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Do M Dwarfs Pulsate? the Search with the Beating Red Dots Project Using HARPS
Highlights on Spanish Astrophysics X, Proceedings of the XIII Scientific Meeting of the Spanish Astronomical Society held on July 16 – 20, 2018, in Salamanca, Spain. B. Montesinos, A. Asensio Ramos, F. Buitrago, R. Schödel, E. Villaver, S. Pérez-Hoyos, I. Ordóñez-Etxeberria (eds.), 2019 Do M dwarfs pulsate? The search with the Beating Red Dots project using HARPS. Zaira M. Berdi~nas 1, Eloy Rodr´ıguez 2, Pedro J. Amado 2, Cristina Rodr´ıguez-L´opez2, Guillem Anglada-Escud´e 3, and James S. Jenkins1 1 Departamento de Astronom´ıa,Universidad de Chile, Camino el Observatorio 1515, Las Condes, Santiago, Chile. 2 Instituto de Astrof´ısica de Andaluc´ıa–CSIC,Glorieta de la Astonom´ıaS/N, E-18008 Granada, Spain 3 School of Physics and Astronomy, Queen Mary University of London, 327 Mile End Rd., London, E1 4NS, UK. Abstract Only a few decades have been necessary to change our picture of a lonely Universe. Nowa- days, red stars have become one of the most exciting hosts of exoplanets (e.g. Proxima Cen [1], Trappist-1 [8], Barnard's star [12]). However, the most popular techniques used to detect exoplanets, i.e. the radial velocities and transit methods, are indirect. As a consequence, the exoplanet parameters obtained are always relative to the stellar parameters. The study of stellar pulsations has demonstrated to be able to give some of the stellar parameters at an unprecedented level of accuracy, thus accordingly decreasing the uncertainties of the mass and radii parameters estimated for their exoplanets. Theoretical studies predict that M dwarfs can pulsate, i.e. -
6 Dec 2019 Is Interstellar Travel to an Exoplanet Possible?
Physics Education Publication Date Is interstellar travel to an exoplanet possible? Tanmay Singal1 and Ashok K. Singal2 1Department of Physics and Center for Field Theory and Particle Physics, Fudan University, Shanghai 200433, China. [email protected] 2Astronomy and Astrophysis Division, Physical Research Laboratory Navrangpura, Ahmedabad 380 009, India. [email protected] Submitted on xx-xxx-xxxx Abstract undertake such a voyage, with hopefully a positive outcome? What could be a possible scenario for such an adventure in a near In this article, we examine the possibility of or even distant future? And what could be interstellar travel to reach some exoplanet the reality of UFOs – Unidentified Flying orbiting around a star, beyond our Solar Objects – that get reported in the media system. Such travels have been in the realm from time to time? of science fiction for long. However, in the last 50 years or so, this question has gained further impetus in the mind of a man on the 1 Introduction street, after the interplanetary travel has become a reality. Of course the distances to In the last three decades many thousands of be covered to reach even some of the near- exoplanets, planets that orbit around stars est stars outside the Solar system could be beyond our Solar system, have been dis- arXiv:1308.4869v2 [physics.pop-ph] 6 Dec 2019 hundreds of thousands of time larger than covered. Many of them are in the habit- those encountered within the interplanetary able zone, possibly with some forms of life space. Consequently, the time and energy evolved on a fraction of them, and hope- requirements for such a travel could be fully, the existence of intelligent life on some immensely prohibitive. -
Pricelist Abstraction (Jean-Marie Gitard (Mr STRANGE))
