Do you have to calibrate a telescope?
Collimation is the process of aligning all components in a telescope to bring light to its best focus. All telescopes need to be collimated at some point; however, it's easy to perform this task on some and a bit more involved for others.
Fortunately, collimating a reflector is simple. Once you get the process down, it takes only a few minutes. A laser collimator emits a beam that bounces off the primary and secondary mirrors in a reflector and (hopefully) back onto the collimator's target.
Without getting into the crazy but cool scientifical physics and math of it, collimation is, simply put, the physical alignment of your telescope's optics. If your telescope is not properly collimated, it will be impossible to properly focus, no matter the sky conditions.
Over time, dirt and dust can build up on the lens of your eyepiece, causing the images you see to be less clear. To clean your eyepiece, all you need is some distilled water and a soft, lint-free cloth. Lastly, make sure you are using the right eyepiece for the job.
The James Webb Space Telescope has reached a new milestone: “Fine-phasing” calibration is now complete, which means all 18 hexagonal submirrors are acting as a single unit, and are now focused and aimed perfectly at a single spot in one of JWST's many scientific cameras.
Collimation is the process of aligning all components in a telescope to bring light to its best focus. All telescopes need to be collimated at some point; however, it's easy to perform this task on some and a bit more involved for others.
I recommend checking collimation every time you take your Newtonian out for observing, as there is usually a 50% chance it needs to be tweaked at the very least.
Experienced planetary observers use 20x to 30x per inch of aperture to see the most planetary detail. Double-star observers go higher, up to 50x per inch (which corresponds to a ½-mm exit pupil). Beyond this, telescope magnification power and eye limitations degrade the view.
Yes, you must align your 'scope with every observing session you embark upon.
That black spot you are seeing is the shadow of the secondary mirror, indicating that you have not achieved correct focus."
Do I need to polar align my telescope?
Polar alignment is an essential first step toward a night of visual observation or astrophotography. Why is it so important? By aligning the axis of your telescope mount with the motion of the sky, you can accurately track objects in space.
Astigmatism causes stars to appear as lines, crosses, or squares at the edge of the field. It is the most significant problem with wide-angle eyepieces, especially with low-f/number telescopes. Using a Barlow lens with the eyepiece will often suppress astigmatism dramatically.

All telescopes, refractors, reflectors, and catadioptrics, as well as all cameras, have inverted images because that's the way all lenses and mirrors work. Even the lenses in your eyes invert the images of the world, and your brain erects them.
The theoretical limit of useful magnification for a telescope is 50 or 60 times the telescope's aperture in inches, or two times the aperture in millimeters.
One disadvantage of this orbit is that, since it's a full 930,000 miles (1.5 million km) from Earth — three times the distance from the Earth to the moon — JWST is too distant for repairs like the ones that Hubble experienced.
The iconic Hubble Telescope and James Webb Space Telescope will be roundly beaten by the new Giant Magellan Telescope. It is expected to be 4 times more powerful than the James Webb Telescope.
In addition to its out-of-this-world mosaic, Webb was also able to take a selfie. Using a specialized pupil imaging lens, the telescope captured the below image of itself.
In the northern hemisphere the best direction to align the telescope is so it has its best view to the south. The reason for this is to do with the tilt of Earth's axis of rotation.
Manually point your telescope as best you can at the target, and then look through the eyepiece. Hopefully, the object will be in the field of view, but if it isn't, use the slow motion control knobs or dials on your telescope's mount to make adjustments until the target is in the center of the eyepiece.
If you are unable to find objects while using your telescope, you will need to make sure the finderscope is aligned with the telescope. The finderscope is the small scope attached near the rear of the telescope just above the eyepiece holder. This is best done when the scope is first set up.
What are the 3 main factors that should be considered when choosing a telescope?
Instead, you should choose a telescope based on your observing interests, lifestyle, and budget.
A telescope's most important attribute is its size, meaning the diameter of its main mirror or lens. The bigger the telescope, the more light it collects, which allows you to see fainter objects. You can observe quite a lot with a telescope just 4 to 6 inches diameter.
A badly collimated telescope will display poor star shapes and other aberrations that will spoil the view. It is also important that the optical elements are aligned with the tube assembly, otherwise there can be problems with aligning the focuser, which is a purely mechanical part of the instrument."
X-ray field collimation differs from the use of electronic magnification in that the acquired field of view remains constant, and there is no improvement in the resultant spatial resolution performance (see below).
Refractors require the least collimation.
What Size Telescope Do I Need To See It? A 4” to 6” scope is adequate to spot Jupiter's Great Red Spot. Jupiter is nearly 390 million miles away from us. The large distance means that you will need to use a minimum 100x magnification to see the Great Red Spot.
The rings of Saturn should be visible in even the smallest telescope at 25x. A good 3-inch scope at 50x can show them as a separate structure detached on all sides from the ball of the planet.
The Andromeda Galaxy looks great through smaller telescope of, say, 4 inches in diameter.
