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Refractor telescopes have long been touted as great optical instruments for studying the planets and Moon. But with its short focal length and generous 120mm aperture, our popular Orion AstroView 120ST (ST for "Short Tube") Equatorial Refractor Telescope takes refractor usage to new depths - as in deep sky!
This compact, rich-field refractor telescope is designed for wide-field observation of nebular clouds, star clusters, and even distant galaxies. The Orion AstroView 120ST Equatorial Refractor Telescope features multi-coated optics and a well-baffled optical tube to ensure good contrast in your views. The refractor telescope optical tube measures just 26" long including the dew shield, so it earns high marks for portability. Not limited to visual use, the fast f/5 optical system makes the AstroView 120ST an excellent refractor telescope to use for wide-field astrophotography in addition to observational astronomy.
The Orion AstroView 120ST EQ Refractor has a big 120mm (4.7") clear aperture for great light gathering and big, bright views. The 120ST refractor telescope's achromatic objective lens has a short focal length of just 600mm (f/5) for exceptional rich-field performance. With the included 25mm Plossl, the AstroView 120ST refractor covers a sprawling 2.1° swath of sky - enough to display the entire Double Cluster of Perseus, Pleiades Cluster, or North America Nebula!
The AstroView 120ST comes with a 6x30 finder scope which lets you accurately aim the refractor anywhere in the sky. The finder features a lightweight, yet sturdy aluminum dovetail bracket with easy two-screw adjustment. Once a simple alignment process is completed, just peer through the finder scope and move the telescope until the cross hairs are centered on the object you want to see. Look in the telescope, and there it is!
Two included 1.25" Sirius Plossl telescope eyepieces provide good, sharp views at 24x (with the 25mm focal length eyepiece) and 60x (with the 10mm focal length eyepiece). Each Sirius Plossl boast a wide, 52° apparent field-of-view. We recommend starting out with the 25mm eyepiece for a wider view, then once you've centered an interesting object, take a closer look by swapping out the 25mm ocular for the more powerful 10mm eyepiece to explore in detail.
A 90° 1.25" mirror star diagonal provides a comfortable angle at night and yields bright views. A diagonal "bends" the light path of a telescope so you can enjoy the view without having to contort yourself into awkward positions to peer into the eyepiece. The cast-metal 2" rack-and-pinion focuser with included step-down 2"-to-1.25" adapter accommodates either a 1.25" or 2" diagonal, so you can use optional 2" gear for an even dreamier wide-field effect! (2" accessories sold separately.)
The AstroView equatorial (EQ) mount provides the stability and smoothness of motion you need for enjoyable wanderings through the heavens. An included polar-axis scope will allow you to achieve polar-alignment quickly and accurately, and manual slow-motion controls let you center objects and track them with minimal effort. To upgrade to motorized tracking, you can add an optional Orion EQ-3M electronic drive for automatic tracking of celestial objects (Orion EQ-3M drive sold separately).
Explore starry skies anytime - even when it's cloudy! The AstroView 120ST Equatorial Refractor Telescope includes a FREE Special Edition download of Starry Night astronomy software. With realistic sky simulations and a many useful features including telescope control, the user-friendly Starry Night Special Edition software will help you plan your observations and understand what you see. Requires PC running Windows 7, 8 or 10. Requires Macintosh running OS X 10.4 or higher. The AstroView 120ST EQ refractor telescope also includes a collimation cap and center-marked primary mirror for easy optical alignment.
Weighs 36.5 lbs. total (optical tube 8 lbs., 9 oz.; mount 28 lbs.).
Limited Warranty against defects in materials or workmanship for one year from date of purchase. This warranty is for the benefit of the original retail purchaser only. For complete warranty details contact us at 800-676-1343.
Please note this product was not designed or intended by the manufacturer for use by a child 12 years of age or younger.
Level 1 Beginner - Suited for a wide range of uses, these telescopes are simple to operate and set up. Some initial assembly may be required. Very good optical and mechanical quality. Great for families, young people, and folks who don't want to mess with equipment but just want to take a look. Any of these scopes will show you countless lunar craters, Saturn's rings and a myriad of star clusters and nebulas! Referring to the manual is recommended.
Level 2 Intermediate - These scopes offer higher performance and more advanced features than Level 1: Beginner models. They typically take a bit longer to learn and need some set-up or adjustments. But anyone with the slightest technical bent will have no problem getting familiar with these models. Referring to the manual is recommended.
Level 3 Advanced - These scopes provide the best performance but may require more skill to master and appreciate. They have exceptionally fine optics and mechanics. Some are easy to use but are but on the large or heavy side. Some are intended for specialized uses. These scopes will appeal to the more technically inclined. Referring to the manual is highly recommended.
Level 4 Expert - Expert telescopes offer uncompromising optical and mechanical quality for the most demanding amateur astronomer. They may be technically involved or designed for specialized use, such as astrophotography or detailed deep sky observation. They carry a premium price, but are designed to provide the ultimate performance in the field. Referring to the manual is highly recommended.
For telescopes, the optical diameter (also known as aperture) is the size of a telescope's main light-collecting lens or primary mirror, measured in millimeters or inches. Telescopes with larger optical diameters collect more light, which leads to an increase in brightness and image resolution compared to smaller instruments.
For binoculars, the optical diameter (also known as objective lens diameter) is the size of each of the front-facing objective lenses of a binocular measured in millimeters. Binoculars with larger objective lenses collect more light, which increases image resolution and brightness. Binoculars with larger objective lenses are recommended for low light situations, and binoculars with at least 50mm or larger objective lenses are recommended for pleasing astronomical observations at night.
Binocular lenses and prisms are often coated with anti-reflective material to minimize light loss as light travels through the multiple optical surfaces of a typical binocular. Coatings help maximize the amount of light transmitted through each glass surface of a binocular, so as much light as possible reaches the observer's eyes to provide a bright and sharp image.
Good lenses are at least "fully coated," with a single layer of magnesium fluoride coating applied to each air-to-glass lens surface. Multiple layers of coatings are even more effective; the term "multi-coated" means one or more air-to-glass lens surface has multiple coatings. "Fully multi-coated" optics are even better, meaning all lens surfaces have multiple layers of anti-reflective coatings applied for maximum light transmission and optimal image quality.
Orion 120mm, f/5 refractor telescope optical tube assembly
25mm Sirius Pl�ssl telescope eyepiece (1.25")
10mm Sirius Pl�ssl telescope eyepiece (1.25")
90� Mirror star diagonal (1.25")
2" - 1.25" telescope eyepiece adapter
Tripod legs
AstroView Equatorial mount
6x30 finder scope
Finder telescope bracket with O-ring
Tube rings
Polar axis finder scope
7.3 lb counterweight
3.8 lb counterweight
Counterweight shaft
Tripod accessory tray
Slow-motion control cables
Dust cap
Polar axis finder scope plastic cover
Accessory tray bracket
Phillips-head screwdriver
Flat-head screwdriver key
Starry Night Special Edition astronomy software download card
Orders received by 1pm Eastern Standard Time for in-stock item the same business day. Order received after noon will ship the next business day. When an item is not in-stock we will ship it as soon as it becomes available. Typically in-stock items will ship first and backordered items will follow as soon as they are available. You have the option in check out to request that your order ship complete, if you'd prefer.
A per-item shipping charge (in addition to the standard shipping and handling charge) applies to this product due to its size and weight. This charge varies based on the shipping method.
Standard Delivery: $0.00Standard Delivery to Canada: $40.003 Day Delivery: $83.002 Day Delivery: $83.00Next Day Delivery: $96.00
How do I align a polar finder?
This procedure is complicated and it is not required for casual observing, but here it goes . . . Remove the cover cap from the front opening in the R.A. axis of the telescope mount. Look through the polar finder at a distant object. Focus the polar finder so that the images and reticle are sharp by rotating the eyepiece end of the finder. Notice that the reticle pattern consists of a crosshair with a circle around the middle. On the circumference of this circle is a tiny circle; this is where Polaris will be placed for accurate polar alignment once the finder is properly aligned. Alignment of the polar finder is best done during the day, before going out into the field at night. Aligning the polar axis finder scope so that it will accurately point at the true north pole is a two-step procedure. First, the polar finder must be rotated in its housing so that the small circle in which Polaris will be placed in is in the proper initial position. Next, the polar axis finder must be adjusted so that it points directly along the mount's R.A. axis. 1. Loosen the R.A. setting circle lock thumb screw, located just above the R.A. setting circle. Rotate the R.A. setting circle until the line above the "0" on the setting circle lines up with the pointed indicator that is cast into the mount. Retighten the thumbscrew. 2. Rotate the date circle until the "0" line on the meridian off-set scale lines up with the time meridian indicator mark. The meridian offset scale is printed on the inner circumference of the date circle, and is labeled "E20" to "W20". The time meridian indicator mark is an engraved line on the exterior of the polar finder's housing. It is on the "ring" of the housing that is closest to the date circle. 3. The R.A. setting circle is labeled in hours, from "0" to "23" (military time). For Northern Hemisphere observers, refer to the top numbers on the setting circle. Each small line represents 10 minutes of R.A. The date circle is labeled from "1" to "12", with each number representing a month of the year ("1" is January, "2" is February, etc.). Each small line represents a two-day increment. 4. Loosen the R.A. lock lever and rotate the mount about the R.A. axis until the March 1 indicating mark (the long line between the "2" and the "3") on the date circle lines up with the 4 PM mark (the long line above the "16") on the R.A. setting circle. You may find it convenient to remove both the counterweights and the telescope optical tube to do this. 5. Now, loosen the three thumbscrews on the polar finder housing and rotate the polar finder so the small circle where Polaris will be centered is located straight down from the intersection of the crosshairs. Retighten the thumbscrews. The polar axis finder scope is now properly set in its initial position. Next, you must align it so that it is exactly parallel to the mount's R.A. axis. 6. Look through the polar finder at a distant object (during the day) and center it in the crosshairs. You may need to adjust the latitude adjustment T-bolts and the tripod position to do this. 7. Rotate the mount 180° about the R.A. axis. Again, it may be convenient to remove the counterweights and optical tube first. 8. Look through the polar finder again. Is the object being viewed still centered on the crosshairs? If it is, then no further adjustment is necessary. If not, then look through the polar finder while rotating the mount about the R.A. axis. You will notice that the object you have previously centered moves in a circular path. Use the three thumbscrews on the housing to redirect the crosshairs of the polar finder to the apparent center of this circular path. Repeat this procedure until the position that the crosshairs point to does not rotate off-center when the mount is rotated in R.A. Once this is accomplished, retighten the thumbscrews. The polar axis finder scope is now ready to be used. When not in use, replace the plastic protective cover to prevent the polar finder from getting bumped, which could knock it out of alignment.
