Update on the Quest for an Earth-Like Planet Update on the Quest for An
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Colors of Extreme Exo-Earth Environments
Colors of Extreme Exo-Earth Environments Siddharth Hegde1,* and Lisa Kaltenegger1,2 1Max Planck Institute for Astronomy, Heidelberg, Germany; 2Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA. *E-mail: [email protected]; [email protected] Abstract The search for extrasolar planets has already detected rocky planets and several planetary candidates with minimum masses that are consistent with rocky planets in the habitable zone of their host stars. A low-resolution spectrum in the form of a color-color diagram of an exoplanet is likely to be one of the first post-detection quantities to be measured for the case of direct detection. In this paper, we explore potentially detectable surface features on rocky exoplanets and their connection to, and importance as, a habitat for extremophiles, as known on Earth. Extremophiles provide us with the minimum known envelope of environmental limits for life on our planet. The color of a planet reveals information on its properties, especially for surface features of rocky planets with clear atmospheres. We use filter photometry in the visible waveband as a first step in the characterization of rocky exoplanets to prioritize targets for follow-up spectroscopy. Many surface environments on Earth have characteristic albedos and occupy a different color space in the visible waveband (0.4-0.9 !m) that can be distinguished remotely. These detectable surface features can be linked to the extreme niches that support extremophiles on Earth and provide a link between geomicrobiology and observational astronomy. This paper explores how filter photometry can serve as a first step in characterizing Earth-like exoplanets for an aerobic as well as an anaerobic atmosphere, thereby prioritizing targets to search for atmospheric biosignatures. -
Universidade De São Paulo Instituto De Astronomia E Geofisica Mestrado Profissional Em Ensino De Astronomia
UNIVERSIDADE DE SÃO PAULO INSTITUTO DE ASTRONOMIA E GEOFISICA MESTRADO PROFISSIONAL EM ENSINO DE ASTRONOMIA JOSÉ IVAN SPINARDI ELABORAÇÃO DE UMA SEQUÊNCIA DIDÁTICA EM ASTROBIOLOGIA PARA O ENSINO FUNDAMENTAL 2 SÃO PAULO 2017 “Versão corrigida. O original encontra-se disponível na Unidade.” JOSÉ IVAN SPINARDI ELABORAÇÃO DE UMA SEQUÊNCIA DIDÁTICA EM ASTROBIOLOGIA PARA O ENSINO FUNDAMENTAL 2 Dissertação apresentada ao Instituto de Astronomia e Geofísica da Universidade de São Paulo obtenção do título de mestre em ensino de Astronomia. Área de concentração: Ensino de Astronomia. Orientador: Prof. Dr. Amâncio Cesar Santos Friaça SÃO PAULO 2017 “O materialismo dialético ensina que a matéria nunca permanece em repouso, mas, pelo contrário, está em constante movimento, desenvolve-se e, evoluindo, eleva-se a níveis cada vez mais altos e adquire formas de movimento cada vez mais complexas. Ao elevar-se de um degrau ao outro, a matéria adquire novos atributos. Um deles é a vida cujo surgimento marca uma etapa, um escalão determinado do desenvolvimento histórico da matéria. Durante o decorrer desse desenvolvimento é que surgiu a vida, como uma nova qualidade.” Alexander Oparin “Se não existe vida fora da Terra, então o Universo é um grande desperdício de espaço” Carl Sagan “Há vidas sim em outros planetas, porém, não desenvolvidas.” Um aluno da 8ª série A. AGRADECIMENTOS À minha família. Ao meu sobrinho Luiz Lucas pelo suporte em informática. Às educadoras Erika Reyes Molina e Giovanni Scataglia Botelho Paz, pelo apoio e confiança. À Professora Maria Helena Pereira, da EMEF João Guimaraes Rosa, pela cessão de suas aulas para a aplicação das atividades. -
Hunting for Transits of Super-Earth GJ 581E 2 June 2011
