Friday, September 30, 2011

Celestron EdgeHD 1100 CGEM Schmidt-Cassegrain Telescope

!9# Celestron EdgeHD 1100 CGEM Schmidt-Cassegrain Telescope

Brand : Celestron | Rate : | Price : $3,499.00
Post Date : Oct 01, 2011 00:24:35 | Usually ships in 2-3 business days

Celestron's innovative new EdgeHD telescopes are aplanatic Schmidt Cassegrain models designed to produce aberration-free images across a wide visual and photographic field of view. Celestron EdgeHD optics produce a focal plane more than three-times flatter than a standard Schmidt Cassegrain telescope. This guarantees you visibly sharp stars across some of the largest CCD chips available today. Superior edge performance not only creates rounder, more pleasing stars but actually improves the resolution and limiting magnitude when compared to telescopes of equal aperture. With Celestron's High Definition optics you will be able to capture the faintest of galaxies all the way to the corner of your full frame camera chip. Coupled with Celestron's XLT coating group on every surface, EdgeHD optics gives you maximum light throughput across the widest visual and photographic spectrum. The EdgeHD tube has been redesigned with top-notch features to make sure you get the most from your optics each and every night. Mirror locks hold the mirror in place and reduce image shift when rotating the tube around the mount. Flexible rods allow the mirror to be held in place without putting any force or pressure on the mirror, keeping the image centered in the eyepiece (or chip). Cooling tube vents located on the rear cell allow hot air to be released from behind the primary mirror. Each vent has an integrated 60 micron mesh filter guaranteed to let warm air out without letting dust in.

  • Celestron 11" aperture aplanatic Schmidt-Cassegrain telescope produces astrograph-quality flat focal plane
  • EdgeHD coma-free Cassegrain optics and a built-in field flattener ensures sharp focus all the way to the edge of the field
  • Flexible tension clutches hold the mirror in place and reduce image shift when rotating the tube around the mount
  • Cooling vents located on the rear cell allow hot air to be released from behind the primary mirror
  • All EdgeHD optical tubes are Fastar compatible for imaging down to f/2 with optional accessories

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Monday, September 26, 2011

Celestron CGEM CPC

Celestron CGEM 1100 Dream Discovery HD show you. El nuevo el Telescope MEGCs HD 1100 Montura de diseño computarizada CGEM Equatorial combination with System of nuevo EdgeHD Optico. Ofrecer Imágenes más hasta 89% of the United Nations de que hasta el 40% más United Nations and these brilliant 8''y 9.25''. El nuevo todo el poder System Optico EgdeHD toma por los popularizado telescopios Schmidt-Cassegrain Compact with the UN System y Mejorada definición de lo combination optics, you Permite que Realizelarge scale de calidad y de campo astrophotography. Puedes buscar como Instrumento de todos los Objetos Messier catalog Observaciones y otros cientos de Objetos de los interesantes Catálogos equally from both NGC, IC y Caldwell. Observaciones para Astronomical imagen, el diseño EdgeHD disminuye Considerable aberración en la la. Even Realize Permite, en el de la Cámara CCD USE, en todas las estrellas buen a fire. Manti and limit difracción de los Objetos en todo el DuringCampo de vista de muchas de las más populares astrofotográficas camara. El más veces UN EdgeHD 11''zu produce que el plano Priority 3 Equivalent to a UN SCT Telescope plano. Junto este nuevo diseño with Optico, el también has EdgeHD rediseñado mecanismos que el mejor ayudarán Get yourself a telescope de Rendimiento you, como lo que en lugar the UN Asegurador espejo y los cambios en mantles of reducing Movement During Observaciones; Ventilacion liberate those allowed el aire caliente ofMain non-espejo, espejo Secundario desprendible ...

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Thursday, September 22, 2011

Celestron CGEM 1100 - 11" SCT Telescope on CGEM Equatorial Mount 11099

!9# Celestron CGEM 1100 - 11" SCT Telescope on CGEM Equatorial Mount 11099


Rate : | Price : $3,399.00 | Post Date : Sep 22, 2011 08:37:02
Usually ships in 1-2 business days


Celestron's CGEM-1100 features Celestron's high-end 11" Schmidt Cassegrian OTA with XLT coatings mounted on our brand new CGEM mount.

