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Cosmology Handouts
Cosmology Handouts

... Rainbows reveal that white light is a combination of all the colours. In 1666, Isaac Newton showed that white light could be separated into its component colours using glass prisms. Soon scientists were using this new tool to analyze the light coming from several different light sources. Some scient ...
Three of his best known contributions
Three of his best known contributions

Spectroscopy PPT
Spectroscopy PPT

Spectroscopy - Jefferson Lab
Spectroscopy - Jefferson Lab

Exploring the Helium Reionization Era
Exploring the Helium Reionization Era

Lecture - Ann Arbor Earth Science
Lecture - Ann Arbor Earth Science

Exercise 8
Exercise 8

Project Title: Quantitative Galaxy Evolution Supervisor(s): Project
Project Title: Quantitative Galaxy Evolution Supervisor(s): Project

Document
Document

... • Doppler shifting - wavelength emitted by something moving away from us is shifted to a lower frequency • Sound of a fire truck siren - pitch of the siren is higher as the fire truck moves towards you, and lower as it moves away from you • Visible wavelengths emitted by objects moving away from us ...
ASTRONOMY 5
ASTRONOMY 5

CosmologyL2
CosmologyL2

Document
Document

... • Doppler shifting - wavelength emitted by something moving away from us is shifted to a lower frequency • Sound of a fire truck siren - pitch of the siren is higher as the fire truck moves towards you, and lower as it moves away from you • Visible wavelengths emitted by objects moving away from us ...
Abell 1656: the Coma Cluster of galaxies - Euro-VO
Abell 1656: the Coma Cluster of galaxies - Euro-VO

Seminar 2
Seminar 2

... The main point of this paper is that galaxies have different morphologies at different redshifts. This indicates that they have gone through some sort of evolution in the past. The redshift range discussed in detail in this paper is 0 < z < 1. At higher redshifts it becomes very difficult to determi ...
IS AN ALTERNATE COSMOLOGY BECOMING NECESSARY?
IS AN ALTERNATE COSMOLOGY BECOMING NECESSARY?

1_Introduction - The Ohio State University Department of
1_Introduction - The Ohio State University Department of

DETAILED STELLAR POPULATION ANALYSIS OF GALAXY
DETAILED STELLAR POPULATION ANALYSIS OF GALAXY

... ABSTRACT:
The
poster
describe
a
project
of
a
detailed
stellar
population
analysis
for
different
clusters
of
galaxies
with
increasing
 
redshift.
The
selected
clusters
are
part
of
the
 GEMINI/HST
Galaxy
Cluster
Project
(PIs
I.
Jorgensen
&
R.
Davies.
For the Gemini/HST Galaxy Cluster Project, a sample ...
Transparencies - Rencontres de Moriond
Transparencies - Rencontres de Moriond

5.2.1 Doppler Hubble Toil and Trouble
5.2.1 Doppler Hubble Toil and Trouble

...  The inflation hypothesis explains a couple of puzzling things about the Universe, including how patches of space on opposite sides of the Universe can be the same temperature.  Gas clouds separated by tens of billions of lightyears are not just “about the same temperature”. The difference between ...
Document
Document

Estimating the redshift of PKS 0447−439 through its GeV–TeV
Estimating the redshift of PKS 0447−439 through its GeV–TeV

PH607lec11
PH607lec11

... In the absence (or distant from) massive objects. Inertial frames: uniform motion or rest sustained in the absence of a force. There is no absolute inertial frame. ...
GR Cosmology: The Robertson
GR Cosmology: The Robertson

... a circumference drawn around at that distance would be smaller than 2 and the area at that distance would be less than 4 2 . Ultimately when you reached our ‘antipode’ both shrink to zero, and you have discovered there is only a finite volume to the Universe (at fixed cosmological time – see lat ...
The Universe - Cloudfront.net
The Universe - Cloudfront.net

... Concept Check What relationship did Hubble discover between red shifts and the distances of galaxies from Earth?  Galaxies that have the greatest red shifts are the most distant. ...
00:00 [Narrator] 1. The Milky Way galaxy is our cosmic home. But it
00:00 [Narrator] 1. The Milky Way galaxy is our cosmic home. But it

... a glowing band across the night sky. And for a long time it was thought that that the entire Universe consisted of our galaxy alone. This only changed in 1924. In that year Edwin Hubble identified variable stars in several spiral nebulae. He used these stars to calculate the distances to these nebul ...
< 1 ... 34 35 36 37 38 39 40 41 42 ... 52 >

Redshift



In physics, redshift happens when light or other electromagnetic radiation from an object is increased in wavelength, or shifted to the red end of the spectrum. In general, whether or not the radiation is within the visible spectrum, ""redder"" means an increase in wavelength – equivalent to a lower frequency and a lower photon energy, in accordance with, respectively, the wave and quantum theories of light.Some redshifts are an example of the Doppler effect, familiar in the change of apparent pitches of sirens and frequency of the sound waves emitted by speeding vehicles. A redshift occurs whenever a light source moves away from an observer. Another kind of redshift is cosmological redshift, which is due to the expansion of the universe, and sufficiently distant light sources (generally more than a few million light years away) show redshift corresponding to the rate of increase in their distance from Earth. Finally, gravitational redshift is a relativistic effect observed in electromagnetic radiation moving out of gravitational fields. Conversely, a decrease in wavelength is called blueshift and is generally seen when a light-emitting object moves toward an observer or when electromagnetic radiation moves into a gravitational field. However, redshift is a more common term and sometimes blueshift is referred to as negative redshift.Knowledge of redshifts and blueshifts has been applied to develop several terrestrial technologies such as Doppler radar and radar guns. Redshifts are also seen in the spectroscopic observations of astronomical objects. Its value is represented by the letter z.A special relativistic redshift formula (and its classical approximation) can be used to calculate the redshift of a nearby object when spacetime is flat. However, in many contexts, such as black holes and Big Bang cosmology, redshifts must be calculated using general relativity. Special relativistic, gravitational, and cosmological redshifts can be understood under the umbrella of frame transformation laws. There exist other physical processes that can lead to a shift in the frequency of electromagnetic radiation, including scattering and optical effects; however, the resulting changes are distinguishable from true redshift and are not generally referred to as such (see section on physical optics and radiative transfer).
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