Hunting for transits of Super-Earth GJ 581e 2 June 2011 terrestrial-mass exoplanet in the habitable zone". They found that, despite the small amount of light Gliese 581d receives from its star, a carbon dioxide atmosphere could maintain temperatures above the freezing point of water at the surface. If the orbital inclination of a planetary system is just right, then one or more planets may be observed to cross (transit) the disk of the star, dimming the brightness of the star by a tiny fraction. By measuring this effect, it is possible to derive the Artist's concept of Gliese 581 e. Image: size of the planet. JohnVanVliet/Wikipedia. If Gliese 581e transits its host star, then it must have a radius smaller than 1.4 times that of the Earth since a larger planet would have been (PhysOrg.com) -- An international team of detected by MOST. In terms of composition, this astronomers has ruled out transits of a water-rich suggests that planet e does not have a hydrogen or or hydrogen-helium atmosphere planet for Gliese helium atmosphere, nor does it contain more than 581e. The host star itself is relatively quiet which 25% water. Therefore it must be a solid rocky means good news for the potential habitability of at planet. However, if the planet does not transit, its least one of its planets. size and therefore its composition cannot be constrained, but the inclination of its orbit can. The study was conducted using observations acquired by MOST (Microvariability & Oscillations "Although transits were not detected for Gliese of STars), Canada's only space telescope. -
Thea Kozakis
Thea Kozakis Present Address Email: [email protected] Space Sciences Building Room 514 Phone: (908) 892-6384 Ithaca, NY 14853 Education Masters Astrophysics; Cornell University, Ithaca, NY Graduate Student in Astronomy and Space Sciences, minor in Earth and Atmospheric Sciences B.S. Physics, B.S. Astrophysics; College of Charleston, Charleston, SC Double major (B.S.) in Astrophysics and Physics, May 2013, summa cum laude Minor in Mathematics Research Dr. Lisa Kaltenegger, Carl Sagan Institute, Cornell University, Spring 2015 - present Projects Studying biosignatures of habitable zone planets orbiting white dwarfs using a • coupled climate-photochemistry atmospheric model Searching the Kepler field for evolved stars using GALEX UV data • Dr. James Lloyd, Cornell University, Fall 2013 - present UV/rotation analysis of Kepler field stars • Study the age-rotation-activity relationship of 20,000 Kepler field stars using UV data from GALEX and publicly available rotation⇠ periods Dr. Joseph Carson, College of Charleston, Spring 2011 - Summer 2013 SEEDS Exoplanet Survey • Led data reduction e↵orts for the SEEDS High-Mass stars group using the Subaru Telescope’s HiCIAO adaptive optics instrument to directly image exoplanets Hubble DICE Survey • Developed data reduction pipeline for Hubble STIS data to image exoplanets and debris disks around young stars Publications Direct Imaging Discovery of a ‘Super-Jupiter’ Around the late B-Type Star • And, J. Carson, C. Thalmann, M. Janson, T. Kozakis, et al., 2013, Astro- physical Journal Letters, 763, 32 -
The Search for Worlds Like Our Own
ASTROBIOLOGY Volume 10, Number 1, 2010 Education Articles ª Mary Ann Liebert, Inc. DOI: 10.1089=ast.2009.0380 The Search for Worlds Like Our Own Malcolm Fridlund,1 Carlos Eiroa,2 Thomas Henning,3 Tom Herbst,3 Helmut Lammer,4 Alain Le´ger,5 Rene´ Liseau,6 Francesco Paresce,7 Alan Penny,8,9 Andreas Quirrenbach,10 Huub Ro¨ttgering,11 Franck Selsis,12 Glenn J. White,9,13 Olivier Absil,14,15 Denis Defre`re,15 C. Hanot,15 Daphne Stam,16 Jean Schneider,17 Giovanna Tinetti,18 Anders Karlsson,19 Phillipe Gondoin,19 Roland den Hartog,19 Luigi D’Arcio,19 Anna-Maria Stankov,19 Mikael Kilter,19 Christian Erd,19 Charles Beichman,20 Daniel Coulter,21 William Danchi,22 Michael Devirian,21 Kenneth J. Johnston,23 Peter Lawson,21 Oliver P. Lay,21 Jonathan Lunine,24 and Lisa Kaltenegger25 Abstract The direct detection of Earth-like exoplanets orbiting nearby stars and the characterization of such planets— particularly, their evolution, their atmospheres, and their ability to host life—constitute a significant problem. The quest for other worlds as abodes of life has been one of mankind’s great questions for several millennia. For instance, as stated by Epicurus *300 BC: ‘‘Other worlds, with plants and other living things, some of them similar and some of them different from ours, must exist.’’ Demokritos from Abdera (460–370 BC), the man who invented the concept of indivisible small parts—atoms—also held the belief that other worlds exist around the stars and that some of these worlds may be inhabited by life-forms. -
