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PART 3 Galaxies
PART 3 Galaxies

... • We can estimate the mass of the entire galaxy be measuring the orbital velocity of small satellite galaxies in orbit around the Milky Way (2×1012 solar masses) ...
Our Expanding Universe
Our Expanding Universe

... This radiation “interfered” with their radio experiments. Other scientists determined that the static interference represented the remnants of the energy released by the initial expansion of space that followed the Big Bang. The quest for more evidence of the Big Bang theory continued. Physicists Jo ...
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... A black hole can be both very small, and have an accretion disk that can emit enough radiation Likely that at the centers of these galactic nuclei, there are supermassive black holes Intense magnetic fields in the accretion disk pump superheated gas out into jets that leave the nucleus There are sti ...
Copy rights – www.SJJeyanth.yolasite.com 01.Our Solar system
Copy rights – www.SJJeyanth.yolasite.com 01.Our Solar system

... as clearly distinguished as planetary moons, sometimes being almost as large as their partners. The asteroid belt also contains main belt comets which may have been the source of Earth’s water. Trojan asteroids are located in either of Jupiter’s L4 or L5 Points (gravitationally stable regions leadin ...
LIFEPAC® 7th Grade Science Unit 3 Worktext - HomeSchool
LIFEPAC® 7th Grade Science Unit 3 Worktext - HomeSchool

... the Milky Way. Today we know of many other galaxies similar to the Milky Way. To study the Milky Way as a whole is difficult for scientists on the earth because we are located within it. We cannot look at the Milky Way galaxy from the outside to observe its size and shape. It is so large that light ...
Name - crespiphysics
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... The new moons of Jupiter and Saturn have been discovered in the last few years because we have better telescopes in space like the Hubble telescope and we have sent satellites to both Jupiter and Saturn. The Hubble telescope is outside the Earth’s atmosphere and not subjected to atmospheric fluctuat ...
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... Sec 13.4 Active Galaxies I. Active? A. ~ ___ % of galaxies – very ______ B. Wide range of EM radiation II. Types of Active Galaxies A. ___________ galaxies – “normal” galaxies undergoing aggressive star formation due to interactions Ex/ M82 – The ______ Galaxy B. ____________ galaxies – resemble spi ...
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... c. is composed of neutral hydrogen and a fairly dense concentration of dust. d. produces large amounts of 21-cm radiation. e. produces radio waves from CO and other molecules. _______________ is/are believed to be produced by supernova explosions. a. Coronal gas b. HI clouds c. Molecular clouds d. R ...
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... The Earth is surrounded by a blanket of gases, known as the atmosphere. It provides us with the air we breathe and insulates us from drastic changes in temperature. It also protects us from harmful ultraviolet radiation from the Sun. The atmosphere extends for more than 300 miles above the Earth but ...
Earth Sun Relationship
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... The Earth is surrounded by a blanket of gases, known as the atmosphere. It provides us with the air we breathe and insulates us from drastic changes in temperature. It also protects us from harmful ultraviolet radiation from the Sun. The atmosphere extends for more than 300 miles above the Earth but ...
Dark Matter and Dark Energy
Dark Matter and Dark Energy

... Embarrassment with Dark Energy • A naïve estimate of the cosmological constant in Quantum Field Theory: rL~MPl4~10120 times observation • The worst prediction in theoretical physics! • People had argued that there must be some mechanism to set it zero • But now it seems finite??? ...
Unit 8: The Earth is Space
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... A. The Big Bang Theory: the entire universe began with a giant explosion of matter and energy. 1. Explosion occurred about 14 Billion years ago. The Universe has been expanding ever Since (text p.719-720) B. Supporting Evidence (text p.718-720) ...
Chapter 25 Our Solar System - Information Technology Florida Wing
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... glare on its surface. Mercury is slightly larger than our Moon, and it is the second smallest of the nine original planets. Mercury is only 36 million miles from the Sun and orbits it every 88 days. It has a very elliptical orbit and moves approximately 30 miles per second. Mercury rotates very slow ...
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... 1. What is dark matter and dark energy or do we need gravity modified? 2. How do galaxies evolve? (especially radio data applications and simulations) ...
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Astronomy Assignment #1

... The scaled down Local Group of Galaxies would be 60 cm in radius. Solving similar proportions for the Local Super Cluster and Visible Universe yields the following. The Local Super cluster would have a radius of 20 meters and the visible universe would have a radius of about 5.5 km. This last answer ...
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Chapter 1 - Chabot College

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Overview IR Astronomy Explore hidden universe , Cosmic dust, Cool

... line. The infrared glow produced by cosmic dust which has been warmed by all the stars since the beginning of time is shown in red. This 'background glow' of the Universe tells us the total amount of energy released by stars.  But this reveals a very surprising result: the amount of energy radiated ...
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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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