Artmajeur JEAN-MARIE GITARD (MR STRANGE) (FRANCE) ARTMAJEUR.COM/JEANMARIEGITARD Pricelist: Abstraction 22 Artworks Image Title Status Price Spirale For Sale $318.14 Digital Arts, 98x82x0.1 cm ©2020 Ref 13786553 artmajeur.link/l94q4U HERAKLION For Sale $365.45 Digital Arts, 75x100x0.1 cm ©2019 Ref 13659182 artmajeur.link/velV6l PHAEDRA 112 Ca For Sale $259.01 Digital Arts, 50x50x0.1 cm ©2020 Ref 13609553 artmajeur.link/zOOdl6 GLIESE 668 Cc Limited Edition For Sale $259.01 Digital Arts, 50x50x0.1 cm ©2018 Ref 13609547 artmajeur.link/tVScWB KOI-1686.01 For Sale $353.62 Digital Arts, 80x80x0.1 cm ©2018 Ref 12809219 artmajeur.link/lqEm9T 1 / 4 Image Title Status Price LHS 1723 b For Sale $353.62 Digital Arts, 100x75x0.1 cm ©2018 Ref 12809207 artmajeur.link/iEB3Ph Kepler-438 b For Sale $341.8 Digital Arts, 82x82x0.1 cm ©2019 Ref 12300905 artmajeur.link/8D7uGT Luyten b For Sale $365.45 Digital Arts, 100x75x0.1 cm ©2019 Ref 12300896 artmajeur.link/wnZk2l Proxima Centauri b For Sale $341.8 Digital Arts, 82x82x0.1 cm ©2017 Ref 12283532 artmajeur.link/Y8zZkd Gliese 667 Cc For Sale $341.8 Digital Arts, 82x82x0.1 cm ©2018 Ref 12283529 artmajeur.link/LMBNRI K2-72-e For Sale $353.62 Digital Arts, 96x80x0.1 cm ©2018 Ref 12283526 artmajeur.link/FZDM29 2 / 4 Image Title Status Price TRAPPIST-1d For Sale $353.62 Digital Arts, 100x75x0.1 cm ©2018 Ref 12274691 artmajeur.link/xSVnNP Tau Ceti e For Sale $353.62 Digital Arts, 75x100x0.1 cm ©2017 Ref 12274649 artmajeur.link/DbFvHV KOI-3010.01 For Sale $341.8 Digital Arts, 82x82x0.1 cm ©2019 Ref 12274613 artmajeur.link/pGjEoY -
The Detectability of Nightside City Lights on Exoplanets
Draft version September 6, 2021 Typeset using LATEX twocolumn style in AASTeX63 The Detectability of Nightside City Lights on Exoplanets Thomas G. Beatty1 1Department of Astronomy and Steward Observatory, University of Arizona, Tucson, AZ 85721; [email protected] ABSTRACT Next-generation missions designed to detect biosignatures on exoplanets will also be capable of plac- ing constraints on the presence of technosignatures (evidence for technological life) on these same worlds. Here, I estimate the detectability of nightside city lights on habitable, Earth-like, exoplan- ets around nearby stars using direct-imaging observations from the proposed LUVOIR and HabEx observatories. I use data from the Soumi National Polar-orbiting Partnership satellite to determine the surface flux from city lights at the top of Earth's atmosphere, and the spectra of commercially available high-power lamps to model the spectral energy distribution of the city lights. I consider how the detectability scales with urbanization fraction: from Earth's value of 0.05%, up to the limiting case of an ecumenopolis { or planet-wide city. I then calculate the minimum detectable urbanization fraction using 300 hours of observing time for generic Earth-analogs around stars within 8 pc of the Sun, and for nearby known potentially habitable planets. Though Earth itself would not be detectable by LUVOIR or HabEx, planets around M-dwarfs close to the Sun would show detectable signals from city lights for urbanization levels of 0.4% to 3%, while city lights on planets around nearby Sun-like stars would be detectable at urbanization levels of & 10%. The known planet Proxima b is a particu- larly compelling target for LUVOIR A observations, which would be able to detect city lights twelve times that of Earth in 300 hours, an urbanization level that is expected to occur on Earth around the mid-22nd-century. -
Prusaprinters
Exoplanets scaled one in 120 million 3D MODEL ONLY tato_713 VIEW IN BROWSER updated 5. 3. 2021 | published 5. 3. 2021 Summary Some of the most notable Earth-sized exoplanets scaled (smaller than 2.5 Earth diameter). Learning > Physics & Astronomy trappist1h trappist1g trappist1f trappist1e trappist1d trappist1c trappist1b trappist1 trappist terrestrialplanet space scalemodel scaledmodel scale proximacentauri planets planetas planeta planet oceanworld kepler62b kepler62 kepler22b kepler22 kepler11b icegigant extraterrestrial corot7 chthonianplanet chthonian astronomy astronomia Originally published here: Exoplanets scaled one in 120 million by tato_713 - Thingiverse The concept of this post is to compare the size in the same scale of various Earth sized exoplanets with the Earth itself or other astronomical bodies like Neptune. Although there are thousands exoplanets confirmed, I made only some of the most notorious ones with known diameter, and nearly Earth sized (up to 2.5 its diameter). The models are just spheres scaled one in 120 million, to compare with terrestrial planets; one in 250 million; and one in 500 million for the biggest ones. The file's names explained: name_1_x_10_y.stl is 1 : x* 10^y. So _1_6_10_7 is 1:600000000 or one in 60 million. Proxima Centauri b Proxima b is the closest exoplanet known to the Solar System, the closest within the habitable zone of its star, the only known planet in the nearest star, Proxima Centauri, and the only one confirmed in the Alpha Centauri system. As is it said, the host star for the planet is part of the Alpha Centauri system, orbiting the two main stars Alpha Centauri A (Rigil Kentaurus) and B (Toliman). -