The CGEM mount has a fresh, attractive, bold appearance and is capable of carrying Celestron's higher-end SCT optical tubes (up to 11") securely and vibration free which is ideal for both imaging and visual observing.

Ergonomic Design - CGEM was designed to be ergonomically friendly with large Altitude and Azimuth adjustment knobs for quick and easy polar alignment adjustment. The internal RA and DEC motor wiring provides a clean look and an easy and trouble free set up.

Innovation - The CGEM series has a new innovative Polar alignment procedure called All-Star (patent pending). All-Star allows users to choose any bright star, while the software calculates and assists with polar alignment. Another great feature of the CGEM, sure to please astroimagers, is the Permanent Periodic Error Correction (PEC) which will allow users to train out the worm gears periodic errors, while the mount retains the PEC recordings.

Performance - For objects near the Meridian (imaginary line passing from North to South), the CGEM will track well past the Meridian for uninterrupted imaging through the most ideal part of the sky. The CGEM mount has a robust database with over 40,000 objects, 400 user defined programmable objects and enhanced information on over 200 objects.

Celestron's CGEM mount is the perfect fit between the Advanced Series and CGE Series. Offering the portability of the Advanced Series and the precision of the CGE.

Features

* Ultra Sturdy 2" steel tripod with Accessory Tray * Star diagonal provides more comfortable viewing position when observing objects that are high in the sky * 40,000 object database with 400 user-definable objects and expanded information on over 200 objects * Proven NexSt

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Saturday, September 10, 2011

Astronomy homeschool on a budget

!9# Astronomy homeschool on a budget

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First, in astronomy there is a large financial investment. Just go out and look. Immediate success. You see the stars.

But then comes a thirst for more. What are the stars? Why move in the sky? And what has that twinkle in his eyes and glistening all over? Do not ask, since thought Superman wore underwear. These questions are worth a trip just responded to your local library.

Then it happened. Discover has its own cityan astronomy club. "Come and see the stars," he curls up! "Free star party on Saturday!" Armed with a thermos of hot chocolate and cookies your wife trudging the hills star of the party. And you see everything - not just the stars and galactic nuclei, but all the telescopes.

WOW.

Your wife is not happy to trade the car for a telescope. Call them crazy, but a telescope does not collect food or take the kids to ballet. In fact, it's a gadget, the things we were lookingSince one of you were there before. You're only doing it now all fired. And yes, things most of them shining, it's there when you retire, so why not wait until then?

"Since the purpose of life, the happiness that can only be experienced in the actual experience," says the Dalai Lama with a lot of patience.

"But the Dalai Lama has four children and two mortgages," your wife counters. So what will you do?

Astronomy ClubTelescopes are for members, but if you want something right now? (We are Americans, after all.) And you want to share with your children for astronomy, and are not likely to share an expensive telescope with dirty hands. There must be an alternative happy. But what?

Go get a raft. The inflatable kind that you have lurking in the garage already. Put it on the lawn and pull a pair of binoculars. A good pair. Add cocoa and biscuits, andInstant Star have a party worthy of every amateur astronomer.

How to get a good pair of binoculars? Here are some ideas that might work for you (Backyard Astronomer's Guide by extracts from Dyer and Dickinson):

Large main objectives means brighter images, but for most people is a 50 mm lens offers a practical limit to the handheld. Binoculars with a 7 mm exit pupil are easier to get in front of the eye position, an advantage for young people and beginners of all ages to correct.

TopMagnification means better resolution, but it also means the highest standards of optical quality to produce good pictures. It also leads to an increase in shaking in portable mode. This factor alone limits for handheld 10x magnification binoculars for astronomical observations.

All together they are the most common sizes 7x50 and 10x50. If you like smaller and lighter, go for the 7x42 and 8x42. Why not go for the 10x50s, since the largest is called the best? Now that the objectives andObservation with a telescope at night is much easier for some than others. In our experience, are much easier to use 7x50s. On the other hand, made 10x50s weaker stars and the moon and the sky covered in more detail. More specifically it makes sense, but because they are dimmer stars more clearly? Part of the reason for this is that by avoiding the exit pupil smaller edge-of-eye aberrations (which produces crisp stars) helps, but most of all is that the higher magnification, in fact, spreading from the sky in the background, obscuring thein the process.

