Editing 1517: Spectroscopy
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In the first and second panel the singer examines the spectra of a remote planet by ''watching the sunlight'' during the {{w|Transit (astronomy)|transit}} of the planet as this sunlight ''dances across the planet's face''. Finally we determine that breathable oxygen exists. Since we cannot (as Faith can) ''feel'' the planet we have to ''see'' it. And by doing this ''I can see you breathe''. | In the first and second panel the singer examines the spectra of a remote planet by ''watching the sunlight'' during the {{w|Transit (astronomy)|transit}} of the planet as this sunlight ''dances across the planet's face''. Finally we determine that breathable oxygen exists. Since we cannot (as Faith can) ''feel'' the planet we have to ''see'' it. And by doing this ''I can see you breathe''. | ||
β | Measuring the light output of stars (spectra) we are able to determine a number of details of the star, including rotation, relative radial velocity, chemical composition, temperature, and to some degree, distance and size. When a planet, as pictured, moves between the star and the observer, then by looking at the spectrum received, the viewer is able to determine the contents of the planet's atmosphere from the specific wavelengths of light that are {{w|Absorption spectroscopy|absorbed}} in this. If it turns out that the atmosphere absorbs the lines corresponding to molecular oxygen (O<sub>2</sub>) this is a clear indication that the planet has large quantities of breathable oxygen (but {{w|Exoplanet#Abiotic_oxygen|not necessarily life}}). | + | Measuring the light output of stars (spectra) we are able to determine a number of details of the star, including rotation, relative radial velocity, chemical composition, temperature, and to some degree, distance and size. When a planet, as pictured, moves between the star and the observer, then by looking at the spectrum received, the viewer is able to determine the contents of the planet's atmosphere from the specific wavelengths of light that are {{w|Absorption spectroscopy|absorbed}} in this. If it turns out that the atmosphere absorbs the lines corresponding to molecular oxygen (O<sub>2</sub>) this is a clear indication that the planet has large quantities of breathable oxygen (but {{w|Exoplanet#Abiotic_oxygen|not necessarily life}}). Since for most (though {{w|Anaerobic_organism|not all}}) |
+ | forms of life as we know it to exist and breathe, there must be oxygen in large amounts in the atmosphere, it is clear why [[Randall]] would be interested in exoplanets with oxygen. | ||
This comic came out four days after this article about [http://www.huffingtonpost.com/2015/04/23/nasa-nexss-search-for-life_n_7123788.html NASA's New NExSS Initiative]. {{w|NASA}} will search for signs of life on other planets, for instance by using "the light passing through the atmospheres of these exoplanets". And they "will study chemicals that have been detected on other worlds, such as oxygen and methane, to see if they were produced by biology". | This comic came out four days after this article about [http://www.huffingtonpost.com/2015/04/23/nasa-nexss-search-for-life_n_7123788.html NASA's New NExSS Initiative]. {{w|NASA}} will search for signs of life on other planets, for instance by using "the light passing through the atmospheres of these exoplanets". And they "will study chemicals that have been detected on other worlds, such as oxygen and methane, to see if they were produced by biology". |