Chemical Components: Mostly hydrogen, then helium. Since the star is a class
M, its spectrum is expected to have strong absorption lines of helium and TiO. TiO stands
for titanium oxide and it is very common to find TiO in cooler stars such as Antares.
Location: RA = 16h 29m 24.4s, Dec = -26° 25' 55"
Spectrum analysis of most abundant chemical: hydrogen
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Stellar Classification: supergiant star (spectral type M1.5Iab)
http://earthsky.org/brightest-stars/antares-rivals-mars-as-the-scorpions-heart
Castorena, J. (2009, July 27). Spectra of Cool Stars. Retrieved September 25, 2015, from http://cosmos.ucdavis.edu/archives/2009/cluster9/catorena_jackeline.pdf
Espenak, F. (2012, January 21). Antares. Retrieved September 25, 2015, from http://astropixels.com/stars/Antares-01.html
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