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The Hertzsprung–Russell Diagram

Explore 182 stars by temperature and luminosity.

182-star catalogue

Explore the stellar population

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Advanced filtersTemperature, distance, magnitude, radius, age, stellar type, spectral class, and constellation Optional · currently showing all stars

Temperature

2,500–40,000 K

Distance

0–31,623 ly

Apparent magnitude

−27.0–28.0

Radius

0.006–1,778 R☉

Age

1 Myr–12.6 Gyr
Stellar type
Choose one or more
Spectral class
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Constellations

Hertzsprung–Russell diagram of nearby and notable stars A scatter plot with stellar surface temperature decreasing from left to right and luminosity increasing from bottom to top.
Hotter
OBAFGKM
Cooler

Read the lives of stars from one diagram

Each point is a real star. Move over or select a point to inspect it, search by name, isolate a stellar type, limit the sample by distance, and switch between true radius and equal-size markers.

Temperature decreases from left to right, while luminosity rises upwards. This unusual arrangement reveals the diagonal main sequence, swollen giants above it, and faint white dwarfs below it.

Three patterns to look for

01

Follow the main sequence

Most stars form a diagonal band from hot, luminous blue stars to cool, faint red stars. This is where stars spend most of their lives fusing hydrogen.

02

Compare colour and heat

Blue-white stars on the left have hotter surfaces. Orange and red stars on the right are cooler—even when a giant’s large surface makes it extremely luminous.

03

Find the stellar outliers

Giants and supergiants sit above the main sequence. White dwarfs sit below it: very hot, but faint because their radiating surfaces are so small.