How do I align a finder scope?
Before you use the finder scope, it must be precisely aligned with the telescope so they both point to exactly the same spot. Alignment is easiest to do in daylight, rather than at night under the stars. First, insert a low power telescope eyepiece (a 25mm eyepiece will work great) into the telescope's focuser. Then point the telescope at a discrete object such as the top of a telephone pole or a street sign that is at least a quarter-mile away. Position the telescope so the target object appears in the very center of the field of view when you look into the eyepiece. Now look through the finder scope. Is the object centered on the finder scope's crosshairs? If not, hopefully it will be visible somewhere in the field of view, so only small turns of the finder scope bracket's alignment thumb screws will be needed. Otherwise you'll have to make larger turns to the alignment thumb screws to redirect the aim of the finder scope. Use the alignment thumb screws to center the object on the crosshairs of the finder scope. Then look again into the telescope's eyepiece and see if it is still centered there too. If it isn't, repeat the entire process, making sure not to move the telescope while adjusting the alignment of the finder scope. Finder scopes can come out of alignment during transport or when removed from the telescope, so check its alignment before each observing session.
How do I focus the finder scope?
If, when looking through the finder scope, you notice that the image is fuzzy, you will need to focus the finder scope for your eyes. Different finder scopes focus differently; most Orion finder scopes include a lock ring near the objective and focus as follows:
1. Loosen the lock ring that is located behind the finder's objective lens cell
2. Screw the objective lens cell in or out until the image appears sharp.
3. Tighten the lock ring behind the lens cell. If there is no lock ring the finder scope is focused by rotating the eyepiece.
Once the finder scope is now focused it should not need focusing again for your eyes..
Can the finder scope crosshairs be adjusted?
Yes, but before taking this on, regardless of the orientation, the intersection of the crosshairs marks the center and that's what important. However, should you feel the need to change the orientation of the finder scope's crosshairs; you can do so by carefully rotating the finder scope in its bracket. Loosen the adjustment screws or pull on the tensioner (depending on the model) and rotate the finder scope tube in the bracket until the crosshairs are oriented the way you want. You should not need to rotate the finder scope tube more than 1/4 of a turn. For right-angle finder scopes, unthread the eyepiece to re-orient the crosshairs; gently turn the eyepiece until the crosshairs are oriented as you wish. You should not need to rotate the eyepiece more than 1/4 of a turn to do this. This may leave you with a loose eyepiece. If so, you can add an o-ring or shim to tighten it at the new orientation.
How do I calculate the magnification (power) of a telescope?
To calculate the magnification, or power, of a telescope with an eyepiece, simply divide the focal length of the telescope by the focal length of the eyepiece. Magnification = telescope focal length ÷ eyepiece focal length. For example, the Orion Astroview 120mm EQ Refractor Telescope, which has a focal length of 600mm, used in combination with the supplied 25mm eyepiece, yields a power of: 600 ÷ 25 = 24x.
It is desirable to have a range of telescope eyepieces of different focal lengths to allow viewing over a range of magnifications. It is not uncommon for an observer to own five or more eyepieces. Orion offers many different eyepieces of varying focal lengths.
Every telescope has a theoretical limit of power of about 50x per inch of aperture (i.e. 240x for the Orion Astroview 120mm Refractor). Atmospheric conditions will limit the usefullness of magnification and cause views to become blurred. The highest useful magnification of a telescope of the Orion Astroview 120mm is 300x. Claims of higher power by some telescope manufacturers are a misleading advertising gimmick and should be dismissed. Keep in mind that at higher powers, an image will always be dimmer and less sharp (this is a fundamental law of optics). With every doubling of magnification you lose half the image brightness and three-fourths of the image sharpness. The steadiness of the air (the "seeing") can also limit how much magnification an image can tolerate. Always start viewing with your lowest-power (longest focal length) eyepiece in the telescope. It's best to begin observing with the lowest-power eyepiece, because it will typically provide the widest true field of view, which will make finding and centering objects much easier After you have located and centered an object, you can try switching to a higher-power eyepiece to ferret out more detail, if atmospheric conditions permit. If the image you see is not crisp and steady, reduce the magnification by switching to a longer focal length eyepiece. As a general rule, a small but well-resolved image will show more detail and provide a more enjoyable view than a dim and fuzzy, over-magnified image.
What are practical focal lengths to have for eyepieces for my telescope?
To determine what telescope eyepieces you need to get powers in a particular range with your telescope, see our Learning Center article: How to choose Telescope Eyepieces
Why do Orion telescopes have less power than the telescope at department stores?
Advertising claims for high magnification of 400X, 600X, etc., are very misleading. The practical limit is 50X per inch of aperture, or 120X for a typical 60mm telescope. Higher powers are useless, and serve only to fool the unwary into thinking that magnification is somehow related to quality of performance. It is not.
How do I get started with astronomical viewing?
When choosing a location for nighttime stargazing, make it as far away from city lights as possible. Light-polluted skies greatly reduce what can be seen with the telescope. Also, give your eyes at least 20 minutes to dark-adapt to the night sky. You'll be surprised at how many more stars you will see! Use a red flashlight, to see what you're doing at the telescope, or to read star charts. Red light will not spoil your dark-adapted night vision as readily as white light will. To find celestial objects with your telescope, you first need to become reasonably familiar with the night sky. Unless you know how to recognize the constellation Orion, for instance, you won't have much luck locating the Orion Nebula. A simple planisphere, or star wheel, can be a valuable tool for learning the constellations and seeing which ones are visible in the sky on a given night. A good star chart or atlas, like the Orion DeepMap 600, can come in handy for helping locate interesting objects among the dizzying multitude of stars overhead. Except for the Moon and the brighter planets, it is pretty time-consuming and frustrating to hunt for objects randomly, without knowing where to look. It is best to have specific targets in mind before you begin looking through the eyepiece. Practice makes perfect. After a few nights, this will begin to "click" and star-hopping will become easier. See our Learning Center articles: About General Astronomy
How big a telescope do I need?
For viewing craters on the Moon, the rings of Saturn, and Jupiter with its four bright moons, a 60mm or 70mm refractor or a 3-inch reflector telescope does a good job. An 80mm to 90mm refractor or 4.5-inch or 6-inch reflector will show more planetary and lunar detail as well as glowing nebulas and sparkling star clusters. Under dark, non-light-polluted skies, a big scope—8-inch diameter or more—will serve up magnificent images of fainter clusters, galaxies, and nebulas. The larger the telescope, the more detail you will see. But don't bite off more than you can chew, size-wise. Before you buy, consider carefully a telescope's size and weight. Make sure you can comfortably lift and transport it, and that you have room indoors to store it. For more detailed information on this topic see our Learning Center article: Choosing a Telescope for Astronomy - The long Version
Why would I want a manual scope when I can get a Go-To scope?
For the novice stargazer, buying a computer-controlled telescope with a small aperture puts a lot of money into the mechanical and database components of the telescope to locate objects that you can't see with the optics of the telescope. Someone who is inexperienced with astronomy and night sky will spend their time pouring over instruction manuals and text scrolling across a screen instead of exploring the night sky, studying the stars and their patterns and learning how to locate to binary stars and nebula. Our advice . . .go for bigger aperture.
What causes dim or distorted images?
Too much magnification
Keep in mind that at higher powers, an image will always be dimmer and less sharp (this is a fundamental law of optics). The steadiness of the air, the seeing, can also limit how much magnification an image can tolerate. Always start viewing with your lowest-power (longest focal length) eyepiece in the telescope. It's best to begin observing with the lowest-power eyepiece, because it will typically provide the widest true field of view, which will make finding and centering objects much easier After you have located and centered an object, you can try switching to a higher-power eyepiece to ferret out more detail, if atmospheric conditions permit. If the image you see is not crisp and steady, reduce the magnification by switching to a longer focal length telescope eyepiece. As a general rule, a small but well-resolved image will show more detail and provide a more enjoyable view than a dim and fuzzy, over-magnified image. As a rule of thumb, it is not recommended to exceed 2x per mm of aperture.
Atmospheric conditions aren't optimal.
Atmospheric conditions vary significantly from night to night, even hour to hour . "Seeing" refers to the steadiness of the Earth's atmosphere at a given time. In conditions of poor seeing, atmospheric turbulence causes objects viewed through the telescope to "boil." If, when you look up at the sky with just your eyes, the stars are twinkling noticeably, the seeing is bad and you will be limited to viewing with low powers (bad seeing affects images at high powers more severely). Seeing is best overhead, worst at the horizon. Also, seeing generally gets better after midnight, when much of the heat absorbed by the Earth during the day has radiated off into space. It's best, although perhaps less convenient, to escape the light-polluted city sky in favor of darker country skies.
Viewing through a glass window open or closed.
Avoid observing from indoors through an open (or closed) window, because the temperature difference between the indoor and outdoor air, reflections and imperfections in the glass, will cause image blurring and distortion.
Telescope not at thermal equilibrium.
All optical instruments need time to reach "thermal equilibrium." The bigger the instrument and the larger the temperature change, the more time is needed. Allow at least a half-hour for your telescope to cool to the temperature outdoors. In very cold climates (below freezing), it is essential to store the telescope as cold as possible. If it has to adjust to more than a 40 degrees temperature change, allow at least one hour. Time to adjust varies depending on the scope type and aperture.
