star formation 1 Why Should We Expect to Find Other Planets? Planetary system formation is a natural by-product of star formation 2 Why Should We Expect to Find Other Planets? Observations show young stars are surrounded

More information

PERCENTAGE OF STARS WITH PLANETS

PERCENTAGE OF STARS WITH PLANETS 01 March, 2018 PERCENTAGE OF STARS WITH PLANETS Document Filetype: PDF 279.89 KB 0 PERCENTAGE OF STARS WITH PLANETS Astronomers have discovered that terrestrial planets might form around many, if not most,

More information

Hunting Habitable Shadows. Elizabeth Tasker

Hunting Habitable Shadows. Elizabeth Tasker Hunting Habitable Shadows Elizabeth Tasker Saturn Earth Uranus Mercury Mars Jupiter Venus Neptune Saturn Earth Uranus Mercury Mars Jupiter Venus Neptune 2013 2012 2011 2010 2009 2008 2007 2006 2005 2004

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

Life on Trappist-1-like Planets Impossible, Possible or Likely?

Life on Trappist-1-like Planets Impossible, Possible or Likely? ESA NL 2017 Life on Trappist-1-like Planets Impossible, Possible or Likely? Joe Gale, Institute of Life Sciences Amri Wandel, Racach Institute of Physics The Hebrew University of Jerusalem Israel Some

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

The UVES M Dwarf Planet Search Programme

The UVES M Dwarf Planet Search Programme The UVES M Dwarf Planet Search Programme Martin Kürster Mathias Zechmeister Michael Endl 2 Eva Meyer,@W/K@MBJ(MRSHSTSEXQ RSQNMNLHD 'DHCDKADQF&DQL@MX 2,B#NM@KC.ARDQU@SNQX4MHUDQRHSXNE 3DW@R@S TRSHM42 We

More information

The Main Point(s) Lecture #36: Planets Around Other Stars. Extrasolar Planets! Reading: Chapter 13. Theory Observations

The Main Point(s) Lecture #36: Planets Around Other Stars. Extrasolar Planets! Reading: Chapter 13. Theory Observations Lecture #36: Planets Around Other Stars Extrasolar Planets! Theory Observations Detection methods Results to date... Implications for "Habitable Zones" Reading: Chapter 13 Astro 102/104 1 The Main Point(s)

More information

Astronomy December, 2016 Introduction to Astronomy: The Solar System. Final exam. Practice questions for Unit V. Name (written legibly):

Astronomy December, 2016 Introduction to Astronomy: The Solar System. Final exam. Practice questions for Unit V. Name (written legibly): Astronomy 101 12 December, 2016 Introduction to Astronomy: The Solar System Final exam Practice questions for Unit V Name (written legibly): Honor Pledge: On my honor, I have neither given nor received

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

Searching for extrasolar planets using microlensing

Searching for extrasolar planets using microlensing Searching for extrasolar planets using microlensing Dijana Dominis Prester 7.8.2007, Belgrade Extrasolar planets Planets outside of the Solar System (exoplanets) Various methods: mostly massive hot gaseous

More information

Life in the Universe (1)

Life in the Universe (1) Conditions for the emergence of life and habitability Life in the Universe (1) We call biogenic conditions the set of physico-chemical requirements that must be fulfilled for abiogenesis to take place

More information

Earth-like planets in habitable zones around L (and T) dwarfs

Earth-like planets in habitable zones around L (and T) dwarfs Earth-like planets in habitable zones around L (and T) dwarfs David Montes José A. Caballero Departamento de Astrofísica Universidad Complutense de Madrid Detecting planets around lowmass stars (and brown

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

Extra Solar Planetary Systems and Habitable Zones

Extra Solar Planetary Systems and Habitable Zones Lecture Overview Extra Solar Planetary Systems and Habitable Zones Our Galaxy has 200 Billion Stars, Our Sun has 8 planets. It seems like an awful waste if we are alone Exoplanets Karen J. Meech, Svetlana

More information

Adam Burrows, Princeton April 7, KITP Public Lecture

Adam Burrows, Princeton April 7, KITP Public Lecture Adam Burrows, Princeton April 7, 2010 KITP Public Lecture The Ancient History of Comparative Planetology There are infinite worlds both like and unlike this world of ours...we must believe that in all

More information

The importance of telescopes of all sizes, from small to extremely large: The example of exoplanet rsearch

The importance of telescopes of all sizes, from small to extremely large: The example of exoplanet rsearch The importance of telescopes of all sizes, from small to extremely large: The example of exoplanet rsearch Charles Alcock Director Harvard-Smithsonian Center for Astrophysics With help from: Telescopes

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

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

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

John Barnes. Red Optical Planet Survey (ROPS): A radial velocity search for low mass M dwarf planets

John Barnes. Red Optical Planet Survey (ROPS): A radial velocity search for low mass M dwarf planets Red Optical Planet Survey (ROPS): A radial velocity search for low mass M dwarf planets John Barnes Centre for Astrophysics Research University of Hertfordshire UK -H. Jones, D. Pinfield, M. Tuomi (University

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

The Ultraviolet Radiation Environment in the Habitable Zones Around Low-Mass Exoplanet Host Stars. Kevin France. University of Colorado at Boulder

