• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Project 1. CCD image analysis
Project 1. CCD image analysis

... more  photons  strike  the  surface:  the  brighter  the  illumination  the  greater  the  charge. It is possible to estimate the amount of light that has fallen onto each pixel  by  examining  the  amount  of  charge  it  has  stored  up.  Thus,  the  charge  which  has  accumulated  in  each  pixe ...
Learning goals for Astronomy`s Final 2013
Learning goals for Astronomy`s Final 2013

Galileo Galilei (1564-1642) - Sunshine Coast Centre RASC
Galileo Galilei (1564-1642) - Sunshine Coast Centre RASC

observingopenclusters-2-2-1
observingopenclusters-2-2-1

Ch. 27 Notes
Ch. 27 Notes

Unit 3: Understanding the Universe
Unit 3: Understanding the Universe

... Describe the composition of each of the outer planets. ...
01 - University of Warwick
01 - University of Warwick

... we must emphasize that this is just a hypothesis. No one has The second satellite is fainter than the first, but still detected done rigorous scientific calculations to verify that the hyin three of the five images of the first satellite. You can read pothesis actually works in detail, but our scien ...
Desert Skies - Tucson Amateur Astronomy Association
Desert Skies - Tucson Amateur Astronomy Association

What, and Why, is the International Astronomical Union?
What, and Why, is the International Astronomical Union?

... Hyderabad had originally agreed to do, they took on another later). The Carte du Ciel was, in retrospect, a target at which you threw not only money* but also the irreplaceable time of gifted scientists. Two other turn-of-the-century international projects deserve mention. Astronomers had gradually ...
Falling Stars
Falling Stars

Student Literacy
Student Literacy

... how some stars were always visible at night. Other stars were only visible during certain months of the year. People charted when these stars appeared and how they were positioned. They depended on these stars and star patterns for direction. Skywatchers noticed that during the spring, summer, fall ...
PDF Version
PDF Version

... time always has the same shape. What makes them very useful is that the period of the variation, which is the amount of time before the star’s brightness curve repeats itself, varies with the star’s intrinsic brightness. The star’s apparent brightness, which is the brightness that we can see ourselv ...
First Exam - University of Iowa Astrophysics
First Exam - University of Iowa Astrophysics

... (d) an imaginary point on the celestial sphere which we see as straight overhead (e) an imaginary line of the sky, defined by the right ascension = 0 hours 18. Which of the following planets is most similar to the Earth in mass and diameter? (a) Venus ∗ (b) Jupiter (c) Saturn (d) Uranus (e) Mercury ...
Document
Document

Comet Observers Club Chair
Comet Observers Club Chair

... Of these, 184 are periodic comets (orbital periods less than 200 years); some of the remainder are no doubt periodic as well, but their orbits have not been determined with sufficient accuracy to tell for sure. Comets are sometimes called "dirty snowballs". They are a mixture of ices (both water and ...
The Crab Nebula - Exploring a pulsar up close! - Chandra X
The Crab Nebula - Exploring a pulsar up close! - Chandra X

Studying the Universe Studying the Universe
Studying the Universe Studying the Universe

The Stars - University of Redlands
The Stars - University of Redlands

Dynamite Diameters
Dynamite Diameters

Dorn_projectF08 - Bowling Green State University
Dorn_projectF08 - Bowling Green State University

here - North Central Kansas Astronomical Society
here - North Central Kansas Astronomical Society

... Be careful (still dangerous) and Venus “dot” hard to see. # 14 welding glass Solar Shades from astronomers without borders 10 -4 = 0.01% attenuation ...
Figure 1
Figure 1

Sirius Astronomer - Orange County Astronomers
Sirius Astronomer - Orange County Astronomers

Volume 1 (Issue 7), July 2012
Volume 1 (Issue 7), July 2012

... planned to be established. Research studies pertaining to deep space objects including galaxies, nebulae and variable stars are also being initiated. Search for earth like planets is a hot topic in astrophysics nowadays. It is planned to conduct research studies in this field also. ...
PHY2083
PHY2083

... ii) F = L / 4πr2 c.f. previous example at 1 AU now 10 pc = 2.063 x 106 AU Inverse square law => flux will be 1 / (2.063 x 106)2 times lower => Flux at 10pc = 3.21 x 10-10 W / m2 ...
< 1 ... 46 47 48 49 50 51 52 53 54 ... 95 >

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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report