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The Large Scale Universe As a Quasi Quantum White Hole
International Astronomy and Astrophysics Research Journal 3(1): 22-42, 2021; Article no.IAARJ.66092 The Large Scale Universe as a Quasi Quantum White Hole U. V. S. Seshavatharam1*, Eugene Terry Tatum2 and S. Lakshminarayana3 1Honorary Faculty, I-SERVE, Survey no-42, Hitech city, Hyderabad-84,Telangana, India. 2760 Campbell Ln. Ste 106 #161, Bowling Green, KY, USA. 3Department of Nuclear Physics, Andhra University, Visakhapatnam-03, AP, India. Authors’ contributions This work was carried out in collaboration among all authors. Author UVSS designed the study, performed the statistical analysis, wrote the protocol, and wrote the first draft of the manuscript. Authors ETT and SL managed the analyses of the study. All authors read and approved the final manuscript. Article Information Editor(s): (1) Dr. David Garrison, University of Houston-Clear Lake, USA. (2) Professor. Hadia Hassan Selim, National Research Institute of Astronomy and Geophysics, Egypt. Reviewers: (1) Abhishek Kumar Singh, Magadh University, India. (2) Mohsen Lutephy, Azad Islamic university (IAU), Iran. (3) Sie Long Kek, Universiti Tun Hussein Onn Malaysia, Malaysia. (4) N.V.Krishna Prasad, GITAM University, India. (5) Maryam Roushan, University of Mazandaran, Iran. Complete Peer review History: http://www.sdiarticle4.com/review-history/66092 Received 17 January 2021 Original Research Article Accepted 23 March 2021 Published 01 April 2021 ABSTRACT We emphasize the point that, standard model of cosmology is basically a model of classical general relativity and it seems inevitable to have a revision with reference to quantum model of cosmology. Utmost important point to be noted is that, ‘Spin’ is a basic property of quantum mechanics and ‘rotation’ is a very common experience. -
An Introduction to Our Universe
An Introduction to Our Universe Lyman Page Princeton, NJ [email protected] Draft, August 31, 2018 The full-sky heat map of the temperature differences in the remnant light from the birth of the universe. From the bluest to the reddest corresponds to a temperature difference of 400 millionths of a degree Celsius. The goal of this essay is to explain this image and what it tells us about the universe. 1 Contents 1 Preface 2 2 Introduction to Cosmology 3 3 How Big is the Universe? 4 4 The Universe is Expanding 10 5 The Age of the Universe is Finite 15 6 The Observable Universe 17 7 The Universe is Infinite ?! 17 8 Telescopes are Like Time Machines 18 9 The CMB 20 10 Dark Matter 23 11 The Accelerating Universe 25 12 Structure Formation and the Cosmic Timeline 26 13 The CMB Anisotropy 29 14 How Do We Measure the CMB? 36 15 The Geometry of the Universe 40 16 Quantum Mechanics and the Seeds of Cosmic Structure Formation. 43 17 Pulling it all Together with the Standard Model of Cosmology 45 18 Frontiers 48 19 Endnote 49 A Appendix A: The Electromagnetic Spectrum 51 B Appendix B: Expanding Space 52 C Appendix C: Significant Events in the Cosmic Timeline 53 D Appendix D: Size and Age of the Observable Universe 54 1 1 Preface These pages are a brief introduction to modern cosmology. They were written for family and friends who at various times have asked what I work on. The goal is to convey a geometrical picture of how to think about the universe on the grandest scales. -
Galaxies Through Cosmic Time Illuminated by Gamma-Ray Bursts and Quasars
Galaxies through Cosmic Time Illuminated by Gamma-Ray Bursts and Quasars Kasper Elm Heintz arXiv:1910.09849v1 [astro-ph.GA] 22 Oct 2019 Faculty of Physical Sciences University of Iceland 2019 Galaxies through Cosmic Time Illuminated by Gamma-Ray Bursts and Quasars Kasper Elm Heintz Dissertation submitted in partial fulfillment of a Philosophiae Doctor degree in Physics PhD Committee Prof. Páll Jakobsson (supervisor) Assoc. Prof. Jesús Zavala Prof. Emeritus Einar H. Guðmundsson Opponents Prof. J. Xavier Prochaska Dr. Valentina D’Odorico Faculty of Physical Sciences School of Engineering and Natural Sciences University of Iceland Reykjavik, July 2019 Galaxies through Cosmic Time Illuminated by Gamma-Ray Bursts and Quasars Dissertation submitted in partial fulfillment