Star Log Project

List of Stars Star 1 Star 2 Star 3 Star 4 Star 5 Star 6 Star 7 Star 8 Star 9 Star 10 Star 11 Star 12 Star 13 Star 14 Star 15 Designation	Element	Wavelength (nm)
y	O2	898.765
Z	O2	822.696
A	O2	759.370
B	O2	686.719
C (Hα)	H	656.281
a	O2	627.661
D1	Na	589.592
D2	Na	588.995
D3 or d	He	587.5618
e	Hg	546.073
E2	Fe	527.039
b1	Mg	518.362
b2	Mg	517.270
b3	Fe	516.891
b4	Mg	516.733

Designation	Element	Wavelength (nm)
c	Fe	495.761
F (Hβ)	H	486.134
d	Fe	466.814
e	Fe	438.355
G' (Hγ)	H	434.047
G	Fe	430.790
G	Ca	430.774
h (Hδ)	H	410.175
H	Ca+	396.847
K	Ca+	393.368
L	Fe	382.044
N	Fe	358.121
P	Ti+	336.112
T	Fe	302.108
t	Ni	299.444

Small particles that make up everything imaginable within the universe. Scientists have spent centuries what it is that makes up matter. In recent times, astronomers have studied the chemical composition of distant stars. They are able to do so because, elements when super-heated emit a specific wavelength enabling astronomers to identify them. In this project, we will choose 15 solar bodies and find their chemical composition, just as astronomers do when finding new celestial bodies.

https://www.google.com/url?sa=i&rct=j&q=&esrc=s&source=images&cd=&cad=rja&uact=8&ved=0CAcQjRxqFQoTCMad992XnMgCFcF8kgodi7sL2Q&url=http%3A%2F%2Fscienceblogs.com%2Fstartswithabang%2F2012%2F08%2F14%2Fhow-many-colors-are-really-in-a-rainbow%2F&psig=AFQjCNHaWauD1h9mNXdYeJH0ciPnA1xzOA&ust=1443613984189021

https://en.wikipedia.org/wiki/Astronomical_spectroscopy

https://en.wikipedia.org/wiki/List_of_largest_known_stars

http://www.astronoo.com/en/stars.html