Make sure you are not looking over buildings, pavement, or any other source of heat, which will radiate away at night, causing "heat wave" disturbances that will distort the image you see through the telescope.
Does the atmosphere play a role in how good the quality of the image will be?
Atmospheric conditions play a huge part in quality of viewing. In conditions of good "seeing", star twinkling is minimal and objects appear steady in the eyepiece. Seeing is best over-head, worst at the horizon. Also, seeing generally gets better after midnight, when much of the heat absorbed by the Earth during the day has radiated off into space. Typically, seeing conditions will be better at sites that have an altitude over about 3000 feet. Altitude helps because it decreases the amount of distortion causing atmosphere you are looking through. A good way to judge if the seeing is good or not is to look at bright stars about 40 degrees above the horizon. If the stars appear to "twinkle", the atmosphere is significantly distorting the incoming light, and views at high magnifications will not appear sharp. If the stars appear steady and do not twinkle, seeing conditions are probably good and higher magnifications will be possible. Also, seeing conditions are typically poor during the day. This is because the heat from the Sun warms the air and causes turbulence. Good "transparency" is especially important for observing faint objects. It simply means the air is free of moisture, smoke, and dust. These tend to scatter light, which reduces an object's brightness. One good way to tell if conditions are good is by how many stars you can see with your naked eye. If you cannot see stars of magnitude 3.5 or dimmer then conditions are poor. Magnitude is a measure of how bright a star is, the brighter a star is, the lower its magnitude will be. A good star to remember for this is Megrez (mag. 3.4), which is the star in the "Big Dipper" connecting the handle to the "dipper". If you cannot see Megrez, then you have fog, haze, clouds, smog, light pollution or other conditions that are hindering your viewing. Another hint: Good seeing can vary minute to minute. Watch the planets for a while to pick-up those moments of good seeing.
How long will it take my eyes to dark adapt?
Do not expect to go from a lighted house into the darkness of the outdoors at night and immediately see faint nebulas, galaxies, and star clusters—or even very many stars, for that matter. Your eyes take about 30 minutes to reach perhaps 80 percent of their full dark-adapted sensitivity. Many observers notice improvements after several hours of total darkness. As your eyes become dark-adapted, more stars will glimmer into view and you will be able to see fainter details in objects you view in your telescope. So give yourself at least a little while to get used to the dark before you begin observing. To see what you are doing in the darkness, use a red light flashlight rather than a white light. Red light does not spoil your eyes' dark adaptation like white light does. A flashlight with a red LED light is ideal, or you can cover the front of a regular flashlight with red cellophane or paper. Beware, too, that nearby porch and streetlights and automobile headlights will spoil your night vision. Your eyes can take at least 1/2 hour to re-adjust.
How do I see the best detail on the surface of the Moon?
The Moon, with its rocky, cratered surface, is one of the easiest and most interesting subjects to observe with your telescope. The myriad craters, rilles, and jagged mountain formations offer endless fascination. The best time to observe the Moon is during a partial phase, that is, when the Moon is not full. During partial phases, shadows cast by crater walls and mountain peaks along the border between the dark and light portions of the lunar disk highlight the surface relief. A full Moon is too bright and devoid of surface shadows to yield a pleasing view. Try using an Orion Moon filter to dim the Moon when it is too bright; it simply threads onto the bottom of the eyepiece, you'll see much more detail.
How do I best view Deep-Sky Objects?
Most deep-sky objects are very faint, so it is important that you find an observing site well away from light pollution. Take plenty of time to let your eyes adjust to the darkness. Don't expect these objects to appear like the photographs you see in books and magazines; most will look like dim gray "ghosts." (Our eyes are not sensitive enough to see color in deep-sky objects except in few of the brightest ones.) But as you become more experienced and your observing skills improve, you will be able to coax out more and more intricate details. And definitely use your low-power telescope eyepieces to get a wide field-of-view for the largest of the deep-sky objects.
What will the planets look like through the telescope?
The planets don't stay put like stars do (they don't have fixed R.A. and Dec. coordinates), so you will need to refer to the Orion Star Chart on our website. Venus, Mars, Jupiter, and Saturn are among the brightest objects in the sky after the Sun and the Moon. All four of these planets are not normally visible in the sky at one time, but chances are one or two of them will be.
JUPITER: The largest planetJupiter, is a great subject to observe. You can see the disk of the giant planet and watch the ever-changing positions of its four largest moons, Io, Callisto, Europa, and Ganymede. If atmospheric conditions are good, you may be able to resolve thin cloud bands on the planet's disk.
SATURN: The ringed planet is a breathtaking sight when it is well positioned. The tilt angle of the rings varies over a period of many years; sometimes they are seen edge-on, while at other times they are broadside and look like giant "ears" on each side of Saturn's disk. A steady atmosphere (good seeing) is necessary for a good view. You may probably see a tiny, bright "star" close by; that's Saturn's brightest moon, Titan.
VENUS: At its brightest, Venus is the most luminous object in the sky, excluding the Sun and the Moon. It is so bright that sometimes it is visible to the naked eye during full daylight! Ironically, Venus appears as a thin crescent, not a full disk, when at its peak brightness. Because it is so close to the Sun, it never wanders too far from the morning or evening horizon. No surface markings can be seen on Venus, which is always shrouded in dense clouds. Sometimes using a color filter will lessen the glare of Venus and help you see the crescent.
MARS: If atmospheric conditions are good, you may be able to see some subtle surface detail on the Red Planet, possibly even the polar ice cap. Mars makes a close approach to Earth every two years; during those approaches its disk is larger and thus more favorable for viewing. For more detailed information on this topic see our Learning Center article: What Will You See Through a Telescope
How do I Find Deep-sky Objects: Starhopping?
Starhopping, as it is called by astronomers, is perhaps the simplest way to hunt down objects to view in the night sky. It entails first pointing the telescope at a star close to the object you wish to observe, and then progressing to other stars closer and closer to the object until it is in the field of view of the eyepiece. It is a very intuitive technique that has been employed for hundreds of years by professional and amateur astronomers alike. Keep in mind, as with any new task, that starhopping may seem challenging at first, but will become easier over time and with practice. To starhop, only a minimal amount of additional equipment is necessary. A star chart or atlas that shows stars to at least magnitude 5 is required. Select one that shows the positions of many deep-sky objects, so you will have a lot of options to choose from. If you do not know the positions of the constellations in the night sky, you will need to get a planisphere to identify them. Start by choosing bright objects to view. The brightness of an object is measured by its visual magnitude; the brighter an object, the lower its magnitude. Choose an object with a visual magnitude of 9 or lower. Many beginners start with the Messier objects, which represent some of the best and brightest deep-sky objects, first catalogued about 200 years ago by the French astronomer Charles Messier. Determine in which constellation the object lies. Now, find the constellation in the sky. If you do not recognize the constellation on sight, consult a planisphere. The planisphere gives an all-sky view and shows which constellations are visible on a given night at a given time. Now look at your star chart and find the brightest star in the constellation that is near the object that you are trying to find. Using the finder scope, point the telescope at this star and center it on the crosshairs Next, look again at the star chart and find another suitably bright star near the bright star currently centered in the finder. Keep in mind that the field of view of the finder scope is between 5-deg - 7-deg, so you should choose a star that is no more than 7-deg from the first star, if possible. Move the telescope slightly, until the telescope is centered on the new star. Continue using stars as guideposts in this way until you are the approximate position of the object you are trying to find. Look in the telescope's eyepiece, and the object should be somewhere within the field of view. If it's not, sweep the telescope carefully around the immediate vicinity until the object is found. If you have trouble finding the object, start the starhop again from the brightest star near the object you wish to view. This time, be sure the stars indicated on the star chart are in fact the stars you are centering in the finder scope and telescope eyepiece. Remember the telescope and the finder scope will give you inverted images (unless you are using a correct image finder scope), keep this in mind when you are starhopping from star to star. Observing Hint: Always use your lowest powered eyepiece in your telescope when starhopping . This will give you the widest possible field of view.
Can I wear my glasses when using a telescope?
If you wear eyeglasses, you may be able to keep them on while you observe, if your telescope eyepieces have enough "eye relief" to allow you to see the whole field of view. You can find out by looking through the eyepiece first with your glasses on and then with them off, and see if the glasses restrict the view to only a portion of the full field. If they do, you can easily observe with your glasses off by just refocusing the telescope the needed amount. If your eyes are astigmatic, images will probably appear the best with glasses on. This is because a telescope's focuser can accommodate for nearsightedness or farsightedness, but not astigmatism. If you have to wear your glasses while observing and cannot see the entire field of view, you may want to purchase additional eyepieces that have longer eye relief.
What will a star look like through a telescope?
Stars will appear like twinkling points of light in the telescope. Even the largest telescopes cannot magnify stars to appear as anything more than points of light. You can, however, enjoy the different colors of the stars and locate many pretty double and multiple stars. The famous "Double-Double" in the constellation Lyra and the gorgeous two-color double star Albireo in Cygnus are favorites. Defocusing the image of a star slightly can help bring out its color. For more detailed information on this topic see our Learning Center article: Stars and Deep Sky Objects
Is there an eyepiece available that will rotate the image so that it can be used for scenic viewing?
We carry correct-image prism diagonals which provide right-side up non-reversed images in refractor and cassegrain telescopes. It is not possible to correct the image orientation in a reflector telescope.
How do I clean any of the optical lenses?
