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PSC100 Summary Chapters 10 to Chapter 20
PSC100 Summary Chapters 10 to Chapter 20

... When we look out into space from the Earth, even with our best telescopes, the stars appear to be quite alike. There are, of course, different patterns to be seen in various areas of the sky, but aside from our Sun and the planet of our solar system, all of the other points of light seem much the sa ...
Cosmic Rays
Cosmic Rays

... Galactic cosmic rays (GCRs) come from outside the solar system but generally from within our Milky Way galaxy.  GCRs are atomic nuclei from which all of the surrounding electrons have been stripped away during their high-speed passage through the galaxy.  They have probably been accelerated within ...
THE 3-D UNIVERSE CONCEPTS
THE 3-D UNIVERSE CONCEPTS

... just by how bright it appears from Earth. For instance, a close, faint star can appear just as bright in the sky as a brighter star that is farther away. The difference between a star’s actual brightness and its apparent brightness when seen from Earth indicates how far away it is. To judge a star’s ...
AMPTE:  NOTES  ON  THE  INITIAL ... WORK  IN  PROGRESS _ _ _ _ _... _
AMPTE: NOTES ON THE INITIAL ... WORK IN PROGRESS _ _ _ _ _... _

... They'd put up with nature's whims long enough. This time the scientists would do it their way. For two decades they had patiently been observing the vast stream of charged particles spewed by the sun into space. This hot "solar wind" produced brilliant auroras over the Earth's poles, disrupted radio ...
Primary-centric World-View proposes a Fractal Architecture
Primary-centric World-View proposes a Fractal Architecture

... the Great Wall form along and follow web-like threads of dark matter. • It is thought that this dark matter dictates the structure of the Universe on the grandest of scales. • Dark matter gravitationally attracts baryonic matter, and it is this normal matter that astronomers see forming long, thin f ...
The First Stars - Amazon Web Services
The First Stars - Amazon Web Services

... stronger than the attractive gravitational force by about 40 powers of ten, if we consider enough atoms, with protons and electrons whose charges cancel, the forces can balance each other. When we turn on gravity many of the atoms are destroyed by the immense pressure that itself opposes the force o ...
EarthComm_c1s3
EarthComm_c1s3

... matter is continuously created out of empty space. The matter created out of empty space is mostly hydrogen. The rate at which new matter appears is in balance with the expansion of the universe. Therefore, the average density of the universe remains constant. There are arguments against the steady- ...
Presentation - The Stimulating Physics Network
Presentation - The Stimulating Physics Network

... Some people say that there are benefits of living with no gravity such as relief to back pain, poor circulation being improved in addition to with some surgeries becoming simpler to perform. This however, is not true as low gravity would cause its own problems. Bones would become brittle as they wou ...
Long-Time Data Storage: Relevant Time Scales
Long-Time Data Storage: Relevant Time Scales

... The memory of our personal lives goes back a little beyond our actual lifespan: we heard stories told by our parents and grandparents, only occasionally has someone the luck of great-grand parents. Beyond theses generations the past becomes very abstract. We oversee only a small fraction of the roug ...
News Release - האוניברסיטה העברית
News Release - האוניברסיטה העברית

... the most powerful supercomputers in Europe, made it possible in an unprecedented manner to carry out a detailed investigation of how galaxies formed in the early Universe. The picture that emerges is of galaxy-building that results from a continuous flow of cold gas along a few narrow streams rather ...
Soal Short
Soal Short

... 2. On April 2, 2008 a telescope (10 cm diameter, f /10) at the Bosscha Observatory was used to observe the Sun and found an active region 0987 (based on the NOAA number) at 8o South and 40o West from the center of the solar disk. The region was recorded with a CCD SBIG ST-8 Camera (1600  1200 pixel ...
class 1,S11
class 1,S11

... —No, the observable portion of the universe is about 14 billion light-years in radius because the universe is about 14 billion years old. ALSO (not in Ch. 1 of the book), we can “see” only about 4% of the universe, 96% is made of “dark matter” and “dark energy”. ...
Star Dust By the Rev. Tom Garrison
Star Dust By the Rev. Tom Garrison