Esocast Episode 6: Lightest Exoplanet Found 00:00 [Visual Starts]
ESOcast Episode 6: Lightest exoplanet found 00:00 [Visual starts] [Narrator] A: Artist’s impression of Gliese 581e 1. The holy grail of current exoplanet research is the detection of a rocky, Earth-like planet in the ‘habitable zone,’ region around the host star with the right conditions for water to be liquid on their surface. The latest result from the European Southern Observatory comes closer than ever to attaining these goals. 00:25 ESOcast intro This is the ESOcast! Cutting-edge science and life behind the scenes of ESO, the European Southern Observatory. Exploring the Universe’s ultimate frontier with our host Dr. J, a.k.a. Dr. Joe Liske. 00:42 [Dr. J] 2. Hello and welcome to another episode of the ESOcast. This time we have some very exciting A: Artist’s impression of Gliese 581e news for you, it’s another major ESO discovery. We’d like to tell you about the discovery of the B: Artist’s impression of Gliese 581d smallest, or rather lightest, and possibly most Earth- like planet so far discovered outside of our own Solar System. We’d also like to report on yet another planet within the same system that has now been shown to lie within the habitable zone of its parent star, meaning that it could host liquid water and possibly even life. 01:13 [Narrator] 3. Gliese 581 is a seemingly inconspicuous red C: Zoom-in on Gliese 581e dwarf star located 20.5 light-years away in the constellation Libra, or “the Scales”. It is among the 100 closest stars to us and weighs only one third the mass of the Sun. -
SARA SEAGER Physics and Planetary Science, Massachusetts Institute of Technology, Cambridge
21 10 meters SARA SEAGER Physics and planetary science, Massachusetts Institute of Technology, Cambridge We picnicked inside a fiberglass radome (a portmanteau of radar and dome), atop the tallest building in Cambridge. The Green Building, otherwise known as Building 54, houses the fields of Geology and Earth Sciences on the lower floors and Astronomy and Atmospheric Sciences on the upper floors. It was only late October, but the temperature was already below freezing, so we bundled up in fur caps and heavy jackets to endure the cold inside the dome. We sat next to a defunct radar satellite that had recently been hacked by students to bounce beams off the moon. 1 Sara requested high-protein brain food, so we made hard-boiled eggs and prepared them so that each egg was boiled for a different increment of time, which was an- notated on each of the dozen eggshells: 5 min, 6 min, 7 min, 8 min, 9 min, 10 min, 11 min, 12 min, 13 min, 14 min, MICHAEL: Do you know the early astronauts like Buzz 15 min, 16 min what your kids are going to Aldrin. Buzz Aldrin can be dress up as for Halloween? alternately outspoken, rude, Sara ate a twelve-minute egg to test her theory that there is a threshold beyond obnoxious, and fun, while the which there is no effect on the egg, so boiling longer only serves to waste energy. SARA: Yes, one son is going to be current astronauts typically Buzz Aldrin, an astronaut, and appear to be more conforming (FIG. -
High-Resolution Spectra and Biosignatures of Earth-Like Planets Transiting White Dwarfs