Any quality optical lens cleaning tissue and optical lens cleaning fluid specifically designed for multi-coated optics can be used to clean the exposed lenses of your eyepieces or finder scope. Never use regular glass cleaner or cleaning fluid designed for eyeglasses. Before cleaning with fluid and tissue, blow any loose particles off the lens with a blower bulb or compressed air. Then apply some cleaning fluid to a tissue, never directly on the optics. Wipe the lens gently in a circular motion, then remove any excess fluid with a fresh lens tissue. Oily finger-prints and smudges may be removed using this method. Use caution; rubbing too hard may scratch the lens. On larger lenses, clean only a small area at a time, using a fresh lens tissue on each area. Never reuse tissues.
How do I Polar Align an Equatorial Mount?
For Northern Hemisphere observers, approximate polar alignment is achieved by pointing the mount's R.A. axis at the North Star, or Polaris. It lies within 1° of the north celestial pole (NCP), which is an extension of the Earth's rotational axis out into space. Stars in the Northern Hemisphere appear to revolve around Polaris..
To find Polaris in the sky, look north and locate the pattern of the Big Dipper. The two stars at the end of the "bowl" of the Big Dipper point right to Polaris. Observers in the Southern Hemisphere aren't so fortunate to have a bright star so near the south celestial pole (SCP). The star Sigma Octantis lies about 1° from the SCP, but it is barely visible with the naked eye (magnitude 5.5)..
For general visual observation, an approximate polar alignment is sufficient: 1. Level the equatorial mount by adjusting the length of the three tripod legs.
2. Loosen one of the latitude adjusting T-bolts and tighten the other to tilt the mount until the pointer on the latitude scale is set at the latitude of your observing site. This may vary depending on the mount, some have one bolt and a tightening screw instead. If you don't know your latitude, consult a geographical atlas to find it. For example, if your latitude is 35° North, set the pointer to +35. The latitude setting should not have to be adjusted again unless you move to a different viewing location some distance away.
3. Loosen the Dec. lock lever and rotate the telescope optical tube until it is parallel with the R.A. axis. The pointer on the Dec. setting circle should read 90-deg. Retighten the Dec. lock lever.
4. Move the tripod so the telescope tube (and R.A. axis) points roughly at Polaris. If you cannot see Polaris directly from your observing site, consult a compass and rotate the tripod so the telescope points north. Using a compass is a less desirable option, a compass points about 16° away from true north and requires you to compensate foe accurate polar alignment.
The equatorial mount is now approximately polar-aligned for casual observing. More precise polar alignment is required for astrophotography and for use of the manual setting circles. From this point on in your observing session, you should not make any further adjustments to the latitude of the mount, nor should you move the tripod. Doing so will undo the polar alignment. The telescope should be moved only about its R.A. and Dec. axes.
How do I point the telescope on an Equatorial Mount?
Beginners occasionally experience some confusion about how to point the telescope overhead or in other directions. At the zenith: You want to view an object that is directly overhead, at the zenith. DO NOT make any adjustment to the latitude adjustment T-bolts. That will spoil the mount's polar alignment. Remember, once the mount is polar aligned, the telescope should be moved only on the R.A. and Dec. axes. To point the scope overhead, first loosen the R.A. lock lever and rotate the telescope on the R.A. axis until the counterweight shaft is horizontal (parallel to the ground). Then loosen the Dec. lock lever and rotate the telescope until it is pointing straight overhead. The counterweight shaft is still horizontal. Then retighten both lock levers. Directly north at an object that is nearer to the horizon than Polaris: You can't do it with the counterweight down. You have to rotate the scope in R.A. so that the counterweight shaft is positioned horizontally. Then rotate the scope in Dec. so it points to where you want it near the horizon. Directly south: The counterweight shaft should again be horizontal. Then you simply rotate the scope on the Dec. axis until it points in the south direction. East or west: To point the telescope to the east or west, or in other directions, you rotate the telescope on its R.A. and Dec. axes. Depending on the altitude of the object you want to observe, the counterweight shaft will be oriented somewhere between vertical and horizontal. Another hint: On some smaller scopes the RA slow-motion shaft can get in the way of some orientations. If this occurs, simply remove the slow-motion knobs and re-attach to the other side of the RA axis.
How do I track Celestial Objects with an Equatorial Mount?
When you observe a celestial object through the telescope, you'll see it drift slowly across the field of view. To keep it in the field, if your equatorial mount is polar-aligned, just turn the R.A. slow-motion control. The Dec. slow-motion control is not needed for tracking, but may be required to center the object. Objects will appear to move faster at higher magnifications, because the field of view is narrower. A DC motor drive system can be mounted on all Orion equatorial mounts to provide hands-free tracking. Motor drive systems are typically offered as an optional accessory. Objects will then remain stationary in the field of view without any manual adjustment of the R.A. slow-motion control. A dual-axis motor drive is necessary for astrophotography.
What is the advantage of a dual axis electronic drive over a single axis drive?
A dual axis drive motorizes both axes of motion of the equatorial mount. It provides the basic tracking function as well as fine control of the telescope position in any direction. A dial axis system comes in especially handy foot observing at high powers and is a must for long-exposure astrophotography.
What are the Setting Circles and what do they do?
The setting circles on an equatorial mount enable you to locate celestial objects by their "celestial coordinates". Every object resides in a specific location on the "celestial sphere". That location is denoted by two numbers: its right ascension (R.A.) and declination (Dec.). In the same way, every location on Earth can be described by its longitude and latitude. R.A. is similar to longitude on Earth, and Dec. is similar to latitude. The R.A. and Dec. values for celestial objects can be found in any star atlas or star catalog. The R.A. setting circle is scaled in hours, from 1 through 24, with small marks in between representing 10 minute increments (there are 60 minutes in 1 hour of R.A.). The upper set of numbers apply to viewing in the Northern Hemisphere, while the numbers below them apply to viewing in the Southern Hemisphere. The Dec. setting circle is scaled in degrees, with each mark representing 2-deg increments. Values of Dec. coordinates range from +90-deg to -90-deg. The 0-deg mark indicates the celestial equator. When the telescope is pointed north of the celestial equator, values of the Dec. setting circle are positive, while when the telescope is pointed south of the celestial equator, values of the Dec. setting circle are negative. So, the coordinates for the Orion Nebula listed in a star atlas will look like this: R.A. 5h 35.4m Dec. -5-deg 27' That's 5 hours and 35.4 minutes in right ascension, and -5 degrees and 27 arc-minutes in declination (there are 60 arc-minutes in 1 degree of declination). Before you can use the setting circles to locate objects, the mount must be well polar aligned, and the R.A. setting circle must be calibrated. The Dec. setting circle has been calibrated at the factory, and should read 90-deg whenever the telescope optical tube is parallel with the R.A. axis.
How do I find objects with the setting circles?
Look up in a star atlas the coordinates of an object you wish to view. 1. Loosen the Dec. lock lever and rotate the telescope until the Dec. value from the star atlas matches the reading on the Dec. setting circle. Remember that values of the Dec. setting circle are positive when the telescope is pointing north of the celestial equator (Dec. = 0-deg), and negative when the telescope is pointing south of the celestial equator. Retighten the lock lever. 2. Loosen the R.A. lock lever and rotate the telescope until the R.A. value from the star atlas matches the reading on the R.A. setting circle. Remember to use the upper set of numbers on the R.A. setting circle. Retighten the lock lever. The lower set is for the Southern Hemisphere. Most setting circles are not accurate enough to put an object dead-center in the telescope's eyepiece, but they should place the object somewhere within the field of view of the finder scope, assuming the equatorial mount is accurately polar aligned. Use the slow-motion controls to center the object in the finder scope, and it should appear in the telescope's field of view. The R.A. setting circle must be re-calibrated every time you wish to locate a new object. Do so by calibrating the setting circle for the centered object before moving on to the next one.
When I use my motor drive, the moon drifts from the field of view.
The moon moves at a slightly slower rate from East to West than sidereal rate, so the motor speed needs to be reduced. If it North or South, the polar alignment should be checked.
Is there an image quality difference between a short-tube and long-tube?
Short refractors have more visible chromatic aberration than long refractors. You're likely to see purple or orange halos around bright planets and the lunar limb. With short reflectors, "coma" comes into play: stars appear like "commas" or "seagulls" near the edge of the eyepiece field. For most people, a little color fringing or coma is no big deal. These aberrations are less noticeable at low magnifications, which is one reason not to push the power higher than about 100x in most short-tube telescopes. High-end short-tubes made with exotic glasses or with corrector lenses can handle higher power. For more detailed information on this topic see our Learning Center article: Short Tube vs Long Tube- What's the Difference
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Online or in your mailbox. Check out our colorful catalog, filled with hundreds of quality products.
Please send me email about sales, new products, and astronomy.
Since 1975 Orion Telescopes & Binoculars has been offering telescopes for sale direct to customers, with an unswerving commitment to best quality products, value and unmatched customer care. Our 100% satisfaction guarantee says it all.
Orion offers telescopes for every level: Beginner, Intermediate, Advanced, and Expert. From our entry level beginner telescopes for amateur astronomers to our Dobsonian telescopes to our most advanced Cassegrain telescopes and accessories, you can find the best telescope for you. Because we sell direct, we can offer you tremendous value at a great price. Not sure how to choose a telescope? Orion's Telescope Buyer's Guide is a great place to start.
Orion binoculars are known for quality optics at a great price. We offer binoculars for every viewing interest, including astronomical binoculars, compact binoculars, waterproof binoculars, birding binoculars, and sport and hunting binoculars.
Orion's telescope and astrophotography accessories will enhance your telescope enjoyment without breaking the bank. Expand your viewing experience with accessories ranging from moon filters to power-boosting Barlow lenses to advanced computerized telescope mounts. Capture breathtaking photos with our affordable astrophotography cameras. And when you're stargazing, Orion's telescope cases and covers, observing gear, red LED flashlights, astronomy books and star charts will make your observing sessions more convenient, comfortable and meaningful.
At Orion, we are committed to sharing our knowledge and passion for astronomy and astrophotography with the amateur astronomy community. Visit the Orion Community Center for in-depth information on telescopes, binoculars, and astrophotography. You can find astrophotography "how to" tips and share your best astronomy pictures here. Submit astronomy articles, events, & reviews, and even become a featured Orion customer!


