The light-gathering power of an objective lens or mirror is proportional to its area, or equivalently,
to the square of its linear dimensions (radius, diameter, circumference).
If the focal ratios ('f' number) are the same, then the 1-m scope scoops up 102 = 100 times as much light
as the 10-cm job.
100 times difference in brightness is exactly the mathematical definition of six (6) magnitudes brighter/dimmer.
The diameter of the telescope aperture determines how much light the telescope can gather, which impacts the brightness and detail of the images it can produce. A larger aperture means more light can be collected, allowing for clearer and sharper views of celestial objects.
Newtonian telescope
Refracting telescope.
The size of a telescope almost invariably refers to the size of it's objective lens, or mirror. It translates to how much light the telescope can gather, not "how big it can magnify", which is very secondary.
A larger telescope has a greater light-collecting area, which allows it to gather more light from faint objects in space. This increased light-gathering ability improves the telescope's sensitivity and ability to detect fainter objects, providing astronomers with clearer and more detailed images. Additionally, a larger telescope can have higher resolution, allowing for sharper and more detailed observations of celestial objects.
The diameter of the telescope aperture determines how much light the telescope can gather, which impacts the brightness and detail of the images it can produce. A larger aperture means more light can be collected, allowing for clearer and sharper views of celestial objects.
A reflecting telescope.
Newtonian telescope
A radio telescope.
Refracting telescope.
Refracting Telescope.
It can gather more light
radiotelescope
Yes.
telescope
the reflecting telescope uses mirrors and lenses. The refracting telescope does not include the mirrors.
the reflecting telescope uses mirrors and lenses. The refracting telescope does not include the mirrors.