GED® Science: Stars, Galaxies & the Universe › 2. Properties of Stars: Temperature, Color, and Brightness
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2. Properties of Stars: Temperature, Color, and Brightness

GED® Science: Stars, Galaxies & the Universe · preview lesson

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Not all stars look the same in the night sky — some are bright, some dim, some bluish-white, some orange-red. These differences reflect real physical properties.

Temperature and Color:
A star's surface temperature controls its color. This follows the same physics as a heating metal:

ColorTemperatureExample
Blue-whiteVery hot (~20,000–50,000 K)Rigel
WhiteHot (~7,500–10,000 K)Sirius
YellowMedium (~5,500–6,000 K)Sun
OrangeCooler (~3,500–5,000 K)Arcturus
RedCoolest (~2,500–3,500 K)Betelgeuse

Brightness — Luminosity vs. Apparent Magnitude:

  • Luminosity is the total energy a star actually emits — its true brightness.
  • Apparent magnitude is how bright a star looks from Earth. A very luminous star far away can look dimmer than a less luminous star nearby.

A star appears bright if it is intrinsically luminous, or if it is close to Earth — or both.

Size matters too: a star of the same temperature but larger surface area emits more total light. Giant and supergiant stars can be hundreds of times larger than the Sun.

Quick Check

Two stars have the same temperature. Star A is much larger than Star B. Which one is more luminous?

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