of a Philosophiae Doctor degree in Physics Copyright © Kasper Elm Heintz 2019 All rights reserved Faculty of Physical Sciences School of Engineering and Natural Sciences University of Iceland Dunhagi 107, Reykjavik Iceland Telephone: 525-4000 Bibliographic information: Kasper Elm Heintz, 2019, Galaxies through Cosmic Time Illuminated by Gamma-Ray Bursts and Quasars, PhD disserta- tion, Faculty of Physical Sciences, University of Iceland, 71 pp. ISBN 978-9935-9473-3-8 Printing: Háskólaprent Reykjavik, Iceland, July 2019 Contents Abstract v Útdráttur vii Acknowledgments ix 1 Introduction 1 1.1 The nature of GRBs and quasars 1 1.1.1 GRB optical afterglows...................................2 1.1.2 Late-stage emission components associated with GRBs..............3 1.1.3 Quasar classification and selection............................4 1.1.4 GRBs and quasars as cosmic probes..........................5 1.2 Damped Lyman-α absorbers 7 1.2.1 Gas-phase abundances and kinematics........................ 10 1.2.2 The effect of dust..................................... -
The W. M. Keck Observatory Scientific Strategic Plan
The W. M. Keck Observatory Scientific Strategic Plan A.Kinney (Keck Chief Scientist), S.Kulkarni (COO Director, Caltech),C.Max (UCO Director, UCSC), H. Lewis, (Keck Observatory Director), J.Cohen (SSC Co-Chair, Caltech), C. L.Martin (SSC Co-Chair, UCSB), C. Beichman (Exo-Planet TG, NExScI/NASA), D.R.Ciardi (TMT TG, NExScI/NASA), E.Kirby (Subaru TG. Caltech), J.Rhodes (WFIRST/Euclid TG, JPL/NASA), A. Shapley (JWST TG, UCLA), C. Steidel (TMT TG, Caltech), S. Wright (AO TG, UCSD), R. Campbell (Keck Observatory, Observing Support and AO Operations Lead) Ethan Tweedie Photography 1. Overview and Summary of Recommendations The W. M. Keck Observatory (Keck Observatory), with its twin 10-m telescopes, has had a glorious history of transformative discoveries, instrumental advances, and education for young scientists since the start of science operations in 1993. This document presents our strategic plan and vision for the next five (5) years to ensure the continuation of this great tradition during a challenging period of fiscal constraints, the imminent launch of powerful new space telescopes, and the rise of Time Domain Astronomy (TDA). Our overarching goal is to maximize the scientific impact of the twin Keck telescopes, and to continue on this great trajectory of discoveries. In pursuit of this goal, we must continue our development of new capabilities, as well as new modes of operation and observing. We must maintain our existing instruments, telescopes, and infrastructure to ensure the most efficient possible use of precious telescope time, all within the larger context of the Keck user community and the enormous scientific opportunities afforded by upcoming space telescopes and large survey programs. -
ELBERTH MANFRON SCHIEFER.Pdf
UNIVERSIDADE FEDERAL DO PARANA´ ELBERTH MANFRON SCHIEFER INSTABILIDADE DE JEANS PARA SISTEMAS ESFERICOS´ EM UM UNIVERSO EM EXPANSAO˜ A PARTIR DAS EQUAC¸ OES˜ DE BOLTZMANN E DE POISSON CURITIBA 2019 ELBERTH MANFRON SCHIEFER INSTABILIDADE DE JEANS PARA SISTEMAS ESFERICOS´ EM UM UNIVERSO EM EXPANSAO˜ A PARTIR DAS EQUAC¸ OES˜ DE BOLTZMANN E DE POISSON Disserta¸c˜ao apresentada ao curso de P´os-Gradua¸c˜ao em F´ısica, Setor de Ciˆencias Exatas, Universidade Federal do Paran´a, como requisito parcial `aob- ten¸c˜ao do t´ıtulo de Mestre em F´ısica. Orientador: Prof. Dr. Gilberto Medeiros Kremer CURITIBA 2019 ! "#$ %$" & #$ ' ( )$ #*$ , , -$ .) )$$ /,0 1 2$,$ $3 4 5 %$" & #$ "#$6 7 ,$ !89:6 ;$ < -$ $ $ = $ %. $$ ><?$, @ !89:6 B$ $ ?$ &$ C$$ 6 96 $ $ )$6 !6 %/, 6 6 %)" D@E6 F6 ' ( 6 '6 -$ $ $ =6 ''6 C$$ ?$ &$6 '''6 @,6 ;; G 869!F =$ % $ - <:59H:F Aos que se mantiveram ao meu lado. AGRADECIMENTOS • Ao Professor Doutor Gilberto Medeiros Kremer pela orienta¸c˜ao, apoio e, acima de tudo, compreens˜ao. • A` Andressa Flores Santos pelo apoio infinito. • Aos meus pais, familiares e amigos que sempre estiveram l´a quando precisei. • Ao Programa de P´os-gradua¸c˜ao em F´ısica e `a CAPES pelo suporte financeiro. ”Eu n˜ao sou livre, e sim `as vezes constrangido por press˜oes estranhas a mim, outras vezes por convic¸c˜oes ´ıntimas.”A. Einstein RESUMO A instabilidade de Jeans ´e investigada para um sistema esf´erico por interm´edio das equa¸c˜oes de Boltzmann e de Poisson a partir de um m´etodo rec´em desenvolvido que utiliza os inva- riantes de colis˜ao da equa¸c˜ao de Boltzmann. -
