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IOSR Journal of Applied Physics (IOSR-JAP) e-ISSN: 2278-4861.
IOSR Journal of Applied Physics (IOSR-JAP) e-ISSN: 2278-4861.

... hydrogen atoms per cubic meter. All the dark energy in our solar system amounts to the mass of a small asteroid [which is much smaller than our planet], making it an utterly inconsequential player in the dance of the planets. Its effects stand out only when viewed over vast distances and spans of ti ...
Slide 1
Slide 1

... What is the ultimate fate of our universe? A Big Crunch? A Big Freeze? A Big Rip? or a Big Bounce? Measurements made by WMAP or the Wilkinson Microwave Anisotropy Probe favor a Big Freeze. But until a deeper understanding of dark energy is established, the other three still cannot be totally ignored ...
Spiral galaxies: Spiral galaxies: Inclination Spiral galaxies: Internal
Spiral galaxies: Spiral galaxies: Inclination Spiral galaxies: Internal

... • In denser regions of the ISM, collisions between atoms become frequent enough to form molecules. • The most common molecule is H2, but since H2 is a symmetric molecule, it has no rotational quantum transitions. It is therefore extremely difficult to detect. • As a tracer of H2, astronomers usually ...
Word version of Episode 704
Word version of Episode 704

... The CLEA software enables you to simulate controlling a telescope so that it points at a selected galaxy, and then using a spectrometer to record the light received over a range of wavelengths. From this spectrum you can measure the observed wavelengths of one or more absorption lines in the galaxy’ ...
Universe, Dark Energy and Dark Matter
Universe, Dark Energy and Dark Matter

... the galaxies we can express their gravitational interacttions by Newton’s laws of gravitation as attraction between individual galaxies in our spherical cavity. Such an approach to the galaxies inside an imaginary spherical cavity which interact with each other by the law of gravitation but not with ...
Galaxies - WordPress.com
Galaxies - WordPress.com

... wavelength shortens, and the light shifts towards the blue end of the color spectrum. If an object is moving away fom us, its wavelength gets longer, and the light shifts towards the red end of the ...
Long Ago and Far Away
Long Ago and Far Away

... infrared telescope in astronomy. Figure 2 shows distant galaxies as seen by Spitzer in infrared light and by the Hubble Space Telescope (HST) in visible light. HST makes distant galaxies look almost nearby! But some infrared-bright galaxies are hard to see in the HST image, because dust obscures vis ...
Static, Infinite, Etern and Auto sustentable Universe
Static, Infinite, Etern and Auto sustentable Universe

... exist, but a fight of forces that determines if this one expands or is contracted. That fight could be eternal and/or to have a beginning in the past (as George Lemaitre together with Friedman proposed in 1929) where all the matter and energy would be concentrated in a singular point and it would in ...
project.generative.interactive.music
project.generative.interactive.music

... of 200 miles per second, astronomers believe that the description as a supersuper-sonic jet exhaust is quite apt. Ground-based studies have shown that the nebula's size increases with time, suggesting that the stellar outburst that formed the lobes occurred just 1,200 years ago. M2-9 is 2,100 light- ...
Age Estimates of Globular Clusters in the Milky Way
Age Estimates of Globular Clusters in the Milky Way

... Hubble’s first measurement of the expansion of the Universe in 1929 also resulted in an embarrassing contradiction: Working backward, on the basis of the expansion rate he measured, and assuming that the expansion has been decelerating since the Big Bang—as one would expect given the attractive natu ...
Cosmology
Cosmology

... C. Dust prevents us from seeing beyond a certain distance. D. There are so many galaxies in the universe that they block our view. ...
Earth apart.
Earth apart.

... density could change over time or from one place to another in the universe. Vacuum energy gets its name from its role as the energy of "empty" space. Space is filled with a smooth energy density of virtual particles (particle-antiparticle pairs) that pop in and out of existence. Vacuum energy can b ...
Will Dark Energy Tear the Universe Apart?
Will Dark Energy Tear the Universe Apart?

... density could change over time or from one place to another in the universe. Vacuum energy gets its name from its role as the energy of "empty" space. Space is filled with a smooth energy density of virtual particles (particle-antiparticle pairs) that pop in and out of existence. Vacuum energy can b ...
dark matter. - Gordon State College
dark matter. - Gordon State College

... • Scientists predict that if the Big Bang occurred, there would not have been enough time to form any heavy elements due to the rapidly expanding universe; only hydrogen and helium could have been formed. • Strong evidence for the Big Bang came when scientists measured that about 75% of all the matt ...
Nucleosynthesis in the Early Universe.
Nucleosynthesis in the Early Universe.

