2. Properties of Stars: Temperature, Color, and Brightness
GED® Science: Stars, Galaxies & the Universe · preview lesson
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:
| Color | Temperature | Example |
|---|---|---|
| Blue-white | Very hot (~20,000–50,000 K) | Rigel |
| White | Hot (~7,500–10,000 K) | Sirius |
| Yellow | Medium (~5,500–6,000 K) | Sun |
| Orange | Cooler (~3,500–5,000 K) | Arcturus |
| Red | Coolest (~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.
Two stars have the same temperature. Star A is much larger than Star B. Which one is more luminous?
More surface area at the same temperature means more total light emitted — Star A is more luminous.
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