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The objective focal length of the Hubble Space Telescope is approximately 57.6 meters (or 188 feet). This long focal length allows Hubble to capture high-resolution images of astronomical objects, making it one of the most powerful space telescopes. The design includes a primary mirror with a diameter of 2.4 meters, which contributes to its ability to observe in various wavelengths, including visible, ultraviolet, and near-infrared light.
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What is the power of the eyepiece?
The magnification, or power, at which a telescope is operating is a function of the focal length of the telescope's main (objective) lens (or primary mirror) and the focal length of the eyepiece employed.
How does the eyepiece affect the total magnifacation in a telescope?
A telescope consists of two lenses. 1) The main lens which collects the light ( it is relatively bigger that eyepiece). 2) Eye piece , through which we see. Magnification of a telescope depends on the focal length of the eye piece and the main lens. Magnification = Focal length of the main lens / Focal length of the eyepiece . For example : If the focal length of the main lens is 12 units and the focal length of the eyepiece is 2 units , then the magnification will be 12/2 = 6.When the focal length of the main lens is constant , the focal length of the eyepiece is inversely proportional to the magnification.
How does a refracting telescope work to magnify distant objects?
A refracting telescope uses lenses to bend and focus light, which magnifies distant objects by making them appear closer and larger. The objective lens gathers and focuses light, while the eyepiece lens further magnifies the image for the viewer to see.
Why the aperture and focal length of objective of a telescope are large?
The aperture of a telescope is large to collect more light, which enhances the clarity and brightness of the observed images, especially for faint celestial objects. A larger aperture also allows for better resolution, enabling the telescope to distinguish fine details in astronomical objects. The focal length, on the other hand, is large to provide higher magnification and to create a more detailed image by allowing better separation of closely spaced objects. Together, these characteristics improve the overall performance and effectiveness of the telescope in astronomical observations.
How does a convex telescope work to magnify distant objects?
A convex telescope uses a converging lens to gather and focus light from distant objects. This lens bends the light rays towards a focal point, creating a magnified image that can be viewed through the eyepiece.
What will decreasing a telescope's eyepiece focal length?
The magnification of the telescope image is(focal length of the objective) divided by (focal length of the eyepiece).The focal length of the objective is fixed.Decreasing the focal length of the eyepiece increases the magnification of the image.(But it also makes the image dimmer.)
If a telescope has an objective with a focal length of 50 centimeters and an eyepiece with a focal length of 25 millimeter what will be the magnification?
20
What is the formula for calculating the angular magnification of a telescope?
The formula for calculating the angular magnification of a telescope is: Magnification focal length of the objective lens / focal length of the eyepiece.
What happens if you decrease a telescopes eyepiece focal length?
The magnification of the telescope image is(focal length of the objective) divided by (focal length of the eyepiece).The focal length of the objective is fixed.Decreasing the focal length of the eyepiece increases the magnification of the image.(But it also makes the image dimmer.)
Which lens in a refracting telescope has a shorter focal length?
The objective lens in a refracting telescope typically has a shorter focal length compared to the eyepiece lens. This is because a shorter focal length allows for higher magnification and better light gathering capabilities.
What is the power of the eyepiece?
The magnification, or power, at which a telescope is operating is a function of the focal length of the telescope's main (objective) lens (or primary mirror) and the focal length of the eyepiece employed.
How is magnifying power of telescope and a microscope are a affected by increasing the focal length of their objectives?
The magnification of a telescope M is the the focal length of the objective Fo over the focal length of the eyepiece Fe so increasing the focal length of the objective increases the magnification. The magnification of a microscope M is approximately tube length L/Fo x 25/Fe. Therefore increasing the focal length of the objective reduces the magnification.
What would be the effect on magnification to increase the focal length of microscope and telescope?
The focal length of a telescope is directly related to the magnification in that the longer the focal length, the more magnification you get from the telsceope. How the focal length of a telescope relates to the length of the telescope itself depends on the design of the telescope. In a refracting telescope, the focal length is approximately the length of the telescope. In a reflecting telescope, the focal length is roughly two time the length of the telescope.
What is the magnification of a reflecting telescope with an eyepiece of focal length 25 mm and an objective lens of focal length 2000 mm?
That's 80 power.
The magnification of a telescope is changed by changing the what?
The magnification of a telescope is the ratio of the effective focal length of the objective to the focal length of the eyepiece. For example, a small telescope's objective may have a focal length of 800mm. When an eyepiece with a focal length of 25mm is used, the magnification is 800/25 = 32. The term "effective focal length" refers to the focal length of the objective as affected by any "focal extender". Many telescopes are designed to have a short total size, but high power, by "folding" the optical path. A mirror-type objective with a focal length of perhaps 800mm is coupled with a smaller curved mirror that intercepts the last 200mm and extends it to 800mm, a 4x extension, so that the effective focal length of that objective is 3200mm. Use that with a 25mm eyepiece and the magnification is 3200/25 = 128. By the way, if a telescope is smaller than you are, it is seldom much use to view using a magnification greater than 50 to 100. Most objects are best viewed at relatively low powers such as 30 or so.
The magnification of a telescope is changed by changing the?
The magnification of a telescope is the ratio of the effective focal length of the objective to the focal length of the eyepiece. For example, a small telescope's objective may have a focal length of 800mm. When an eyepiece with a focal length of 25mm is used, the magnification is 800/25 = 32. The term "effective focal length" refers to the focal length of the objective as affected by any "focal extender". Many telescopes are designed to have a short total size, but high power, by "folding" the optical path. A mirror-type objective with a focal length of perhaps 800mm is coupled with a smaller curved mirror that intercepts the last 200mm and extends it to 800mm, a 4x extension, so that the effective focal length of that objective is 3200mm. Use that with a 25mm eyepiece and the magnification is 3200/25 = 128. By the way, if a telescope is smaller than you are, it is seldom much use to view using a magnification greater than 50 to 100. Most objects are best viewed at relatively low powers such as 30 or so.
How do you calculate the power of magnificaiton?
The power of magnification is calculated by dividing the focal length of the objective lens by the focal length of the eyepiece lens in a microscope or telescope. The formula is: Magnification = Focal Length of Objective Lens / Focal Length of Eyepiece Lens. For example, if the objective lens has a focal length of 10 mm and the eyepiece lens has a focal length of 25 mm, the magnification would be 10/25 = 0.4x. Additionally, in microscopy, total magnification can also be determined by multiplying the magnification of the objective lens by that of the eyepiece lens.
