If the surface temperature of a star is 5,800K and the temperature within this same star is 10,000K, what type of spectra do we expect to see? Is it continuous, absorption, or emission?
in 3rd law:u told that cold gas will absorb photon then it would go 2nd orbit.as a result absorption spectrum will produce.but electron is not stable in that orbit.it will come down in his first orbit.then.would the absorption spectrum will produce????
I have a small doubt, • why do hot & dense sources (example - SUN) have continuous spectrum ? • why do hot and less dense sources (example - hydrogen gas in discharge tube) have line spectrum ? As all of them emit ElectroMagnetic radiation 🙄, so where comes the boundary ?
Thanks so much for the video. Very helpful, especially with the examples!
Extremely Helpful thank you
Well explained!
I love you! Thanks for the videos!!
Nice explanation and I loved your voice
Thank you for the video
If the surface temperature of a star is 5,800K and the temperature within this same
star is 10,000K, what type of spectra do we expect to see? Is it continuous,
absorption, or emission?
thank u bro
Thank u so much for video..
Thank you!
Last line is not visible
Sorry - got lost in the video conversion. A future update should fix the presentation.
Great
thank you sir
in 3rd law:u told that cold gas will absorb photon then it would go 2nd orbit.as a result absorption spectrum will produce.but electron is not stable in that orbit.it will come down in his first orbit.then.would the absorption spectrum will produce????
Anyone here from mr. Stover!!?
I have a small doubt,
• why do hot & dense sources (example - SUN) have continuous spectrum ?
• why do hot and less dense sources (example - hydrogen gas in discharge tube) have line spectrum ?
As all of them emit ElectroMagnetic radiation 🙄, so where comes the boundary ?