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Photoelectric Photometry of the Pleiades
Photoelectric Photometry of the Pleiades

Chapter 1 Seeing the Light: The Art and Science of Astronomy
Chapter 1 Seeing the Light: The Art and Science of Astronomy

... and Saturn. These celestial bodies aren’t wandering through the stars; they orbit around the Sun, our solar system’s central star. Today astronomers know that planets can be smaller or bigger than Earth, but they all are much smaller than the Sun. The planets in our solar system are so close to Eart ...
What is an astrolabe
What is an astrolabe

December 2011
December 2011

Spectral resolution, wavelength coverage, the atmosphere and
Spectral resolution, wavelength coverage, the atmosphere and

Aryabhatta Research Institute of Observational Sciences
Aryabhatta Research Institute of Observational Sciences

The double-degenerate, super-Chandrasekhar nucleus of the
The double-degenerate, super-Chandrasekhar nucleus of the

Oldest SN
Oldest SN

... One of the objects is either the Sun or the (near) full moon and second object is relatively close to the first. If we assume one of the objects is the Sun then the second object cannot be the moon, since, with such proximity to the Sun, the moon would be in a partial phase around the new the moon a ...
Astronews - Hawaiian Astronomical Society
Astronews - Hawaiian Astronomical Society

... Lacy Veach Day of Discovery – President Chris Peterson reported that the club will take part in the upcoming annual Lacy Veach Day of Discovery at Punahou School. It will take place during October 31, 2015. Gretchen West will have a sign up page at the next general membership meeting, as we need to ...
November - LVAstronomy.com
November - LVAstronomy.com

Electronic version
Electronic version

Temperate Earth-sized planets transiting a nearby ultracool
Temperate Earth-sized planets transiting a nearby ultracool

ppt document
ppt document

orion® starseekers - NexStar Resource Site
orion® starseekers - NexStar Resource Site

key - Scioly.org
key - Scioly.org

2010-02 LAAS Bulletin I - Los Angeles Astronomical Society
2010-02 LAAS Bulletin I - Los Angeles Astronomical Society

... the surface temperature of Earth will be about 6 times its current value. That’s about 1728 Kelvins or 2650 Fahrenheit. That’s far above the melting point for lead, copper, zinc, silver, gold, aluminum, silicon, nickel, iron, titanium, and a host of other materials that we, and our technology, depen ...
Spectroscope Lab
Spectroscope Lab

... How fast a heavenly body moves and in which direction (red shift/blue shift). How hot a star is. If a star is rotating. If a star has a magnetic field ...
The Sun - Sophia
The Sun - Sophia

The Evening Sky Map
The Evening Sky Map

Patterns in the Night Sky
Patterns in the Night Sky

... saw thousands of years ago, their component stars are not in exactly the same location as they were then. Precise observations of stars reveal that they move relative to each other in space, but these changes in position occur slowly, over many years. Since most stars are so far away from Earth, whe ...
Mar 2016 - Bays Mountain Park
Mar 2016 - Bays Mountain Park

Document
Document

... http://images.google.com/imgres?imgurl=http://www.wisegorilla.com/images/solarsystem/MoonPhases.gif&imgrefurl=htt p://www.wisegorilla.com/images/solarsystem/solarsystem.html&h=540&w=720&sz=41&hl=en&start=11&tbnid=9sM05 oBriZfI2M:&tbnh=105&tbnw=140&prev=/images%3Fq%3Dmoon%2Bphases%26svnum%3D10%26hl%3 ...
night sky a field guide to the heavens
night sky a field guide to the heavens

... things were now for the first time, if, I say, they were now suddenly presented to mortals beyond all expectation, what could have been named that would be more marvelous than these things, or that nations beforehand would less venture to believe could be? Nothing, me thinks: so wonderous strange ha ...
Lecture 6-Spectral resolution, wavelength coverage, the atmosphere
Lecture 6-Spectral resolution, wavelength coverage, the atmosphere

3. The MONS Telescope requirements
3. The MONS Telescope requirements

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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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