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The Sun: Source of heat and light
The Sun: Source of heat and light

Mass Segregation in Globular Clusters
Mass Segregation in Globular Clusters

Planning Observations
Planning Observations

Stars Names - astrofoto.org
Stars Names - astrofoto.org

... Stars Names ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

... care. The extra publicity may have caused more people to go out and look at totality (or perhaps let their kids stay up late to see it), and who knows — maybe a few of them got turned on to astronomy as a result. My only real annoyance was with the news media. Sloppy writing (and no fact checking) o ...
This document was created for people who do not have access to
This document was created for people who do not have access to

... of North America, the Crab Nebula would be approximately one quarter of a mile across and 160 miles away from our Solar System. The Crab Nebula is the remains of an exploded star that was once 8-12 times the mass of our Sun. Very massive stars end their lives in a gigantic explosion, known as a supe ...
Feb 2017 - Astronomical Society of Northern New England
Feb 2017 - Astronomical Society of Northern New England

Reach for the Stars B
Reach for the Stars B

Down Under from North Florida
Down Under from North Florida

Telescopic Drawings or Photographs of Celestial
Telescopic Drawings or Photographs of Celestial

IYA 2009 - AAVSO Beginner/Intermediate Amateur Astronomer
IYA 2009 - AAVSO Beginner/Intermediate Amateur Astronomer

Why Spectroscopy?
Why Spectroscopy?

Binary Beauties: By John R - Black River Astronomical Society
Binary Beauties: By John R - Black River Astronomical Society

... The second polarized filter type is comprised of two layers of polarized material. The 2nd layer is mounted immediately above the 1st and is meant to be rotated. The filter is designed to act as a light "spigot", able to meter incoming light. As fields cross, the filter darkens. This is handy to red ...
View the sky`s greatest nebula
View the sky`s greatest nebula

... Draper used an 11-inch Alvan Clark refractor with a triplet objective. He also used a new “dry-plate” photographic technique to make his images. The exposure lasted 50 minutes. Since that night in 1880, M42 has been scrutinized through every size telescope and in every available band of the electrom ...
Dec 2016 - Astronomical Society of Northern New England
Dec 2016 - Astronomical Society of Northern New England

... down to the size of a city and only occur after a supernova explosion, which is much more powerful and rarer than the common explosion of an average star, which is called a planetary nebula. Every white dwarf is basically pure carbon and some oxygen, but much more dense and valuable than the best di ...
Diapositiva 1
Diapositiva 1

presentation source
presentation source

Universe Discovery Guides: January
Universe Discovery Guides: January

Light
Light

The Dimensions Program - Asnuntuck Community College
The Dimensions Program - Asnuntuck Community College

... In order to know more about a star, we need astronomy. Astronomy is the study of stars, planets, galaxies, comets, gaseous clouds, the space between the galaxies, and any other celestial objects. Astronomers, the scientists that do astronomy, use telescopes to make images of celestial objects that a ...
orion® starBlast™ - Spectrum Scientifics
orion® starBlast™ - Spectrum Scientifics

June 2015 - Bristol Astronomical Society
June 2015 - Bristol Astronomical Society

What is Epsilon Aurigae?
What is Epsilon Aurigae?

March
March

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Larger, high-res file, best for printing

... easy-to-find deep-sky objects. Some of them you can see even from a lightfilled city sky. Well, I guess I have to qualify that statement. Ken’s deep-sky objects can be seen from many, though not all, city locales. Xi’an, China, in July 2008 — two hours after sunrise. I was reminded of the problem la ...
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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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