... There are some 59 elements in the human body that are also found on the earth’s crust. iv And scientists like Margaret Meixner say the “earth on which we stand is made almost entirely of ...
neuroaesthetics, neurological disorders and creativity
neuroaesthetics, neurological disorders and creativity

... The cosmic particle detection is based on standard techniques used for decades in high energy particle physics. Muons are detected by the very faint bluish light they generate in plastic scintillator strips deployed as two detector arrays located on the ceiling and the floor of the installation. The ...
Chapter 29 Notes-
Chapter 29 Notes-

... represents the speed of light, which is about 300,000 km/s. • Einstein’s equation can be used to calculate the amount of energy produced from a given amount of matter. • By using Einstein’s equation, astronomers were able to explain the huge quantities of energy produced by the sun. The Sun’s Interi ...
Earth`s Moon
Earth`s Moon

... Concept 3: Earth in the Solar System PO1: Explain the phases of the Moon in terms of the relative positions of the Earth, Sun, and Moon. Earth’s Moon  Our moon is the closest celestial object to Earth.  A moon is a naturally occurring satellite or an object that orbits another object.  It takes o ...
PHYS2160 Notes 4
PHYS2160 Notes 4

... stars (Hartmann 1904) – that is stars where the velocities of the two stellar componentises varied, but there was a third component that did not move.. Total dust mass is small, but its impact on astronomy is significant – it stops us seeing the Galactic centre in visible light, or seeing the dense ...
Finding planets and life among the stars
Finding planets and life among the stars

... of planetary systems that it revealed, gave impetus to NASA’s Kepler mission— the first space telescope dedicated solely to detecting planets more like ours. Kepler uses a different detection technique, which only works for planets whose orbits happen to be edge-on, as seen from the Earth. As the pl ...
The Life Cycle of Spiral Arm Galaxies
The Life Cycle of Spiral Arm Galaxies

... The  observed  speed  of  the  Smith  Cloud  (0.001c)  may  not  just  be  a  random  number  but   might  have  significance.    It  might  correspond  to  the  speed  that  protons  are  traveling  in  the   outer  shell  of  th ...
Perfect Little Planet
Perfect Little Planet

... can reach temperatures around 700 degrees Fahrenheit, while the side away from the Sun has temperatures of about -330 degrees Fahrenheit. Venus has thick clouds of sulfur that trap the Sun’s heat and make it the hottest planet in the Solar System. It also rotates in the opposite direction as most of ...
strolympics - Chandra X
strolympics - Chandra X

... these amazing athletes compare to other rotating things that we know about? Ferris wheels rotate about relatively slowly making one revolution every 600 seconds or so. A ceiling fan, on the other hand, typically rotates twice around every second. This translates into a rotational speed of 0.5 Hertz, ...
Structure of the respiratory system: lungs, airways and dead space 1
Structure of the respiratory system: lungs, airways and dead space 1

... increased numbers more than make up for their reduced size. Generations 5–11 are small bronchi, the smallest being 1 mm in diameter. The lobar, segmental and small bronchi are supported by irregular plates of cartilage, with bronchial smooth muscle forming helical bands. Bronchioles start at about g ...
powerpoint - High Energy Physics at Wayne State
powerpoint - High Energy Physics at Wayne State

... violent weather patterns. Chromosphere contains jet-like spikes of gas – called spicules. Spicules rise vertically through the chromosphere. Last 10 minutes Consist of gas jets, at 30 km/s Rise to heights of 5000 to 20000 km. T ~ chromosphere. ...
Lecture 7
Lecture 7

... 4) Galaxies, groups, clusters, walls, and superclusters all formed from gravity acting on matter in the Universe, much as stars form from clumps of gas within galaxies. We will see computer simulations of this later. 5) The density of neighbors around a galaxy is called its environment. These range ...
How Big is the Solar System?
How Big is the Solar System?

... I mean that we can only see out about 6,000 light years into the disk of our own galaxy in the visible spectrum, and the galaxy is about 100,000 light years across! The dust and gas makes up a whopping 10-15% of the "normal matter" in the galaxy, with the remainder being stars. The thickness of the ...
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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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