-- A concave mirror gathers the light and bunches it up all in one place, called
the "focus" of the mirror. There's a "real image" at that place, and you can
capture it with a piece of ground glass, tissue, photo-film, or light-sensitive device
at that place.
-- A plane mirror doesn't gather anything. It just kind of sends the light back
toward where it came from. It doesn't form any real image, and there's nothing
to capture.
To find the aperture of a reflecting telescope, you would measure the diameter of the primary mirror. The aperture of a telescope is the diameter of its primary light-gathering element, which in the case of a reflecting telescope, is the primary mirror.
Yes, the light gathering power of a telescope is directly proportional to the surface area of its objective lens or mirror. A larger objective can collect more light, allowing for brighter and clearer images to be observed. This increased light gathering power is beneficial for viewing faint or distant objects in space.
Inner curved surface is known as concave mirror because inner side of the spherical mirror is polished to reflect the light is called concave mirror,and concave mirror is know because concave mirror converges parallel beam of light.
Astronomical telescopes use a large concave mirror, a plane mirror, and a convex lens in their design. The concave mirror gathers light, the plane mirror reflects it to a more convenient viewing location, and the convex lens magnifies and focuses the image for observation.
To see an upright image of yourself in a concave mirror you must be closer than the principal focus. Hope this helps.
The size of a reflecting telescope is typically indicated by its aperture, which is the diameter of the primary mirror. Aperture size plays a crucial role in determining the light-gathering ability and resolving power of the telescope.
The telescope is cylindrical. Its primary mirror is concave.
A reflecting telescope.
mirror with a concave parabolic figure
a concave mirror and an angled plane mirror
Concave mirror of a reflecting telescope
In front of the mirror
In front of the mirror
Concave means bulging inward - reflecting telescopes use this sort of mirror. The first telescope designed to use one was invented by Isaac Newton and they are therefore called "Newtonian" telescopes.
a. concave mirror b. a convex lens c. a plane mirror or d. all the above.
70 mm. The numbers refer to the diameter of the main lens or mirror; the larger this number, the more light-gathering the telescope is, and also, the higher its resolution will be.70 mm. The numbers refer to the diameter of the main lens or mirror; the larger this number, the more light-gathering the telescope is, and also, the higher its resolution will be.70 mm. The numbers refer to the diameter of the main lens or mirror; the larger this number, the more light-gathering the telescope is, and also, the higher its resolution will be.70 mm. The numbers refer to the diameter of the main lens or mirror; the larger this number, the more light-gathering the telescope is, and also, the higher its resolution will be.
concave mirror