44 Closest Stars and How They Compare to Our Sun
44 CLOSEST STARS AND HOW THEY COMPARE TO OUR SUN R = Solar radius (a unit of distance to express the size of stars relative to the sun) L = Solar luminosity (a unit of radiant flux used SUN System/constellation to compare the luminosity of stars, galaxies, Solar System Potential planets and other celestial objects in terms of the sunʼs output) 8 Distance From Earth 8.317 light-minutes EARTH 1R (432,288 miles) s) -year (light Proxima Centauri TH EAR Alpha Centauri OM E FR 1 ANC DIST 4.244 light-years 0.001 0.01 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10 25 0.1542R 0.00005L L <=0.0001 α Centauri A (Rigil Kentaurus) 1 Alpha Centauri L 4.365 light-years 1.223R 1.519 L α Centauri B (Toliman) 5 Alpha Centauri light-years 4.37 light-years 0.863R 0.5002L Bernard’s Star Ophiuchus 1 5.957 light-years 0.196R 0.0035L Wolf 359 (CN Leonis) Leo 2 7.856 light-years 0.16R 0.0014L Lalande 21185 Ursa Major 1 8.307 light-years 0.393R 0.026L Sirius A Canis Major Luyten 726-8A 8.659 light-years Cetus 1.711 R 25.4L 8.791 light-years 0.14R 0.00004L Sirius B Canis Major 8.659 light-years Luyten 726-8B 0.0084R 0.056L Cetus 8.791 light-years 0.14R 0.00004L Ross 154 Sagittarius 9.7035 light-years 0.24R 0.0038L 10 light-years Epsilon Eridani Eridanus Ross 248 2 Andromeda 10.446 light-years 10.2903 light-years 0.735R 0.34L 0.16R 0.0018L Lacaille 9352 Piscis Austrinus 3 10.7211 light-years Ross 128 0.47R 0.0367L Virgo 1 EZ Aquarii A 11 light-years Aquarius 61 Cygni A 0.1967R 0.00362L 11.1 light-years Cygnus 0.175R 0.000087L 3 (part of triple star system) 11.4 light-years -
Ground-Based Capabilities for General Astrophysics and Exoplanets Science
Ground-based capabilities for general astrophysics and exoplanets science Olivier Guyon University of Arizona Subaru Telescope, National Astronomical Observatory of Japan, National Institutes for Natural Sciences Astrobiology Center, National Institutes for Natural Sciences JAXA HabEx meeting, Aug 3, 2016 HabEx Uniqueness HabEx unique capabilities (not accessible from ground): ● Largest UV-Opt astronomical aperture in space ● Spectral coverage: UV not accessible from ground, continuous NIR coverage ● Angular resolution in UV .. and optical ? ● Ultra-high contrast ● High stability → astrometry → precision photometry, spectroscopy Major ground facilities (Opt-NIR) ELTs coming online in mid-2020s: ● E-ELT: 39m aperture, Chile ● TMT: 30m, Hawaii(?) ● GMT: 25m, Chile 8-m class survey telescope/instruments: ● Imaging: LSST ● Spectroscopy: Subaru-PFS + other dedicated survey facilities (LAMOST, PAN-STARRS PTF etc…) Wide FOV optical imaging: Subaru HSC 8m aperture, 1.5deg diam FOV 104 4kx2k CCDs LSST 8m aperture, 3.5deg diam FOV 189 4kx4k CCDs Subaru Prime Focus Spectrograph 2,400 fibers over 1.3 deg diam FOV 0.38 – 1.26 um Increased image quality over moderate FOV in near-IR with GLAO example: ULTIMATE-Subaru ELTs E-ELT first light instruments E-ELT – First Light instruments MAORY + MICADO (Multi-conjugate Adaptive Optics RelaY for the E-ELT) (Multi-AO Imaging Camera for Deep Observations) 0.8 – 2.4 um diffraction-limited imaging (6 – 12 mas) R=8000 spectroscopy HARMONI (High Angular Resolution Monolithic Optical and Near-infrared Integral field -
Astronomical Considerations Relating to the Choice of Target Star
