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Habitability on Local, Galactic and Cosmological Scales
Habitability on local, Galactic and cosmological scales Luigi Secco1 • Marco Fecchio1 • Francesco Marzari1 Abstract The aim of this paper is to underline con- detectable studying our site. The Climatic Astronom- ditions necessary for the emergence and development ical Theory is introduced in sect.5 in order to define of life. They are placed at local planetary scale, at the circumsolar habitable zone (HZ) (sect.6) while the Galactic scale and within the cosmological evolution, translation from Solar to extra-Solar systems leads to a as pointed out by the Anthropic Cosmological Princi- generalized circumstellar habitable zone (CHZ) defined ple. We will consider the circumstellar habitable zone in sect.7 with some exemplifications to the Gliese-667C (CHZ) for planetary systems and a Galactic Habitable and the TRAPPIST-1 systems; some general remarks Zone (GHZ) including also a set of strong cosmologi- follow (sect.8). A first conclusion related to CHZ is cal constraints to allow life (cosmological habitability done moving toward GHZ and COSH (sect.9). The (COSH)). Some requirements are specific of a single conditions for the development of life are indeed only scale and its related physical phenomena, while others partially connected to the local scale in which a planet are due to the conspired effects occurring at more than is located. A strong interplay between different scales one scale. The scenario emerging from this analysis is exists and each single contribution to life from individ- that all the habitability conditions here detailed must ual scales is difficult to be isolated. However we will at least be met. -
Exodata: a Python Package to Handle Large Exoplanet Catalogue Data
ExoData: A Python package to handle large exoplanet catalogue data Ryan Varley Department of Physics & Astronomy, University College London 132 Hampstead Road, London, NW1 2PS, United Kingdom [email protected] Abstract Exoplanet science often involves using the system parameters of real exoplanets for tasks such as simulations, fitting routines, and target selection for proposals. Several exoplanet catalogues are already well established but often lack a version history and code friendly interfaces. Software that bridges the barrier between the catalogues and code enables users to improve the specific repeatability of results by facilitating the retrieval of exact system parameters used in an arti- cles results along with unifying the equations and software used. As exoplanet science moves towards large data, gone are the days where researchers can recall the current population from memory. An interface able to query the population now becomes invaluable for target selection and population analysis. ExoData is a Python interface and exploratory analysis tool for the Open Exoplanet Cata- logue. It allows the loading of exoplanet systems into Python as objects (Planet, Star, Binary etc) from which common orbital and system equations can be calculated and measured parame- ters retrieved. This allows researchers to use tested code of the common equations they require (with units) and provides a large science input catalogue of planets for easy plotting and use in research. Advanced querying of targets are possible using the database and Python programming language. ExoData is also able to parse spectral types and fill in missing parameters according to programmable specifications and equations. Examples of use cases are integration of equations into data reduction pipelines, selecting planets for observing proposals and as an input catalogue to large scale simulation and analysis of planets. -
© in This Web Service Cambridge University