Binoculars with roof prisms are more compact than Porro smaller than 42 and usually are more expensive. For general astronomy binoculars at a reasonable price, we recommend Porro 7x50 and 10x50 models

General recommendations for glasses Astronomy:

These two differ is in the range $ 200: Orion Vista 10x50 and 10x50 Celestron Ultima. Both are 27 ounces (exceptionally easy for binoculars 50mm) and a very sharp and a good range of 5.3 degreesInterocular distance. In the range of $ 100 is the Bausch & Lomb Legacy 7x50 and 10x50 binoculars ideal for beginners in astronomy. A lightweight tripod and L-adapter are a great addition to an update. Go enjoy your night sky!


Astronomy homeschool on a budget

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Monday, September 5, 2011

Telescopes - How to Select a Spotting Scope

!9# Telescopes - How to Select a Spotting Scope

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Welcome to the understanding of a telescope. This wonderful device has been specially developed for daily use to increase your enjoyment outdoors and wildlife viewing. This tool allows you to remotely wildlife in their natural environment to enjoy. Enjoy the beauty of undisturbed and learn more about their unique habits.

A telescope is an abridged version of a telescope to be used in daylight. Its smaller size allows greater flexibility and portability. It differswith a telescope, as it always produces a vertical image. It 'was designed to be mounted on a standard tripod or one of the media window. Enjoy a need for more magnification binoculars so you can see objects at a greater distance. For our hunter, a telescope is a great tool for the evaluation of your goals on the shooting range.

We wish you a basic understanding of the numbers of your telescope is labeled. Here you will find three numbersconnected to the same extent. The first two numbers indicate the magnification. For example, a reading area is a 18-36x50 zoom range of 18 to 36 The last number is the diameter of the front lens. The 18-36x50, it would be the size of the 50mm objective lens. The bigger your goal, the more detail you can see from your perspective.

Most telescopes are refractors, which means that using a prism to rotate the image right and correct from left to right.There are two types of prisms are available: Porro prism and roof prism. Porro prisms are by far the most popular, because they are cheaper to produce and easier. A roof prism allows the producer of a sleek, compact design, therefore, to improve portability to produce. There is a wide variance in performance capability between low quality and high-quality spotting scope purchase, so according to your needs. It will certainly be able to notice the difference inQuality.

We hope that this information can be found in the decision to support what the telescope for sale and we will continue to keep us updated with future articles on understanding your telescope.


Telescopes - How to Select a Spotting Scope

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Friday, September 2, 2011

Physics IB - IA Example: data collection and processing

!9# Physics IB - IA Example: data collection and processing

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For those who have difficulty writing their internships, this article allows for data collection and processing component to write a physics IB explain practical.

In principle, the practical calculations of the dynamics involved is allowed with the help of a machine, collisions with minimal friction. The objective was to examine the law of conservation of momentum.

Below is an example of this practice:

Data collection and processing:

Qualitative observations:

It 'wasnoticed that the metal ramp would be a bit 'after each shot and that if the ramp was adjusted heated, the plane because of the movement that changes shape metal. By adjusting the slider at the bottom of the ramp, the height can move the ramp so that the ramp approximately parallel to the ground, but as a vocation, railways, planes are likely to be influenced by the effects of gravity on the sides of the ramp. This would increase the uncertainties of this experiment, because theEffects of gravity would have taken hours.

Moreover, it records the acceleration of the infrared light SAILING readings during two distinct periods. The screen consists of two metal parts, which block infrared light and the time is blocked by the machine is used to calculate the acceleration. However, the two pieces of metal can reflect light and give back a part of the natural light in the room have on the reader. This may have added to the uncertaintyexperiment.

If the ramp has been set, so it was horizontal and the plane was placed in the middle, the plane rocked back and forth. The air rising from the holes of the ramp would push the brush against the edge of the wing and rear. Then push the air behind the shield against the edge of the wing and the brush.

After the collision of two gliders, it was found that the terminal velocity gliders' (separation after the collision) was similartheir initial velocity (before the collision). This indicates that the value should be the last trip similar to the value of the first lap.

After the string was cut between the slides, causing the magnetic force of repulsion between the magnets attached to them, go in different directions. It was found that the plane was heavier than the lightest shade slower. This is the same for the dynamism necessary (and as well as their directionsvice versa), since p = mv. If m is larger, v must be smaller to be the same for both p for gliders.

