Want this question answered?
Lippershey first discovered a dark-line spectrum.
No, its an absorption spectrum
We can see non-luminous objects because the light reflect off the object and into our eyes that's why at night you can only see a faint out line of the objects around you
Dark-line spectrum is a "photo-negative" of emission spectrum. It is the gaps that appear in precisely the same location as corresponding bright lines. produced by a cool gas with a hot solid and you
Intensity of spectral line show the abundance of different elements in the light source. Every element has its own "fingerprint" which can indicate its presence.
1. Glow discharge lamp 2. Electrode discharge in spectrometry
There are several kinds of spectra. Bright line spectrum, or emission spectrum, is when light emitted by a gas has an electrical discharge going through it, and it produces a spectrum of just a few isolated parallel lines.
Lippershey first discovered a dark-line spectrum.
Line Spectrum
No, its an absorption spectrum
Dark lines especially in solar spectrum have been named as Fraunhofer lines. These line are good examples for line absorption spectrum
dark-line spectrum...
atom give line spectrum because it is sharukh khan and molecule is salman khan that is why it give continiuos spectrum
We can see non-luminous objects because the light reflect off the object and into our eyes that's why at night you can only see a faint out line of the objects around you
The spectrum of sunlight is continuous while for hydrogen is line spectrum (discontinuous)
No. Atomic emission spectrum is non-contiuous and it is named as line spectrum.
Wavelengths of absorbed or emitted photons Every line in a line spectrum is caused by a transition, from one quantum state to another quantum state, involving electrons.