The W. M. Keck Observatory Scientific Strategic Plan
The W. M. Keck Observatory Scientific Strategic Plan A.Kinney (Keck Chief Scientist), S.Kulkarni (COO Director, Caltech),C.Max (UCO Director, UCSC), H. Lewis, (Keck Observatory Director), J.Cohen (SSC Co-Chair, Caltech), C. L.Martin (SSC Co-Chair, UCSB), C. Beichman (Exo-Planet TG, NExScI/NASA), D.R.Ciardi (TMT TG, NExScI/NASA), E.Kirby (Subaru TG. Caltech), J.Rhodes (WFIRST/Euclid TG, JPL/NASA), A. Shapley (JWST TG, UCLA), C. Steidel (TMT TG, Caltech), S. Wright (AO TG, UCSD), R. Campbell (Keck Observatory, Observing Support and AO Operations Lead) Ethan Tweedie Photography 1. Overview and Summary of Recommendations The W. M. Keck Observatory (Keck Observatory), with its twin 10-m telescopes, has had a glorious history of transformative discoveries, instrumental advances, and education for young scientists since the start of science operations in 1993. This document presents our strategic plan and vision for the next five (5) years to ensure the continuation of this great tradition during a challenging period of fiscal constraints, the imminent launch of powerful new space telescopes, and the rise of Time Domain Astronomy (TDA). Our overarching goal is to maximize the scientific impact of the twin Keck telescopes, and to continue on this great trajectory of discoveries. In pursuit of this goal, we must continue our development of new capabilities, as well as new modes of operation and observing. We must maintain our existing instruments, telescopes, and infrastructure to ensure the most efficient possible use of precious telescope time, all within the larger context of the Keck user community and the enormous scientific opportunities afforded by upcoming space telescopes and large survey programs. -
Effects of Rotation Arund the Axis on the Stars, Galaxy and Rotation of Universe* Weitter Duckss1
Effects of Rotation Arund the Axis on the Stars, Galaxy and Rotation of Universe* Weitter Duckss1 1Independent Researcher, Zadar, Croatia *Project: https://www.svemir-ipaksevrti.com/Universe-and-rotation.html; (https://www.svemir-ipaksevrti.com/) Abstract: The article analyzes the blueshift of the objects, through realized measurements of galaxies, mergers and collisions of galaxies and clusters of galaxies and measurements of different galactic speeds, where the closer galaxies move faster than the significantly more distant ones. The clusters of galaxies are analyzed through their non-zero value rotations and gravitational connection of objects inside a cluster, supercluster or a group of galaxies. The constant growth of objects and systems is visible through the constant influx of space material to Earth and other objects inside our system, through percussive craters, scattered around the system, collisions and mergers of objects, galaxies and clusters of galaxies. Atom and its formation, joining into pairs, growth and disintegration are analyzed through atoms of the same values of structure, different aggregate states and contiguous atoms of different aggregate states. The disintegration of complex atoms is followed with the temperature increase above the boiling point of atoms and compounds. The effects of rotation around an axis are analyzed from the small objects through stars, galaxies, superclusters and to the rotation of Universe. The objects' speeds of rotation and their effects are analyzed through the formation and appearance of a system (the formation of orbits, the asteroid belt, gas disk, the appearance of galaxies), its influence on temperature, surface gravity, the force of a magnetic field, the size of a radius. -
Interpreting the Spitzer/IRAC Colours of 7 ≤ Z ≤ 9 Galaxies: Distinguishing Between Line Emission and Starlight Using ALMA