Raw data:

Note: The units are in SI units are converted to proper treatment.

There were two gliders, gliders A and B. A glider glider had a mass of 261G. Glider B had a mass of 309g. Let the uncertainty of half of the body, because the scales used to measure only possible up to 1 gram

A glider is always first and always on the left side Glider Bon the right side first. Let the direction of the velocity on the right side must be positive.

The uncertainty of the mass of each glider is + / - 0.5 grams, since the scale can be measured with precision at this level. 0.05 mm-1 - The uncertainty of the initial velocity and final would, in theory, be + /. This will be recorded in the raw data.

However, there are more uncertainties in this measurement is involved. It is not possible for the slope of the ramp, perfectly horizontal, soGravity has no effect. In addition, the air rising from the holes would also measure a few changes. The light reflecting off the metal plates can also influence the outcome. In addition, the recorder speed of light calculated from the length of the plates. The length of these plates is 100 mm + / - 0.5 mm. So there is much uncertainty over + /-0.05mms-1.

The uncertainty can not be quantified, but that would mean that the data can not be determined at 4significant digits. A rough estimate of the uncertainty will be 5mm-1. This is half the final digit of a measurement to 3 significant figures.

The correct number of significant digits will be used the processed data. For now, it will be left with four significant figures, since the raw data.

Experiment collision

Glider

Fair + / -0.05 (g)

u + / -5 (mms-1)

v+ / -5 (Mms-1)

A

261

1493

-836.0

B

309

-1186

780.0

Experiment magnetic repulsion

Glider

Fair + / -0.05 (g)

u + / -5 (mms-1)

v + / -5 (mms-1)

A

261

0.000

-280.0

B

309

0.000

230.0

Data processed: The data will now be converted to SI units and their uncertainties.

The mass of raw data must be converted to kilograms. Thus, the uncertainty isby + /-0.0005kg.

The speed of the raw data will be converted to ms-1. This will be only three significant digits, as explained above and the uncertainty is 0.005 ms-1.

Experiment collision

Glider

Fair + / -0.0005 (kg)

u + / -0005 (ms-1)

v + / -0005 (ms-1)

A

0.261

1.49

-0.836

B

0.309

-1.19

0.780

Magnetic RepulsionExperiment

Glider

Fair + / -0.0005 (kg)

u + / -0005 (ms-1)

v + / -0005 (ms-1)

A

0.261

0.000

-0.280

B

0.309

0.000

0.230

Momentum calculation:

Let A be the mass of the sail and its initial velocity uA mA and VA Let UB be its final speed and its top speed will be the mass of the BB B mB glider and its initial velocity

Be the first sweep of the screen of a PIA and his last race pfa. Leave the firstB PiB dynamic momentum of the sail and pfb are final.

Collision experiment:

pia = 1.49 = 0.389 = 0.261x Maua Ns

The uncertainty can be calculated by adding the uncertainties of the masses and the initial velocity:

Relative error = 0.002 mass = 0.0005/0.261 relative error of the initial velocity = 0.005/1.49 = 0.003 Total relative error = 0.005 or 0.5% absolute error = 0.005 x 0.389 = 0.002

Sun pious = 0.39 + / - 0.002 Ns

Using the same method, theother values ​​of momentum, and their absolute error can be calculated:

MAVA PFA = = (0.261 + / -0.0005) x (-0.836 + / -0.005) = - 0.22 + / - 0.002 Ns

PIB Mbube = = (0.309 + / -0.0005) x (-1.19 + / -0.005) = - 0.36 + / - 0.002 Ns

pfb mBvB = = (0.309 + / -0.0005) x (0.780 + / -0.005) = 0.24 + / - 0.002 Ns

Experiment magnetic repulsion:

Since UA and UB are both equal to 0, the first sweep of the A and B glider glider is equal to mu = 0 This is because most ex 0 = 0

PFA =MAVA = (0.261 + / -0.0005) x (-0.280 + / -0.005) =- 0.07 + / - 0.001 Ns

pfb mBvB = = (0.309 + / -0.0005) x (0.230 + / -0.005) = 0.07 + / - 0.002 Ns


Physics IB - IA Example: data collection and processing

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