For OmCheeto (astrospectroscopy)

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In summary, tried to do some astrospectroscopy last night (fail), but figured I'd share the results anyway. Taped a diffraction grating onto the lens flange (lens side, not camera side) to image some spectra- Sony worked much better for this- ended up having to use a wide-angle lens to capture the spectrum. Images from my backyard- one of a streetlight (with Jupiter and Spica visible), and the other a neighbor's back porch light. These are 6s ISO 1000 exposures: Unfortunately, the planet/starlight was just too faint for me to capture. The lights, however, have measurably different spect
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Tried to do some astrospectroscopy last night (fail), but figured I'd share the results anyway.

I taped a diffraction grating onto the lens flange (lens side, not camera side) to image some spectra- I was hoping to compare Jupiter, Spica, and Arcturus. For whatever reason, my old Sony worked much better for this- I think that Sony puts their sensor much closer to the lens flange than Nikon so the spectra still fall onto the chip. I ended up having to use a wide-angle lens to capture the spectrum, the trade-off being much less throughput. Images from my backyard- one of a streetlight (with Jupiter and Spica visible), and the other a neighbor's back porch light. These are 6s ISO 1000 exposures:

DSC_1799_zpsurajoicq.jpg


DSC_1810_zpsbfzsmxww.jpg


Unfortunately, the planet/starlight was just too faint for me to capture. The lights, however, have measurably different spectra (first one is the streetlight, most likely a Sodium lamp), the second an LED. Note also, the horizontal axis goes from red to blue and you can clearly see the Sodium lamp spectral peaks:

Plot%20of%20DSC_1799_zpsj5e4fhsk.jpg


Plot%20of%20DSC_1810_zps2lqsimfr.jpg


(for comparison: https://image.slidesharecdn.com/201...-all-you-need-to-know-7-638.jpg?cb=1358421058)
 
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A guy at my local Astro Society gave a talk about Spectroscopy and he had some great pictures and graphs of spectra he'd obtained with a diffraction grating, using a section of the digital colour i mage. You could distinctly see the overall curve which corresponded to the temperature of the chosen star and also some absorption lines. All from a humble back yard!
Andy Resnick said:
I think that Sony puts their sensor much closer to the lens flange than Nikon so the spectra still fall onto the chip.
We didn't discuss the optical arrangement but I sort of assumed he was using prime focus and just put the grating 'somewhere' up the tube and it all came out right. (I should have known better. Nothing just comes out right with Astrophotography.
 
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  • #4
I carved my diffraction grating to fit my lens.

2017.05.16.camera.customized.diffraction.grating.png


I'm also a big fan of "night lights" spectroscopy:

2017.01.09.0306.OmCheeto.porch.light.spectroscopy.png


hmmmm...
Was this thread inspired by the Pamela Gay interview from yesterday?
By the end of it, I had half a dozen new tabs on my browser open.
 
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  • #5
OmCheeto said:
<snip>
Was this thread inspired by the Pamela Gay interview from yesterday?

Nope- I was photographing the Markarian Chain and clouds started to move in, so I grabbed the opportunity to goof around.
 
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  • #6
Andy Resnick said:
Nope- I was photographing the Markarian Chain and clouds started to move in, so I grabbed the opportunity to goof around.
The last thing she mentioned was the upcoming eclipse.
That prompted me to check out the society she mentioned that she belongs to; "...I’m the Director of Technology and Citizen Science at the Astronomical Society of the Pacific."
There I found that they had the RSpec Explorer Spectrometer for sale. Only $440.
I thought that would be cool to own, but the price was a bit too much, so I'll probably stick with my $1.25 diffraction grating.
The RSpec Spectrometer also doesn't appear to have the range I'm looking for:
Spectral range is approximately 390 to 700 nanometers. Accuracy is generally 1% or better. Spectroscopic features as narrow as 3 nanometers can be measured.
That looks suspiciously like the visual range. If I'm going to spend more than $100 on something, it had better also measure IR & UV.
Perhaps 200 to 1500 nanometers.
I'm not really sure. Some day I'll research that.
(google google google)