Always use your telescope outside. Poking your telescope out of the window just doesn't work. The wave of heat or cool leaving your house will definitely interfere big time with what you're trying to view.
Choose firm, stable but soft ground such as the lawn. Make sure to place the telescope in an area shielded from local light sources, like the street lights. Simply placing the telescope nearer to a fence, for example, to shield it from the neighbor's security light can make a big difference.
Do you close one eye when looking through a telescope?
Close one eye at a time and the eye that still sees the object is the dominant eye.
The Sun is extremely bright and you can damage your eyes within a few seconds if you look at the Sun without protection. To view the Sun during a partial or annular eclipse you need to either look at a projection of the Sun or use a special-purpose solar filter—very dark sunglasses do NOT protect your eyes.
Telescopes work wonderfully but can they really see through clouds?! Of course not! Although surprisingly, there are probably a few people who honestly believe that a telescope is capable of revealing objects otherwise masked by cloud cover.
The brighter view and lower magnification can make Jupiter just look like a bright white featureless disk to your dark adapted eyes. Picking the right magnification is a balance between what the atmosphere will support, what the telescope will support, view brightness, and image scale.
Rotate the protractor until the string's shadow points to the Sun's known azimuth (measured from north through east) plus 180°. Finally, swivel the mount until the polar axis stands directly above 0° on the protractor. You are now polar-aligned.
If you are expecting to observe the stars and other celestial objects as you would at night, you are likely to be disappointed. Indeed, telescopes collect light from objects in the sky and magnify it, so it is important to have a dark sky to see more detail.
You should wear glasses for all low-power observing, but you can probably get away with taking them off when you are examining the Moon, planets, or anything else at high magnification.
Astigmatism occurs when either the front surface of the eye (cornea) or the lens inside the eye has mismatched curves. Instead of having one curve like a round ball, the surface is egg-shaped. This causes blurred vision at all distances.
By far the most common reason for non-round stars in a Newtonian telescope is poor collimation. This produces an optical aberration called coma. Some examples of the appearance of coma in images can be found in the diagram to the right. Keep in mind that coma may be combined with other optical problems.
Telescopes help us see objects more clearly. But if you look through the wrong end of the telescope, it does just the opposite: instead of seeing objects more clearly, you see them less clearly – and they seem even farther away. Think of your Bible as a telescope.
Why can't my telescope see a planet?
Even with a lower-power eyepiece like the 20mm, a view can be blurry because of the Earth's atmosphere. Heat waves and high-altitude winds move air around and cause differing temperatures of air to mix. This makes the air act like a weak lens that interferes with the light from a planet or a star by de-focusing it.
A low magnification of around 50x will show you the whole moon and give you the "big picture." But to see the moon at its best, try a high magnification, at least 150x. The moon can tolerate high magnification better than any object in the sky.
Optimum Magnification
Observational experiments usually find that, for deep-sky observing, the best detail can be seen with an exit pupil of between 2mm and 3mm. This would be a magnification of around 35-50x on a 4" scope, 70-100x on an 8" scope, and 120-175x on a 14" scope.
You want to see a diffraction pattern of concentric circles appear around it. Basically, this refers to circles around the star that might look a little wiggly. If the circles you see are not concentric, then your telescope needs to be collimated.
That black spot you are seeing is the shadow of the secondary mirror, indicating that you have not achieved correct focus."
Is your image out of focus? If the stars in your image appear fat, or they have a doughnut/ring shape to them, then your image is out of focus. The example shown above is a section of an image of NGC6025, taken by a 0.4m telescope. The image is out of focus due to a focussing issue with the telescope.
As a rule of thumb, get stargazing binoculars with an aperture of 35 mm to 60 mm aperture and a magnification of 7x to 10x. A pair of 7×35's is about the minimum acceptable for astronomical observing; 7×50's are better… this will give you the same magnification but a wider field of view.
- Step 1: Align the Finder Scope With the Eyepiece. ...
- Step 2: Orientate Yourself to the Image. ...
- Step 3: Locaton, Location, Location. ...
- Step 4: Give the Telescope Time to Acclimate to the Outdoor Conditions. ...
- Step 5: Clear Skies.
Collimating a Refractor
An out-of-collimation refractor will usually show elongated stars like coma in a Newtonian, like in the image below. The bottom images show what a star with a mis-collimated refractor looks like out of focus. The in-focus images are at the top.
They are artifacts caused by light diffracting around the support vanes of the secondary mirror in reflecting telescopes, or edges of non-circular camera apertures, and around eyelashes and eyelids in the eye.
Why can I see Jupiter through my telescope?
Jupiter is an interesting telescopic target thanks to its surface features made of different coloured bands and belts. Even in a small telescope, you will be able to see the different belts and zones along with the planet's north and south pole.
All telescopes, refractors, reflectors, and catadioptrics, as well as all cameras, have inverted images because that's the way all lenses and mirrors work. Even the lenses in your eyes invert the images of the world, and your brain erects them.
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