MNRAS 497, 3440–3450 (2020) doi:10.1093/mnras/staa2085 Advance Access publication 2020 July 16 Interpreting the Spitzer/IRAC colours of 7 ≤ z ≤ 9 galaxies: distinguishing between line emission and starlight using ALMA G. W. Roberts-Borsani ,1,2‹ R. S. Ellis2 and N. Laporte3,4,2 1Department of Physics and Astronomy, University of California, Los Angeles, 430 Portola Plaza, Los Angeles, CA 90095, USA 2Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK 3Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK 4 Cavendish Laboratory, University of Cambridge, 19 JJ Thomson Avenue, Cambridge CB3 0HE, UK Downloaded from https://academic.oup.com/mnras/article/497/3/3440/5872501 by UCL, London user on 09 December 2020 Accepted 2020 July 13. Received 2020 June 30; in original form 2020 January 7 ABSTRACT Prior to the launch of JWST, Spitzer/IRAC photometry offers the only means of studying the rest-frame optical properties of z >7 galaxies. Many such high-redshift galaxies display a red [3.6]−[4.5] micron colour, often referred to as the ‘IRAC excess’, which has conventionally been interpreted as arising from intense [O III]+H β emission within the [4.5] micron bandpass. An appealing aspect of this interpretation is similarly intense line emission seen in star-forming galaxies at lower redshift as well as the redshift-dependent behaviour of the IRAC colours beyond z ∼ 7 modelled as the various nebular lines move through the two bandpasses. In this paper, we demonstrate that, given the photometric uncertainties, established stellar populations with Balmer (4000 Å rest frame) breaks, such as those inferred at z>9 where line emission does not contaminate the IRAC bands, can equally well explain the redshift-dependent behaviour of the IRAC colours in 7 z 9 galaxies. -
How Are the Spiral and Other Types of Galaxies Formed?
GSJ: Volume 5, Issue 10, October 2017 16 GSJ: Volume 5, Issue 10, October 2017, Online: ISSN 2320-9186 www.globalscientificjournal.com HOW ARE THE SPIRAL AND OTHER TYPES OF GALAXIES FORMED? Author: Weitter Duckss (Slavko Sedic) Zadar Croatia The goal of this article is to prove the formation of galaxies via rotation of objects around their axis, with the strict abiding of the law of universal gravitation. Rotation of objects (smaller objects, stars, galaxies,...) is analysed through the effects of rotation 1 in the formation of objects and in processes that follow, due to: the rotation around the axis; the effects on the other orbiting objects or on binary objects; the effect of rotation on the displacement of an incoming object into the orbit; the influence of the speed of rotation on the quantity and mass of particles and objects orbiting around a main object 2; its influence on the radius, temperature, and accordingly on the color and surface gravity of a star 3. First of all, let's get rid of the Big Bang. If the official science claims, „The universe is spreading“, then there should be a small universe (with a small diameter) 300-400 thousand years after the so-called Big Bang, and a big universe, in which „...the most distant objects in the universe are the galaxies GN-z11 13,39 bn. ly (billion light years), EGSY8p7 13,23 bn. ly, GRB 090423 13,18 bn. ly, etc.“ „The light that comes from the "edges" of the universe started on your way to us at the time of last scattering of photons at 3000 K. -
Light Speed Expansion and Rotation of a Primordial Black Hole Universe Having Internal Acceleration
International Astronomy and Astrophysics Research Journal 2(2): 9-27, 2020; Article no.IAARJ.57955 Light Speed Expansion and Rotation of a Primordial Black Hole Universe having Internal Acceleration U. V. S. Seshavatharam1* and S. Lakshminarayana2 1Honorary Faculty, I-SERVE, Survey no-42, Hitech City, Hyderabad-84, Telangana, India. 2Department of Nuclear Physics, Andhra University, Visakhapatnam-03, Andhra Pradesh, India. Authors’ contributions This work was carried out in collaboration between both authors. Author UVSS designed the study, performed the statistical analysis, wrote the protocol and wrote the first draft of the manuscript. Author SL managed the analyses of the study. Both authors read and approved the final manuscript. Article Information Editor(s): (1) Dr. Swarniv Chandra, Techno India University, India. (2) Dr. Hadia Hassan Selim, National Research Institute of Astronomy and Geophysics, Cairo, Egypt. Reviewers: (1) Hidirova Mohiniso Bahromovna, Tashkent University of Information Technologies named