text:
In a video that covers a wide range of lip-synched performances of the tune from sassy to silly, their fellow artists show Little Big Town and "Pontoon" some love with their unique interpretations of the song that has quickly coasted up the charts.
The all-star cast includes the quartet's labelmates Darius Rucker, Luke Bryan and Lady Antebellum, along with Carrie Underwood (performing it live in concert), Wynonna, Pistol Annies, Charlie Daniels, Sara Evans, Jake Owen, Hunter Hayes and more.
Click ***HERE*** to watch!

subset: commoncrawl


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So how many chances do we get? How many mistakes are we allowed to make? At what time does our Character start to erode beyond the point of repair?
These are questions that are always out there.. but no one seems to want to answer. In our society today it seems that we are willing to give chance after chance with no expectation of demonstrating good character.
We allow athletes, movie stars, musicians, and other folks in the lime light opportunity after opportunity to "make things right" and the message that we send is "Anything goes, don't worry about consequences". You can get away with anything as long as you say you are sorry.
I spent some time in Southwest Asia, justice is swift and unforgiving there. Consequences are dire and without remorse. I am not suggesting we should be that harsh, but at what point do we start to worry about the erosion of the character of the people of our country.
We see politicians that lie, cheat, and steal from our country.. only to be reelected. We see rock stars that are clearly into a life style that I would not want my kids to live. Money is the answer.. "Well, they make millions, they are exempt…. or cool" What's the message?
Now before anyone says that I am ranting on the rich and famous.. NO I AM NOT… I am ranting on the general public that allows the erosion of character to happen. It is our fault for letting this happen and we need to wake up.
Mike Vic kills dogs for eight years.. In Philadelphia, number 7 Jersey's are the number one selling jersey. WHY? The University of Oregon is pushing to reinstate a player that demonstrated a terrible lack of judgement, not only at a game, but being suspended from practice and many off the field infractions. WHY? Brittany Spears is in and out of rehab, seemingly not bucking for mom of the year, but her concerts are full and record sales up. WHY? And let's not get into politics. I googled "Political Scandal… Page after page of politicians that should all be in jail.
The point here is how many chances do we give? What is kind of mistakes are we allowed to make, especially if we have no intent on learning from them and doing better? And how far are we going to let our Character slip?
You need to answer these questions.. Each of you.
Live the Scout Oath and Law.
Have a Great Scouting Day!
Mistakes, Chances, and Chipping away at Character
So how many chances do we get? How many mistakes are we allowed to make? At what time does our Character start to erode beyond the point of repair?


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Binghamton University professor leads national public affairs organization
BINGHAMTON, NY – Binghamton University faculty member, Nadia Rubaii-Barrett, is now serving as the 2011-12 president of the National Association of Schools of Public Affairs and Administration (NASPAA).
"It's exciting and really quite humbling," said Rubaii-Barrett, an associate professor of public administration. "Some of the people who have been past NASPAA presidents are prominent individuals in our field who I put on a pedestal. In that sense, it's a little daunting to be in the same position as people you hold in very high regard."
NASPAA is an international membership organization of programs in public administration, public policy and public affairs. Its 280 members confer more than 10,000 master's degrees annually. NASPAA's mission is to ensure excellence in public service education and promote the ideal of public service. It also serves as the accrediting body for master's programs in public affairs. More than half of its member programs are accredited.
Rubaii previously served on NASPAA's Executive Council and chaired the Commission on Peer Review and Accreditation.
"Nadia has been a leader in the public affairs education community for almost 15 years," NASPAA Executive Director Laurel McFarland said. "We are honored to have someone with her experience and commitment to educating the next generation of public sector professionals, and to social equity, as our president."
The position carries a great amount of time and subject commitment. Besides teaching her regular classes, Rubaii conducts conference calls with the association's executive committee and speaks with McFarland by phone at least two to three times per week. Rubaii also uses Skype to oversee several task forces and works to draft various proposals.
"This is when you have the opportunity to really shape the agenda and priorities for the association," she said. "I don't want this to be a year of being a place-holder. I want to go out on a limb and say what we need to be doing. I'm only going to have one opportunity to make a mark on what the association does."


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Improv Comedy at the Uptown TheaterLocation: Uptown Theater at Myrtle Beach Mall
Come out to the Uptown Theater located at Myrtle Beach Mall for some completely made up laughs! Based on the styling of the hit TV show 'Whose Line is it Anyway', Carolina Improv brings you two different shows entitled "Whose Beach Is It Anyway" and "Who's Night Out is It Anyway".
All shows begin at 7:30. Tickets are available at the door or online at http://www.carolinaimprov.com/Next Date:


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Despite what my biographers here on POTUS say, I still hold to many conservative values. The problem is, there has been NO party of candidate that upholds them. Who has been fiscally responsible lately? Bush? (I won't even mention Obama) The current or recent republican congress? (I won't even mention the recent democratic congress)
Really? Besides Ron Paul, who do you see coming close to making the necessary budget cuts to bring our financial house under control?
All the non-military, non-entitlement spending COMBINED, even if cut drastically, will not be enough.
I will respectfully disagree on another point. The crowd at CPAC IS the conservative voice. Heckles and jeers should not be dismissed. Especially if its not just one isolated voice, but many. Also, if the mainstream GOP was living up to its conservative principles, do you think the TeaParty would even exist in its current form and strength?
I think I've raised some valid questions. I hope they don't just generate personal attacks that add nothing to the discussion. (not you, we've had many good discussions here)


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Log In now to add this Gigapan to a group gallery.
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About This GigapanToggle
- Taken by
- Explore score
- 2
- Size
- 0.10 Gigapixels
- Views
- 16024
- Date added
- Nov 14, 2008
- Date taken
- Nov 13, 2008
- Categories
- Galleries
- Mars, Astrology and Space ...MARS
- Competitions
- Tags
- nasa, mars, mer, rover, spirit, columbia, hills
- Description
This stunning image mosaic of the "Columbia Hills" is the first 360-degree panorama taken since the Mars Exploration Rover Spirit arrived at the hills over a month ago. The rover has been busy studying the rocks here, which show evidence of past alteration by water. The dark patch of soil to the right is the spot where Spirit stopped for engineering work on its right front wheel. Spirit's tracks can be followed from there all the way back to "Bonneville Crater" and the original landing site, more than 3 kilometers (1.86 miles) away.
This approximate true-color image, nicknamed the "Cahokia panorama" after the Native American archaeological site near St. Louis, was acquired between sols 213 to 223 (Aug. 9 to 19, 2004). The panorama consists of 470 images acquired through six panoramic camera filters (750 to 480 nanometers). It took until the week of sol 237 (Sept. 2) to downlink all the data back to Earth. Several more weeks of image processing and geometric mapping by team members at Jet Propulsion Laboratory, Pasadena, Calif., and Cornell University, Ithaca, N.Y., were required to stitch all the images together into this spectacular mosaic.
Image credit: NASA/JPL/Cornell