Cambridge University Press 978-1-107-09161-0 - Planetary Sciences: Updated Second Edition Imke de Pater and Jack J. Lissauer Index More information Index D region, 263 Airy hypothesis, 252–253, 280 I/F,59 Aitken basin, 266 β-effect, 109 albedo γ -ray fluorescence, 571 Bond albedo, 58, 77, 144 3He, 386 geometric albedo, 59 ν6 resonance, 581 giant planets, 77 monochromatic albedo, 58 ’a’a, 168f, 168 terrestrial panets, 77–78 ablation, 184 albite, 162, 239 absorption, 67 Aleutan islands, 167 absorption coefficient, 67, 71 Alfven´ velocity; see velocity absorption line, 85 Alfven´ waves, 291, 306 accretion zone, 534 ALH84001, 342 achondrites, 337, 339, 358 allotropes, 217 eucrite, 339 α decay, 352, 365 HED, 358 Amalthea, 227f, 455, 484 acid rain, 194 amorphous ice, 412, 438 activation energy, 127 Ampere’s law, 290 active region, 283 amphibole, 154 active sector, 317, 319 andesite, 156f Adams–Williams equation, 261, 281 angle of repose, 163 adaptive optics (AO), 104, 194, 494, 568f, 568–569 angular momentum, 521 adiabatic invariants anhydrous rock, 550 first invariant, 297 anion, 153 second invariant, 297–298 anomalous cosmic rays, 311f, 312 third invariant, 298 anorthite, 162, 197 adiabatic lapse rate, 63–64, 80–81, 149 anorthosite, 197 dry, 64, 80 ansa, 459 giant planets, 77 antapex, 189 superadiabatic, 64, 70, 111 Antarctica, 214 wet, 101–102 anticyclone, 111f, 112 Adrastea, 225, 227f, 454f, 484 antipode, 183, 197, 316 advection, 61 apex, 189 advective derivative, 108 Apollo program, 16 aeolian processes, 173 Apollo spacecraft, 95, 185, 196–197, 267f, 316, 341 aerodynamic drag, 49, 55, 102, 347–348, 416 apparition, 407 aerogel, 432f, 432 aqueous alteration, 401 AGB star (asymptotic giant branch), 527 arachnoid, 201, 202f agregates, 528 Archimedean spiral, 287f airglow, 135 Archimedes principle, 251 625 © in this web service Cambridge University Press www.cambridge.org Cambridge University Press 978-1-107-09161-0 - Planetary Sciences: Updated Second Edition Imke de Pater and Jack J. -
Les Exoplanètes
LESLES EXOPLANEXOPLANÈÈTESTES Introduction Les différentes méthodes de détection Le télescope spatial Kepler Résultats et typologie GAP 47 • Olivier Sabbagh • Avril 2016 Les exoplanètes I Introduction Une exoplanète, ou planète extrasolaire, est une planète située en dehors du système solaire, c’est à dire une planète qui est en orbite autour d’une étoile autre que notre Soleil. L'existence de planètes situées en dehors du Système solaire est évoquée dès le XVIe siècle par Giordano Bruno. Ce moine novateur et provocateur du XVI° siècle a eu des intuitions foudroyantes qu’il assénait avec force et conviction, en opposition farouche contre le dogme du géocentrisme qui prévalait depuis Aristote et Ptolémée. Son entêtement lui vaudra le bûcher pour hérésie en 1600. Voir le paragraphe qui lui est consacré dans notre document « une histoire de l’astronomie ». Dès 1584 (Le Banquet des cendres), Bruno adhère, contre la cosmologie d'Aristote, à la cosmologie de Copernic (1543), à l'héliocentrisme : double mouvement des planètes sur elles-mêmes et autour du Soleil, au centre. Mais Bruno va plus loin : il veut renoncer à l'idée de centre : « Il n'y a aucun astre au milieu de l'univers, parce que celui-ci s'étend également dans toutes ses directions ». Chaque étoile est un soleil semblable au nôtre, et autour de chacune d'elles tournent d'autres planètes, invisibles à nos yeux, mais qui existent. « Il est donc d'innombrables soleils et un nombre infini de terres tournant autour de ces soleils, à l'instar des sept « terres » [la Terre, la Lune, les cinq planètes alors connues : Mercure, Vénus, Mars, Jupiter, Saturne] que nous voyons tourner autour du Soleil qui nous est proche ». -
THE KINEMATICS and AGES of STARS in GLIESE's CATALOGUE 1. Introduction This Contribution Gives Some Results on the Kinematics An
THE KINEMATICS AND AGES OF STARS IN GLIESE'S CATALOGUE R. WIELEN Astronomisches Rechen-Institut, Heidelberg, F.R.G. 1. Introduction This contribution gives some results on the kinematics and ages of stars near the Sun. These results are mainly based on the catalogue of nearby stars compiled by Gliese (1957, 1969 and minor recent modifications). Table I shows the number of objects under consideration. While the old catalogue (1957) contained only stars with distances r up to 20 pc, the new edition (1969) includes many stars with slightly larger distances. In Table I, a 'system' is either a single star or a binary or a multiple system. The number of systems with known space velocities nearer than 20 pc has increased by about 30% from 1957 to 1969. The first edition of Gliese's catalogue (1957) has been analyzed in detail by Gliese (1956) and von Hoerner (1960). TABLE I Gliese's Catalogue of Nearby Stars Number Edition 1969 1957 All j-s=20pc r<20 pc Stars 1890 1277 1095 Systems 1529 1036 916 Systems with known space velocity 1131 770 598 Although Gliese's catalogue is the most complete collection of stars within 20 pc, this sample of stars is severely biased by selection effects and is not fully representative for all the nearby stars. Only the stars brighter than M„~ +7 are almost completely known within 20 pc. For the fainter stars, the following selection effects occur: (a) The southern sky is deficient in detected faint nearby stars; (b) Since most of the faint nearby stars are found by their high proper motions, the sample is deficient in stars with small tangential components of their space velocities (measured with respect to the Sun); (c) Due to incomplete detection, the apparent space density of faint stars decreases rapidly with increasing distance r, and this effect becomes stronger with increasing M„. -
