The Hertzsprung-Russell Diagram

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Plotting Stars on the HR Diagram

For this activity, you will plot stars on a simply HR Diagram, based on absolute magnitude and spectral type. There are two tables below, one of the brightest stars visible from Earth, and one of the nearest stars to Earth. Print out the HR Diagram template and then plot the stars from the first table in one color (say blue). Next plot the stars from the second table in a different color (say red). Once you have plotted all the stars note any patterns you see, and see if you can understand why or why not the patterns are there.

Note that there is some overlap between the two tables. For instance, the star Sirius A (being the brightest star visible from Earth and the 9th closest star to the Sun) is on both. You might want to use a third color to plot these. It likely will be cumbersome to put all the star names and/or designations on the chart (unless you have very small handwriting!). In fact, you don't really need them anyway, as all you are looking for are patterns. (After you have thought about the patterns, if any, and what may cause them, click here: Patterns.)

Note on the Spectral Types. The Sun is a G2V, meaning that it is a "G" star, subclass 2, and of a luminosity class V, signifying Main Sequence. Canopus is an A9II, meaning that it is an "A" star, subclass 9, with a luminosity class II, signifying a "bright" giant star. You also will notice some with designations such as "DA." These are white dwarf stars with no luminosity class ranking. Many of the spectral types end with a small letter such as "m" or "e." These are additional classifications indicating specific characteristics of the star's spectrum. You needed be concerned about them -- just consider the main spectral type. Now will you need the distances in light years, which are provided for your edification. Also, a few stars appear in both tables, and some stars do not have names per se, so their alphanumeric designation is provided instead.

Star data adapted from a list on Chris Nolan's Constellations site, originally from Norton's 2000.0, 18th edition.

The Brightest Stars:

Common Name Distance (light years) Absolute Magnitude Spectral Type
Sun - 4.8 G2V
Sirius A 8.6 1.4 A1Vm
Canopus 74 -2.5 A9II
Rigil Kentaurus 4.3 4.4 G2V + K1V
Arcturus 34 0.2 K1.5IIIp
Vega 25 0.6 A0Va
Capella 41 0.4 G6III + G2III
Rigel ~1400 -8.1 B81ae
Procyon 11.4 2.6 F5IV-V
Achernar 69 -1.3 B3Vnp
Betelgeuse ~1400 -7.2 M2Iab
Hadar 320 -4.4 B1III
Acrux 510 -4.6 B0.5Iv + B1Vn
Altair 16 2.3 A7Vn
Aldebaran 60 -0.3 K5III
Antares ~520 -5.2 M1.5Iab
Spica 220 -3.2 B1V
Pollux 40 0.7 K0IIIb
Fomalhaut 22 2.0 A3Va
Becrux 460 -4.7 B0.5III
Deneb 1500 -7.2 A2Ia
Regulus 69 -0.3 B7Vn
Adhara 570 -4.8 B2II
Castor 49 0.5 A1V + A2V
Gacrux 120 -1.2 M3.5III
Shaula 330 -3.5 B1.5IV

 


The Nearest Stars

Common Name Distance (light years) Absolute Magnitude Spectral Type
Sun - 4.8 G2V
Proxima Centauri 4.2 15.5 M5.5Vc
Rigil Kentaurus 4.3 4.4 G2V
Alpha Cen B 4.3 5.7 K1V
Barnard's Star 6.0 13.2 M3.8V
Wolf 359 7.7 16.7 M5.8Vc
BD +36 2147 8.2 10.5 M2.1Vc
Luyten 726-8A 8.4 15.5 M5.6Vc
Luyten 726-8B 8.4 16.0 M5.6Vc
Sirius A 8.6 1.4 A1Vm
Sirius B 8.6 11.2 DA
Ross 154 9.4 13.1 M3.6Vc
Ross 248 10.4 14.8 M4.9Vc
Epsilon Eri 10.8 6.1 K2Vc
Ross 128 10.9 13.5 M4.1V
61 Cyg A 11.1 7.6 K3.5Vc
61 Cyg B 11.1 8.4 K4.7Vc
Epsilon Ind 11.2 7.0 K3Vc
BD +43 44 A 11.2 10.4 M1.3Vc
BD +43 44 B 11.2 13.4 M3.8Vc
Luyten 789-6 11.2 14.5  
Procyon A 11.4 2.6 F5IV-V
Procyon B 11.4 13.0 DF
BD +59 1915 A 11.6 11.2 M3.0V
BD +59 1915 B 11.6 11.9 M3.5V
CoD -36 15693 11.7 9.6 M1.3Vc

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