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Recent Developments in Cosmology
Recent Developments in Cosmology

... From our vantage point 13 billion years after the Big Bang, we are now trying to unravel what happened in the earliest tiny fraction of a second, when the Universe was 0.000000000000000000000000000000000001 seconds old! We can test our ideas about the Very Early Universe by observing the distributio ...
TRANSIT
TRANSIT

... and data reduction; there will be something for everyone from the very beginner to the ambitious student. Apart from the astronomical program, there are many non-astronomical activities such as group games, sporting events, singing evenings, hiking tours and an excursion. Since it is an internationa ...
Our galaxy, the Milky Way, has about 3 billion solar masses of HI
Our galaxy, the Milky Way, has about 3 billion solar masses of HI

... The distance of individual neutral hydrogen clouds in the galaxy’s disk can be determined using their radial velocities (that are determined from their Doppler shifts). Thus, astronomers can determine both the distance to these clouds of hydrogen and their velocity. With the hydrogen cloud’s velocit ...
Unit I Geography, Its Nature and Perspectives
Unit I Geography, Its Nature and Perspectives

... The Köppen system divides the world into six main climate regions. Tropical (A), Dry (B), Temperate (C), Continental (D), Cold Polar (E), and Highland (H). Terrain
 This is the setting within which human action occurs – They help shape (not dictate) how people live – The resource base can shape a gr ...
Talk - Otterbein University
Talk - Otterbein University

... far away (1000 ly) • This means that some stars appear dim but are actually very bright • That means that stars have different sizes, ...
unit1-outline notes - Monarch High School AP Human Geography
unit1-outline notes - Monarch High School AP Human Geography

... The Köppen system divides the world into six main climate regions. Tropical (A), Dry (B), Temperate (C), Continental (D), Cold Polar (E), and Highland (H). Terrain
 This is the setting within which human action occurs – They help shape (not dictate) how people live – The resource base can shape a gr ...
Cosmology - 2015 - johndistefano.com.au
Cosmology - 2015 - johndistefano.com.au

... came in the 1930’s when the Swiss astronomer Fritz Zwicky , while working at the Mount Wilson Observatory measured the speed at which galaxies in the Coma cluster, 321 million light years from away, orbit the centre of the cluster. He calculated that unless the cluster contained mush more mass than ...
Cycles: Earth, Sun, Moon by MTDavis
Cycles: Earth, Sun, Moon by MTDavis

... ONE ROTATION of the earth on it’s axis = ONE DAY ONE MOON CYCLE =about 29.5 DAYS, which should be ONE MONTH. 12 X 29.5 = 354 days, 11 days short of the real SOLAR CALENDAR, so Julius Caesar, with the help of Greek science, changed our months to 30 or 31 day months which no longer match the moon cyc ...
Test 4 Review
Test 4 Review

... • Write out and bubble your last name, space, first name and Exam color in the name space of the scantron form. Write out and bubble your Banner ID in the ID space. • Draw simple sketches to help visualize problems • Solve numerical problems in the margin • Come up with your answer first, then look ...
ISP 205: Visions of the Universe
ISP 205: Visions of the Universe

... Earth orbits the Sun (revolves) once every year… • at an average distance of 1 AU ≈ 150 million km. • with Earth’s axis tilted by 23.5º (pointing to Polaris). • and rotates in the same direction it orbits, counterclockwise as viewed from above the North Pole. ...
Weighing a Galaxy—11 Nov Ast 207 F2005 Nov-09 • Schedule
Weighing a Galaxy—11 Nov Ast 207 F2005 Nov-09 • Schedule

... 1. What are the fossils (something that can be examined) from the universe at 3 min? 2. The amount of helium in the sun depends on the properties of deuterium. If deuterium is less tightly bound, would there be more or less helium on the surface of the sun? ...
Rocky Planets Gas Giants
Rocky Planets Gas Giants

... The purpose of a refracting telescope is to collect light from distant objects. All refracting telescopes are the same. It works just like a magnifying glass. It is made up of lenses. As light passes through the lens, it is refracted (this means the light is bent). It has two lenses. The first is th ...
Between the Stars: Gas and Dust in Space
Between the Stars: Gas and Dust in Space