[Final] Origin of Oceans and Waterworlds
Origin of oceans and waterworlds Boris Pestoni, Vytenis Šumskas University of Zürich AST 202 The Universe: Contents, Origin, Evolution and Future March 22, 2016 S Contents S Origin of water on Earth S How did the oceans form? S States of matter of water S Is water a peculiarity of the Earth? S Extreme worlds: ice planets and ocean planets Water on Earth S ~71% of the Earth’s surface is covered with water. Water on Earth S Only 0,02% - 0,06% of our planet’s total mass is water. S Nonetheless, Earth is called “The blue planet”. Oceans on Earth S The age of Earth’s oceans is estimated to be nearly the same as the age of Earth: 4 - 4,4 billion years. Oceans on Earth S The planet cooled. S It became covered in gas. Oceans on Earth S The longest rain in the history of Earth. S Eventually water gathered in the deepest parts of surface. Other sources of water S ≥50% of Earth’s water came from outer space. Water in asteroids S How do we even know it? States of matter of water Water in the universe Until now we have found water in the following objects / regions: Out of Proto_ Rings the planetary disk Asteroid Comets of Mars Moon Earth Milky of the Milky belt Saturn Way Way Water of ✓ ✓ ✓ ✓ crystallization Water ice ✓ ✓ ✓ ✓ ✓ ✓ ✓ Liquid water ✓ ✓ ✓ ✓ Steam ✓ ✓ ✓ ✓ ✓ ✓ Supercritical ✓ water Overview of the Solar System Imbalance of water on planets S The reason that there is clearly more liquid water on the Earth than on the other rocky planets of the Solar System is, until now, not completely understood. -
Taking the Measure of the Universe: Precision Astrometry with SIM
Accepted for publication in PASP, January 2008 issue A Preprint typeset using LTEX style emulateapj v. 08/22/09 TAKING THE MEASURE OF THE UNIVERSE: PRECISION ASTROMETRY WITH SIM PLANETQUEST Stephen C. Unwin1, Michael Shao2, Angelle M. Tanner2, Ronald J. Allen3, Charles A. Beichman4, David Boboltz5, Joseph H. Catanzarite2, Brian C. Chaboyer6, David R. Ciardi4, Stephen J. Edberg2, Alan L. Fey5, Debra A. Fischer7, Christopher R. Gelino8, Andrew P. Gould9, Carl Grillmair8, Todd J. Henry10, Kathryn V. Johnston11,12, Kenneth J. Johnston5, Dayton L. Jones2, Shrinivas R. Kulkarni4, Nicholas M. Law4, Steven R. Majewski13, Valeri V. Makarov2, Geoffrey W. Marcy14, David L. Meier2, Rob P. Olling15, Xiaopei Pan2, Richard J. Patterson13, Jo Eliza Pitesky2, Andreas Quirrenbach16, Stuart B. Shaklan2, Edward J. Shaya15, Louis E. Strigari17, John A. Tomsick18,19, Ann E. Wehrle20, and Guy Worthey21 Accepted for publication in PASP, January 2008 issue ABSTRACT Precision astrometry at microarcsecond accuracy has application to a wide range of astrophysical problems. This paper is a study of the science questions that can be addressed using an instrument with flexible scheduling that delivers parallaxes at about 4 microarcsec (µas) on targets as faint as V = 20, and differential accuracy of 0.6 µas on bright targets. The science topics are drawn primarily from the Team Key Projects, selected in 2000, for the Space Interferometry Mission PlanetQuest (SIM PlanetQuest). We use the capabilities of this mission to illustrate the importance of the next level of astrometric precision in modern astrophysics. SIM PlanetQuest is currently in the detailed design phase, having completed in 2005 all of the enabling technologies needed for the flight instrument. -
Discoveries by Astronomer Thomas Scott Zolotor
