Webb image archive
Continuous Spectra (Blackbody Curves) of Stars
Graphs of brightness vs. wavelength of three objects of different temperature. A blackbody curve is a type of continuous spectrum that is directly related to the temperature of an...
- Date
- Dec 13, 2023
- Observatory
- James Webb Space Telescope
- Credit
- NASA / ESA / CSA / STScI
- Archive ID
- 01F8GF8WYBCQVKTGPX3MA58182
Graphs of brightness vs. wavelength of three objects of different temperature. A blackbody curve is a type of continuous spectrum that is directly related to the temperature of an object. A star with a temperature of 8,000 kelvins (roughly 8,000 degrees Celsius or 14,000 degrees Fahrenheit) is brighter and looks bluer than a star that is 3,000 K (2,700°C or 5,000°F ), which is dimmer and redder. A blackbody spectrum can be used to calculate the temperature of an object. (Although stars are not perfect blackbodies, the blackbody curve describes the shape of a star’s overall spectrum quite well.)
Credits
Illustration
NASA, ESA, Leah Hustak (STScI), Andi James (STScI)