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Preface
Preface

... in the rest frame of the galaxies and has been shown to have a stronger wavelength dependence than the dust extinction ...
AS 4022: Cosmology - ASTRONOMY GROUP – University of St
AS 4022: Cosmology - ASTRONOMY GROUP – University of St

... – moving in a slow dance around the center of galaxies. ...
Unit 7A Cells
Unit 7A Cells

... gets less if two objects get closer together. B gets bigger if two objects get further apart. C gets less if two objects get further apart. D does not depend on distance. ...
Book: Introduction to Matter (in
Book: Introduction to Matter (in

... 4. What tools are used to measure mass and weight? What units are used? 5. The amount of space occupied by an object is defined as… ?? How does one calculate it? What is the formula? (Be able to manipulate the formula to solve for the other 2 variables AND know what the appropriate units of measurem ...
Multiple Choice, continued
Multiple Choice, continued

... • The galaxy in which we live, the Milky Way, is a spiral galaxy in which the sun is one of hundreds of billions of stars. • Two irregular galaxies, the Large Magellanic Cloud and Small Magellanic Cloud, are our closest neighbors. • These three galaxies are called the Local Group. ...
Stellar Dynamics
Stellar Dynamics

... medium) flows into the centre of the cluster, falling into the gravitational potential well. As a result this gas gets heated up and emits copious amount of X-rays through which it can be observed. Near the centre of rich clusters the gas becomes dense and its cooling time is estimated to be shorter ...
Coding Einstein`s Legacy - the Neukom Institute
Coding Einstein`s Legacy - the Neukom Institute

... that the planets left alone in space move in circles around the Sun2 ! Could it be that the reason planets have this path was the geometry on the scales of the solar system being different from Euclid’s? Einstein speculated that this was indeed the case. But how does the geometry changes? Einstein e ...
Galaxies - science9atsouthcarletonhs
Galaxies - science9atsouthcarletonhs

... Galaxy Clusters • Most galaxies are not alone in the vast expanse of space, but are connected to one or more other galaxies by gravity • These collections of galaxies are known as galaxy clusters and they too appear to be organized into larger “superclusters” ...
Chapter 2 Text - UW Atmospheric Sciences
Chapter 2 Text - UW Atmospheric Sciences

... When averaged over a year, more solar energy is absorbed near the equator than near the poles. The atmosphere and the ocean transport energy poleward to reduce the effect of this heating gradient on surface temperature. Much of the character of Earth’s evolution and climate has been determined by it ...
AST 207 Final Exam 14 December 2009
AST 207 Final Exam 14 December 2009

... c. (1 pts.) What will the sun become when it completely exhausts its fuel? (1 pt.) How big will it be? (1 pt.) What will prevent gravity from making it collapse? d. (2 pts.) The sun is losing more mass than can be accounted with the loss of protons, neutrons, and electrons. Explain how that is possi ...
DSSU, the Non-Expanding Universe: Structure, Redshift, Distance
DSSU, the Non-Expanding Universe: Structure, Redshift, Distance

... cannot fail. By adjusting the value of Ω0 the distance can always be made to agree with the supernovae distance measurements. That, however, is also the problem; different regions of the BB universe require different Ω density values. A major ongoing effort in astrophysics is to come to some agreeme ...
THE SUN - OoCities
THE SUN - OoCities

... R{Sun symbol}, so it subtends an angle of only 1/25 in the sky, roughly the same as that of the Moon. By comparison, the next closest star to the Earth is 250,000 times farther away, and its relative apparent brightness is reduced by the square of that ratio, or 62 billion times. The temperature of ...
LNP fulldome show catalog
LNP fulldome show catalog

... seemed to us we could give everybody what they need by designing the shows to offer both MINI and FULL versions, averaging 7 and 14 minutes respectively, and they are all included in the package. It's win-win all the way around! Two Voices, More Choices The days of debating “which voice is better, m ...
The Galaxy Luminosity Function
The Galaxy Luminosity Function

... effectively zero in dense clusters. This is because the velocity dispersions of clusters are extremely high (≥ 1000 km/s), which is higher than the escape velocity of galaxy flybys. ...
From Spyglasses to Space Telescopes
From Spyglasses to Space Telescopes