after Muhammad Al-Khwarizmi, Uzbekistan. (2) Valery Timkov, Institute of Telecommunications and Global Information Space, The National Academy of Sciences of Ukraine, Ukraine. (3) Alesandro Ferreira dos Santos, Instituto de Física, Universidade Federal de Mato Grosso, Brasil. (4) Maliki Olaniyi Sadik, Michael Okpara Federal University Umudike, Nigeria. (5) Tritos Ngampitipan, Chandrakasem Rajabhat University, Thailand. Complete Peer review History: http://www.sdiarticle4.com/review-history/57955 Received 23 April 2020 Accepted 29 June 2020 Review Article Published 07 July 2020 ABSTRACT With reference to primordial black holes, an attempt has been made to develop a practical model of cosmology. Main features of this integrated model are: Eternal role of Planck scale, light speed expansion and rotation of a primordial cosmic black hole, slow thermal cooling, internal acceleration and anisotropy. -
Chronology of the Universe - Wikipedia
7/1/2018 Chronology of the universe - Wikipedia Chronology of the universe The chronology of the universe describes the history and future of the universe according to Big Bang cosmology. The earliest stages of the universe's existence are estimated as taking place 13.8 billion years ago, with an uncertainty of around 21 million years at the 68% confidence level.[1] Contents Outline A more detailed summary Very early universe Diagram of evolution of the (observable part) of the universe from the Big Planck epoch Bang (left) to the present Grand unification epoch Electroweak epoch Inflationary epoch and the metric expansion of space Nature timeline Baryogenesis Supersymmetry breaking view • discuss • (speculative) 0 — Electroweak symmetry breaking Vertebrates ←Earliest mammals – Cambrian explosion Early universe ← ←Earliest plants The quark epoch -1 — Multicellular ←Earliest sexual Hadron epoch – L life reproduction Neutrino decoupling and cosmic neutrino background -2 — i f Possible formation of primordial – ←Atmospheric oxygen black holes e photosynthesis Lepton epoch -3 — Photon epoch – ←Earliest oxygen Nucleosynthesis of light Unicellular life elements -4 —accelerated expansion←Earliest life Matter domination – ←Solar System Recombination, photon decoupling, and the cosmic -5 — microwave background (CMB) – The Dark Ages and large-scale structure emergence -6 — Dark Ages – Habitable epoch -7 — ←Alpha Centauri https://en.wikipedia.org/wiki/Chronology_of_the_universe 1/26 7/1/2018 Chronology of the universe - Wikipedia -7 — p a Ce tau -
Hubble Breaks Cosmic Distance Record 3 March 2016
Hubble breaks cosmic distance record 3 March 2016 Using the NASA/ESA Hubble Space Telescope an international team of astronomers has measured the distance to this new galaxy, named GN-z11. Although extremely faint, the galaxy is unusually bright considering its distance from Earth. The distance measurement of GN-z11 provides additional strong evidence that other unusually bright galaxies found in earlier Hubble images are really at extraordinary distances, showing that we are closing in on the first galaxies that formed in the Universe. Previously, astronomers had estimated GN-z11's distance by analysing its colour in images taken with both Hubble and the NASA Spitzer Space Telescope. Now, for the first time for a galaxy at This image shows the position of the most distant galaxy such an extreme distance, the team has used discovered so far within a deep sky Hubble Space Hubble's Wide Field Camera 3(WFC3) to precisely Telescope survey called GOODS North (Great measure the distance to GN-z11 spectroscopically Observatories Origins Deep Survey North). The survey field contains tens of thousands of galaxies stretching far by splitting the light into its component colours. back into time.The remote galaxy GN-z11, shown in the inset, existed only 400 million years after the Big Bang, "Our spectroscopic observations reveal the galaxy when the Universe was only 3 percent of its current age. to be even further away than we had originally It belongs to the first generation of galaxies in the thought, right at the distance limit of what Hubble Universe and its discovery provides new insights into the can observe," explains Gabriel Brammer of the very early Universe.