Ok. After I win the lottery.
Low Cost GREEN-Wave Spectrometer
350-1150nm wavelength range
$1,948.00​
 
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  • #7
OmCheeto said:
There I found that they had the RSpec Explorer Spectrometer for sale. Only $440.
I thought that would be cool to own, but the price was a bit too much, so I'll probably stick with my $1.25 diffraction grating.`

Yeah, I'm with you- we hand out those cheap gratings to students (we buy in bulk, I think they end up about $0.50 each) and let them look at spectra themselves- why involve a computer?

Just decided to get a big sheet/roll of grating (like https://www.onlinesciencemall.com/p...=27348598342&gclid=CLOsw_nn-dMCFY-BaQod4x0CuA) to put over the front element of my telephoto. Not sure it will work, but I can afford the $6.50 to try. Science!
 
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  • #8
Success!

As per the image in post #4, I put a grating sheet in front of the lens and was easily able to get spectra of Jupiter, Spica, and Arcturus. The spectra are about 10 degrees off normal, so it took me a bit to realize that I can't look at the object itself in order to capture the spectra. By happenstance, the spectra of Jupiter and Spica appear together- Jupiter is off the frame to the upper right, Spica is off to the left to the lower left:
Jupiter%20and%20Spica_zpsutluojmu.jpg


Here's Arcturus:
Arcturus_zpsh1hguf8k.jpg


Now, using this to make quantitative measurements is tricky: Bayer filter, etc. Here are RGB lineplots through the spectra of Jupiter, Spica, and Arcturus:

Profiles%20of%20Jupiter_zpsd3boo5ah.jpg


Profiles%20of%20Jupiter%20and%20Spica_zpsrfzg9vrn.jpg


Profiles%20of%20Arcturus_zpsyxqjqcl1.jpg


You can see where Jupiter's spectrum overlapped Spica's (the narrow peak). It's not immediately obvious how these correspond to the different colors, but if I plot the spectral intensity ('brightness') rather than the actual colors in the same order, the difference is more clear:

Plot%20of%20Jupiter_zpsihbcwm7y.jpg


Plot%20of%20Jupiter%20and%20Spica_zpslwvlkf8o.jpg


Plot%20of%20Arcturus_zpsmvmo9y7x.jpg


Now, Spica's curve shows how predominantly blue it is, while Arcturus emphasizes the red end. Not sure why there is a 'notch' in the yellow band...
 
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1. What is astrospectroscopy?

Astrospectroscopy is a scientific technique used to study the composition and properties of objects in outer space, such as stars, planets, and galaxies. It involves analyzing the light emitted or absorbed by these objects to gather information about their chemical composition, temperature, and motion.

2. How does astrospectroscopy work?

Astrospectroscopy works by collecting and analyzing light from astronomical objects using specialized instruments called spectrographs. The light is split into different wavelengths, or colors, and then measured and recorded. This data can be used to identify the chemical elements present in the object and other physical characteristics.

3. What can astrospectroscopy tell us about the universe?

Astrospectroscopy can tell us a lot about the universe, including the chemical composition and physical properties of objects in space, the temperature and movement of stars and galaxies, and the evolution of the universe over time. It also allows us to study the formation of planets and the potential for life in other solar systems.

4. What are some practical applications of astrospectroscopy?

Astrospectroscopy has many practical applications, including helping astronomers better understand the origins and evolution of the universe, aiding in the search for habitable planets, and providing crucial data for space exploration missions. It is also used in industries such as medicine and environmental science to analyze the composition of materials and substances.

5. What are the challenges of using astrospectroscopy?

One of the main challenges of using astrospectroscopy is the vast amount of data that needs to be collected and analyzed. This requires advanced technology and computational power. Another challenge is the interference from Earth's atmosphere, which can distort the light from astronomical objects. This can be overcome by using telescopes in space or by using sophisticated correction techniques.

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