Astrophysics (13) Flashcards
Lens
can be used to refract light. Lenses are used to focus light and to produce images of various objects.
The Universe
made up of billions of stars and galaxies. The distance between galaxies is measured in millions of light years. The Universe is about 13.8 billion years old.
Converging lens
refracts rays of light to a point.
Principal axis
the principal axis of a lens is an imaginary line that passes through the centre of a lens and through the centres of curvature of the faces of the lens.
Focal point
the focal point of a lens is the point at which rays parallel to the principal axis of the lens are brought to a focus.
Focal length
the focal length of a lens is the distance between the centre of the lens and the point at which rays parallel to the principle axis are brought to a focus.
Collecting power
is a measure of the light intensity gathered by a telescope. This is proportional to the square of the telescope’s diameter.
Brightness
the brightness of a star is a measure of how much visible light from the star reaches our eyes.
Luminosity
the luminosity of a star is the energy it emits per second, in all wavelengths.
Apparent magnitude
a star’s apparent magnitude is a measure of its brightness as it appears on the sky.
Astronomical unit
the average distance from the Earth to the Sun (AU) = 1.5×〖10〗^11m (2sf).
Light year (ly)
the distance travelled by light in one year = 9.46×〖10〗^15m.
Parallax
nearby objects appear to move relative to far-away objects, when viewed from a different angle. If the measured parallax angle is smaller, then the distance to the star is further.
Parsec (pc)
1pc = 3.26ly
Absolute magnitude
a star’s absolute magnitude is the apparent magnitude the star would have if it were 10pc away.