Project Icarus: Astronomical Considerations RelangJBIS, to the Vol. Choice 63, pp. of 419-425Target Star, 2010 PROJECT ICARUS: ASTRONOMICAL CONSIDERATIONS RELATING TO THE CHOICE OF TARGET STAR I.A. CRAWFORD Department of Earth and Planetary Sciences, Birkbeck College London, Malet Street, London, WC1E 7HX, UK. In this paper we outline the considerations required in order to select a target star system for the Icarus interstellar mission. It is considered that the maximum likely range for the Icarus vehicle will be 15 light-years, and a list is provided of all known stars within this distance range. As the scientific objectives of Icarus are weighted towards planetary science and astrobiology, a final choice of target star(s) cannot be made until we have a clearer understanding of the prevalence of planetary systems within 15 light-years of the Sun, and we summarize what is currently known regarding planetary systems within this volume. We stress that by the time an interstellar mission such as Icarus is actually undertaken, astronomical observations from the solar system will have provided this information. Finally, given the high proportion of multiple star systems within 15 light- years (including the closest of all stars to the Sun in the α Centauri system), we stress that a flexible mission architecture, able to visit stars and accompanying planets within multiple systems, is desirable. This paper is a submission of the Project Icarus Study Group. Keywords: Interstellar travel; nearby stars; extrasolar planets; astrobiology 1. INTRODUCTION The Icarus study is tasked with designing an interstellar space 2. STARS WITHIN 15 LIGHT-YEARS OF THE SUN vehicle capable of making in situ scientific investigations of a nearby star and accompanying planetary system [1, 2]. -
Habitable Planet – a Rocky, Terrestrial-Size Planet in a Habitable Zone of a Star
Habitable Exoplanets Margarita Safonova M. P. Birla Institute of Fundamental Research Indian Institute of Astrophysics Bangalore There are countless suns and countless earths all rotating round their suns in exactly the same way as the seven planets of our system…. The countless worlds in the universe are no worse and no less inhabited than our earth. — Giordano Bruno (circa 1584) Margarita Safonova. Habitable exoplanets: Overview. C. Sivaram. Astrochemistry and search for biosignatures on exoplanets. 11 May, 2018 Snehanshu Saha. Exploring habitability of exoplanets via modeling and machine learning. June 15, 2018 Exoplanets – extra solar planets But we cannot exclude Solar System objects. Firstly, some can be habitable, or even inhabited. Mars may still have subterranean kind of life, Europa&Enceladus have subsurface oceans kept warm by the tidal stresses. Titan has essentially Earth-like surface, albeit with lakes and rivers of liquid methane, and thick organic hazy atmosphere. Secondly, they can be used as calibrators. E.g., based on the composition, the simplified planet taxonomy using the SS: Rocky (>50% silicate rock), but Mercury ~64% iron core. Icy (>50% ice by mass), but both N&U have significant rock and gas. Gaseous (>50% H/He). Thousands of detected exoplanets now called as super-earths, hot earths, mini-neptunes, hot neptunes, sub-neptunes, saturns, jupiters, hot jupiters, jovians, gas giants, ice giants, rocky, terrestrial, terran, subterran, superterran, etc… Exoplanets Is there a limit on the size/mass of a planet? The lower mass limit may be assumed as of Mimas (3.7x1019 kg) – approx. min mass required for an icy body to attain a nearly spherical hydrostatic equilibrium shape. -
Olivier Guyon [email protected]
WATCH Olivier Guyon [email protected] Breakthrough Watch Advisory Committee chair Subaru Telescope, NAOJ, NINS University of Arizona Japanese Astrobiology Center, NINS BREAKTHROUGH WATCH Identify and chararacterize nearby habitable planets Targets: Nearest stars < ~5pc → search for biomarkers → Future exploration (Starshot) Approaches Ground and space Detection and spectroscopic characterization BTW key effort Task R&D, Design, instrument work On-sky observations force CY2016 CY2017 CY2018 CY2019 CY2020 CY2021 CY2022 CY2023 CY2024 CY2025 CY2026 Searching for Earth-mass planets in the habitable zones of Alpha Cen A & B Alpha Cen Thermal Imaging Uses existing large ground-based telescopes Instruments/cameras development