... many spacecraft designed to exploit the advantages of being outside Earth’s atmosphere have been launched. The Chandra X-ray Observatory, the Spitzer Space Telescope, and the Hubble Space Telescope (HST) were particularly powerful. Turbulence in the Earth’s atmosphere blurs astronomical images. Beca ...
GCR Neon Isotopic Abundances: Comparison with Wolf
GCR Neon Isotopic Abundances: Comparison with Wolf

... formed ~2 kpc closer to the galactic center than our present galactocentric radius of 8.5 kpc, based on the higher metallicity of the Sun relative to that of nearby stars [34]. Wolf-Rayet Stars-The overabundance of 22Ne in OCRs may be a result of the acceleration of WR star material as first suggest ...
Cosmological principle and the Cosmic microwave
Cosmological principle and the Cosmic microwave

... early universe Hot Big Bang model Post-recombination :Freely propagating through (weakly perturbed) homogeneous & isotropic cosmos. Pre-recombination : Tightly coupled to, and in thermal equilibrium with, ionized matter. ...
What makes a planet habitable?
What makes a planet habitable?

... heating due to O2 and O3 photodissociation by solar UV radiation (1250 ≤ λ ≤ 3500 Å), ...
Early Star-Forming Galaxies
Early Star-Forming Galaxies

... However, at the target distance (corresponding to the epoch 9 billion to 11 billion years ago), Herschel  could only spot bright galaxies producing stars at a rate of 50 or more Sun-like stars a year. To analyze galaxies creating stars below this threshold, the astronomers added more than 18,000 sta ...
Cosmic rays: the centenary of their discovery
Cosmic rays: the centenary of their discovery

... The Positron and the Muon Skobelzyn seems to have been the first to recognize a high-energy cosmic ray track in a magnet-cloud chamber [5] (see Figure 2) but pride of place for recognizing the positron goes to Anderson [6]. Fig 3 gives the evidence – surprisingly, a particle travelling upwards but r ...
Test#4
Test#4

... PH109 Exploring the Universe, Test #4, Spring 2012 Please indicate the best answer to the following question on the answer sheet provided. 1. What kind of galaxy do we live in? a) Spiral, b) elliptical, c) spherical, d) irregular 2. The size of our galaxy is about a) 3 light years, b) 100 thousand l ...
beyond the light barrier
beyond the light barrier

... There are three categories which classify all observed particle motions: slower-than-light (subluminal), light speed (luminal), and faster-than-light (superluminal). Subluminal particles, called tardyons, consist of everything made from the most elementary states of matter and can be quantified thro ...
J: Chapter 3: The Solar System
J: Chapter 3: The Solar System

... part of a nebula of gas, ice, and dust, like the one shown in Figure 2, about 4.6 billion years ago. Follow the steps shown in Figures 3A through 3D, which illustrate how this might have happened. A cloud of material in this nebula was rotating slowly in space. A nearby star might have exploded, and ...
Unit 7A Cells
Unit 7A Cells

... gets less if two objects get closer together. B gets bigger if two objects get further apart. C gets less if two objects get further apart. D does not depend on distance. ...
Large-scale, Optical/Near-IR Galaxy Surveys with a 4
Large-scale, Optical/Near-IR Galaxy Surveys with a 4

... surveys, or ~6000 hours per year over a mission lifetime of 5 years. The availability of telescopes with a large, diffraction-limited field of view provides a stimulus to innovative instrument concepts (Robberto 2009). In particular, the commercial development of digital micromirror devices (DMD’s) ...
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Outer space



Outer space, or just space, is the void that exists between celestial bodies, including the Earth. It is not completely empty, but consists of a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium as well as electromagnetic radiation, magnetic fields, neutrinos, dust and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvin (K). Plasma with a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvin in the space between galaxies accounts for most of the baryonic (ordinary) matter in outer space; local concentrations have condensed into stars and galaxies. In most galaxies, observations provide evidence that 90% of the mass is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Data indicates that the majority of the mass-energy in the observable Universe is a poorly understood vacuum energy of space which astronomers label dark energy. Intergalactic space takes up most of the volume of the Universe, but even galaxies and star systems consist almost entirely of empty space.There is no firm boundary where space begins. However the Kármán line, at an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which was passed by the United Nations in 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights, followed by manned rocket launches. Earth orbit was first achieved by Yuri Gagarin of the Soviet Union in 1961 and unmanned spacecraft have since reached all of the known planets in the Solar System. Due to the high cost of getting into space, manned spaceflight has been limited to low Earth orbit and the Moon.Outer space represents a challenging environment for human exploration because of the dual hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is high.
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