High-resolution Spectra and Biosignatures of Earth-like Planets Transiting White Dwarfs Thea Kozakis, Zifan Lin, Lisa Kaltenegger Carl Sagan Institute, Cornell University, Ithaca, New York, USA ABSTRACT With the first observations of debris disks as well as proposed planets around white dwarfs, the question of how rocky planets around such stellar remnants can be char- acterized and probed for signs of life becomes tangible. White dwarfs are similar in size to Earth and have relatively stable environments for billions of years after initial cooling, making them intriguing targets for exoplanet searches and terrestrial planet atmospheric characterization. Their small size and the resulting large planet transit signal allows observations with next generation telescopes to probe the atmosphere of such rocky planets, if they exist. We model high-resolution transmission spectra for planets orbiting white dwarfs from as they cool from 6,000-4,000 K, for i) planets re- ceiving equivalent irradiation to modern Earth, and ii) planets orbiting at the distance around a cooling white dwarf which allows for the longest continuous time in the hab- itable zone. All high-resolution transmission spectra will be publicly available online upon publication of this study and can be used as a tool to prepare and interpret up- coming observations with JWST, the Extremely Large Telescopes as well as mission concepts like Origins, HabEx, and LUVOIR. Subject headings: White dwarf stars, Habitable zone, Habitable planets, Stellar evolution, Exoplanet atmospheres, Astrobiology, Biosignatures, Transmission spectroscopy, Extrasolar rocky planets 1. Introduction Zwart 2016; Malamud & Perets 2016) indi- cate debris disks or planets around a high The first discovery of a planetestimal or- percentage of WDs of up to 50% (Schreiber arXiv:2001.00049v3 [astro-ph.EP] 17 Jan 2020 biting a white dwarf (WD) in 2015 (Van- et al. -
Model Spectra of the First Potentially Habitable Super-Earth - Gl581d
Model Spectra of the First Potentially Habitable Super-Earth - Gl581d Lisa Kaltenegger Harvard Smithsonian Center for Astrophysics, 60 Garden st., 02138 MA Cambridge, USA also MPIA, Koenigstuhl 17, 69117 Heidelberg, Germany [email protected] Antígona Segura Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, México Subhanjoy Mohanty Imperial College London, 1010 Blackett Lab., Prince Consort Road, London SW7 2AZ, UK Abstract Gl581d has a minimum mass of 7 MEarth and is the first detected potentially habitable rocky Super-Earth. Our models confirm that a habitable atmosphere can exist on Gl581d. We derive spectroscopic features for atmospheres, assuming an Earth-like composition for this planet, from high oxygen atmosphere analogous to Earth’s to high CO2 atmospheres with and without biotic oxygen concentrations. We find that a minimum CO2 partial pressure of about 7 bar, in an atmosphere with a total surface pressure of 7.6 bar, are needed to maintain a mean surface temperature above freezing on Gl581d. We model transmission and emergent synthetic spectra from 0.4µm to 40µm and show where indicators of biological activities in such a planet’s atmosphere could be observed by future ground- and space-based telescopes. The model we present here only represents one possible nature – an Earth-like composition - of a planet like Gl581d in a wide parameter space. Future observations of atmospheric features can be used to examine if our concept of habitability and its dependence on the carbonate-silicate cycle is correct, and assess whether Gl581d is indeed a habitable super-Earth. Subject headings: astrobiology, Planets and satellites: atmospheres, composition, detection, individual: Gl581d, Earth, Instrumentation: spectrographs 1. -
De Natura Rerum: Exoplanets and Exoearths Pierre Léna Que L’Homme Contemple La Nature Dans Sa Haute Et Pleine Majesté… Que La Terre Lui Paraisse Comme Un Point
De Natura Rerum: Exoplanets and ExoEarths Pierre Léna Que l’homme contemple la nature dans sa haute et pleine majesté… que la Terre lui paraisse comme un point. Blaise Pascal (1623-1662) Pensées Introduction At the 2004 Plenary Session of the Pontifical Academy of Sciences on Paths of Discovery, I presented a paper with the title The case of exoplanets [Léna 2005]. It was then close to the 10th anniversary of the discovery of the first exoplanet in 1995. There is no point in repeating here this paper. But in the last decade, the discoveries on this subject have been so considerable that, the 20th anniversary coming, it is worth addressing the topic again. During the first decade 1995-2004, only 133 exoplanets had been