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The Expanding Universe
The Expanding Universe

... The universe started with a sudden appearance of energy which consequently became matter and is now everything around us. There were two theories regarding the universe The Steady State Universe: where the universe had always been and would always continue to be in ...
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6-Where to Survey - The Challenger Learning Center

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Lecture 1 - Department of Physics and Astronomy
Lecture 1 - Department of Physics and Astronomy

... over time or from place to place. Thought Experiment: imagine two teams of scientist measuring the speed of a beam of light. One team measures the speed from a ground. The second team measures the speed from a fast moving airplane following the light beam. Do the two ...
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Chapter 26

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Lecture 1 Coordinate Systems - Department of Physics & Astronomy
Lecture 1 Coordinate Systems - Department of Physics & Astronomy

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Where do we come from?

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24.1 The Study of Light

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The Hubble Ultra Deep Field Project Overview

... The velocity you calculated for this star is much less than the speed of light, so we could have found a decent approximation to the answer using z = v/c. But, if you use the approximation equation to calculate the recession velocity based on the spectral shift from the spectrum of a distant galaxy ...
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Handout from Allaire Star Party

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Doppler Effect - Sciwebhop.net

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Lecture 7 Stars and Galaxies and Nebula, (Oh My!) Feb 18 2003

... They orbit in the disk of our galaxy and don't last very long, members escape the group over time. All about the same age and composition so it is likely that they formed around the same time. ...
Astronomy 170: Aug. 24 10am class
Astronomy 170: Aug. 24 10am class

Before people could understand the history of the universe, they had
Before people could understand the history of the universe, they had

Sirius Astronomer - Orange County Astronomers
Sirius Astronomer - Orange County Astronomers

Not a limitation
Not a limitation

... • EVERYTHING was in one small point (singularity) that “blew up” and is still moving outwards today • Not really an explosion, so much as a very rapid expansion…like blowing up a balloon • About 13.7 billion years ago • Microwave radiation detected in the 1960’s supports this theory. It’s left over ...
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Hubble Deep Field



The Hubble Deep Field (HDF) is an image of a small region in the constellation Ursa Major, constructed from a series of observations by the Hubble Space Telescope. It covers an area 2.5 arcminutes across, about one 24-millionth of the whole sky, which is equivalent in angular size to a 65 mm tennis ball at a distance of 100 metres. The image was assembled from 342 separate exposures taken with the Space Telescope's Wide Field and Planetary Camera 2 over ten consecutive days between December 18 and December 28, 1995.The field is so small that only a few foreground stars in the Milky Way lie within it; thus, almost all of the 3,000 objects in the image are galaxies, some of which are among the youngest and most distant known. By revealing such large numbers of very young galaxies, the HDF has become a landmark image in the study of the early universe, with the associated scientific paper having received over 900 citations by the end of 2014.Three years after the HDF observations were taken, a region in the south celestial hemisphere was imaged in a similar way and named the Hubble Deep Field South. The similarities between the two regions strengthened the belief that the universe is uniform over large scales and that the Earth occupies a typical region in the Universe (the cosmological principle). A wider but shallower survey was also made as part of the Great Observatories Origins Deep Survey. In 2004 a deeper image, known as the Hubble Ultra-Deep Field (HUDF), was constructed from a few months of light exposure. The HUDF image was at the time the most sensitive astronomical image ever made at visible wavelengths, and it remained so until the Hubble Extreme Deep Field (XDF) was released in 2012.
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