Tuesday, November 25, 2014

Astronomy Tools - Equipment

Astronomy Tools - Equipment

Astronomers use various types of equipment based on the portion of the E-M Band to be observed.Telescopes and radio dishes are used from the surface of the Earth to study visible light, near infrared light, and radio waves.
Attached to these telescopes are various tools like special made CCD cameras, a wide variety of filters, photometers and spectrometers. These various instruments are designed to record what we normally cannot see with our eyes.
From space, astronomers use special telescopes to study X-ray and gamma ray emissions. In addition,space based telescopes like the Hubble Space Telescopecan peer deep into the Universe without atmospheric interference.
Other specialized instruments are also finding their way into main stream astronomy, like neutrino detectors deep underground and gravity wave detectors.
Telescopes and radio dishes are also pairing up to create interferometers to increase the resolutioncapabilities. Radio dishes are often found as members of a group like the VLA in Socorro, New Mexico.
The following sections will look into the more common pieces of equipment used today to gather valuable data.
Telescopes

This section on telescopes is not designed to serve as a buyers guide, but to outline the popular styles of telescopes used today.For tips and advice on what type of telescope is good for you, a good starting point is Best Telescope Guide.
In order to see faint celestial objects, or if you want to look closely at the moon and the other planets of our Solar System, you need a telescope. It important to know that while magnification can seem like a good thing, the important issue to consider when looking for a telescope is aperture - the diameter of the telescope. The larger the aperture, the more light can be seen. Some rules of thumb:
  • Aperture dictates how much light can be seen
  • Focal length is the length of the refracted or reflected light path at focus
  • If you will take your telescope to remote locations, consider carefully your choice of aperture - weight considerations
  • Short focal lengths equal brighter images - not recommended for looking at planets (image too washed out)
  • Shorter focal lengths also equal larger field of view
  • Long focal lengths equal dimmer image and narrow field of view
  • NEVER USE A TELESCOPE TO LOOK AT THE SUN - without a proper solar filter.
There are essentially three groups of telescopes: refractors, reflectors, and compound.
Refracting telescopes use lenses to focus and magnify an object. There are two classes of refractors:
  • Achromatic - single objective lens
  • Apochromatic - multiple objective lenses

A typical refractor will usually come looking like this. I think anyone who had an interest in astronomy as a kid had one of these - I know I did. I remember the first object I wanted to see which was - you guessed it - Saturn, everyone's favorite through a telescope. Image provided byCelestron.
A common issue with any standard refractor is something called chromatic aberration. Recall a prism and how light is separated into fundamental colors of the rainbow. As such, a single lens will have difficulty focusing the red and blue (either side of the visible spectrum) to a single point. In an effort to correct this flaw, a second and sometimes third lens are placed together to ensure single focus. This is the apochromatic and not surprisingly the price can double or triple compared to a standard achromat.
Reflecting telescopes use mirrors to focus light and an eyepiece to magnify. There are two common classes of reflecting telescopes:
  • Newtonian
  • Ritchey-Chretien
Image of the light path involved with a Newtonianstyle telescope. Image provided by Celestron.
The light path of a Ritchey-Chretiendesign is similar to aSchmidt-Cassegrainbut without a corrector plate.
A style of Newtonian telescope called the Dobson - named after the style of mount - is a popular first choice for a beginning telescope. It offers a large aperture for a modest price. Image provided by Celestron.
Reflecting telescopes eliminate any chromatic aberrations since lightdoes not pass through anything - only reflected. There is another issue with reflecting (and poorly designed refractors) telescopes called coma. Stars will appear stretched towards the edge of the field of view. Coma is eliminated in the Ritchey-Chretien design since hyperbolic mirrors are used - and result in a higher manufacturing cost.
This image illustrates what coma could look like. When looking though a Newtonianreflector, the stars the edge of view will look almost like comas, or comets. This affect is more pronounced during astrophotography. The view at the center will be unaffected.
Compound telescopes use a combination of lenses and mirrors to focus the light.
  • Schmidt-Cassegrain
  • Maksutov-Cassegrain
This image is of a Schmidt-Cassegrain type of telescope. A corrector plate eliminates the coma introduced by the standard Newtonian. Image provided by Celestron.
The Maksutov-Cassegraintelescope uses a lens in place of a corrector plate. This helps overall color and eliminates coma. Image provided by Celestron.
This image is typical of the Schmidt-Cassegrain type of telescopes available today. Celestron was nice enough to let use their images on this portion of the website, but oddly enough I have never looked through aCelestron telescope. This particular model is their NexStar series that boasts a fiber woven tube for light weight portability and faster cool-down times and also features the ease of GPS alignment and a computer for finding and tracking your favorite objects. These features are common on a wide variety of manufactures.
While the Schmidt-Cassegrain's corrector plate eliminates the issues of coma, it does not eliminate coma completely. This is evident isastrophotography, and many seasoned imagers prefer the Ritchey-Chretien because its design eliminates coma completely. The Maksutov-Cassegrain uses a lens instead of a corrector plate to reduce coma, but to eliminate chromatic aberration, long focal lengths are required. As such, the Maksutov-Cassegrain really is best suited for planetary work - and the optics can be quite good.
So what telescope is best? There really isn't one, but there are some guidelines:
  • For an inexpensive achromatic refractor, stay away from short focal lengths - anything greater than a focal length of f6.5 is good.
  • Apochromatic telescopes are very expensive, and just like high end audio equipment, have their faithful following. Read reviews and look for yourself! However, if you plan to use the telescope for astrophotography, an apochromatic telescope is necessary.
  • Meade and Celestron are the two main producers of theSchmidt-Cassegrain telescope. There is not a clear winner as to who is best, but Meade tends to include more electronic wizardry into their scopes - which is fine if you like that sort of thing. Truth is, competition between these two companies is good for the consumer as the need for better and cheaper telescopes are released often.
  • Go to a local Astronomy Club or "Star Party" - a gathering of like minded folks flocking to a dark location for a night of fun filled observing. There are sure to be a variety of telescopes, and most are willing to let you take a peek. Astronomy and Sky and Telescope magazines will have a list of national events.
To help determine choice, you may want to know how faint your telescope choice can see - keeping in mind this is mathematical and may vary depending on central obstruction of the telescope and the atmospheric conditions:
An example: a 10" telescope has a diameter of 254 mm:
The faintest object a 10" telescope can see is with a visual magnitudeof 14.7 (Pluto has a magnitude of around 13.8).
A nice summary of each style of telescope and its application is:
Telescope StyleThe Good:The Bad:
AchromaticInexpensive, good first scope, great portabilityChromatic aberration, often heavy and poorly designed tubes, not upgradeable
ApochromaticExcellent color, perfect forphotography andplanetary workExpensive
NewtonianInexpensive, available up to 20" or moreNot for photography, coma, large size difficult to transport, collimation required often
Ritchey-ChretienExcellent deep sky work andphotographyExpensive, not really suited for visual observation
Schmidt-CassegrainGood all-around telescopeLarge central obstruction, needs collimation often
Maksutov-CassegrainGood planetary work, boasts image quality like an apochromatExpensive, high focal length unsuited for deep sky observing
Collimation means adjustment of the light path. Reflecting telescopes use a small secondary mirror to focus the light toward an eyepiece, and the alignment can suffer due to excessive movement of even violent temperature changes. Devices are available at your local telescope store to help correct this condition.

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