Emission Spectra of Common Elements

What Stars Are Made Of

Atoms and elements are found throughout the universe. We know this because the same spectra seen in laboratories are also seen in light from the stars. The discovery of Helium was a surprising result of this knowlege. We now know it as the second most common element. We did not detect it on Earth until its spectrum was discovered in light from the Sun.

Atoms and Elements

The atoms are the building blocks of matter. Atoms have a nucleus of protons and neutrons and are surrounded by rapidly moving electrons. There are only 92 naturally occuring types of atoms. Substances made from each of the different types of atoms are called elements: hydrogen, oyxgen, carbon and gold are some well known examples.

How Elements Produce Emission Spectra

When elements are vapourised and heated, their electrons jump in energy level. When the electrons fall back to their resting states, they emit photons of light. When such light is passed through a spectroscope, the photons produced by the different jumps appear as coloured bands of light.

Elements Can Be Identified From Their Spectra

Each element produces its own set of spectral lines. Like finger prints for humans, spectra can identify elements. Elements in a star's atmosphere can be identified from lines in the spectrum of the star's light.

The Emission Spectra Of The Most Common Elements

The spectra of the sixteen most abundant elements in the universe are given below. Apart from Iron - Fe and Xenon - Xe, they are located in the first four rows of the periodic table of elements.

1
H

The First Twenty Elements

2
He

3
Li

4
Be

5
B

6
C

7
N

8
O

9
F

10
Ne

11
Na

12
Mg

13
Al

14
Si

15
P

16
S

17
Cl

18
Ar

19
K

20
Ca

31
Ga

32
Ge

33
As

34
Se

35
Br

36
Kr

Hydrogen H
Helium He
Oxygen O
Carbon C
Nitrogen N
Neon Ne
Magnesium Mg
Silicon Si
Sulfur S
Iron Fe
Aluminum Al
Calcium Ca
Argon Ar
Sodium Na
Krypton Kr
Xenon Xe

References


This page re-presents material from J Talbot's Laser Stars site.

The data for the spectra is from the Astronomical Data Center and the National Space Science Data Center through the World Data Center for Rockets and Satellites.