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Sportscasters highlighted in Boston Globe
July 08, 2013
July 08, 2013
In a July 8 article, the Boston Globe featured the growing successes of students in the Journalism Department pursuing sports journalism.
Janet Kolodzy, journalism professor and internship coordinator whose students frequently intern at ESPN, NESN, and WEEI radio said, "We have an under-the-radar and consistently strong program."
With ample internship and work opportunities in the sports-dominated city of Boston, students are armed with hands-on instruction from professors in the field. John Rooke, part-time faculty member and an ESPN sportscaster, stresses the importance of knowing online formats such as podcasts and the strengths of social media.
Ross Lippman '13 was recently named the Sportscasters Talent Agency of America's top collegiate sports broadcaster, also known as the Jim Nantz award. He attributed his success to his training in the journalism program, calling it, "Emerson's best-kept secret." Two other Emerson students are ranked in the top 20.
Read the Boston Globe article online, or download the PDF »
View the Boston Globe video slideshow »


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Size matters.
There is no shame in liking a little extra padding around your bars. We've lost count of the number of pro bikes we've seen with double-wrapped bars, ready to tackle the spring classics. And for those who dislike wearing cycling gloves, a nicely padded handlebar is de rigueur. Lizard Skins DSP 2.5 Handlebar Tape offers the same super grip that the 1.8 variation does, but with the added comfort of 0.8mm more padding.
Now, 0.8mm might not sound like a lot, and indeed Lizard Skins is careful not to give it a foamy, slightly blundering feel. It's just a whisper of extra padding, but it could make the difference between numb hands and all day comfort. The DSP 2.5 Bar Tape shares the same high tech feel that their 1.8 tape has, but with a different design pattern. In fact, if you take a close look, it resembles a file tread pattern like you might see on an all-weather road tire. It has more texture than other tapes we've used, and that's not by accident. The tape is intended to facilitate the movement of your hands form one position to the other, but there is no hint of unwanted slip, even with ungloved hands.
Each roll of tape is 82 inches long, so you'll be able to wrap your bars without having to resort to overly pulling and stretching the tape. In fact, that is something that the folks at Lizard Skins are keen to caution you against doing. Be firm in pressing the tape into place and space it evenly, but don't pull at it too much because that will reduce its durability.
Lizard Skins DSP 2.5 Handlebar Tape comes in Black, Blue, Green, Orange, Red, and White. The package includes 2 rolls of tape, 2 bar-end plugs, and 2 finishing strips. Its claimed weight is only 50 grams per set, which means even weight-weenies can get the ultimate comfort without sacrificing a gram.
- 0.8mm more padding than Lizard Skin's 1.8 tape
- File tread pattern
- 82 inches long
- Package includes 2 rolls of tape, 2 bar-end plugs, and 2 finishing strips
Tech Specs
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Reviews & Community
Worst tape I ever bought
After 30 rides the bar tape started to show white spots. For a tape this expensive, I expected a lot more life from it. I like the feel of the tape, but that does not make up for such a short life. I emailed lizard skins twice to inform them of this problem, but both went unanswered. If this is how a company treats and feels about their customers......I'd rather move on and continue to support fizik which I've never had an issue with. Stay away at all costs, do not buy this tape.
Lizard Skinz 2.5 Bar Tape
- Familiarity: I've put it through the wringer
White wear spots appearing after 6 weeks of riding. too bad as it feels great when new. Would not recommend buying. Use the new Fizik Enduro bar tape. Doesn't wear out like the Lizard Skinz.
Hey there!
One thing you might want to try is picking up another set of this stuff and not stretching it at all when installing. I've installed countless sets on bikes of customers of mine, and if the tape is stretched, the layers separate and those white wear marks appear way sooner than they should.
Comfort and Quality
- Familiarity: I've put it through the wringer
This bar tape is definitely my favorite. I have used it for a few years now and have been very satisfied with it. I prefer using the 2.5mm tape as it is just the right amount of cushioning for my preference. I would highly recommend this bar tape if you are looking for something new or if you have not yet tried it out!
Nice feel, didn't last
- Familiarity: I've put it through the wringer
I put Lizard Skins on one of my bikes. Loved the feel so much I put it on the other one. Then, the first bike started showing significant wear on the right side, after about 9 months. I typically ride 3x per week, maybe 150 miles a week. Bike was not crashed or leaned on anything. Just worn out from riding. The second set of Lizard Skins also now shows significant wear in the same area. Vary disappointing for such an expensive tape. I won't be replacing with more Lizard Skin.
Best tape available but pricey
- Familiarity: I've put it through the wringer
Tape is the best but the price sucks. But the best in grip and comfort
Feels Great, Didn't Hold Up
- Familiarity: I've put it through the wringer
I wanted to love this tape. I mean, it was 2x as much as the Fizik Microtex I had been using. It was love at first sight and first ride. There was enough pad to feel it, and the grip was much better than the Fizik. However, only about 2k miles in, and they're starting to wear through and the black tape is now white where I hold the bars just below the shifters. For $40, this shouldn't last 1/2 a season, when I was getting 2 years on my old tape. If it were $10 cork that'd be one thing, but for this price, no thanks. I'll unfortunately be going back to my old tape that didn't feel as nice, but lasted longer.
Totally agree. I posted a similar review above before I saw yours. Very disappointed with how long they last. Nice feel though.
Do you ride with gloves?
Yes, i use the Giro LTZ 95% of the time, and no gloves the other 5% of the time.
Don't think about it, BUY THEM!!!
- Familiarity: I've put it through the wringer
Great feel with this tape. Soft grip, dampens any chatter, cleans super easy, adds a ton of personality with the different color combinations. Stop you search for new tape right here and BUY THEM!
It's the best
- Familiarity: I've put it through the wringer
Favorite bar tape out there for soft feel and tacky grip. I don't wear gloves when I ride, and Lizard Skin is one of the only tapes I've found that still holds it's texture all the same even when under heavy fire from sweat, rain or other road debris. Only complaint is it gets dirty really fast, especially the white. It looks great at first, but it's so tacky that it does pick up debris really quickly. Fairly easy to clean, but it doesn't really bother me to just replace it pretty regularly. Worth it to keep my ride looking good, and hands feeling fresh.
So comfy
- Familiarity: I've used it several times
I run this tape on both of my bikes that have drop bars and don't think I would ever bother with a different tape. It is very comfortable and doesn't get sticky from glue bleeding in the heat like I've had happen on other tape. It wraps pretty smooth and looks nice. Good grip. Get some
Not real lizard skin.
Not only is this tape tacky and durable, but it's surprisingly cushy. The colors are also nice and tacky, which is important if (like me) you appreciate a well-matching bike.
The pink really pops, btw.
Love it!
These tape is almost perfect. It is soft, extremely durable, and Looks really awesome. I gave it four star instead of 5 as it does not clean as well as i thought it was going to. Don't get me wrong it cleans well, but my expectations where set high by what people had told me. Other than that nothing to complain about with these.
new favorite bar tape
- Familiarity: I've put it through the wringer
I changed out of traditional cork to this stuff about a month ago. I ride daily. Over the last 30 days, Ive gone from complaining about the price to wondering how I got along without it. Super tacky feel, grips well even in rain. Cushy as heck. Very comfortable ride. Dampens some road vibration at the bars. Overall, a great product.
Don't Judge Before You Ride It
- Familiarity: I've put it through the wringer
While most know Lizard Skins as a mountain bike brand, this is a legit product for your road or cross bike. I've used this almost exclusively the last couple years for a few basic reasons:
1/ It's durable. More than most any cork tape. Really
2/ It's incredibly comfortable. If the 2.5 isn't your jam, there is a cushier size just for you.
3/ It's easy to keep clean, so you can run the euro white all day long, and your bike will look great.
In short, I highly recommend you give it a whirl. Your bike will look great, and your hands will love you for it.
best bar tape
- Familiarity: I've put it through the wringer
when your bar tape starts to fall of or is just time to change it, you need to pick up this bar tape, not only does it look good, its super comfy, has a lot of padding, and is very easy to wrap on your bars.
Lizard Skin
- Familiarity: I've used it several times
I have been a fan for this tape for some time. It is very comfortable; has excellent grip, and cool colors. Now the negative. It is does not have very good durability; developes gaps; and discolors or shows dirt readily. I have also used Cinelli and Arundel, both of which have strengths and weaknesses.
Opinion has Changed
- Familiarity: I've put it through the wringer
I have been using this tape for years. At first I loved it. I could get two seasons out of it and 10K miles easy. Excellent feel. The last four or so rolls I've bought have been a little short for my Time bars and the tape has not adhered well, gapping on the tops after only a month of use. I think DSP may be using a different adhesive. Disappointed that I have to look for a new favorite tape.
Top layer prone to peeling
Tape feels good but starting peeling fairly quickly in a few months. Google it. Went with Fizik Performance 3mm.
DSP Tape
- Familiarity: I've used it several times
This stuff kicks just as much ass as everyone else says. Super tacky and comfortable. Depending on how you tape it you can keep it relatively thin or bulk up in certain areas by overlapping it closer. I knew it would be the perfect grip for my girlfriends first road bike to help kill road chatter. Mission accomplished.
Thanks for this pic, really helped me out!
Comfy, thick
- Familiarity: I've used it several times
The extra padding is nice for riding without gloves, but interferes with the shifters on my SRAM Red levers. Have to adjust the braking to keep the shift levers from getting stuck on the bar tape. Have not had this problem with thinner bar tape.
Had plenty of length to do my bars. Like really plenty, discarded about a foot on each side when I finished, and I use continuous multiple wraps around the brake hoods rather than use the short strip that comes with the kit. Finishing tape is nice, sticky to both the tape to finish it off, and to my hands when riding.
It's sticky, providing a good grip, even with sweaty hands.
I'll likely use Lizard Skins again, but a thinner tape next time.
Super Comfy
I just used this tape for the first time and I have to say, it's amazing. It's really comfortable and I love the grip on it. I'll definitely keep using this tape from here on out, I'm really happy with this purchase!


