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Study Guide: Use your notes and handouts to
Study Guide: Use your notes and handouts to

... What is a spectroscope? How do scientists use it to learn what elements are in the stars? ...
Descriptions For Posters
Descriptions For Posters

1 - BYU Physics and Astronomy
1 - BYU Physics and Astronomy

Astrophysics Outline—Option E
Astrophysics Outline—Option E

... E.3.14 State the relationship between period and absolute magnitude for Cepheid variables E.3.15 Explain hoe Cepheid variables may be used as “standard candles” E.3.16 Determine the distance to a Cepheid variable using the luminosity-period relationship E.4 Cosmology Assessment Statement Olbers’ par ...
Bang To Sol - Transcript
Bang To Sol - Transcript

Topic Outline - Physics Rocks!
Topic Outline - Physics Rocks!

... E.6.1 Describe the distribution of galaxies in the universe E.6.2 Explain the red-shift of light from distant galaxies E.6.3 Solve problems involving red-shift and the recession speed of galaxies Hubble’s Law E.6.4 State Hubble’s Law E.6.5 Discuss the limitations of Hubble’s law E.6.6 Explain how th ...
The Milky Way Galaxy
The Milky Way Galaxy

Astronomy and Space Science
Astronomy and Space Science

The Milky Way Galaxy is Heading for a Major Cosmic Collision
The Milky Way Galaxy is Heading for a Major Cosmic Collision

... –  Bright new regions of star formation appear, as gas gets compressed by the collision –  Star formation ceases, as gas and dust are expelled –  An elliptical light concentration remains on the night sky, having replaced today’s familiar Milky Way ...
Galaxy Questions Info
Galaxy Questions Info

... (pinwheel-shaped) arms, a bulge at its center, and a halo. Spiral galaxies have a variety of shapes, and they are classified according to the size of the bulge and the tightness and appearance of the arms. The spiral arms, which wrap around the bulge, contain many young blue stars and lots of gas an ...
Intro to Astronomy
Intro to Astronomy

... would take millions years in our fastest spaceship to leave our galaxy so we could turn around and look back at it. ...
Student Worksheet - Indiana University Astronomy
Student Worksheet - Indiana University Astronomy

... to dense. The size of the grains and their composition also vary from place to place. Some form into aggregates of grains, and others become coated with mantles of ice. Both silicate and carbon grains can be found in interstellar space. Dust interacts with light by both scattering and by absorption. ...
Fundamental properties of the Sun - University of Iowa Astronomy
Fundamental properties of the Sun - University of Iowa Astronomy

... • A wind past the Earth at 400 km/sec • The Sun is “melting away” • Density 19 orders of magnitude less than atmosphere • A medium for solar events • May have “sandblasted” the early atmosphere of Mars ...
Introduction and first data set
Introduction and first data set

... In addition to stars, some curious fuzzy objects are seen scattered, with roughly uniform number density, all around the sky. They are similar to the jet-like features extending from the Southern Blue Spot (SBS). They vary enormously in brightness and size, though the larger ones tend to be brighter ...
Concept map-Rubric-final - Berkeley Center for Cosmological
Concept map-Rubric-final - Berkeley Center for Cosmological

... of matter contained or that accelerated expansion may be related to dark energy or other specific evidence, key objects, spectural ...
Justin Linford (MSU)
Justin Linford (MSU)

...  The angular resolution is then determined by the largest distance between two dishes. ...
The Electro-Magnetic Spectrum - EHS
The Electro-Magnetic Spectrum - EHS

... As frequency decreases, energy increases E = h • h = 6.626 x 10-34 Joules *second ...
Stellar Explosions
Stellar Explosions

Solar System, Galaxy, and Universe (ES) V.4
Solar System, Galaxy, and Universe (ES) V.4

Why Aren`t All Galaxies Barred?
Why Aren`t All Galaxies Barred?

radio_poster
radio_poster

... (1University of Tsukuba, Japan; 2Firenze, Italy) Abstract: We investigate the radio spectral energy distributions (SEDs) of young starforming galaxies. The duration and luminosity of the nonthermal radio emission from supernova remnants (SNRs) are constrained by using the observed radio SEDs of SBS ...
WHERE DO ELEMENTS COME FROM?
WHERE DO ELEMENTS COME FROM?

ies la arboleda – centro tic - plurilingüe
ies la arboleda – centro tic - plurilingüe

... (A)- The universe was contained in a single point in space. All of the matter and energy of space was then contained at this point. What existed prior to this event is completely unknown. About 13.73 billion years (13.730.000.000 years) ago a tremendous explosion started the expansion of the univers ...
Origins of the Universe - Fraser Heights Chess Club
Origins of the Universe - Fraser Heights Chess Club

The Scales of Things
The Scales of Things

< 1 ... 94 95 96 97 98 99 100 101 102 ... 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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