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Original file (SVG file, nominally 576 × 432 pixels, file size: 49 KB)
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Summary
| Description |
English: Plot shows the temperature a black-body would need to be to emit a given amount of thermal radiation. This is sometimes referred to as the "effective temperature." The effective temperature is typically close to the actual temperature of the matter emitting the radiation. The temperature range includes temperatures commonly relevant to Earth's atmosphere.
The curve simply follows from the Stefan-Boltzmann law, with emissivity taken to be 1. |
| Date | |
| Source | Own work |
| Author | Rhwentworth |
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File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 19:48, 11 June 2023 | | 576 × 432 (49 KB) | Rhwentworth | Adjusted text |
| 12:22, 11 June 2023 |  | 576 × 432 (44 KB) | Rhwentworth | Fixed typo | |
| 12:11, 11 June 2023 |  | 576 × 432 (44 KB) | Rhwentworth | Uploaded own work with UploadWizard |
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