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Skin lesions of histoplasmosis are a symptom of widespread infection with the fungus Histoplasma capsulatum.
This article talks about skin lesions due to histoplasmosis only. For more general information on the disease, see: Histoplasmosis
Histoplasmosis is a fungal infection. It occurs throughout the world. In the United States, it is most common in the southeastern, mid-Atlantic, and central states.
Histoplasma fungus grows in soil. When particles become airborne, they can be breathed into the lungs, causing infection. Soil contaminated with bird or bat droppings may have a higher concentration of the fungus.
After infecting the lungs, the fungus travels to distant areas of the body, including the skin. This is a sign of widespread (disseminated) infection. Skin lesions can be caused by an immune response to the infection (usually a rash called erythema nodosum or erythema multiforme), or by the fungus itself when it spreads to the skin.
Widespread infection is most common in immunosuppressed people, such as those with AIDS or cancer, or those who have had a transplant.
The symptoms may include:
In some cases, a biopsy of the skin lesion can identify the fungus. Rashes due to erythema nodosum and erythema multiforme, however, usually do not have fungus in them. Blood and urine tests may help detect the fungus in some cases.
Antifungal drugs, such as amphotericin B, itraconazole, and ketoconazole, are the usual treatments. Antifungals may be given intravenously depending on the form or stage of disease. In some cases, long-term treatment with antifungal drugs may be needed.
The outlook depends on the form of histoplasmosis and the condition of the individual's immune system. Death can occur in some cases.
The skin lesions may be similar to skin problems from other infections or illnesses. Notify your health care provider if you develop any suspicious lesions on your skin, so that you may be tested correctly.
Histoplasmosis may be prevented by reducing exposure to dust in chicken coops, bat caves, and other high-risk locations. Wear masks and other protective equipment if you work in these environments.
Kauffman CA. Histoplasmosis. In: Goldman L, Ausiello D, eds. Cecil Medicine. 23rd ed. Philadelphia, Pa: Saunders Elsevier; 2007:chap 353.
A.D.A.M., Inc. is accredited by URAC, also known as the American Accreditation HealthCare Commission (www.urac.org). URAC's accreditation program is an independent audit to verify that A.D.A.M. follows rigorous standards of quality and accountability. A.D.A.M. is among the first to achieve this important distinction for online health information and services. Learn more about A.D.A.M.'s editorial policy, editorial process and privacy policy. A.D.A.M. is also a founding member of Hi-Ethics and subscribes to the principles of the Health on the Net Foundation (www.hon.ch)
The information provided herein should not be used during any medical emergency or for the diagnosis or treatment of any medical condition. A licensed medical professional should be consulted for diagnosis and treatment of any and all medical conditions. Call 911 for all medical emergencies. Links to other sites are provided for information only -- they do not constitute endorsements of those other sites. © 1997- 2013 A.D.A.M., Inc. Any duplication or distribution of the information contained herein is strictly prohibited.


text: Saguna, a pioneer of Mobile Edge Computing (MEC), makes mobile broadband faster, simpler and more economical with smart NFV software solutions. With Saguna, mobile operators improve user experience, network economics and monetization by bringing internet content and applications into the Radio Access Network (RAN); as close as possible to mobile users. Read more


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Sept. 6, 1962- Jan. 19, 2014
Angel Perez Jr. (Yuyi) passed away peacefully on Sunday, Jan. 19, 2014 at his home, surrounded by his family and friends. He was born in Havana, Cuba and came to the United States in 1980. Through his jewelry business, Angel gained many friends he considered part of his family. He loved dancing, gardening, reading, art, music, comedy, antiques and had a strong Catholic faith. He will be best remembered for his keen sense of humor, positive attitude, and unconditional love for his family and friends.
He is survived by his parents Angel and Elsa Perez; his loving wife of 27 years, Maribel Perez; daughter, Barbara (Ernesto) Balmaceda; sister, Raquel (Jorge) Galvan; nieces and nephew, Briana, Katia and Kayla Galvan, and Alyssa and David Payne; sister-in-law Marylin (Joshua) Payne; mother and father-in-law Yiyi and Luis Perez and many loving aunts, uncles and cousins.
Funeral services will be held at 1 p.m. Wednesday, Jan. 22, 2014 at The Basilica of St. Mary Star of the Sea.
In lieu of flowers, donations may be made to Hospice/VNA of the Florida Keys.


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it is really frustrating watching Jozy struggle on the USMNT because of Jurgy. he is trying to force his style instead of putting the players in the best situation.
quote:Possibly but the podcast I listened to yesterday Jurgy is very high on Shea right now, he's making the most of his minutes at Stoke and I bet Jurgy calls him in and starts him wide left for the Costa Rica game. Jurgy also is dead set on the Jones/Bradley combo in the midfield and said with time if they learn to play together and can grasp the concept that when one pushes forward the other holds that he would love to play without a true 6... The thought of that scares me
Joe Benny Corona has been starting and playing exceptional well as a left sided midfielder for Xolos in the Copa Libertadores. Maybe, just maybe, Klinsmann will call him and actually play him.
Wahl said he expects Boca to be left off the upcoming rosters.
He hasn't even been making the bench for his second division club. I'm thinking his ship is sailing. Preciate the years Carlos. Thank you for all your espn the body magazine spreads
I'm going to shite myself if Bradley is not the captain.
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Arizona Cardinals
Jeff King: Players 'take a lot of ownership' for 'Black Monday' decisions
Veteran tight end Jeff King has seen a lot in his seven NFL seasons, so when news came down Monday morning that the Arizona Cardinals had relieved head coach Ken Whisenhunt and general manager Rod Graves of their duties, he wasn't all that shocked.
"You always know that it's a possibility, but until the reality comes down you don't want to believe it," King said.
This is nothing new for Arizona's veteran tight end, though. King was a member of the 2010 Carolina Panthers that went 2-14 before canning head coach John Fox on "Black Monday" after nine years of service.
Even so, King admitted to Arizona Sports 620's Doug & Wolf that the news was still upsetting to hear from a player's perspective.
"I've been part of one of these before in Carolina when John Fox got let go and it's always a little bit unsettling," King said. "To some degree you take a lot of ownership in why a coach got fired."
There are plenty of reasons that likely led to the decision to fire Whisenhunt Monday, but as King noted, at the end of the season all that matters are wins and losses. While 2012 began with so much promise as the Cardinals raced out to a 4-0 record, a 1-11 finish combined with season-long issues at quarterback and along the O-line didn't help matters for the offensive-minded Whisenhunt.
"Ultimately, it falls on the players to make plays, and we didn't make enough for coach and Rod Graves to keep their jobs in the eyes of Mr. Bidwill," said King. "It's a bittersweet day.
"We just finished another season in the NFL, which you should be proud to do. But on the other hand, a guy who you looked up to [in Ken Whisenhunt], and for me, a guy who brought me to Arizona [in Rod Graves] were fired, which makes it tough."
King, who had 17 catches for 129 yards in 2012, was signed by Graves to a three-year deal in July 2011.
While Arizona finished 2012 with a higher win total than Carolina had in 2010, the former Virginia Tech star said he did see parallels between Fox's and Whisenhunt's departures.
"There are a lot of parallels between the two from the way they both went out to the uncertainty we had at the quarterback position in Carolina those last couple of years," said King. "Now, with what we are going through in Arizona, it's very similar to what happened before."
For fans in the Valley, the parallels between the two teams will hopefully end there. The Panthers hired Ron Rivera to replace Fox in 2011. In two seasons under Rivera, Carolina is just 11-21.
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Topics include all things NFL Draft. It's sports news skewered.
Haason Reddick, Cardinals linebacker + 1st Rd pick
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The Cardinals get their guy in Haason Reddick.
Doug Franz, Host: The Doug & Wolf Show
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Doug and B-Train talk about the impact of Haason Reddick on the Cardinals
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Matt tells B-Train about the 49ers big night in the first round of the draft


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23:36. Ensure all the information you provide is accurate.
Please enter the details of the car, driver and championship / series. It is important that all boxes are completed with as much information as possible to ensure that your car is placed into the correct group.
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Books for Christian Teens
Browse our broad selection of Christian books for teens. Whether you are looking for a fiction or nonfiction book to read, Family Christian has you covered. Christian teen books are available in a wide variety of topics and genres. Look through our selection to find the book you are looking for.
There are no products matching the selection.


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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.3 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the page "GNU Free Documentation License".
The copyright and license notices on this page only apply to the text on this page. Any software or copyright-licenses or other similar notices described in this text has its own copyright notice and license, which can usually be found in the distribution or license text itself.