On-sky observations Alpha Cen Astrometry (TOLIMAN) 30cm space telescope Design Fabrication, testing Science operation [3yr] If planet found Alpha Cen planet characterization task force Alpha Cen planet characterization mission(s) – BTW-led or BTW-assisted Finding and characterizing habitable worlds within 5pc Indirect detection, mass & orbit measurements of habitable planets within 5pc Strategic investments in existing and future RV and astrometry projects BTW participation to ground-based near-IR RV campaign (likely near-IR, possibly optical) RV & Astrometry task force BTW participation to space-based astrometry mission Imaging & spectroscopy of habitable planets within 5pc with ELTs Targets Development and deployment of instrumentation for spectroscopic characterization of rocky planets in habitable zones of -
Imaging Exoplanets
Imaging Exoplanets Olivier Guyon University of Arizona Subaru Telescope, National Astronomical Observatory of Japan, National Institutes for Natural Sciences (NINS) Astrobiology Center, National Institutes for Natural Sciences (NINS) Habitable zone of a star Every star has a habitable zone How do astronomers identify exoplanets ? HIGH PRECISION OPTICAL MEASUREMENTS OF STARLIGHT (indirect techniques) Earth around Sun at ~30 light year → Star position moves by 0.3 micro arcsecond (thickness of a human hair at 30,000 km) → Star velocity is modulated by 10cm / sec (changes light frequency by 1 part in 3,000,000,000) If Earth-like planet passes in front of Sun-like star, star dims by 70 parts per million (12x12 pixel going dark on a HD TV screen 70 miles away) Habitable Zones within 5 pc (16 ly): Astrometry and RV Signal Amplitudes for Earth Analogs Star Temperature [K] Approximate Sirius detection limit for ground-based α Cen A optical RV F, G, K stars Approximate expected detection α Cen B limit for space astrometry Procyon A Proxima Cen Eps Eri Barnard's star CN Leonis Circle diameter is proportional to 1/distance Circle color indicates stellar temperature (see scale right of figure) Astrometry and RV amplitudes are given for an Earth analog receiving the same stellar flux as Earth receives from Sun (reflected light) Expected detection limit for near-IR RV surveys, M-type stars Why directly imaging ? Woolf et al. Spectrum of Earth (taken by looking at Earthshine) shows evidence for life and plants 5 Exoplanet transit If the planet passes in front of its star, we see the star dimming slightly Transit of Venus, June 2012 Taking images of habitable exoplanets: Why is it hard ? 7 8 Coronagraphy … Using optics tricks to remove starlight (without removing planet light) ← Olivier's thumb.. -
World Ships: Feasibility and Rationale Andreas Makoto Hein, Cameron Smith, Frédéric Marin, Kai Staats
World ships: Feasibility and Rationale Andreas Makoto Hein, Cameron Smith, Frédéric Marin, Kai Staats To cite this version: Andreas Makoto Hein, Cameron Smith, Frédéric Marin, Kai Staats. World ships: Feasibility and Rationale. ACTA Futura, European Space Agency, Advanced Concepts Team, 2020. hal-02561266 HAL Id: hal-02561266 https://hal.archives-ouvertes.fr/hal-02561266 Submitted on 3 May 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. World ships: Feasibility and Rationale Andreas Makoto Hein,∗ Cameron Smith, Fred´ eric´ Marin, Kai Staats Initiative for Interstellar Studies, 27-29 South Lambeth Road, London SW8 1SZ, United Kingdom Department of Anthropology, Portland State University Portland, OR, 97207, USA Universite´ de Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, UMR 7550, F-67000 Strasbourg, France Arizona State University Interplanetary Initiative, Phoenix, Arizona, USA April 5, 2020 Abstract Key roadblocks for world ships are the large amount of required resources, shifting its eco- World ships are hypothetical, large, self- nomic feasibility beyond the year 2300 and the contained spacecraft for crewed interstellar development of a maintenance system capable travel, taking centuries to reach other stars. of detecting, replacing, and repairing several Due to their crewed nature, size and long trip components per second.