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ISP 205: Visions of the Universe
ISP 205: Visions of the Universe

20_Testbank
20_Testbank

... 7) Massive-star supernovae and white-dwarf supernovae work equally well as standard candles for measuring cosmic distances. Answer: FALSE 8) The larger the value of Hubble's constant, the more rapid the expansion of the universe and hence the younger the universe. Answer: TRUE ...
Living Things - Fairfield-Suisun Unified School District
Living Things - Fairfield-Suisun Unified School District

... at different wavelengths. Astronomers are able to learn a great deal about the Crab Nebula by examining these different images. The images are shown at different scales. ...
Starburst Galaxies - Beck-Shop
Starburst Galaxies - Beck-Shop

... Thirdly, the rate of star formation greatly exceeds the rate sustainable over the galaxy’s lifetime, so that the starburst event must be a relatively transient episode. A classical galaxy like our own has a star-formation rate within the disk of a few solar masses per year, equivalent to perhaps 100 ...
Introduction to Astronomy - Northumberland Astronomical Society
Introduction to Astronomy - Northumberland Astronomical Society

... Telescope (2 inch / 50mm) Telescope (4 inch / 100mm) Telescope (6 inch / 150mm) Telescope (10 inch / 250mm) Telescope (16 inch / 406mm) ...
Poster 49 | PDF (852 kB)
Poster 49 | PDF (852 kB)

... been subject to possible dynamical ejection from their clusters. We have recently conducted a methane imaging survey of the Rho Ophiuchi cloud for T dwarfs using the IRIS2 near-infrared imaging spectrograph on the Anglo-Australian Telescope. The Rho Ophiuchi cloud is the closest (d ~ 120 parsecs) st ...
Standing in Awe - Auckland Astronomical Society
Standing in Awe - Auckland Astronomical Society

... the photos in full colour. Congratulations once again to the winners and thanks to all those that entered. ...
Brown et al. 2008 Studying Resolved Stellar
Brown et al. 2008 Studying Resolved Stellar

... near-infrared sensitivity of JWST will be a major asset. For others, observations will have to take place at optical wavelengths where the atomic physics of stellar atmospheres places important diagnostics. We will show how even an infrared-optimized JWST, thanks to its larger aperture, will be able ...
Supermassive Black Holes in Inactive Galaxies Encyclopedia of Astronomy & Astrophysics eaa.iop.org
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... Maximally anisotropic models allow smaller masses, M• ~ 108M⊙, but isotropy is more likely given the rapid rotation. Since that time, two generations of improved observations have become available. The full circles in figure 2 were obtained with the Subarcsecond Imaging Spectrograph (SIS) and the Ca ...
HNRS 227 Lecture #2 Chapters 2 and 3
HNRS 227 Lecture #2 Chapters 2 and 3

...  The Tully-Fisher relation, which correlates the width of the 21cm line of hydrogen in a spiral galaxy with its luminosity, can also be used for determining distance  A method that can be used for elliptical galaxies is the fundamental plane, which relates the galaxy’s size to its surface brightne ...
A new view of galaxy evolution
A new view of galaxy evolution

... was obvious that fainter, and presumably more distant galaxies, look and are quite different from the galaxies we see in today’s universe. Understanding what this means, and how we can understand the physics of galaxy formation from these objects, have been major goals in astronomy for the past 15 y ...
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The Galaxy Presentation 2011
The Galaxy Presentation 2011

...  Extinction makes optical studies impossible - use radio or IR  Observe ionized gas, line emission, dust, star clusters  Resolution greatly improved with VLA and VLBI observatories, plus sensitive IR arrays ...
PHYS 2410 General Astronomy Homework 8
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2010_02_04 LP08 Our Galactic Home

... Up to 100 pc (parsecs) = 326 ly (light years) Up to 1000 pc (nearby in our galaxy) Up to 10,000 pc (104 pc) (into our galaxy) Up to 105 pc (100,000 pc) (through our galaxy) Up to 107 pc (far out into our galaxy and into other galaxies) ...
CO 2 Cycle
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... Bright new deposits seen in NASA images of two gullies on Mars suggest liquid water carried sediment in the past several years…The atmosphere on Mars is so thin that liquid water cannot persist at the surface. However, researchers propose that water could remain liquid long enough, after breaking ou ...
Astronomy - Wappingers Central School District
Astronomy - Wappingers Central School District

... are constantly being made. This often makes the internet a more powerful resource than a well developed textbook. The course is designed to be flexible enough that the students will be able to review and discuss some of these ground breaking topics as they are happening. At the other end of the spec ...
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... What are the factors to determine the chance there is advanced intelligent life out there? ...
June 2016 - Flint River Astronomy Club
June 2016 - Flint River Astronomy Club

... fusion at their cores does not stop when they run out of hydrogen atoms to fuse into helium. The process continues as helium converts into other, progressively heavier elements such as lithium, beryllium, carbon, neon, oxygen, silicon, and eventually iron. Every step in the process re-ignites the st ...
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Chapter 1: Introduction to Galaxies File - QMplus
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... Ellipticals are classified by their observed shapes. They are given a type En where n is an integer describing the apparent ellipticity defined as n = int[10(1 − b/a)] where b/a is the axis ratio (the ratio of the semi-minor to semi-major axes) as seen on the sky. In practice we observe only types E ...
The Great Nebula in Orion
The Great Nebula in Orion

... Hubble’s high resolution enables us to separate the light of the closely packed stars in Orion. Its high stability and lightmeasuring accuracy overcome the challenge of the non-uniform brightness of nebula. In the Hubble images, we can precisely compare the stellar signals through many filters. We c ...
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Linking Asteroids and Meteorites through Reflectance
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... • Milky Way is 100,000 light years in diameter • There are ~100 billion stars in the Milky Way ...
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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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