... interpretation of the overall curvature of the spacetime continuum.  Later we will use it to consider the question of whether the Universe is “closed or open”. •Overall there are three possibilities which we can see as being similar to the question of “Escape velocity” for an object leaving a plane ...
Space Science Chapter 10.1 textbook
Space Science Chapter 10.1 textbook

... knowledge would grow only when you had better ways of leaving your island and exploring new areas. Earth is like an island in the universe, and humans are constantly looking for ways to explore and learn more about the universe and Earth’s place in it. Step by step, as our technology has improved, w ...
Absolute Magnitudes of Supernovae
Absolute Magnitudes of Supernovae

... Summary Using the Hubble Law, determine the absolute magnitudes of Type Ia supernovae occurring in distant galaxies. Background - During a three-week period in 1997, the Hubble Space Telescope was used to observe a supernova - an exploding star in a distant galaxy. These exploding stars appear sudde ...
file - University of California San Diego
file - University of California San Diego

... is a phenomenon called redshift. Elements such as hydrogen and iron emit light at specific wavelengths or spectral lines when tested in the laboratory. Yet the light from objects such as galaxies and quasars is skewed from these laboratory values and shifted toward longer wavelengths--the red end of ...
TR-16
TR-16

... Dark energy seems to have become effective 5-10 billion years ago. Dark energy can be generalized to quintessence, which is a dynamic time-evolving spatially-changing form of energy that could have negative pressure. Another explanation of dark energy to a cosmic field associated with inflation. The ...
Here - gcisd
Here - gcisd

... universe must be expanding. He also discovered galaxies farther from Earth experience greater redshift. In other words, the farther a galaxy is from Earth, the faster it is moving away from Earth. Not only is the universe expanding, Hubble concluded that it must be expanding more quickly all the tim ...
Document
Document

... • For nearby stars, use opposite points of Earth’s orbit around the ...
Cosmology and Particle Physics
Cosmology and Particle Physics

... The Russian-born American physicist George Gamow (19041968) was among the rst to note that, if there was a Big Bang, the remnants of the primordial reball should still be evident and should be blackbody radiation. Since the radiation from this reball has been traveling to us since shortly after ...
Galaxies - Indiana University Astronomy
Galaxies - Indiana University Astronomy

... the radiation, and  is the amount the radiation has been shifted towards longer wavelengths ( = the observed wavelength minus the rest wavelength). For these spectra, wavelengths are usually measured in Angstroms (Å), rather than nanometers. An Angstrom is 1/10 of a nanometer, 10-10 meters. The ...
Expanding Universe and Big Bang
Expanding Universe and Big Bang

... In the 20th century, as theory and technology advanced, Doppler techniques began to be used widely. Vesto Slipher, from 1912, made a series of astounding measurements which showed galaxies racing around the universe. The Andromeda galaxy was racing towards us at 300 km/s; but almost every other gala ...
a MS Word version.
a MS Word version.

... 11. Use the figure linked to "XI. ....click here for video-text comparison..." to describe all the steps of the Big Bang. Make sure to describe what is meant by GUTs and TOEs and the epochs related to these theories. What major early epoch is not mentioned by the video but is now a very important pa ...
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Hubble's law

Hubble's law is the name for the observation in physical cosmology that: Objects observed in deep space (extragalactic space, ~10 megaparsecs or more) are found to have a Doppler shift interpretable as relative velocity away from the Earth; This Doppler-shift-measured velocity, of various galaxies receding from the Earth, is approximately proportional to their distance from the Earth for galaxies up to a few hundred megaparsecs away. Hubble's law is considered the first observational basis for the expansion of the universe and today serves as one of the pieces of evidence most often cited in support of the Big Bang model.The motion of astronomical objects due solely to this expansion is known as the Hubble flow.Although widely attributed to Edwin Hubble, the law was first derived from the general relativity equations by Georges Lemaître in a 1927 article where he proposed the expansion of the universe and suggested an estimated value of the rate of expansion, now called the Hubble constant. Two years later Edwin Hubble confirmed the existence of that law and determined a more accurate value for the constant that now bears his name. Hubble inferred the recession velocity of the objects from their redshifts, many of which were earlier measured and related to velocity by Vesto Slipher in 1917.The law is often expressed by the equation v = H0D, with H0 the constant of proportionality (Hubble constant) between the ""proper distance"" D to a galaxy (which can change over time, unlike the comoving distance) and its velocity v (i.e. the derivative of proper distance with respect to cosmological time coordinate; see Uses of the proper distance for some discussion of the subtleties of this definition of 'velocity'). The SI unit of H0 is s−1 but it is most frequently quoted in (km/s)/Mpc, thus giving the speed in km/s of a galaxy 1 megaparsec (3.09×1019 km) away. The reciprocal of H0 is the Hubble time.
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