discovered by an indirect method, and the first direct image of an exoplanet was not even confirmed. Today in our Galaxy containing the Earth, statistics begin to indicate that on average every star has a planet, which means over 100 billions of exoplanets for this galaxy alone, of which nearly 2000 are now identified and more or less characterized. How does the subject of exoplanets relate with the Evolving concepts of nature, the title of this Plenary Session? In the 2005 paper, I recalled the long history of a quest which began metaphysically with Democritus, was disputed theologically during the Middle Age, provided phantasies to poets and writers, until it emerged as a scientific problem, to be addressed with the investigative methods of astronomy during the 19th century. Along this path, Giordano Bruno, who expressed ideas close to Lucretius’s ones, was condemned to the fire for multiple reasons, including this one. -
Extrasolar Planets
Extrasolar Planets Dieter Schmitt Lecture Max Planck Institute for Introduction to Solar System Research Solar System Physics Katlenburg-Lindau Uni Göttingen, 8 June 2009 Outline • Historical Overview • Detection Methods • Planet Statistics • Formation of Planets • Physical Properties • Habitability Historical overview • 1989: planet / brown dwarf orbiting HD 114762 (Latham et al.) • 1992: two planets orbiting pulsar PSR B1257+12 (Wolszczan & Frail) • 1995: first planet around a solar-like star 51 Peg b (Mayor & Queloz) • 1999: first multiple planetary system with three planets Ups And (Edgar et al.) • 2000: first planet by transit method HD 209458 b (Charbonneau et al.) • 2001: atmosphere of HD 209458 b (Charbonneau et al.) • 2002: astrometry applied to Gliese 876 (Benedict et al.) • 2005: first planet by direct imaging GQ Lupi b (Neuhäuser et al.) • 2006: Earth-like planet by gravitational microlensing (Beaulieu et al.) • 2007: Gliese 581d, small exoplanet near habitability zone (Selsis et al.) • 2009: Gliese 581e, smallest exoplanet with 1.9 Earth masses (Mayor et al.) • As of 7 June 2009: 349 exoplanets in 296 systems (25 systems with 2 planets, 9 with 3, 2 with 4 and 1 with 5) www.exoplanet.eu Our Solar System 1047 MJ 0.39 AU 0.00314 MJ 1 MJ 0.30 MJ 0.046 MJ 0.054 MJ 1 AU 5.2 AU 9.6 AU 19 AU 30 AU 1 yr 11.9 yr 29.5 yr 84 yr 165 yr Definition Planet IAU 2006: • in orbit around the Sun / star • nearly spherical shape / sufficient mass for hydrostatic equilib. • cleared neighbourhood around its orbit Pluto: dwarf planet, as Ceres Brown -
Extrasolar Planets
Extrasolar Planets Dieter Schmitt Lecture Max Planck Institute for Introduction to Solar System Research Solar System Physics KatlenburgLindau Uni Göttingen, 8 June 2009 Outline • Historical Overview • Detection Methods • Planet Statistics • Formation of Planets • Physical Properties • Habitability Historical overview • 1989: planet / brown dwarf orbiting HD 114762 (Latham et al.) • 1992: two planets orbiting pulsar PSR B1257+12 (Wolszczan & Frail) • 1995: first planet around a solarlike star 51 Peg b (Mayor & Queloz) • 1999: first multiple planetary system with three planets Ups And (Edgar et al.) • 2000: first planet by transit method HD 209458 b (Charbonneau et al.) • 2001: atmosphere of HD 209458 b (Charbonneau et al.) • 2002: astrometry applied to Gliese 876 (Benedict et al.) • 2005: first planet by direct imaging GQ Lupi b (Neuhäuser et al.) • 2006: Earthlike planet by gravitational microlensing (Beaulieu et al.) • 2007: Gliese 581d, small exoplanet near habitability zone (Selsis et al.) • 2009: Gliese 581e, smallest exoplanet with 1.9 Earth masses (Mayor et al.) • As of 7 June 2009: 349 exoplanets in 296 systems (25 systems with 2 planets, 9 with 3, 2 with 4 and 1 with 5) www.exoplanet.eu Our Solar System 1047 MJ 0.39 AU 0.00314 MJ 1 MJ 0.30 MJ 0.046 MJ 0.054 MJ 1 AU 5.2 AU 9.6 AU 19 AU 30 AU 1 yr 11.9 yr 29.5 yr 84 yr 165 yr Definition Planet IAU 2006: • in orbit around the Sun / star • nearly spherical shape / sufficient mass for hydrostatic equilib. • cleared neighbourhood around its orbit Pluto: dwarf planet, as Ceres Brown