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Drupalevents.ch Codesprint 2012: Translation management & workflows
This Drupal code sprint in Switzerland is a week-long event which will define and implement tools that will let organisations efficiently translate content on websites powered by the open source Drupal content management system. The resulting plug-in, the Translation Management Module, will be a key tool for reducing both the cost and effort in maintaining multilingual Drupal websites.
Drupal already powers multilingual websites today, but the translation and maintenance processes can be challenging and complex. The goal of this code sprint is to enable anyone with the requisite language skills to be able to translate and maintain multilingual content–its articles, pages, blog entries, and so on–on a Drupal website without having to learn any Drupal-specific skills. Professional translation services will be able to connect to their customers' Drupal websites to provide language services directly fro their own systems. The Translation Management Module will also provide translation-, quality-, and financial-control functionality, putting it in a position to become the standard solution for multilingual Drupal websites.
Miro Dietiker, Partner at MD Systems, and co-organiser of the code sprint, comments: "The code sprint will create and standardise important functionality for Drupal. The translation service providers we have contacted thus far are very supportive of this work and are working to adapt and reprogram their own systems to work seamlessly work with our standardized translation management functionality. I guess that there are at least 150 thousand multilingual Drupal sites online and we are looking forward to maintaining and expanding this functionality for a long time to come to help all these sites manage their multilingual content."
About Drupal: Drupal is free, open-source software that powers over a million websites and online applications. It runs on industry-standard hosting platforms and connects to virtually all legacy systems. Drupal's success has spawned an enormous business ecosystem, and thousands of pieces of add-on software extend what it can do. Learn more at drupal.org.
About the code sprint: Drupalevents.ch is bringing together 21 Drupal developers for seven days of intense coding. At standard rates, these 147 work-days of Drupal development to create seamless APIs for website translation and workflow management are worth roughly a quarter of a million dollars. Sponsors of the code sprint include Supertext, Microsoft, and Acquia.


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quote:You white?
Well I made the first layaway payment anyway
quote:buds what? Link?
Just ordered Glockzilla from buds
quote:I know the feeling.
Christmas breaks me every year and I didn't want to fork out that kind of money in one payment. I don't "need" a pistol right now, so layaway was the best option.
buds what? Link?
Also,whats with the auction shite on LINK
You white?
quote:basically QuiBids for guns.
It's a high risk/high reward site. You can pick up a brand new pistol for irt cheap, but you can also lose 325 dollars and have nothing to show for it
Christmas breaks me every year and I didn't want to fork out that kind of money in one payment.
quote:I have the exact one sitting on my kitchen table right now. Also have a .40 barrel for it that makes it shoot almost like a .22. It is heavy so there isnt much kick with the .40 shooting through it.
BTW-Why did you choose to purchase from them?
I also have a longer barrel that I am waiting to try out on some deerz
quote:Just got the regular extension. Will post pics in a little bit. It isn't really my "thing" to post what I have, but I will hook it up this once b/c the 10mm club is small
Yea I'm going to see how it shoots at 50-60 and determine whether to get the barrel extension. Did you buy from lone wolf with external ports?
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Taken in the rocks above Lower North Canyon Camp. Our party was camped at the upper camp. High winds frustrated my efforts to GigaPan. The entire setup was blown over by the wind during an earlier attempt even up in the canyon with my TrekPod walking stick/tripod. Tough as nails, the GigaPan was undamaged and took ...


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It's my understanding that GW did not pardon the two agents, but simply commuted thier sentences. Is that not correct?
Matt McKenzie
"Thinking is the hardest work there is, which is probably the reason why so few engage in it." Henry Ford
That is correct. That is what they (agents and their lawyers) applied for, not a pardon. Given the fact it took so long and the conspiracy necessary to get them convicted in the first place they felt it was not realistic to get a pardon so they went with the commutation instead.
Scooter Libby has spent enough time in jail for his perjury. Commuting his sentence was the correct thing to do IMHO.
I recall there was a president who lied consistently until a little blue dress shed new light on his story. He never spent a minute in jail.
Don's girls:
FC AFC Flyway's Ruby B. Gonia - a Carbon daughter and now a grandma (my avatar)
FC AFC Flyway's Long Tall Sally - Ruby's daughter. Bred to FC AFC Nike which produced Maggie.
Flyway's Iron Lady (Maggie) - Ruby's granddaughter. Maggie's the new puppy in the house. She is now running in the Derby.
1. Obstruction of Justice
2. False statements to FBI investigators (Concerning conversations with Tim Russert)
3. Perjury to the Grand Jury (Russert conversation)
4. Perjury to the Grand Jury (Cooper conversation)
Your statement " His supposed crime came after the investigation was underway and the prosecutor knew that Richard Armitage was the leaker" infers that once a investigation is underway, anything that is discovered after it is started is something you can't be charged with is just not true.
Let's not forget that the perjury charges are the same offenses that Bill Clinton commited and was impeached for. If I remember right it was the right wingers screaming that the rule of law must be upheld and that justice must be served.
I think the Plame matter was so badly handled that the only decent thing was to commute Libby's sentence. Novak and Armitage were more culpable than Libby and they skated. Libby was protecting Old Sureshot. I think he knew he was headed for a fall.
in the next four years we will look back and think w was a great president


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November 7, 2009: New Urban Legend?
Gnomes. Yes, gnomes. Apparently unhappy with being demoted from "player character race" to "monster" in the latest edition of that game, they've begun terrorizing teens in Argentina. The Sun has the story; YouTube has the blurry videos.
-- Paul Chapman
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Web Stories
Brentano String Quartet to perform, Feb. 23
Posted January 13, 2006; 12:49 p.m.
The Brentano String Quartet will perform the works of Princeton faculty members and graduate students in a Composers' Ensemble concert scheduled for 8 p.m. Thursday, Feb. 23, in Taplin Auditorium, Fine Hall.
The award-winning Brentano String Quartet became the first quartet-in-residence at Princeton in 1999. The quartet will perform works by Princeton faculty members Paul Lansky, Martin Scherzinger and Dan Trueman and graduate students David Little, Betsey Biggs and Miriama Young.
Admission is free.


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About Laminate Flooring
At Bestlaminate, we know that the width of laminate planks can make or break your room's design. Consider your room's size and personal preference when ordering narrow plank laminate flooring or wide plank flooring, but don't fret. We have free samples available, so you can easily determine what laminate flooring is right for you!
Choosing Wide or Narrow Plank Laminate Flooring
Classic laminate flooring adds an upscale look to any home. Choosing a suitable board width, however, can sometimes feel like an overwhelming challenge with so many available options, which range from very narrow (less than three inches across) to wide planks (which may be five to seven inches, on average).
When deciding on your ideal floor, consider your existing decor, room size and personal preference to help you determine whether narrow plank laminate flooring or wide plank flooring will be the best fit for you.


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Dear Mr. Dad: My seven-year old is very stressed. He's constantly worried, can't seem to focus in school, and almost always seems to be on edge. A friend suggested that we get our daughter to meditate. Sounds kind of kooky to me, but my friend insists that it's a good thing. What do you think?
A: Despite having spent a good portion of my life either in Berkeley or just a few miles away, I used to be very skeptical about meditation and all the supposed benefits. It's always sounded a bit too good to be true. After all, how could something so simple reduce stress and anxiety, lower your blood pressure and your risk of having a heart attack or stroke, cure insomnia, reduce chronic pain, help you fight off illness, combat depression , improve your memory and your grades, and make you taller, smarter, and better looking? But the reality is that with the exception of the taller and better looking parts, there's actually scientific evidence behind all of the claims (and one could argue that reducing your stress, anxiety, and depression might make you walk a little taller and smile a lot more, which could improve your looks). Oh, and just so you know, these benefits have been found in children as well as adults.
While there's little argument that meditating produces some pretty spectacular results, the problem has always been to explain exactly why it works. Some recent research has found that meditation helps open blood vessels, which in turn reduces blood pressure. And that reduces the risk of heart attack and stroke. Other studies have found that meditators are able to control certain brain waves that help brain cells communicate with each other and make it easier to concentrate. But does it really matter why it works? Bottom line is that it's not going to hurt to give it a shot, and it could very well help a lot.
Okay, now that you know that meditation isn't as kooky as you'd thought, let's talk about how to make it part of your child's life.
- Start by making it a part of your life too. Young children learn by imitating and if you're doing it, they'll want to join. The steps below will work just as well for you as for your child.
- Don't get bogged down by the name. There are all sorts of meditation styles: Transcendental, Zen, Mindfulness, to name just a few.
- Block out some time. 15-20 minutes at a stretch is good for adults. For kids, 5-10 minutes is plenty, especially when you're just starting.
- Find a quiet place. The fewer outside distractions (TV, radio, conversations, etc), the better.
- Get comfortable. You don't have to be twisted into some painful pretzel-like pose or levitate a foot off the ground. You can meditate sitting in a comfortable chair, lying down, walking, or even swimming.
- Focus on something. That could be a "mantra" (a word or phrase) or an object. But my suggestion is that you start with the simplest thing of all: your breath. Slowly count "one" for the first inhale, hold for two seconds, then exhale. Then "two" for the next set, and so on. I'm betting you won't get to "three" before your mind starts heading off in 127 different directions at the same time. When that happens, resist the urge to criticize yourself for losing focus. Everyone does, so just observe that your mind has wandered and gently bring yourself back to your breathing and start counting again.