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The Earth
The Earth

ASTRONOMY WEBQUEST…… EXPLORE THE UNIVERSE
ASTRONOMY WEBQUEST…… EXPLORE THE UNIVERSE

... Universe - http://starchild.gsfc.nasa.gov/docs/StarChild/universe_level2/universe.html Using the website find the following box and Click on the topics to find your answers: The Milky Way ...
PDF - Florida State University
PDF - Florida State University

... Astronomy 1002 is a science class in which we will study what the universe is made of There are a wide range of objects out there, ...
Name
Name

... 32. The first evidence of solid matter around a star other than our sun was discovered on the star called ___________________________ This solid material is expected to some day form ______________________. 33. Our sun and planets were believed to have started forming about ____________years ago. 34 ...
Astrophysics Presentation
Astrophysics Presentation

Into the sub-mm
Into the sub-mm

... Andrew Blain (MRAO) followed with a discussion of the results of a SCUBA pilot survey for previously unknown galaxies. The results and implications of Smail, Ivison and Blain’s observations of distant lensing clusters, revealing the first sub-millimetre selected objects (including a redshift 2 galax ...
Gugus Bintang [Compatibility Mode]
Gugus Bintang [Compatibility Mode]

PDF
PDF

... In contrast, the best HST images permit reliable classifications to be made to epochs corresponding to redshifts of 1–2, some 60–70% of the way back to the Big Bang. Early work with HST concentrated on randomly chosen small fields observed with the Wide Field Planetary Camera 2 (WFPC-2) in parallel, ...
Galaxies
Galaxies

... Often: result of galaxy collisions / mergers Often: Very active star formation (“Starburst galaxies”) Some: Small (“Dwarf galaxies”) satellites of larger galaxies ...
Galaxy
Galaxy

...  When one star hides another star it is called an eclipsing star  Astronomers know there are actually 2 stars by looking at the effects of gravity  Our solar system is not the only solar system with planets revolving around a star  In 2000, astronomers discovered a solar system about 10.5 light- ...
Stars and Galaxies
Stars and Galaxies

... galaxy cluster named the Local Group  Spiral galaxies—spiral arms wind out from inner section; some have barred spirals with stars and gas in a central bar  Elliptical galaxies—large, three-dimensional ellipses; most common shape  Irregular galaxies—smaller, less common galaxies with various diff ...
Studying Science
Studying Science

...  Study visible light from objects in the universe  Helps to see so much more ...
High School Science Essential Curriculum - Astronomy
High School Science Essential Curriculum - Astronomy

... Explain the role of natural forces and the conservation of angular momentum as they apply to the objects in our Universe including the formation of planets and satellites and the retention of an atmosphere. b. Describe and compare Earth’s physical properties to the other planets’ physical properties ...
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File

Light and Telescopes
Light and Telescopes

... – Cannot see all parts of the sky ...
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Review_game_and_answers

... Blue-white ...
30galaxies and the universe
30galaxies and the universe

... Black holes in the centers of giant galaxies—some more than one billion solar masses—had enough infalling gas to once blaze as quasars. The final mass of a black hole is not primordial, but instead is determined during the galaxy formation process. This shows that there is a close relationship betwe ...
Topic 3 – Waves and the Universe
Topic 3 – Waves and the Universe

Topic 3 notes - WordPress.com
Topic 3 notes - WordPress.com

... o Millions of stars make up our galaxy - the Milky Way (The Solar System is just a small part of the Milky Way galaxy) o The Milky Way is just one of billions of other galaxies (some of the nebulae seen from Earth are these other galaxies) that together make up the Universe o In other words…:  Gala ...
Tools of Modern Astronomy Slide Show
Tools of Modern Astronomy Slide Show

... 1. A light year is a unit of ______ and is the distance light travels in one year. Light travels at a rate of _________ and travels 1.5 x 1015 m/year. At that speed light travels almost 6 trillion miles in one _____! 2. It takes light from the Sun about ___ minutes to reach the Earth. It takes light ...
Astronomy_Stars_n_Galaxies_PowerPoint
Astronomy_Stars_n_Galaxies_PowerPoint

talk
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... – 5 kpc versus 900 pc for nine galaxies • 5 local galaxies have two nuclei separated by 4-32 kpc • These galaxies are at faint luminosity end of our sample ...
Chapter 26.4
Chapter 26.4

... http://www.cita.utoronto.ca/~dubinski/tflops/ ...
Diapositiva 1
Diapositiva 1

Chapter 26
Chapter 26

...  Gravity started pulling elements together to ...
< 1 ... 119 120 121 122 123 124 125 126 127 ... 141 >

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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