The angular size of the smallest features that the telescope can see
;-)
Angular resolution can be calculated by dividing the wavelength of light by the diameter of the aperture. The formula is: Angular resolution = 1.22 x (wavelength of light / diameter of aperture). This formula gives the smallest resolvable angle that can be distinguished between two closely spaced objects.
Angular resolution refers to the ability of an optical instrument, such as a telescope or camera, to distinguish between two closely spaced objects in the field of view. It is a measure of the smallest angle between two point sources that can still be resolved as separate entities. Higher angular resolution means better ability to distinguish fine details in an image.
Angular acceleration and linear acceleration are related through the radius of the rotating object. The angular acceleration is directly proportional to the linear acceleration and inversely proportional to the radius of the object. This means that as the linear acceleration increases, the angular acceleration also increases, but decreases as the radius of the object increases.
When an object spins its wheels, it creates angular momentum. This is because the spinning motion generates a rotational force that causes the object to keep spinning. So, spinning the wheels is a way to introduce and demonstrate the concept of angular momentum.
Linear acceleration and angular acceleration are related in rotational motion through the concept of tangential acceleration. In rotational motion, linear acceleration is the rate of change of linear velocity, while angular acceleration is the rate of change of angular velocity. Tangential acceleration is the component of linear acceleration that is tangent to the circular path of rotation, and it is related to angular acceleration through the equation at r , where at is the tangential acceleration, r is the radius of the circular path, and is the angular acceleration. This relationship shows that as the angular acceleration increases, the tangential acceleration also increases, leading to changes in the linear velocity of the rotating object.
Angular resolution can be calculated by dividing the wavelength of light by the diameter of the aperture. The formula is: Angular resolution = 1.22 x (wavelength of light / diameter of aperture). This formula gives the smallest resolvable angle that can be distinguished between two closely spaced objects.
For telescopes of the same size: if the wavelength gets longer, the maximum theoretical angular resolution gets larger (i.e., worse).
The resolution of a camera with a 12MP sensor is 12 megapixels.
No, they do not. The angular resolution of a telescope is determined by the wavelength of the radiation it is measuring and its diameter. Since optical telescopes detect shorter wavelengths than radio telescopes, they generally have better angular resolution for viewing fine details.
Angular resolution refers to the ability of an optical instrument, such as a telescope or camera, to distinguish between two closely spaced objects in the field of view. It is a measure of the smallest angle between two point sources that can still be resolved as separate entities. Higher angular resolution means better ability to distinguish fine details in an image.
Stars are very far away. Eyes just haven't got enough angular resolution. You can help it artificially with technology. Larger the thing, better the angular resolution.
The resolution of a camera with a 12MP sensor is 4000 pixels by 3000 pixels.
the lens and eye piece
Optical
The angular resolution formula in astronomy is given by the equation: θ = 1.22 * λ / D, where θ is the angular resolution, λ is the wavelength of light, and D is the diameter of the telescope. This formula determines the smallest angle at which two objects can be distinguished by a telescope. A smaller angular resolution means better clarity in celestial observations, allowing for finer details to be seen.
If the angular separation of two stars is smaller than the angular resolution of your eyes, they will appear as a single point of light rather than two distinct stars. This is due to the limit of your eyes' ability to resolve fine details at such a close angular distance.
a light-collecting area equivalent to that of a much larger telescope.an angular resolution equivalent to that of a much larger telescope.both the light-collecting area and angular resolution of a much larger telescope.Correct answer: an anguar resolution equivalent to that of a much larger telescope. ;-)