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The Early Universe and the Big Bang
The Early Universe and the Big Bang

... temperature, even though they seem too far apart for light (and heat) to have traveled from one side to the other in the age of the universe? ...
The evolution of Supernova 1987A probed by Hubble Space
The evolution of Supernova 1987A probed by Hubble Space

... will go through all the possible burning stages (H, He, C, O and Si) leading up to an iron core. Between each stage the core contracts when the nuclear burning has stopped, since the outward radiation pressure decreases. This contraction stops when the temperature in the core is high enough to start ...
Chemical Evolution
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Chapter1 - A Modern View of the Univserse -pptx
Chapter1 - A Modern View of the Univserse -pptx

... Question: When will we be able to see what it looks like now? ...
Chapter 23 The Milky Way Galaxy
Chapter 23 The Milky Way Galaxy

... A. An enormous luminous cloud of gas and dust in the interstellar space. B. A collection of planets with a parent star similar to the solar system. C. A collection of hundreds of billions of stars sometimes called a galaxy. D. A figment of the imagination of early astronomers like, the "seas" of the ...
Chapter 19 Stars Galaxies and the Universe
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... a region that is a little more than 10% of the distance between the Sun and the Earth (approximately 15 million kilometers in diameter) (Zimmerman, 2001). Confirming that a black hole exists at the center of the Milky Way galaxy has proven to be quite challenging. Because black holes are dark object ...
Discovery of a candidate inner Oort cloud planetoid
Discovery of a candidate inner Oort cloud planetoid

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FREE Sample Here
FREE Sample Here

... 2) Briefly explain what we mean by the statement "The farther away we look in distance, the further back we look in time." Answer: It means that when we look at a distant object, we see it as it was some time in the past, rather than as it is now. This is because the light we see has taken time to t ...
ATA2010
ATA2010

... of the star forming events which built up our Galaxy Galaxies like the Milky Way are believed to form by • the infall of gas which then turns gradually to stars (most of which form in the disk of the Galaxy, in open star clusters which quickly dissolve), and also by • the accretion of smaller galaxi ...
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Manual - TUM

... receives to much light during an exposure, it will saturate. Saturation is when a pixel’s counting value exceeds 215 , in which case the image cannot be used, if the saturated pixels are within the object of interest. Be mindful of this when taking your images: do not allow pixels of your object of ...
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Gone in a flash: supernovae in the survey era
Gone in a flash: supernovae in the survey era

... brighter than a Type Ia supernova). The first of SLSN (Gal-Yam 2012), commonly defined as CFHT, or DECam on the Cerro Tololo Interevent, SCP 06F6, was identified in 2009 and had being brighter than –21 in absolute magnitude American Observatory 4 m Blanco telescope), broad, unexplained spectral abso ...
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ULXs: General Properties and Variability - X

Bill Gray 168 Ridge Road Bowdoinham, ME 04008 ph (207) 666
Bill Gray 168 Ridge Road Bowdoinham, ME 04008 ph (207) 666

... hit 'c' (for 'centroid'). Given this hint that "yes, there is an object here", CHARON will find the object's position and add a red circle there. You can then make an MPC report as before. (2) The MPC report for comets will not contain the comet designation. The COMET.DAT file on the CD-ROM doesn't ...
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AS 4022: Cosmology - ASTRONOMY GROUP – University of St

... each containing thousands of galaxies and stretching many hundreds of millions of light years. are arranged in filament or sheet-like structures, between which are gigantic voids of seemingly empty space. ...
Doppler Effect Demo
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... that are close to the Milky Way actually move toward us and are blue-shifted. However, all galaxies beyond a certain distance are red-shifted. Is it possible to see any planets orbiting other stars? As of the time of this writing (August 2002) no planets have been directly observed. Most extra-solar ...
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FREE Sample Here - Find the cheapest test bank for your

... 2) Briefly explain what we mean by the statement "The farther away we look in distance, the further back we look in time." Answer: It means that when we look at a distant object, we see it as it was some time in the past, rather than as it is now. This is because the light we see has taken time to t ...
Measuring the Milky Way
Measuring the Milky Way

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Dynamical models of the nucleus of M31

How to Directly Image a Habitable Planet Around Alpha Centauri
How to Directly Image a Habitable Planet Around Alpha Centauri

... to be capable of directly imaging potentially habitable worlds. WFIRST-AFTA has not, but some simulations show that it may be able to directly image such worlds [1]. The 2030s may prove to be an exciting era of an even larger high contrast space telescope of 4m or higher aperture [4,5], capable of s ...
A Modern View of the Universe
A Modern View of the Universe

... shrunk down to a scale that would allow you to walk through it. The Voyage scale model solar system in Washington, D.C., makes such a walk possible (Figure 1.4). The Voyage model shows the Sun and the planets, and the distances between them, at one ten-billionth of their actual sizes and distances. ...


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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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