Model of the Solar Neighborhood

This is a model of the stars that are at most 12 light years from the sun (except for a few brown dwarfs recently discovered by WISE). I built the model in the winter of 2012-13. The stars it represents, along with their spectral types and distances from the sun in light years, are listed towards the bottom of this page.

The model is composed of painted solid wooden balls and dowels. The balls represent stars, and are sized and colored, to represent the stellar diversity in the solar neighborhood, according to the following scheme.

Spectral Type

brown dwarf

red dwarf

orange dwarf

yellow dwarf

blue-white dwarf

white dwarf

Ball Size

1-inch

1-inch

1.5-inch

1.5-inch

2-inch

1-inch

Ball Color

purple

red

orange

yellow

blue-white

white

Two stars are connected by a dowel if and only if they are no more than 10 light years away from one another. The longest dowel, which is also the only rod connected to only one ball (which represents the sun), indicates the direction of the galactic center. The surface of the table runs parallel to the galactic plane.

To construct the model, I calculated the necessary angles by transforming the coordinates from polar equatorial with 0 degrees at the vernal equinox (those that are found in most ephemerides) to polar galactic with the sun as origin and 0 degrees along the line that connects the sun to the galactic center. See the transformations here. I then drilled the holes at appropriate places in the balls and cut the dowels to appropriate lengths. I then painted the balls according to the scheme above, and painted each of the dowels. The model can be taken apart and put back together (as long as one is careful about keeping track of which dowels connect which holes in which balls).

The stars represented in the model are:

Star

Sol

Proxima Centauri

Alpha Centauri A

Alpha Centauri B

Bernard's Star

Wolf 359

Lalande 21185

Sirius A

Sirius B

Luyten 726-8 A

Luyten 726-8 B

Ross 154

Ross 248

Epsilon Eridani

Lacaille 9352

Ross 128

EZ Aquarii A

EZ Aquarii B

EZ Aquarii C

Procyon A

Procyon B

61 Cygni A

61 Cygni B

Struve 2398 A

Struve 2398 B

Groombridge 34 A

Groombridge 34 B

Epsilon Indi A

Epsilon Indi Ba

Epsilon Indi Bb

DX Cancri

Tau Ceti

GJ 1061

Spectral Type

yellow dwarf

red dwarf

yellow dwarf

orange dwarf

red dwarf

red dwarf

red dwarf

blue-white dwarf

white dwarf

red dwarf

red dwarf

red dwarf

red dwarf

orange dwarf

red dwarf

red dwarf

red dwarf

red dwarf

red dwarf

blue-white dwarf

white dwarf

orange dwarf

orange dwarf

red dwarf

red dwarf

red dwarf

red dwarf

orange dwarf

brown dwarf

brown dwarf

red dwarf

yellow dwarf

red dwarf

Distance (ly)

0.00

4.24

4.37


5.96

7.78

8.29

8.58


8.73


9.68

10.32

10.52

10.74

10.92

11.27



11.40


11.40


11.53


11.62


11.82



11.83

11.89

11.99

There are four brown dwarfs that were discovered by WISE, and were announced in the spring of 2013, not long after I finished constructing the model. As a result, they are not depicted. Those stars are:

Star

Luhman 16 A

Luhman 16 B

WISE 0855-0714

WISE 1506+7027

Spectral Type

brown dwarf

brown dwarf

brown dwarf

brown dwarf

Distance (ly)

6.59

7.20

11.09

I plan to integrate these newly discovered neighbors into a future version of the model.

© 2016 T. Scott Dixon All Rights Reserved