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CCD PHOTOMETRY OF OPEN STAR CLUSTER M67
CCD PHOTOMETRY OF OPEN STAR CLUSTER M67

... created on the basis of CCD photometry. They are illustrated with theoretical isochrones in Figures 1, 2, 3, where on the vertical axis is placed the measured stellar size in the filter V and on the horizontal axis is the corresponding colour index. On these diagrams can be seen the main sequence di ...
as a PDF
as a PDF

The Zodiac - Alchemical.org
The Zodiac - Alchemical.org

... constellations associated with water, the Water Goat, the Water Bearer, and the Fishes. The ancient Babylonians saw the constellation as representing Ea, the fish-god who they also associated with an antelope. Earlier, the Sumerians had seen these stars as Enki, their river god. He was the ruler of ...
Workbook IAC
Workbook IAC

View
View

BMAC Newsletter 201105
BMAC Newsletter 201105

The Milky Way Galaxy
The Milky Way Galaxy

Astronomical Toolkit
Astronomical Toolkit

... need to know its distance from Earth. Historically, the stars visible to the naked eye were put into six different brightness classes, called magnitudes. This system was originally devised by the Greek astronomer Hipparchus about 120 BC and is still in use today in a slightly revised form. Hipparchu ...
targets - siamois
targets - siamois

Gone in a flash: supernovae in the survey era
Gone in a flash: supernovae in the survey era

... luminous supernovae (SLSNe) are a new class of high-redshift universe – beyond of space must be searched in order to find significant numextreme supernova that have emerged over the the reach of our current best tool, past five years (for a review, see Gal-Yam 2012), SNe Ia. bers. But with very larg ...
doc - Eu-Hou
doc - Eu-Hou

Lecture02: Astronomical Distance
Lecture02: Astronomical Distance

From the reviews - Astrofoto Portugal
From the reviews - Astrofoto Portugal

Colours of the rainbow
Colours of the rainbow

Learning Objectives - UNC Physics and Astronomy
Learning Objectives - UNC Physics and Astronomy

IAA-B4-0709P
IAA-B4-0709P

... The AADM is capable of attitude initialisation without any external support (lost in space solution). The NEAT mode performs attitude tracking, once initial attitude has been computed. The HEAT mode performs in a similar way to the NEAT, but operates with a reduced number of tracking windows of larg ...
P1 topic 3 - WordPress.com
P1 topic 3 - WordPress.com

... Two major theories about the origin of the Universe are the Big Bang and the Steady State theories. Some evidence supports both theories. Other evidence supports only one theory. By considering the evidence, discuss why one of these theories is preferred by most scientists. ...
Stars, Constellations, and Quasars
Stars, Constellations, and Quasars

Unit H557/02 - Advance Notice Article - June 2017
Unit H557/02 - Advance Notice Article - June 2017

... OCR is committed to seeking permission to reproduce all third-party content that it uses in its assessment materials. OCR has attempted to identify and contact all copyright holders whose work is used in this paper. To avoid the issue of disclosure of answer-related information to candidates, all co ...
Unit 6: Astronomy
Unit 6: Astronomy

Detection Technique for Artificially-Illuminated Objects in the Outer
Detection Technique for Artificially-Illuminated Objects in the Outer

... an object at a distance D ≫ 1 AU scales as D −4 due to the combination of the inverse square dependence of the solar flux which illuminates it combined with the inverse square dependence of the scattered component of that incident flux which reaches an observer on Earth. Thus, the observed flux from ...
Angular measurements
Angular measurements

Here - Astrophysics Research Institute
Here - Astrophysics Research Institute

... Coordinates of Solar System Objects All the objects considered so far have been "fixed stars", which keep almost constant values of Right Ascension and Declination. But bodies within the Solar System move a lot within the equatorial coordinate system. The most important one to consider is the Sun. ...
The Milky Way Model - University of Chicago
The Milky Way Model - University of Chicago

... debated the true nature of this cosmic smear: was it a cloud of gas and dust or a collection of closely packed stars, was it part of the Earth’s atmosphere or at great astronomical distances? These days, looking up at the sky from even a small city or suburb, the Milky Way isn’t even visible anymore ...
Lecture 3
Lecture 3

... This is the law of inertia, which was actually discovered by Galileo.  The second law concerns the force associated with its effect on the acceleration (increase of speed) of a mass. A larger force will make that the same mass is accelerate more (F = ma, where F is the force, m is the mass, and a i ...
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Astrophotography



Astrophotography is a specialized type of photography for recording images of astronomical objects and large areas of the night sky. The first photograph of an astronomical object (the Moon) was taken in 1840, but it was not until the late 19th century that advances in technology allowed for detailed stellar photography. Besides being able to record the details of extended objects such as the Moon, Sun, and planets, astrophotography has the ability to image objects invisible to the human eye such as dim stars, nebulae, and galaxies. This is done by long time exposure since both film and digital cameras can accumulate and sum light photons over these long periods of time. Photography revolutionized the field of professional astronomical research, with long time exposures recording hundreds of thousands of new stars and nebulae that were invisible to the human eye, leading to specialized and ever larger optical telescopes that were essentially big cameras designed to collect light to be recorded on film. Direct astrophotography had an early role in sky surveys and star classification but over time it has given way to more sophisticated equipment and techniques designed for specific fields of scientific research, with film (and later astronomical CCD cameras) becoming just one of many forms of sensor.Astrophotography is a large sub-discipline in amateur astronomy where it is usually used to record aesthetically pleasing images, rather than for scientific research, with a whole range of equipment and techniques dedicated to the activity.
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