Disclaimer: This blog does not contain full documentation of the laboratory procedures, neither does it pretend to provide a complete lab instruction. Instead, it is designed to document special moments in the physics lab. Enjoy!
Showing posts with label Light spectrum. Show all posts
Showing posts with label Light spectrum. Show all posts
Spectrum Lab
As
you can see from the three pictures above, when using the spectrometer towards
the sunlight (1), ceiling light (2), and lamp light (3) they each have different
emission spectra.
Reema
Daylight vs. ceiling light
This is a picture of the spectrometer on daylight/natural light. The colors of the wavelength of the light gradually and seamlessly change from one color to the other without any kind of division.
To the right is a picture of the spectrometer on a fluorescent ceiling light. The colors of the wavelength are divided and the separation between the colors are distinct. Unlike the colors from natural light which have colors, red to yellow, to green, to light blue, to dark blue, the picture of the fluorescent light only has colors red, green, and blue.
Post and photos:
Marjorie
Line Spectra
The
purpose of this lab is to measure wavelengths of different light sources using
a device called a spectroscope. I have provided sample pictures containing the wavelength
measurements of the following light sources taken with a camera through a
spectroscope.
Wavelength measurements are measured by
nanometers (nm) (x10^9). The purpose of measuring wavelengths is used to
specify the strength of the colors measured by their peaks to relate to
specific elements on the periodic table of elements. Each element has its own
wavelength frequency, and by using a spectroscope you are able to identify
which element is present. Astrophysicists and space explorers use this in search
of planets for inhabitability and resources. If a planet contains too many
poisonous gases it would be identified using spectroscopy and we would better
know to avoid landing on those planets or sending humans to explore those
planets.1. Scattered Sunlight
Wavelength Measurements: Red- 6.7nm-6.2nm, Orange- 6.1nm-5.9nm, Yellow- 5.9nm-5.8nm, Green- 5.8nm-5.3nm, Blue- 5.2nm-4.8nm, Indigo- 4.8nm-4.0nm, Violet- 4.0nm->
2. Light Bulb
Wavelength Measurements: Red- 6.1nm, Orange- 6.0nm-5.8nm, Yellow- (not visible), Green- 5.5nm, Blue- 5.0nm-4.8nm, Indigo- 4.4nm, Violet- (not visible)
3. Fluorescent
Light
Wavelength
Measurements: Red-
6.7nm-6.2nm, Orange- 6.2nm-6.0nm, Yellow-
5.9nm, Green-
5.8nm-5.5nm, Blue-
5.2nm-4.9nm, Indigo-
4.8nm-4.5nm, Violet-
4.4nm
By Nicholas
Spectrometer
The differences between the two observations is the sunlight spectrometer, light blends together and is hard to notice distinct changes where the light bulb shows clear lines and distinct changes through the spectrum.
It is this way due to elements from the sun have
much more where light bulbs are artificially made.
In the pictures below the left picture notes that is a picture of spectrometer at the light bulb, where the picture on the right is the sun.We can learn about the bulb or the sun is that
there are clear distinctions of measuring in nanometers through the
spectrometer.
Gian
Gian
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