... To understand how stars form, we need to know the raw material from which they are made All the gas and dust material that lies in the region between stars is referred to as interstellar matter The entire collection of interstellar matter is called the interstellar medium The interstellar medium acc ...
Third Grade Science
Third Grade Science

... animals and plants alive today, others were quite different • Compare modern ecosystems with similar ecosystems from Earth’s geologic past (for example, reef, tundra, and forest) • Recognize methods (fossils, tree rings, and ice) scientists use to study past ecosystems ...
Earth and Beyond - Swinton Community School
Earth and Beyond - Swinton Community School

Solar System Teacher Tips
Solar System Teacher Tips

... Meteorite: a meteoroid that hits the surface of a planet. Meteoroid: dust or small chunks of rock in orbit around the Sun. Moon: a naturally occurring satellite in orbit around a planet or planetoid. Orbit: the path of an object in space, as it travels around another object. Oort Cloud: an area well ...
Space (Part 1)
Space (Part 1)

... Gravity and satellites A satellite is any object that orbits another object. The Moon is a natural satellite of the Earth and is kept in orbit by the attraction of the Earth’s gravity and by its motion. An artificial satellite is an object made by, and put into orbit by, humans. Why do you think sa ...
Star Formation 1 - Center for Astrostatistics
Star Formation 1 - Center for Astrostatistics

... where n is the density of atoms, k is Boltzmann's constant, and T is the temperature (Ideal gas law, Boltzmann mid-1800s) So, the cloud of atoms starts gravitational collapse, gas heats up as density increase, and collapse stops when hydrostatic equilibriumis achieved; that is, when the inward pull ...
The Solar System: Cosmic encounter with Pluto
The Solar System: Cosmic encounter with Pluto

... The Voyagers successfully completed their mission making discoveries such as the active volcanoes on Jupiter's moon, Io, and learning details about Saturn's rings. They had only been made to last five years but were still both going strong, so NASA extended their mission. Voyager 2 went on to take a ...
BIG BANG ACOUSTICS – SOUND IN THE EARLY UNIVERSE
BIG BANG ACOUSTICS – SOUND IN THE EARLY UNIVERSE

... For terrestrial sounds, there is always a driving mechanism – the air blown across the flute, or the stick which strikes the drum. What drives the primordial sound? The kneejerk thought that “the initial explosion was simply a big BANG”, while superficially satisfying, fundamentally misunderstands t ...
Chapter 12 Our Place in the Universe
Chapter 12 Our Place in the Universe

... The Universe as a perfect (black-body) radiator at 2.7 K This question is about the temperature of the Universe and the radiation that has filled it since neutral atoms were first produced. Plasma absorbs photons It is thought that the early Universe was too hot for electrons and protons to combine ...
Using Galaxy Clusters to Study Structure Evolution
Using Galaxy Clusters to Study Structure Evolution

... universe is expanding homogeneously and is not static. »The universe was denser in the past »The universe had a beginning….? ...
What is the Shape of the Universe?
What is the Shape of the Universe?

... with the pair of points (starting at the north pole as a single point – a degenerate S0) getting farther and farther apart until they reach a maximum distance (at the equator), thereafter getting increasingly close until they come together at the south pole (again a ...
Study Guide 4 Part A Outline
Study Guide 4 Part A Outline

... ƒ Universe is expanding ƒ The expansion started at some definite time in the past (the Big Bang)Universe expands away from every galaxy. Every galaxy would see its own version of the Hubble Law. Quasars & Active Galactic Nuclei o Quasars and other active galaxies emit large amounts of energy from re ...
Spiralicity and Motion on Cosmic Scale
Spiralicity and Motion on Cosmic Scale

... circular motion and properties of visible, baryonic matter. General relativity has recently been confirmed on the nearby universe [4]. The predicted gravitational redshift of relativity has been found from the astronomical findings on galactic clusters, where groups of thousands galaxies are held to ...
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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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