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Ground-Based Astrometry 2010-2020
Ground-Based Astrometry 2010-2020

a to z of astronomy
a to z of astronomy

Lecture Topics 1023
Lecture Topics 1023

Lecture 6-Spectral resolution, wavelength coverage, the atmosphere
Lecture 6-Spectral resolution, wavelength coverage, the atmosphere

An Expanded View of the Universe
An Expanded View of the Universe

... Way. Trying to understand galaxy formation and evolution has become one of the most active fields of astronomical research over the last few decades, as large telescopes have reached out beyond the Milky Way. Yet, even nearby giant galaxies have remained diffuse nebulae that cannot be resolved into ...
VERA Project : overview and current status
VERA Project : overview and current status

... Simultaneous observations of two adjacent sources can cancel out atmospheric fluctuation target accuracy : 10 micro-arcsec ! Target source ...
DSLR photometry - British Astronomical Association
DSLR photometry - British Astronomical Association

... Even today, many amateur astronomers still measure magnitudes using their eyes and submit data to an organization such as the AAVSO (American Association of Variable Star Observers) which can be used by professional astronomers for research. ...
SXVR-H814 handbook
SXVR-H814 handbook

WhyIYA - DEP
WhyIYA - DEP

... Dialogues Concerning Two New Sciences was published by Elzevier in Leiden, because it could, of course, not be published in Catholic lands. The book convincingly argued against the Earth centered universe and upheld the scientific sprit. No wonder the 400th annivesary of Galileo’s use of telescope i ...
High-Energy Astrophysics with Gamma
High-Energy Astrophysics with Gamma

... detected as gamma-ray sources  Starburst activity – cosmic ray populations – difussion Detailed analysis for ULIRG Arp 220 confirms this. Many other LIRGs (several tens) may appear in the forthcoming catalogs  first multiwavelength analysis of Arp 220 (the strongest site of star formation known, t ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

8.1 Radio Emission from Solar System objects
8.1 Radio Emission from Solar System objects

PoS(EVN 2014)058 - Proceeding of science
PoS(EVN 2014)058 - Proceeding of science

... Email: [email protected] The e-MERLIN Cyg OB2 Radio Survey (COBRaS) is designed to exploit e-MERLIN’s enhanced capabilities to provide substantial deep-field mapping of one of the most massive OB associations in our Galaxy, offering direct comparison to not only massive clusters in general, but als ...
The History of Infrared Spectroscopy
The History of Infrared Spectroscopy

... (Herschel 1800). Much to his surprise, he found that not only did thermometers register heat beyond the red end of the visible spectrum, but the greatest amount of heat was found in this region. After an initial claim that these “heat rays” were just extensions of visible light, he became convinced ...
Between the Stars: Gas and Dust in Space
Between the Stars: Gas and Dust in Space

... To understand how stars form, we need to know the raw material from which they are made All the gas and dust material that lies in the region between stars is referred to as interstellar matter The entire collection of interstellar matter is called the interstellar medium The interstellar medium acc ...
November - LVAstronomy.com
November - LVAstronomy.com

... found in Cassiopeia. One of the finest, but often overlooked, is NGC-7789. Cassiopeia is one of the most recognized constellations. The constellation is circumpolar for anyone north of a line from San Francisco to Baltimore. When high above Polaris, five of its brightest stars roughly trace out the ...
Does gravity conserve angular momentum
Does gravity conserve angular momentum

... surroundings by gravity, and form the rings of Saturn and the disc galaxies. In this paper, we analyze what happens with the gravity fields of collapsing stars. It is found that not only the mechanical angular momentum is regulating the orientation of disc galaxies. The magnetic-like component of gr ...
Unit 6: Astronomy
Unit 6: Astronomy

Astronomical Picture of the Day
Astronomical Picture of the Day

Lecture 1a
Lecture 1a

z= 1000 - z= 10
z= 1000 - z= 10

... •Metals usually dominate the cooling --- but there are no metals •Molecular hydrogen is the only significant cooling in primordial gas ...
Chapter 15: The Milky Way Galaxy
Chapter 15: The Milky Way Galaxy

... How many stars does the Milky Way Galaxy contain? The Milky Way has about 200 billion stars. Where is our solar system located in the Milky Way Galaxy? The solar system is between the Sagittarius and Perseus spiral arms about 26,000 ly from the center of the Galaxy. Is the Sun moving through the Mil ...
X-ray output should be time variable
X-ray output should be time variable

11 Celestial Objects and Events Every Stargazer Should See
11 Celestial Objects and Events Every Stargazer Should See

Stargazer - Everett Astronomical Society
Stargazer - Everett Astronomical Society

< 1 ... 30 31 32 33 34 35 36 37 38 ... 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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