| x-ray wavelengths |
| ultraviolet wavelengths |
| optical wavelengths |
| infrared wavelengths |
| radio wavelengths |
| the temperature of the Earth's upper atmosphere is different from that of the atmosphere near the ground. |
| the absorption lines of gases in the upper atmosphere are different from those of gases near the ground. |
| the emission lines produced gases in the upper atmosphere are different from those of gases near the ground. |
| the upper atmosphere is reflecting more moonlight than the atmosphere near the ground. |
| dust in the atmosphere is scattering sunlight. |
| It will look like Spectrum A. |
| It will look like Spectrum B. |
| It will look like Spectrum C. |
| It will look like Spectrum D. |
| It will look like Spectrum E. |
| It will look like Spectrum F. |
| It will look like Spectrum G. |
| 8 days |
| 8 hours |
| 8 minutes |
| 8 seconds |
| No time at all. You are already getting hit by the x-rays and gamma-rays. |
| A 1-in sphere of iron heated to a temperature of 4000 degrees |
| A 1-in sphere of lead heated to a temperature of 3000 degrees |
| a 1-in sphere of hydrogen gas heated to a temperature of 6000 degrees |
| A 1-in sphere of liquid mercury heated to a temperature of 5000 degrees |