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Pocket: The Ten Greatest Steps Of The Last Ten Decades
Pocket: The Ten Greatest Steps Of The Last Ten Decades

... observing some of the spiral nebulae in the sky, he was able to pinpoint individual, variable stars of the same type that were known in the Milky Way. Only, their brightness was so low that they needed to be millions of light years away, placing them far outside the extent of our galaxy. Hubble didn ...
Checklist for Geo- vs. Heliocentric Model of Universe
Checklist for Geo- vs. Heliocentric Model of Universe

... before they could grow; nevertheless, galaxies did evolve, but no one could explain how Young galaxies existed in the early universe and should therefore be observable only at great distances, which effectively provides a window onto the early universe This echo of the Big Bang should still be detec ...
Andrew Sonnenschein: The level of poetry…
Andrew Sonnenschein: The level of poetry…

... galaxies, and in the middle of these concentrations of mass there are enormous spaces in which there is nothing, completely empty, and the average distance between each atom is also very big. The Universe today is much rougher and more knotty, at least on a small scale, there are stars, planets and ...
ASTR-100 - Jiri Brezina Teaching
ASTR-100 - Jiri Brezina Teaching

... (such as Venus, 177.3°; Uranus, 97.86°; and Pluto 112.52°; C. D. MURRAY & S. F. DERMOTT (CUP, 1999), Solar System Dynamics, Tab. A.4, p. 531). The revolution (orbiting) is ccw when seen from north on all planets and most of their satellites; the axial rotation is ccw when seen from north only on 6 f ...
Review Sheet and Study Hints - Tufts Institute of Cosmology
Review Sheet and Study Hints - Tufts Institute of Cosmology

...  How does this age differ for an open critical and closed universe  B able to calculate the age of the critical Universe  The need for an accelerating universe  Ho, qo and   Definitions of all of them  Be able to summarize efforts and challenges in determining Ho  Be able to summarize (at le ...
Ch 28-31 Lessons
Ch 28-31 Lessons

... 5. Of the orbits that you drew, which loop size and what color created the most eccentric (oval) ellipse? (Hint – the one with the biggest # in Column 5.) _______________________________________________________________ 6. Look at Appendix J on p. 921. There is a row labeled Orbital eccentricity. Loo ...
Atoms, Einstein, Universe
Atoms, Einstein, Universe

... changed our understanding of energy, mass, light, space, and time. Einstein’s most famous equation E=mc2 provides a deeper understanding of mass and energy that can lead us to develop dramatically more abundant and less polluting sources of energy. Future energy production can be a million times mor ...
Episode 705: Cosmology - Teaching Advanced Physics
Episode 705: Cosmology - Teaching Advanced Physics

... because even nearby stars are very distant compared with the Earth’s orbital diameter. Small angles can be expressed in minutes and seconds; one minute of arc is 1 / 60 of a degree; one second of arc is 1 / 60 of a minute. If the radius of the Earth’s orbit is R then the distance to a star with para ...
ppt
ppt

... • How are heavy elements distributed through galaxies? • What are the progenitors of Type Ia SNe? • What is the effect of a low-metallicity environment on star formation and gas tracers? ...
Word version of Episode 705
Word version of Episode 705

... because even nearby stars are very distant compared with the Earth’s orbital diameter. Small angles can be expressed in minutes and seconds; one minute of arc is 1 / 60 of a degree; one second of arc is 1 / 60 of a minute. If the radius of the Earth’s orbit is R then the distance to a star with para ...
Oct 2012 - Bays Mountain Park
Oct 2012 - Bays Mountain Park

... fifty years ago. This was comprise only one of many a time when scientists categories of radio science were first learning that Venus experiments. Others include might not harbor jungles under its tests of General Relativity, thick atmosphere after studying the solar corona, all. A Russian mapping g ...
Olbers` Paradox - NMSU Astronomy
Olbers` Paradox - NMSU Astronomy

... the line of sight argument: In an infinite, homogeneous Universe every line of sight will end upon the surface of a Star. So why is the sky dark at night? The advantage offered by this argument is that it doesn’t require the stars to be randomly scattered in space, but also works if the stars are g ...
The Earth in Context - Washington State University
The Earth in Context - Washington State University

... frequency that happens when a wave source moves is now known as the Doppler effect. Light energy also moves in the form of waves. We can represent light waves symbolically by a periodic succession of crests and troughs (Fig. 1.4c). Visible light comes in many colors—the colors of the rainbow. The co ...
Sample pages 1 PDF
Sample pages 1 PDF

... of life, then they must have been inherited from a planetary body, from which the Orgueil meteorite originated. However, most bodies in the asteroid belt are believed to be too small and too dry to harbor life. He even speculated that the Orgueil meteorite could have been sent from the primitive Ear ...
Let`s discuss some problems of Physics and Astronomy
Let`s discuss some problems of Physics and Astronomy

... forces were turned off. In order to keep its movement along the orbit the satellite has to have a jet which would reconstruct the force equal to former gravitational with value and direction. And the satellite will fly along its orbit again while the jet is working (and performs its work!). What oth ...
Galaxy interaction and transformation
Galaxy interaction and transformation

... simulations are used to understand the properties of merger remnants. Some of the most important results obtained are 1. Major mergers of galaxies generally lead to elliptical-like remnants, with some irregular structures in the outer regions. Depending on the orbital geometry of the merger, the rem ...
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... CO fundamental spectral line profile emitted by gas in gap produced by giant planet ...
Test #4
Test #4

... a) too many stars, b) glowing interstellar gas, c) interstellar dust, d) planetary nebulae 13. The mass of the galaxy has been found by a) counting the stars it contains, b) determining its gravitational force on nearby galaxies c) estimating the number of interstellar clouds, d) applying Kepler’s 3 ...
Lecture 14
Lecture 14

... Or even still embedded in the gas. ...
Slide 1 - Lawrencehallofscience
Slide 1 - Lawrencehallofscience

... The sky is shown in an aitoff projection, where the equator is the midplane of the Milky Way Galaxy. The spots most covered are the ecliptic poles (the spots 90 degrees away from the plane of Earth’s orbit around the Sun). They are basically seen every orbit. The least covered areas are along the ec ...
Dark Matter: What is it?
Dark Matter: What is it?

... (Weakly Interacting Massive Particles). 3) The universe contains five times as much dark matter as “ordinary” luminous matter. ...
Question 1 The rings of Saturn are seen by Answer 1. reflected and
Question 1 The rings of Saturn are seen by Answer 1. reflected and

... . 
 In a binary star system, one component is found to have about 3 solar masses, the other about 7 solar masses. The 3-solar-mass star is visible from Earth, but the 7solar-mass star is not. Theoretical considerations tell us that the 7-solar-mass star must be a 
 
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Physical structure of the local interstellar medium
Physical structure of the local interstellar medium

... JILA, University of Colorado and NIST, 440 UCB, Boulder, CO 80309, USA Received 19 October 2002; received in revised form 27 January 2003; accepted 13 February 2003 ...
Response to Dr. Laurence Krauss of the
Response to Dr. Laurence Krauss of the

... another subatomic particle. His discovery was another crossroads for science, perhaps equal to the 1887 Michelson-Morley experiment. As in 1887, everything depended on the interpretation given to the experiment. The wrong interpretation, which is inevitably based on the wrong presuppositions, would ...
The Sun Notes
The Sun Notes

... b) Every 11-year cycle, the north magnetic pole and south magnetic pole on the Sun reverse; what had been a north magnetic pole is then a south magnetic pole and vice versa. c) Therefore it is 22 years before the Sun returns to its original state making the real period of the solar-activity cycle 22 ...
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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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