The Ultraviolet Radiation Environment in the Habitable Zones Around Low-Mass Exoplanet Host Stars. Kevin France. University of Colorado at Boulder The Ultraviolet Radiation Environment in the Habitable Zones Around Low-Mass Exoplanet Host Stars Kevin France University of Colorado at Boulder NUVA Challenges in UV Astronomy 07 October 2013 Co-authors

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

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

The effect of stellar activity on radial velocities. Raphaëlle D. Haywood Sagan Fellow, Harvard College Observatory

The effect of stellar activity on radial velocities. Raphaëlle D. Haywood Sagan Fellow, Harvard College Observatory The effect of stellar activity on radial velocities Raphaëlle D. Haywood Sagan Fellow, Harvard College Observatory Mass and radius are the most fundamental parameters of a planet Main inputs for models

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

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

Exoplanet Host Stars

Exoplanet Host Stars Exoplanet Host Stars The Hertzsprung-Russel (HR)Diagram The Hertzsprung-Russel (HR)Diagram Standard Doppler Surveys The Hertzsprung-Russel (HR)Diagram Direct Imaging detections Standard Doppler Surveys

More information

Detecting Earth-Sized Planets with Laser Frequency Combs

Detecting Earth-Sized Planets with Laser Frequency Combs Detecting Earth-Sized Planets with Laser Frequency Combs Hayley Finley Department of Physics, Drexel University, 3141 Chestnut Street, Philadelphia, Pennsylvania 19104 Abstract Detection of Earth-mass

More information

ASTR-1020: Astronomy II Course Lecture Notes Section III

ASTR-1020: Astronomy II Course Lecture Notes Section III ASTR-1020: Astronomy II Course Lecture Notes Section III Dr. Donald G. Luttermoser East Tennessee State University Edition 4.0 Abstract These class notes are designed for use of the instructor and students

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

Probing the Galactic Planetary Census

Probing the Galactic Planetary Census Probing the Galactic Planetary Census Greg Laughlin -- UCSC Astronomy Exoplanet News from the AAS meeting (New York Times) The finding was called exciting by Dr. Kenneth Franklin of the American Museum-Hayden

More information

Parallax: Measuring the distance to Stars

Parallax: Measuring the distance to Stars Measuring the Stars Parallax: Measuring the distance to Stars Use Earth s orbit as baseline Parallactic angle = 1/2 angular shift Distance from the Sun required for a star to have a parallactic angle of

More information

EarthFinder A NASA-selected Probe Mission Concept Study for input to the 2020 Astrophysics Decadal Survey

EarthFinder A NASA-selected Probe Mission Concept Study for input to the 2020 Astrophysics Decadal Survey EarthFinder A NASA-selected Probe Mission Concept Study for input to the 2020 Astrophysics Decadal Survey Peter Plavchan Assistant Professor George Mason University 1 @PlavchanPeter http://exo.gmu.edu

More information

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

Lecture Outlines. Chapter 15. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 15. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 15 Astronomy Today 8th Edition Chaisson/McMillan Chapter 15 Exoplanets Units of Chapter 15 15.1 Modeling Planet Formation 15.2 Solar System Regularities and Irregularities 15.3

More information

Newly discovered planet may support life, scientists say

Newly discovered planet may support life, scientists say Newly discovered planet may support life, scientists say By Scientific American, adapted by Newsela staff on 08.30.16 Word Count 781 The two bright stars are (left) Alpha Centauri and (right) Beta Centauri.

More information

The formation & evolution of solar systems

The formation & evolution of solar systems The formation & evolution of solar systems Content expectations Birth of the Solar System What did the material that eventually became the Sun and planets look like originally? Interstellar clouds like

More information

Exoplanets and The Transiting Exoplanet Survey Satellite (TESS)

Exoplanets and The Transiting Exoplanet Survey Satellite (TESS) Exoplanets and The Transiting Exoplanet Survey Satellite (TESS) Ryan J. Oelkers Monday, June 25, 2018 QuarkNET 2018 It is estimated that nearly all stars in the Milky Way Galaxy have 1-1.5 planets orbiting

More information

The Composition and Evolutionary Status of Proxima Centauri

The Composition and Evolutionary Status of Proxima Centauri American Journal of Astronomy and Astrophysics 2017; 5(1): 1-5 http://www.sciencepublishinggroup.com/j/ajaa doi: 10.11648/j.ajaa.20170501.11 ISSN: 2376-4678 (Print); ISSN: 2376-4686 (Online) Letter The

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

PLATO. revealing the interior of planets and stars completing the age of planet discovery for Earth-sized planets constraining planet formation

PLATO. revealing the interior of planets and stars completing the age of planet discovery for Earth-sized planets constraining planet formation PLATO PLAnetary Transits and Oscillations of Stars revealing the interior of planets and stars completing the age of planet discovery for Earth-sized planets constraining planet formation The PLATO Consortium:

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

Date of delivery: 29 June 2011 Journal and vol/article ref: IAU Number of pages (not including this page): 5

Date of delivery: 29 June 2011 Journal and vol/article ref: IAU Number of pages (not including this page): 5 Date of delivery: 29 June 2011 Journal and vol/article ref: IAU 1101538 Number of pages (not including this page): 5 Author queries: Typesetter queries: Non-printed material: The Physics of the Sun and

More information