Discoveries by Astronomer Thomas Scott Zolotor July 30, 2013 at 12:38pm https://www.facebook.com/notes/tom-freethesouls-zolotor/discoveries-by-astronomer-thomas-scott-z olotor/10151738488524144 THOMAS ZOLOTOR IS A FINANCIAL POLICE® DEPUTY AGENT HE ALSO A SEA CAPTAIN AND ORDINATED MINISTER AS WELL AS AN ASTRONOMER. HE SOMETIMES GOES BY CAPTAIN FREE THE SOULS. Astronomer, Thomas Scott Zolotor, is helping to map and study parts of Mars, Mercury, Vesta and the Moon. Thomas is also studying how galaxies form and has classified and discovered never before seen galaxies. He is searching for gravitational waves around pulsars, and has produced a better understanding of how the Milky Way formed. Thomas is seeking to better define dark matter as well as how the universe formed after the big bang. In his studies, Thomas searches for planets around other star systems. In 1991, Thomas found an asteroid. He has discovered several asteroids and stellar clusters to date.Captain Thomas Zolotor took part in the Andromeda Project which produce the largest catalog of star clusters known in any spiral galaxy. He was one of the very first to find undiscovered stellar clusters in this program. He found a stellar cluster that looks like the letter"N" and another that looks like the number 2. He has discovered many more stellar clusters in the galaxy Andromeda. He has published numerous theories about the universe that are supported by recent research. 1. Captain Zolotor discovered never before seen galaxies. 2. Captain Zolotor discovered never before seen stellar clusters and was involved in helping to make the largest ever catalog of stellar clusters. -
Part 1: the 1.7 and 3.9 Earth Radii Rule
Hi this is Steve Nerlich from Cheap Astronomy www.cheapastro.com and this is What are exoplanets made of? Part 1: The 1.7 and 3.9 earth Radii rule. As of August 2016, the current count of confirmed exoplanets is up around 3,400 in 2,617 systems – with 590 of those systems confirmed to be multiplanet systems. And the latest thinking is that if you want to understand what exoplanets are made of you need to appreciate the physical limits of planet-hood, which are defined by the boundaries of 1.7 and 3.9 Earth radii . Consider that the make-up of an exoplanet is largely determined by the elemental make up of its protoplanetary disk. While most material in the Universe is hydrogen and helium – these are both tenuous gases. In order to generate enough gravity to hang on to them, you need a lot of mass to start with. So, if you’re Earth, or anything up to 1.7 times the radius of Earth – you’ve got no hope of hanging onto more than a few traces of elemental hydrogen and helium. Indeed, any exoplanet that’s less than 1.7 Earth radii has to be primarily composed of non-volatiles – that is, things that don’t evaporate or blow away easily – to have any chance of gravitationally holding together. A non-volatile exoplanet might be made of rock – which for our Solar System is a primarily silicon/oxygen based mineral matrix, but as we’ll hear, small sub-1.7 Earth radii exoplanets could be made of a whole range of other non-volatile materials. -
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. -
Jeu Complet Recto
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QUALIFIER EXAM SOLUTIONS 1. Cosmology (Early Universe, CMB, Large-Scale Structure)
Draft version June 20, 2012 Preprint typeset using LATEX style emulateapj v. 5/2/11 QUALIFIER EXAM SOLUTIONS Chenchong Zhu (Dated: June 20, 2012) Contents 1. Cosmology (Early Universe, CMB, Large-Scale Structure) 7 1.1. A Very Brief Primer on Cosmology 7 1.1.1. The FLRW Universe 7 1.1.2. The Fluid and Acceleration Equations 7 1.1.3. Equations of State 8 1.1.4. History of Expansion 8 1.1.5. Distance and Size Measurements 8 1.2. Question 1 9 1.2.1. Couldn't photons have decoupled from baryons before recombination? 10 1.2.2. What is the last scattering surface? 11 1.3. Question 2 11 1.4. Question 3 12 1.4.1. How do baryon and photon density perturbations grow? 13 1.4.2. How does an individual density perturbation grow? 14 1.4.3. What is violent relaxation? 14 1.4.4. What are top-down and bottom-up growth? 15 1.4.5. How can the power spectrum be observed? 15 1.4.6. How can the power spectrum constrain cosmological parameters? 15 1.4.7. How can we determine the dark matter mass function from perturbation analysis? 15 1.5. Question 4 16 1.5.1. What is Olbers's Paradox? 16 1.5.2. Are there Big Bang-less cosmologies? 16 1.6. Question 5 16 1.7. Question 6 17 1.7.1. How can we possibly see galaxies that are moving away from us at superluminal speeds? 18 1.7.2. Why can't we explain the Hubble flow through the physical motion of galaxies through space? 19 1.7.3.